<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article">
 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">
    jamp
   </journal-id>
   <journal-title-group>
    <journal-title>
     Journal of Applied Mathematics and Physics
    </journal-title>
   </journal-title-group>
   <issn pub-type="epub">
    2327-4352
   </issn>
   <issn publication-format="print">
    2327-4379
   </issn>
   <publisher>
    <publisher-name>
     Scientific Research Publishing
    </publisher-name>
   </publisher>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="doi">
    10.4236/jamp.2025.1310201
   </article-id>
   <article-id pub-id-type="publisher-id">
    jamp-146908
   </article-id>
   <article-categories>
    <subj-group subj-group-type="heading">
     <subject>
      Articles
     </subject>
    </subj-group>
    <subj-group subj-group-type="Discipline-v2">
     <subject>
      Physics 
     </subject>
     <subject>
       Mathematics
     </subject>
    </subj-group>
   </article-categories>
   <title-group>
    The Quantum-Mechanical Explanation of the Thermal Radiative Behaviour of Helium
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Thomas
      </surname>
      <given-names>
       Allmendinger
      </given-names>
     </name>
    </contrib>
   </contrib-group> 
   <aff id="affnull">
    <addr-line>
     aGlattbrugg, Switzerland
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     10
    </day> 
    <month>
     10
    </month>
    <year>
     2025
    </year>
   </pub-date> 
   <volume>
    13
   </volume> 
   <issue>
    10
   </issue>
   <fpage>
    3596
   </fpage>
   <lpage>
    3615
   </lpage>
   <history>
    <date date-type="received">
     <day>
      20,
     </day>
     <month>
      September
     </month>
     <year>
      2025
     </year>
    </date>
    <date date-type="published">
     <day>
      28,
     </day>
     <month>
      September
     </month>
     <year>
      2025
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      28,
     </day>
     <month>
      October
     </month>
     <year>
      2025
     </year> 
    </date>
   </history>
   <permissions>
    <copyright-statement>
     © Copyright 2014 by authors and Scientific Research Publishing Inc. 
    </copyright-statement>
    <copyright-year>
     2014
    </copyright-year>
    <license>
     <license-p>
      This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/
     </license-p>
    </license>
   </permissions>
   <abstract>
    In order to apply the recently published planar atom model of Helium with well-defined electron trajectories onto the results about the thermal radiative behaviour of gases, which was published by the author in 2016, the latter publication had to be partly questioned since its theoretical evaluation contains several errors. Nevertheless, the basic statements made therein, applying the kinetic gas theory, are still valid. Since they cannot be assumed as commonly known, first, the description of the measurement equipment and the applied light sources, the most relevant results, and the basic theoretical interpretation were recapitulated. The essential empirical result of those measurements was the observation that any gas is warmed up when it is thermally irradiated, but solely up to a limiting temperature where the absorption intensity of the gas is equal to its emission intensity. This effect was first observed in air and in CO
    <sub>2</sub>, whereby the limiting temperatures were nearly equal. But it also occurred in the noble gases Argon, Neon and Helium, whereby the limiting temperatures depended on the type of gas. These differences could be explained by means of the kinetic gas theory, assuming proportionality between the collision wattage of the atoms and the radiation wattage. As a consequence, an additional energy must exist, which does not appear in the classic thermodynamic theory, and which must be due to an oscillating process at the electrons. In order to explain this, using the example of Helium, the said atom model is adduced. Since it exhibits well-defined electron trajectories—in contrast to the orthodox orbital model where the electrons underlie probabilities of presence—such an oscillation process, implicating an excited state of the electrons, is well describable. Thereto, a modified harmonic oscillator comes into question. This oscillator is eccentric since it rotates around the nucleus. Moreover, it is asymmetric since its energetic conditions are asymmetric with respect to the orbit path. In particular, the quantum-mechanical condition of a standing wave must be fulfilled, i.e. the angular velocity ω
    <sub>osc</sub> of the oscillator must be an integer multiple of the angular rotation velocity ω
    <sub>rot</sub>, preferably 2. By equating the oscillation energy of the electrons and the radiation energy, which is determined by Einstein’s equation for the photoelectric effect, and by applying the theorem of conservation of momentum 
    <b>P</b> onto the collision process, thermodynamics could be bridged with quantum mechanics, delivering in the excited state an elliptic orbit. The essential difference between the orthodox and the alternative model consists in the fact that the orthodox model only considers the observers’ point of view, whereas the alternative model distinguishes between object and observer. Thereby, the isolated model is two-dimensional, obeying the here described quantum mechanical computation, whereas from the viewpoint of the observer, it is three-dimensional, due to the thermally induced rotation.
   </abstract>
   <kwd-group> 
    <kwd>
     Kinetic Gas Theory
    </kwd> 
    <kwd>
      2D-Atom Model of Helium
    </kwd> 
    <kwd>
      Thermal Radiation Absorption and Emission by Gases
    </kwd> 
    <kwd>
      Electronic Oscillation
    </kwd> 
    <kwd>
      Bridge Thermodynamics/Quantum-Mechanics
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>1. Introduction</title>
   <p>The adsorption and the emission of thermal radiation by gases both play a major role in atmospheric physics, in particular with respect to climate change, which is commonly ascribed to the increase of CO<sub>2</sub> in the atmosphere. In order to describe the thermal radiation intensity Φ of the atmosphere (measured in Wm<sup>−2</sup>), the Stefan-Boltzmann Relation is applied, which expresses coherence with the absolute temperature according to Φ = 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        σ 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         T 
       </mi> 
       <mn>
         4 
       </mn> 
      </msup> 
     </mrow> 
    </math> (σ = Stefan-Boltzmann constant). This relation was established at the end of the 19<sup>th</sup> century <xref ref-type="bibr" rid="scirp.146908-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.146908-2">
     [2]
    </xref>, being derived from laboratory measurements made by Dulong and Petit in the first quarter of the 19<sup>th</sup> century <xref ref-type="bibr" rid="scirp.146908-3">
     [3]
    </xref>. In fact, it concerns Black Bodies, implying radiation and counter-radiation, but it seems also applicable to the atmospheric radiation, using Equation (1):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         Φ 
       </mi> 
       <mrow> 
        <mi>
          s 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          l 
        </mi> 
        <mi>
          a 
        </mi> 
        <mi>
          r 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mi>
          α 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mi>
        σ 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            s 
          </mi> 
          <mi>
            u 
          </mi> 
          <mi>
            r 
          </mi> 
          <mi>
            f 
          </mi> 
         </mrow> 
         <mn>
           4 
         </mn> 
        </msubsup> 
        <mo>
          − 
        </mo> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            a 
          </mi> 
          <mi>
            m 
          </mi> 
          <mi>
            b 
          </mi> 
         </mrow> 
         <mn>
           4 
         </mn> 
        </msubsup> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (1)</p>
   <p>where α = colour-dependent reflection coefficient;</p>
   <p>T<sub>surf</sub> = temperature of the Earth surface or of an opaque body at the Earth surface;</p>
   <p>T<sub>ambient</sub> = temperature of the ambient atmosphere.</p>
   <p>Even though Equation (1) delivers plausible results for solar heat collectors, it may be a fallacy, due to an accidental coincidence of the atmospheric behaviour with that of a Black Body, since its absorption behaviour does not at all correspond to the absorption behaviour of a Black Body (which is by definition total). Moreover, this relation does not describe the temporal occurrence of this equilibrium state. But in particular, it appears strange that the radiation of a gas (air) would solely depend on the temperature and not on the pressure, too.</p>
   <p>Nevertheless, it was incorporated into the atmosphere theory by Arrhenius <xref ref-type="bibr" rid="scirp.146908-4">
     [4]
    </xref>, describing the counter-radiation of the atmosphere against the Earth surface. Thereby, the additional fault was made by referencing it to the Space-temperature, whereby T<sub>Space</sub> = T<sub>amb</sub> = 0 K (or strictly speaking 2.7 K), thus disregarding the complex influence of the intermediate atmosphere.</p>
   <p>This approach is in principle still in use (see, e.g. <xref ref-type="bibr" rid="scirp.146908-5">
     [5]
    </xref>). Thereby, several theories exist about the so-called radiative heat transfer between Earth surface and Space, implicating the assumption that the atmosphere radiates like a Black Body, and applying the Stefan-Boltzmann Relation. But they disregard the fact that this relation is solely valid under conditions of equilibrium, and in particular that in this regard, the so-called greenhouse gases, such as CO<sub>2</sub>, which are generally blamed for climate change, do not occur. Furthermore, apart from the fact that the CO<sub>2</sub>-concentration is very low (namely about 400 ppm = 0.04%), according to <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref>, the spectrum of solar light loses intensity over its whole—also visible—range, due to absorption by the atmosphere. However, the citation of the diagram depicted in <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref> could not be found. At all, the wave-length-specific light intensity would not be easily detectable. Nevertheless, the considerable intensity difference of sunlight between the extra-terrestrial position and the position at the Earth surface is evident and measurable.</p>
   <fig id="fig1" position="float">
    <label>Figure 1</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-#/media/File:Solar_spectrum_en.svg">
       https://en.wikipedia.org/wiki/Solar_irradiance#/media/File:Solar_spectrum_en.svg
      </xref>.<xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 1. Solar irradiance spectrum above atmosphere and at surface.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId19.jpeg?20251031033236" />
   </fig>
   <p>A further but significant problem arises from the difficulty in transferring photometric or spectroscopic data to the behaviour of thermally irradiated gases. In fact, there is no coherence between the respective results—originally delivered by Tyndall in 1860 <xref ref-type="bibr" rid="scirp.146908-6">
     [6]
    </xref>, and later ascertained by IR-spectra—and the warming-up temperature of gases.</p>
   <p>Consequently, no method for measuring the warming-up of a thermally irradiated gas existed, and it was not evident that this warming-up is due to vibrations of the molecular bonds which are associated with the absorption of infrared rays. Rather, the hypothesis emerged that another cause could be linked to the ability of gases to absorb and emit thermal radiation, namely the oscillation of the atomic electron shell. This proved to be all the more true when the own results, first published in 2016 by the author <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref>, revealed that any gas can absorb and emit thermal radiation, even the noble gases.</p>
   <p>The therein described measurements were made using tubes by Styrofoam, which exhibits a low heat-capacity, minimizing the interference between gas and tube. The measuring equipment and the most important results are recapitulated in Chapter 2. The essential, so far nowhere reported phenomenon was the fact that an irradiated gas attains after a certain time a limiting temperature where the absorption intensity is equal to the emission intensity.</p>
   <p>Similar results for air, carbon-dioxide and Argon were independently reported by Seim and Olsen in 2020 <xref ref-type="bibr" rid="scirp.146908-8">
     [8]
    </xref>, but without an evaluation in the same manner. Besides, the influence of thermal radiation on the thermal behaviour of gases was not considered so far, solely the collision-induced spectral absorption (CIA). It was discovered in 1949 by Crawford and co-workers for forbidden vibrational transitions in compressed O<sub>2</sub> and N<sub>2</sub> gases (so-called super-molecular systems) <xref ref-type="bibr" rid="scirp.146908-9">
     [9]
    </xref>. Till 1993, 800 original papers were published in the field, also including noble gas mixtures <xref ref-type="bibr" rid="scirp.146908-10">
     [10]
    </xref>. Since then, further papers appeared, e.g. <xref ref-type="bibr" rid="scirp.146908-11">
     [11]
    </xref>. But a direct correlation between spectral absorbance and thermal behaviour of gases does not exist.</p>
   <p>Based on the empiric results given in <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref>, an explanation was given using the kinetic gas theory, which connects the heat content of a gas to the kinetic translation energy of its particles (molecules or atoms). And indeed, a correlation was found between the collision wattage and the radiation wattage. Thereby, the different limiting temperatures of Argon, Neon and Helium could be explained.</p>
   <p>However, its theoretical explanation was not feasible since thermal radiation does not occur in thermodynamics. But obviously, an additional energy must exist which is responsible for the electromagnetic radiation, acting as transformer. The only possible cause is an oscillation or pulsation of the electronic shell of the (noble gas) atoms, obeying quantum-mechanical criteria.</p>
   <p>And thereto, the recently published atom model of Helium with well-defined planar electron trajectories <xref ref-type="bibr" rid="scirp.146908-12">
     [12]
    </xref> comes into question, namely by applying an eccentric oscillation process onto the electron rotation and regarding the standing wave condition.</p>
   <p>
    <xref ref-type="bibr" rid="scirp.146908-"></xref>The key principle of that model consists in the hypothesis that both electrons which diametrically circle round the nucleus obey the conservation of momentum ħ (=h/2π). But since their partial three-dimensional pathways proceed orthogonally, the resulting mutual pathway is two-dimensional, exhibiting the angular momentum 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msqrt> 
       <mn>
         2 
       </mn> 
      </msqrt> 
      <mi>
        ℏ 
      </mi> 
     </mrow> 
    </math> (see <xref ref-type="fig" rid="fig2">
     Figure 2
    </xref>).</p>
   <fig id="fig2" position="float">
    <label>Figure 2</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 2. 2D-model of Helium composed by two imaginary orthogonal orbits of the electrons, according to <xref ref-type="bibr" rid="scirp.146908-11">
       [11]
      </xref>.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId23.jpeg?20251031033236" />
   </fig>
   <p>This model is two-dimensional. However, it describes an isolated Helium atom in the ground state. In reality, each atom is part of a gas, being in translation as well as in rotation move. And as a consequence of the latter one, it apparently becomes three-dimensional. Thereby, the stochastic thermodynamics—particularly the kinetic gas theory—and the exact quantum mechanics can be bridged theoretically. This is subject of the following chapters.</p>
  </sec><sec id="s2">
   <title>2. Recapitulation of the Measurements and of the Applied Kinetic Gas Theory</title>
   <p>The respective measurements described in <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref> were carried out by means of one-meter-long quadratic tubes from Styrofoam using sunlight (<xref ref-type="fig" rid="fig3">
     Figure 3
    </xref>) as well as artificial light (<xref ref-type="fig" rid="fig4">
     Figure 4
    </xref>), whereby the light source was positioned at the top. In order to measure the temperature course, three thermometers were mounted at three positions.</p>
   <fig id="fig3" position="float">
    <label>Figure 3</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 3. Solar tube.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId24.jpeg?20251031033237" />
   </fig>
   <fig id="fig4" position="float">
    <label>Figure 4</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 4. Heat radiation tube.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId25.jpeg?20251031033238" />
   </fig>
   <p>The experimental difficulties and the instrumental optimizations are discussed in <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref>. The largest difficulty consisted in the fact that the intensity of artificial light decreases inversely proportional to the square of the distance, even if no absorption occurs. That became apparent while—in the cases where artificial light was used—at the different measuring points, temperature differences arose (<xref ref-type="fig" rid="fig5">
     Figure 5
    </xref>), whereas that was not the case when sunlight was used (<xref ref-type="fig" rid="fig6">
     Figure 6
    </xref>). In any case, the temperature ascent began simultaneously at the three thermometer positions, which delivered evidence that the warming-up was induced by thermal radiation and not by thermal conductivity.</p>
   <fig id="fig5" position="float">
    <label>Figure 5</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 5. Heat radiation tube (not optimized), filled with air, 150 W IR-spot: Temporal courses at the three thermometer positions (Figure 9 in <xref ref-type="bibr" rid="scirp.146908-7">
       [7]
      </xref>).</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId26.jpeg?20251031033238" />
   </fig>
   <fig id="fig6" position="float">
    <label>Figure 6</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 6. Outdoor solar-tube, filled with air, irradiation wattage 1000 Wm<sup>−2</sup> (measured by an electronic pyranometer): Temporal courses at the three thermometer positions (Figure 20 in <xref ref-type="bibr" rid="scirp.146908-7">
       [7]
      </xref>).</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId27.jpeg?20251031033237" />
   </fig>
   <p>Initially focused on CO<sub>2</sub>, which is pivotal for the current climate-change theory, and which was the inducement for these measurements, the investigations were extended to other gases, firstly to air and an artificial Nitrogen/Oxygen 4:1 mixture. Surprisingly, they exhibited a quite similar behaviour as pure CO<sub>2</sub> (<xref ref-type="fig" rid="fig7">
     Figure 7
    </xref>). But even noble gases turned out to be active, namely in such a way: When a gas is thermally irradiated, it is warmed up till a limiting temperature is reached where the absorption intensity of the gas (measured in Wm<sup>−</sup><sup>2</sup>) is equal to its emission intensity. Therefore, it can be concluded that any gas is not only able to absorb but also to emit thermal radiation. However, the limiting temperature depends on the gas type, e.g. it is lower for Helium than for Argon (<xref ref-type="fig" rid="fig8">
     Figure 8
    </xref>).</p>
   <fig id="fig7" position="float">
    <label>Figure 7</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 7. Average warming-up rates for different gases, measured by the heat radiation tube (method A, 150W IR-spot, medium thermometer position) (Figure 25 in <xref ref-type="bibr" rid="scirp.146908-7">
       [7]
      </xref>).</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId28.jpeg?20251031033237" />
   </fig>
   <fig id="fig8" position="float">
    <label>Figure 8</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 8. Average warming-up rates for different gases, measured by the heat radiation tube (method A, 150W IR-spot, medium thermometer position) (Figure 26 in <xref ref-type="bibr" rid="scirp.146908-7">
       [7]
      </xref>).</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId29.jpeg?20251031033237" />
   </fig>
   <p>As already mentioned, these differences could be explained by applying the kinetic gas theory, which assumes correlation between the average kinetic translation energy of the particles (molecules or atoms) and the absolute temperature, according to Equation (2):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mover accent="true"> 
        <mi>
          E 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mi>
          k 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
        <mi>
          t 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          m 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mn>
         2 
       </mn> 
      </mfrac> 
      <mi>
        m 
      </mi> 
      <msup> 
       <mover accent="true"> 
        <mi>
          w 
        </mi> 
        <mo>
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        </mo> 
       </mover> 
       <mn>
         2 
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      </msup> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         3 
       </mn> 
       <mn>
         2 
       </mn> 
      </mfrac> 
      <msub> 
       <mi>
         k 
       </mi> 
       <mi>
         B 
       </mi> 
      </msub> 
      <mi>
        T 
      </mi> 
     </mrow> 
    </math> (2)</p>
   <p>where m = mass of a single particle (atom or molecule) = molar atom mass M/N<sub>A</sub>;</p>
   <p>N<sub>A</sub> = Avogadro Constant = 6.022 × 10<sup>23</sup>;</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
      <mi>
        w 
      </mi> 
      <mo>
        ¯ 
      </mo> 
     </mover> 
    </math> = average velocity of this particle;</p>
   <p>
    <xref ref-type="bibr" rid="scirp.146908-"></xref>k<sub>B</sub> = Boltzmann Constant = 1.381 × 10<sup>−</sup><sup>23</sup> J∙K<sup>−</sup><sup>1</sup>;</p>
   <p>T = absolute temperature.</p>
   <p>This approach is based on the assumption of the molar heat capacity with constant volume C<sub>V</sub> = 3/2R (which is equal for all noble gases). Instead, the heat capacity with constant pressure C<sub>p</sub> = 5/2R could be used. In the present case, both conditions seem to be fulfilled, namely constant volume as well as constant pressure. However, the respective volume is insofar not constant as the measuring tube is not perfectly tight. Thus, in fact, a medium case exists which appears not being exactly describable.</p>
   <p>Based on this and regarding the cross-sectional area σ of the atom, the average collision frequency 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
      <mi>
        z 
      </mi> 
      <mo>
        ¯ 
      </mo> 
     </mover> 
    </math> [s<sup>−</sup><sup>1</sup>] can be deduced (Equation (3)), yielding, in combination with the kinetic energy, the kinetic collision wattage 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mover accent="true"> 
        <mi>
          P 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mi>
          k 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
        <mi>
          t 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          m 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> of each atom (Equation (4)):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mover accent="true"> 
       <mi>
         z 
       </mi> 
       <mo>
         ¯ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mover accent="true"> 
         <mi>
           w 
         </mi> 
         <mo>
           ¯ 
         </mo> 
        </mover> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          σ 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          p 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msqrt> 
         <mn>
           2 
         </mn> 
        </msqrt> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           k 
         </mi> 
         <mi>
           B 
         </mi> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          T 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (3)</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mover accent="true"> 
        <mi>
          P 
        </mi> 
        <mo>
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        </mo> 
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       <mrow> 
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          k 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
        <mi>
          t 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          m 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mover accent="true"> 
        <mi>
          P 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          l 
        </mi> 
        <mi>
          l 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          n 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mover accent="true"> 
        <mi>
          E 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mi>
          k 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
        <mi>
          t 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          m 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mover accent="true"> 
        <mi>
          z 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mi>
          t 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          m 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        3 
      </mn> 
      <mi>
        p 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        σ 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <mi>
            R 
          </mi> 
          <mi>
            T 
          </mi> 
         </mrow> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            M 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> (4)</p>
   <p>where p = pressure [1 bar = 10<sup>5</sup> Pa = 10<sup>5</sup> kg∙m<sup>−</sup><sup>1</sup>∙s<sup>−</sup><sup>2</sup>];</p>
   <p>σ = cross sectional area of the atom = r<sup>2</sup>∙π (r = atomic radius);</p>
   <p>R = universal gas Constant = k<sub>B</sub> · N<sub>A</sub> = 8.314 J∙K<sup>−</sup><sup>1</sup>∙mol<sup>−</sup><sup>1</sup>;</p>
   <p>M = molar atom mass [kg∙mol<sup>−</sup><sup>1</sup>] = m ∙ N<sub>A</sub>.</p>
   <p>When comparative measurements are made under the same conditions (same apparatus, same light source, same pressure), the following relation (5) is valid, making use of the limiting temperatures T<sub>lim</sub>:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mrow> 
        <msub> 
         <mi>
           r 
         </mi> 
         <mn>
           2 
         </mn> 
        </msub> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           r 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
       </mrow> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mroot> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <msub> 
             <mi>
               M 
             </mi> 
             <mn>
               2 
             </mn> 
            </msub> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msub> 
             <mi>
               M 
             </mi> 
             <mn>
               1 
             </mn> 
            </msub> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          ⋅ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <msub> 
             <mi>
               T 
             </mi> 
             <mrow> 
              <mi>
                l 
              </mi> 
              <mi>
                i 
              </mi> 
              <mi>
                m 
              </mi> 
              <mo>
                , 
              </mo> 
              <mn>
                1 
              </mn> 
             </mrow> 
            </msub> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msub> 
             <mi>
               T 
             </mi> 
             <mrow> 
              <mi>
                l 
              </mi> 
              <mi>
                i 
              </mi> 
              <mi>
                m 
              </mi> 
              <mo>
                , 
              </mo> 
              <mn>
                2 
              </mn> 
             </mrow> 
            </msub> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         4 
       </mn> 
      </mroot> 
     </mrow> 
    </math> (5)</p>
   <p>For the noble gases Helium, Neon and Argon, the following plausible atomic radii are obtained:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         r 
       </mi> 
       <mrow> 
        <mtext>
          Ar 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mtext>
          assumed 
        </mtext> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mn>
        1 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          10 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
     </mrow> 
    </math> (=1 Å) 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         r 
       </mi> 
       <mrow> 
        <mtext>
          Ne 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0.85 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          10 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
     </mrow> 
    </math> 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         r 
       </mi> 
       <mrow> 
        <mtext>
          He 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0.57 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          10 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
     </mrow> 
    </math></p>
   <p>The pressure dependency of the atmospheric radiation intensity according to Equation (4) could be demonstrated by later experiments, carried out at different altitudes in order to vary the atmospheric pressure, and described in <xref ref-type="bibr" rid="scirp.146908-13">
     [13]
    </xref>. By the thereby applied method, described in <xref ref-type="bibr" rid="scirp.146908-14">
     [14]
    </xref>, the temperature rise of differently coloured aluminium-plates is measured when they are exposed to solar radiation. Similarly to the case of irradiated gases, in the case of irradiated opaque plates, after a certain time, a limiting temperature is attained whereby the—colour-dependent—absorbed solar radiation is in equilibrium with the—colour-independent—thermal radiation of the plates and the counter-radiation of the atmosphere. However, the time needed to attain the limiting temperature is much longer than in the case of gas-irradiation, namely several hours. The different altitudes implicated different atmospheric pressures, light intensities and temperatures. The thereby measured value for the atmospheric emission constant A was 22 Wm<sup>−</sup><sup>2</sup>∙bar<sup>−</sup><sup>1</sup>∙K<sup>−</sup><sup>0.5</sup>, delivering the thermal radiation intensity Φ = A∙p∙T<sup>0.5</sup>.</p>
   <p>The respective principal assumption consists of a correlation between the collision-wattage and the radiation-wattage, expressed by the transformation coefficient ε:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mover accent="true"> 
        <mi>
          P 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          a 
        </mi> 
        <mi>
          d 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          a 
        </mi> 
        <mi>
          t 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          n 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mover accent="true"> 
        <mi>
          P 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mi>
          e 
        </mi> 
        <mi>
          m 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          n 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        ε 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mover accent="true"> 
        <mi>
          P 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          l 
        </mi> 
        <mi>
          l 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          n 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> (6)</p>
   <p>Thereby, the considerable problem arises that the determinable radiation wattage is normally related to area (Wm<sup>−</sup><sup>2</sup>), whereas Formula (4) is related to a single atom, enabling the computation of a volume-related value since the general gas law delivers the coherence between particle number and volume.</p>
   <p>This problem could not be satisfyingly solved in <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref>. Therefore, a spatial particle model was developed corresponding to a close-packing of equal spheres, as it is usual in crystallography. But since it does not affect the essential objective of this treatise, it is omitted here. Rather, the application of the here used atom model is described next.</p>
  </sec><sec id="s3">
   <title>3. The Eccentric Asymmetric Harmonic Oscillator</title>
   <p>As scheduled in <xref ref-type="fig" rid="fig9">
     Figure 9
    </xref>, the radiation emitted by a spot (or by another light-source which comprises thermal radiation) can be absorbed by atoms which undergo an electronic excitation being able either to emit thermal radiation or to increase the heat content. Conversely, the kinetic heat of the gas leads to an excited state. When the limiting temperature is reached, the heat-content of the gas cannot be increased furthermore, so that the absorption intensity becomes equal to the emission intensity.</p>
   <fig id="fig9" position="float">
    <label>Figure 9</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 9. Schema of the energetic relations at the atom.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId52.jpeg?20251031033238" />
   </fig>
   <p>As a consequence, an electronically excited state of the atom must exist, which implies an energetic elevation. It is characterized by an electronic oscillation that is able to transfer the oscillation energy to kinetic motion as well as to electromagnetic radiation. And this can be modelled by means of an eccentric asymmetric harmonic oscillator, using the recently published planar atom model of Helium <xref ref-type="bibr" rid="scirp.146908-12">
     [12]
    </xref>, already roughly described in Chapter 1. The values of the parameters for this model in the ground state are:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0.5644 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          10 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
     </mrow> 
    </math> 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         u 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          t 
        </mi> 
        <mo>
          , 
        </mo> 
       </mrow> 
      </msub> 
      <msub> 
       <mrow></mrow> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        2.901 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mn>
         6 
       </mn> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mtext>
         s 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        5.14 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          16 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mtext>
         s 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math></p>
   <p>Using this model, an excited electronic state can be supposed which enables absorption as well as emission of electromagnetic radiation, but which—beyond that—is capable to transfer kinetic energy to another atom. And as it would seem obvious, the energy of the excited state should have the character of an eccentric oscillation, superimposed on the rotation of the electrons, and in combination with the rotation, inducing a pulsation.</p>
   <fig id="fig10" position="float">
    <label>Figure 10</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 10. Orbit of the electrons as a result of a collision or a thermal-radiative excitation (= dotted curve; red lines: maximal and minimal positions of the electrons).</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId59.jpeg?20251031033239" />
   </fig>
   <p>This constellation is scheduled for ω<sub>osc</sub> = 2ω<sub>rot</sub> in <xref ref-type="fig" rid="fig10">
     Figure 10
    </xref>, expressing a standing wave. Thereby, it has to be regarded that, due to heat motion, the atoms are not immobile. Rather, they move not only in the form of translation but also in the form of rotation (here called full rotation), which both are not quantised. Thus, viewed from the position of an outside observer, the atom appears to pulsate in all directions due to the oscillation of the electron orbit.</p>
   <p>In contrast, within the atom, the conditions are strictly defined. And since the orbital angular momentum must be constant, the rotation velocity u<sub>rot</sub> as well as the angular velocity ω<sub>rot</sub> depend on the rotation radius R (see Equation (7)):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         u 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        R 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
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         ω 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         R 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mn>
         2 
       </mn> 
      </msqrt> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mi>
         h 
       </mi> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          π 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        → 
      </mo> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mn>
         2 
       </mn> 
      </msqrt> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mi>
         h 
       </mi> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          π 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mi>
           e 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (7)</p>
   <p>Regarding this, it suggests itself to assume an asymmetric harmonic oscillator which can be mathematically formulated by Equation (8) and illustrated in <xref ref-type="fig" rid="fig11">
     Figure 11
    </xref>.</p>
   <fig id="fig11" position="float">
    <label>Figure 11</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 11. General description of an asymmetric harmonic oscillator.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId62.jpeg?20251031033239" />
   </fig>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <mi>
        R 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        A 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        sin 
      </mi> 
      <mi>
        φ 
      </mi> 
      <mo>
        + 
      </mo> 
      <mi>
        B 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            sin 
          </mi> 
          <mi>
            φ 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> (8)</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <mi>
        R 
      </mi> 
     </mrow> 
    </math> = distance deflexion</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        A 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              m 
            </mi> 
            <mi>
              a 
            </mi> 
            <mi>
              x 
            </mi> 
           </mrow> 
          </msub> 
          <mo>
            + 
          </mo> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              m 
            </mi> 
            <mi>
              i 
            </mi> 
            <mi>
              n 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mn>
         2 
       </mn> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        B 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              m 
            </mi> 
            <mi>
              a 
            </mi> 
            <mi>
              x 
            </mi> 
           </mrow> 
          </msub> 
          <mo>
            − 
          </mo> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              m 
            </mi> 
            <mi>
              i 
            </mi> 
            <mi>
              n 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mn>
         2 
       </mn> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        φ 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math></p>
   <p>However, this approach is not strictly correct since—as mentioned above—ω<sub>rot</sub> is not constant. Nevertheless, it seems advisable to make such an approximation by assuming ω<sub>rot</sub> as constant and u<sub>rot</sub> as variable in order to give a basic idea of the whole process. Thereby, the boundary condition must be observed that ω<sub>osc</sub> has to be in a distinct ratio to ω<sub>rot</sub><sub>,</sub><sub>0</sub> in order to enable a standing wave condition. In the simplest case, ω<sub>osc</sub> is twice as big as ω<sub>rot</sub><sub>,</sub><sub>0</sub>. In principle, other ratios are possible, but they are disregarded here.</p>
   <p>As for any harmonic oscillator, the total energy of an asymmetric harmonic oscillator is given by the kinetic energy of the oscillating electrons at the turning-over point, i.e. at the point where the distance deflexion as well as the potential energy is zero. And since two diametrically running electrons are implied, its double amount must be used.</p>
   <p>As already mentioned—or rather approximately assumed—both angular velocities (ω<sub>rot</sub> and ω<sub>osc</sub>) are considered as constant. Consequently, the oscillation velocity u<sub>osc</sub> results from the mathematical derivation of the distance deflexion ∆R (given by Equation (8)) and becomes a function of time, expressed by Equation (9):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <msub> 
       <mi>
         u 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        Δ 
      </mi> 
      <mover accent="true"> 
       <mi>
         R 
       </mi> 
       <mo>
         ˙ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mi>
        A 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        cos 
      </mtext> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           ω 
         </mi> 
         <mrow> 
          <mi>
            o 
          </mi> 
          <mi>
            s 
          </mi> 
          <mi>
            c 
          </mi> 
         </mrow> 
        </msub> 
        <mi>
          t 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        + 
      </mo> 
      <mn>
        2 
      </mn> 
      <mi>
        B 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        cos 
      </mtext> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           ω 
         </mi> 
         <mrow> 
          <mi>
            o 
          </mi> 
          <mi>
            s 
          </mi> 
          <mi>
            c 
          </mi> 
         </mrow> 
        </msub> 
        <mi>
          t 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        sin 
      </mtext> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           ω 
         </mi> 
         <mrow> 
          <mi>
            o 
          </mi> 
          <mi>
            s 
          </mi> 
          <mi>
            c 
          </mi> 
         </mrow> 
        </msub> 
        <mi>
          t 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (9)</p>
   <p>This yields at the turning-over point where ω<sub>osc</sub> · t = kinetic energy = total energy Equation (10):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             u 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              s 
            </mi> 
            <mi>
              c 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              t 
            </mi> 
            <mi>
              u 
            </mi> 
            <mi>
              r 
            </mi> 
            <mi>
              n 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         A 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             ω 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              s 
            </mi> 
            <mi>
              c 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> (10)</p>
   <p>where m<sub>e</sub> = electron mass = 0.9109 × 10<sup>−</sup><sup>30</sup> kg;</p>
   <p>A = amplitude, according to Equation (8).</p>
   <p>But whereas ω<sub>osc</sub> is given by the here used atom model, the amplitude A is not readily known. If it were known, the proportion of its parts ∆R<sub>max</sub> and ∆R<sub>min</sub> could be determined, as will be demonstrated in Chapter 5.</p>
   <p>However, first of all, a relation between this electronic oscillation energy and the thermally induced kinetic energy has to be found. Thereto, Einstein’s equation E = h · ν<sub>rad</sub> has to be regarded, being already presented in <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref> but exhibiting considerable errors which are discussed in the next chapter.</p>
   <p>Besides, in <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref>, the relevant frequency (or the respective wave length) was not precisely known but roughly estimated by comparing the results obtained by sunlight and by artificial light, using Planck’s distribution law and the producer’s specifications, yielding 1.9 μm. This value seems quite low since it is not far from the visible (red) light at 0.78 μm. Subsequent experiments with air and with CO<sub>2</sub> <xref ref-type="bibr" rid="scirp.146908-15">
     [15]
    </xref>, using a hot-plate as thermal radiation source, mounted below, let suppose that higher electronic absorption (and emission) wave lengths are possible. However, an exact evaluation like the one applied in <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref> was not possible.</p>
  </sec><sec id="s4">
   <title>4. The Bridge between Thermal Motion and Electronic Oscillation</title>
   <p>In the fundamental publication <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref>, at least two significant errors were made when trying to establish a connection between the kinetic energy E<sub>kin</sub><sub>,</sub><sub>atom</sub>, expressed by Equation (11), being identical with Equation (2):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          k 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
        <mi>
          t 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          m 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         3 
       </mn> 
       <mn>
         2 
       </mn> 
      </mfrac> 
      <msub> 
       <mi>
         k 
       </mi> 
       <mi>
         B 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        Δ 
      </mi> 
      <mi>
        T 
      </mi> 
     </mrow> 
    </math> (11)</p>
   <p>and the radiation energy E<sub>rad</sub>, expressed by Einstein’s formula for the photoelectric effect:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          a 
        </mi> 
        <mi>
          d 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        h 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         ν 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          a 
        </mi> 
        <mi>
          d 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> (12) with 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        6.626 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          34 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        J 
      </mtext> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        s 
      </mtext> 
     </mrow> 
    </math>.</p>
   <p>Since ν<sub>rad</sub> · λ<sub>rad</sub> = c<sub>light</sub> = 3.0 × 10<sup>8</sup> ms<sup>−</sup><sup>1</sup>, ν<sub>rad</sub> becomes 1.58 × 10<sup>14</sup> s<sup>−</sup><sup>1</sup> when λ<sub>rad</sub> = 1.9 μm, while E<sub>rad</sub> becomes 1.05 × 10<sup>−</sup><sup>19</sup> J.</p>
   <p>In the first case, the absolute temperature T = 300 K was used instead of the temperature difference ∆T = T<sub>lim</sub> – T<sub>amb</sub>, while in the second case, a calculation error was made by the factor of 1000.</p>
   <p>But even when the corrected values are used, i.e. ∆T = 26 K (according to <xref ref-type="fig" rid="fig12">
     Figure 12
    </xref>), the quotient ∆E<sub>kin</sub>/∆E<sub>rad</sub> = 5.4 × 10<sup>−</sup><sup>22</sup> J/1.04 × 10<sup>−</sup><sup>19</sup> J = 5.2 × 10<sup>−</sup><sup>3</sup> (instead of 6.3 × 10<sup>−</sup><sup>5</sup> as indicated in <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref>) is too low since it should be 1, which cannot be easily explained.</p>
   <fig id="fig12" position="float">
    <label>Figure 12</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 12. Comparison of Argon and Helium (method B2, 150 W, medium pos.) (Figure 27 in <xref ref-type="bibr" rid="scirp.146908-7">
       [7]
      </xref>).</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId83.jpeg?20251031033240" />
   </fig>
   <p>A plausible explanation can be given by the previously described eccentric asymmetric harmonic oscillator, which is applicable on the planar atom model of Helium.</p>
   <p>First of all, the model-specific expression for the oscillation energy according to Equation (10) can be compared with Einstein’s expression for the radiation energy resulting in Equation (13), whereby the factor 1/2 is omitted since there are two electrons per atom:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             u 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              s 
            </mi> 
            <mi>
              c 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         A 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             ω 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              s 
            </mi> 
            <mi>
              c 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mi>
        h 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         ν 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          a 
        </mi> 
        <mi>
          d 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> (13)</p>
   <p>where m<sub>e</sub> = electron mass = 0.9109 × 10<sup>−</sup><sup>30</sup> kg;</p>
   <p>A = amplitude.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        2 
      </mn> 
      <mi>
        π 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         v 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        2 
      </mn> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        10.28 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          16 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mtext>
         s 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math></p>
   <p>In this equation, the two frequencies ν<sub>osc</sub> and ν<sub>rad</sub> occur, but not within the same mathematical power. Both are known (ν<sub>osc</sub> according to the quantum mechanical supposition, and ν<sub>rad</sub> according to the empirical estimation), while the unknown parameter A exists. However, it can be computed using Equation (13). To verify it, regarding the uncertain character of ν<sub>rad</sub>, an additional relationship based on the kinetic gas theory would be needed.</p>
   <p>But even if such a relationship were not available, it is possible to assess its plausibility. Using the above parameters, the value obtained for A is 0.0327 × 10<sup>−</sup><sup>10</sup> m, which corresponds to 5.8 % of the atomic radius R<sub>0</sub> = 0.5644 × 10<sup>−</sup><sup>10</sup> m, appearing to be plausible. It also allows to compute the electron velocity at the turning-over point u<sub>osc</sub> = A · ω<sub>osc</sub>, yielding 0.336 × 10<sup>6</sup> m∙s<sup>−</sup><sup>1</sup>. This value can be used for comparison with the kinetic gas theory.</p>
   <p>Thereto, it seems obvious to apply the theorem of conservation of momentum P to the collision process, i.e. to the transfer of atomic motion to electronic motion, which is expressed by Equation (14):</p>
   <p>
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   <p>with 
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    </math> according to Equation (2)</p>
   <p>
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   <p>(In order to distinguish between both velocities, the different terms w (for the atoms) and u (for the electrons) are used).</p>
   <p>Thereby, it has to be considered that 
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   <p>But as <xref ref-type="fig" rid="fig13">
     Figure 13
    </xref> reveals, within the range of the near-ground atmospheric temperature the two differences are proportional to one another, according to Equation (15):</p>
   <p>
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   <fig id="fig13" position="float">
    <label>Figure 13</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 13. Plot of T<sub>lim</sub> – T<sub>amb</sub> versus 

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    </caption>
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   </fig>
   <p>Moreover, the temperature difference ∆T = T<sub>lim</sub> – T<sub>amb</sub> can be related to the area-related wattage of the spot by introducing the factor f according to Equation (16), which can be evaluated using a time-temperature diagram as the one depicted in <xref ref-type="fig" rid="fig12">
     Figure 12
    </xref>.</p>
   <p>
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   <p>For Helium, f amounts to 0.0073 Km<sup>2</sup>∙W<sup>−</sup><sup>1</sup>, and when Φ<sub>apparent,area</sub> = 3556 Wm<sup>−</sup><sup>2</sup>, ∆T<sub>He</sub> becomes 26 K = 26˚C.</p>
   <p>Using these relations, the values A = 0.0355 × 10<sup>−</sup><sup>10</sup> m and E<sub>osc</sub> = 0.121 × 10<sup>−</sup><sup>18</sup> J are obtained, which yield for ν<sub>rad</sub> = 1.83 × 10<sup>14</sup> s<sup>−</sup><sup>1</sup> and for λ<sub>rad</sub> = 1.67 μm, being very close to the estimated value of 1.9 μm. Thus, the here used modelling method is in principle validated.</p>
   <p>The energy conservation law appears not to be fulfilled here. However, this is due to the circumstance that two different energies are involved, namely the kinetic energy of the whole atom and the oscillation energy of the electrons, implying a splitting of the collision energy.</p>
  </sec><sec id="s5">
   <title>5. The Determination of the Asymmetric Parts at the Oscillator</title>
   <p>In order to determine the maximal distances R<sub>out</sub> = R<sub>0</sub> + ∆R<sub>max</sub> and R<sub>in</sub> = R<sub>0</sub> – ∆R<sub>min</sub> of the two diametrically running electrons at the eccentric asymmetric harmonic oscillator, described by Equation (8), their energy contents have to be computed as a function of T and equated at their relevant value. Their energy contents are given by the sum of the potential energy and the rotation energy, while the oscillation energy E<sub>osc</sub> is zero at these positions.</p>
   <p>The potential energy can be computed using the expression for the Coulomb-force, which can be derived from Figure 11 and Formula (4) of <xref ref-type="bibr" rid="scirp.146908-12">
     [12]
    </xref>, here designated as Formula (17):</p>
   <p>
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    </math> (17)</p>
   <p>where R = total radius between the nucleus and the electrons.</p>
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   <p>The computation of the kinetic energy requires the implementation of the angular momentum 
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        </mo> 
        <mn>
          34 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        J 
      </mtext> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        s 
      </mtext> 
     </mrow> 
    </math> (which is characteristic for the here applied atom model of Helium) in order to determine the rotation velocity u<sub>rot</sub> according to Equation (18):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         u 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mn>
         2 
       </mn> 
      </msqrt> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mi>
         h 
       </mi> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          π 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mi>
         R 
       </mi> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mi>
           e 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (18)</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0.9109 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          30 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        kg 
      </mtext> 
     </mrow> 
    </math></p>
   <p>Thereby, it has to be regarded that both electrons contribute to the kinetic energy, thus</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          k 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             u 
           </mi> 
           <mrow> 
            <mi>
              r 
            </mi> 
            <mi>
              o 
            </mi> 
            <mi>
              t 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mn>
        2 
      </mn> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mi>
             h 
           </mi> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <mi>
              π 
            </mi> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mi>
           e 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (19)</p>
   <p>Using these relations, the energies ∆E<sub>tot</sub> = ∆E<sub>pot</sub> + ∆E<sub>kin</sub> can be computed for the outer position as well as for the inner position of the electrons, according to the Equations (20) - (22) and plotted as a function of the deflexion ∆R (<xref ref-type="fig" rid="fig14">
     Figure 14
    </xref>). Then, the ∆R-values which are relevant for E<sub>osc</sub>, being determined in the previous chapter and amounting to 0.121 × 10<sup>−</sup><sup>18</sup> J, can be graphically determined, yielding 0.068 × 10<sup>−</sup><sup>10</sup> m for ∆R<sub>max</sub><sub>,</sub><sub>in</sub> and 0.1035 × 10<sup>−</sup><sup>10</sup> m for ∆R<sub>max</sub><sub>,</sub><sub>out</sub>:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          t 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          o 
        </mi> 
        <mi>
          u 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          15 
        </mn> 
        <mi>
          K 
        </mi> 
       </mrow> 
       <mn>
         8 
       </mn> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
         </mrow> 
        </mfrac> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mo>
            + 
          </mo> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              u 
            </mi> 
            <mi>
              t 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (20)</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          t 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          15 
        </mn> 
        <mi>
          K 
        </mi> 
       </mrow> 
       <mn>
         8 
       </mn> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
         </mrow> 
        </mfrac> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mo>
            − 
          </mo> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              i 
            </mi> 
            <mi>
              n 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (21)</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          k 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          o 
        </mi> 
        <mi>
          u 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        2 
      </mn> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mi>
             h 
           </mi> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <mi>
              π 
            </mi> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <msub> 
               <mi>
                 R 
               </mi> 
               <mn>
                 0 
               </mn> 
              </msub> 
              <mo>
                + 
              </mo> 
              <mi>
                Δ 
              </mi> 
              <msub> 
               <mi>
                 R 
               </mi> 
               <mrow> 
                <mi>
                  o 
                </mi> 
                <mi>
                  u 
                </mi> 
                <mi>
                  t 
                </mi> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msubsup> 
           <mi>
             R 
           </mi> 
           <mn>
             0 
           </mn> 
           <mn>
             2 
           </mn> 
          </msubsup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (22)</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          k 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        2 
      </mn> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mi>
             h 
           </mi> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <mi>
              π 
            </mi> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <msub> 
               <mi>
                 R 
               </mi> 
               <mn>
                 0 
               </mn> 
              </msub> 
              <mo>
                − 
              </mo> 
              <mi>
                Δ 
              </mi> 
              <msub> 
               <mi>
                 R 
               </mi> 
               <mrow> 
                <mi>
                  o 
                </mi> 
                <mi>
                  u 
                </mi> 
                <mi>
                  t 
                </mi> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msubsup> 
           <mi>
             R 
           </mi> 
           <mn>
             0 
           </mn> 
           <mn>
             2 
           </mn> 
          </msubsup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (23)</p>
   <fig id="fig14" position="float">
    <label>Figure 14</label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 14. Plot of ∆R<sub>deflection</sub> versus ∆E<sub>deflection</sub><sub>,</sub><sub>tot</sub>.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId127.jpeg?20251031033240" />
   </fig>
   <p>Based on these results, and approximately assuming that ω<sub>rot</sub> and ω<sub>osc</sub> = 2ω<sub>rot</sub> are constant, the calculation of the electron orbit in the excited state is possible, using Equation (8), and regarding that the rotation angle φ = ω<sub>rot</sub> · t (t = time), which implicates that ω<sub>osc</sub> · t = 2φ. Thereby, the synonymous abbreviations ∆R<sub>max,in</sub> ≡ ∆R<sub>min</sub> and ∆R<sub>max,out</sub> ≡ ∆R<sub>max</sub> are assumed. As a consequence, the following values are obtained for the constants A and B:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        A 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              m 
            </mi> 
            <mi>
              a 
            </mi> 
            <mi>
              x 
            </mi> 
           </mrow> 
          </msub> 
          <mo>
            + 
          </mo> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              m 
            </mi> 
            <mi>
              i 
            </mi> 
            <mi>
              n 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mn>
         2 
       </mn> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mn>
        0.08575 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          10 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        B 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              m 
            </mi> 
            <mi>
              a 
            </mi> 
            <mi>
              x 
            </mi> 
           </mrow> 
          </msub> 
          <mo>
            − 
          </mo> 
          <mi>
            Δ 
          </mi> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mi>
              m 
            </mi> 
            <mi>
              i 
            </mi> 
            <mi>
              n 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mn>
         2 
       </mn> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mn>
        0.01775 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          10 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
     </mrow> 
    </math></p>
   <p>The total radius of the electron orbit R = R<sub>0</sub> + ∆R (whereby R<sub>0</sub> = 0.5644 × 10<sup>−</sup><sup>10</sup> m) can be expressed by these constants and by the oscillating angle 2φ, according to Equation (24):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        R 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        + 
      </mo> 
      <mi>
        A 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        sin 
      </mi> 
      <mn>
        2 
      </mn> 
      <mi>
        φ 
      </mi> 
      <mo>
        + 
      </mo> 
      <mi>
        B 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            sin 
          </mi> 
          <mn>
            2 
          </mn> 
          <mi>
            φ 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> (24)</p>
   <p>Now, the electron orbit can be expressed in Cartesian coordinates as follows:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        x 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        R 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        sin 
      </mi> 
      <mi>
        φ 
      </mi> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        y 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        R 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        cos 
      </mi> 
      <mi>
        φ 
      </mi> 
     </mrow> 
    </math></p>
   <p>which yields the relations (25a) and (25b):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        x 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          + 
        </mo> 
        <mi>
          A 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          sin 
        </mi> 
        <mn>
          2 
        </mn> 
        <mi>
          φ 
        </mi> 
        <mo>
          + 
        </mo> 
        <mi>
          B 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mi>
              sin 
            </mi> 
            <mn>
              2 
            </mn> 
            <mi>
              φ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        sin 
      </mi> 
      <mi>
        φ 
      </mi> 
     </mrow> 
    </math> (25a)</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        y 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          + 
        </mo> 
        <mi>
          A 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          sin 
        </mi> 
        <mn>
          2 
        </mn> 
        <mi>
          φ 
        </mi> 
        <mo>
          + 
        </mo> 
        <mi>
          B 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mi>
              sin 
            </mi> 
            <mn>
              2 
            </mn> 
            <mi>
              φ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        cos 
      </mi> 
      <mi>
        φ 
      </mi> 
     </mrow> 
    </math> (25b)</p>
   <p>and which is illustrated in <xref ref-type="fig" rid="fig15(a)">
     Figure 15(a)
    </xref> and <xref ref-type="fig" rid="fig15(b)">
     Figure 15(b)
    </xref>, whereby the “ground state” means the non-excited equilibrium state at ambient temperature. They resemble the elliptic orbit shown in<xref ref-type="fig" rid="fig10">
     Figure 10
    </xref> and thus confirm this approach, too.</p>
   <fig id="fig15" position="float">
    <label>Figure 15</label>
    <caption>
     <title>(a) (b)<xref ref-type="bibr" rid="scirp.146908-"></xref>Figure 15. (a) Orbit of the electrons in the ground state (units at both axis: 10<sup>−10</sup> m); (b) Orbit of the electrons in the thermally excited state (units at both axis: 10<sup>−10</sup> m).</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724362-rId142.jpeg?20251031033241" />
   </fig>
  </sec><sec id="s6">
   <title>6. Conclusions</title>
   <p>In order to apply the recently published planar atom model of Helium <xref ref-type="bibr" rid="scirp.146908-11">
     [11]
    </xref> onto the results about the thermal behaviour of gases under the influence of infrared radiation, which was published by the author in 2016 <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref>, the latter publication had to be partly questioned since its theoretical evaluation contains several errors. Nevertheless, the basic statements made therein, applying the kinetic gas theory, are still valid. Since they cannot be assumed as commonly known, the description of the measurement equipment and the applied light sources (sunlight and IR-spot-light), the most relevant results, and the basic theoretical interpretation were recapitulated in Chapter 2.</p>
   <p>The essential empirical result of those measurements was the observation that any gas is warmed up when it is thermally irradiated, but solely up to a limiting temperature where the absorption intensity of the gas (measured in Wm<sup>−</sup><sup>2</sup>) is equal to its emission intensity. This effect was first observed with air (or a nitrogen/oxygen mixture) and with CO<sub>2</sub>, whereby the limiting temperatures were nearly equal. But it also occurred at the noble gases Argon, Neon and Helium, whereby the limiting temperatures depended on the type of gas. These differences could be explained by means of the kinetic gas theory (which correlates the absolute temperature of a gas to the kinetic energy of the particles), assuming proportionality between the collision wattage of the atoms and the radiation wattage. Thereby, dependency of the radiation intensity on the gas pressure and on the absolute temperature was found.</p>
   <p>As a consequence, an additional energy must exist, which does not appear in the classic thermodynamic theory, and which must be due to an oscillating process at the electrons. Hereto, solely a modified harmonic oscillator comes into question, preferably applied onto the simplest case—namely onto the planar atom model of Helium—and described in Chapter 3. This oscillator, illustrated in <xref ref-type="fig" rid="fig10">
     Figure 10
    </xref> and mathematically expressed by Equation (9), is eccentric since it rotates around the nucleus. Moreover, it is asymmetric since its energetic conditions are asymmetric with respect to the orbit path. In particular, the quantum-mechanical condition of a standing wave must be fulfilled, i.e. the angular velocity ω<sub>osc</sub> of the oscillator must be an integer multiple of the angular rotation velocity ω<sub>rot</sub>, preferably 2. But since the conservation of angular momentum 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msqrt> 
       <mn>
         2 
       </mn> 
      </msqrt> 
      <mi>
        ℏ 
      </mi> 
     </mrow> 
    </math> must be fulfilled, the difficulty arises that both angular velocities are not constant since they depend on the (variable) radius. In order to eliminate this difficulty, the approximation of a constant ω<sub>osc</sub> was made, which delivered plausible results. Particularly, it implied an expression for the oscillation energy E<sub>osc</sub> as a function of the electronic mass m<sub>e</sub>, the amplitude A, and the angular velocity ω<sub>osc</sub> = 2ω<sub>rot</sub>:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         A 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             ω 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              s 
            </mi> 
            <mi>
              c 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> (26)</p>
   <p>which enables to compute A (if E<sub>osc</sub> is known), or to compute E<sub>osc</sub> (if A is known).</p>
   <p>By equating the oscillation energy and the radiation energy, which was determined by Einstein’s formula E = h · ν<sub>rad</sub>, thermodynamics could be bridged with quantum mechanics. Such computations were made in Chapter 4. On the one hand, ν<sub>rad</sub> (or λ<sub>rad</sub>, due to the relation ν<sub>rad</sub> · λ<sub>rad</sub> = c<sub>light</sub>) was predetermined in the form of the λ<sub>rad</sub> value, which had been estimated in <xref ref-type="bibr" rid="scirp.146908-7">
     [7]
    </xref>, namely 1.9 μm. It yielded an A-value of 0.0327 × 10<sup>−</sup><sup>10</sup> m = 5.8% of R<sub>0</sub>.</p>
   <p>On the other hand, the theorem of conservation of momentum P was applied to the collision process which occurs according to the kinetic gas theory, i.e. to the transfer of atomic motion (velocity w) to electronic motion (velocity u), expressed by Equation (27):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         P 
       </mi> 
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      </mo> 
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         u 
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      </mo> 
      <msub> 
       <mover accent="true"> 
        <mi>
          P 
        </mi> 
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        </mo> 
       </mover> 
       <mrow> 
        <mi>
          a 
        </mi> 
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          t 
        </mi> 
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        </mi> 
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          m 
        </mi> 
       </mrow> 
      </msub> 
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      </mo> 
      <msub> 
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        <mtext>
          He 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mover accent="true"> 
        <mi>
          w 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mtext>
          He 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        → 
      </mo> 
      <msub> 
       <mi>
         u 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mrow> 
          <mtext>
            He 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mi>
           e 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mover accent="true"> 
        <mi>
          w 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mrow> 
        <mtext>
          He 
        </mtext> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> (27)</p>
   <p>The calculation yielded the values A = 0.0355 × 10<sup>−</sup><sup>10</sup> m and E<sub>osc</sub> = 0.121 × 10<sup>−</sup><sup>18</sup> J, which correspond to ν<sub>rad</sub> = 1.83 × 10<sup>14</sup> s<sup>−</sup><sup>1</sup> and to λ<sub>rad</sub> = 1.67 μm, being very close to the estimated value of 1.9 μm. Thus, the here used modelling method was validated in principle.</p>
   <p>Finally, in Chapter 5, the asymmetric parts of the oscillator were computed, regarding the condition that the total outer and inner energies must be equal. For ∆R<sub>max,in</sub> and ∆R<sub>max</sub><sub>,</sub><sub>out</sub>, the values 0.068 × 10<sup>−</sup><sup>10</sup> m and 0.1035 × 10<sup>−</sup><sup>10</sup> m were obtained. Using these values, the electron orbit in the excited state could be computed and compared to that in the ground state (<xref ref-type="fig" rid="fig15(b)">
     Figure 15(b)
    </xref> and <xref ref-type="fig" rid="fig15(a)">
     Figure 15(a)
    </xref>). They resembled the elliptic orbit shown in <xref ref-type="fig" rid="fig10">
     Figure 10
    </xref>and thus confirmed this approach, too.</p>
   <p>The essential difference between the orthodox and the alternative model consists in the fact that the orthodox model only considers the observer’s point of view, whereas the alternative model distinguishes between object and observer. Thereby, the isolated model is two-dimensional, obeying strict quantum-mechanical regularities. However, from the viewpoint of the observer, it appears three-dimensional, since it rotates as a whole due to heat-induced movement, and thus obeys stochastic regularities. But the nucleus/electron distances are not identical: while this distance varies in the orthodox model—even in the ground state—it is constant and well-defined in the alternative model. As a consequence, the alternative model allows computing the electron oscillation, due to the well-defined electron radius, whereas the orthodox model would be unable to do so in default of a well-defined electron radius.</p>
  </sec><sec id="s7">
   <title>Acknowledgment</title>
   <p>I thank Johan M. van der Wiel, Andreas Rüetschi, Harald von Fellenberg, Emil Roduner and Dieter Meschede for their critical objections.</p>
  </sec>
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