<?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">OPJ</journal-id><journal-title-group><journal-title>Optics and Photonics Journal</journal-title></journal-title-group><issn pub-type="epub">2160-8881</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/opj.2019.99013</article-id><article-id pub-id-type="publisher-id">OPJ-94989</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Chemistry&amp;Materials Science</subject><subject> Engineering</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Detection of Casimir Radiation from Our Sun
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Richard</surname><given-names>A. Hutchin</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Optical Physics Company, Simi Valley, CA, USA</addr-line></aff><pub-date pub-type="epub"><day>11</day><month>09</month><year>2019</year></pub-date><volume>09</volume><issue>09</issue><fpage>141</fpage><lpage>154</lpage><history><date date-type="received"><day>1,</day>	<month>August</month>	<year>2019</year></date><date date-type="rev-recd"><day>9,</day>	<month>September</month>	<year>2019</year>	</date><date date-type="accepted"><day>12,</day>	<month>September</month>	<year>2019</year></date></history><permissions><copyright-statement>&#169; 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><p>
 
 
  This paper extends the previous experimental work on Planck’s constant h and the vacuum field, whose spectrum is determined by h. In particular it adds additional experimental evidence supporting temporal and spatial variations in the vacuum field, including the Sun as a source at 13 sigmas of certainty. The vacuum field has long been a mystery of physics, having enormous theoretical intensity set by Planck’s constant h and yet no obvious physical effect. Hendrick Casimir first proposed that this form of E &amp; M radiation was real in 1948 and suggested an experiment to verify its existence. Over 50 experiments since then have confirmed that this vacuum radiation is real, is a form of electro-magnetic radiation, and varies in time and space over 10:1 in our laboratory compared to its standard QM spectrum. Two other authors have found the fine structure constant α (proportional to 1/h) is varying across the cosmos at up to 4.2 sigma certainty. All these results suggest that the vacuum field (and thus h) varies in time and space. In a previous paper we reported our tunnel diode experimental results as well as the results of six other organizations (including German, Russian and US national labs).The six organizations reported sinusoidal annual variations of 1000 - 3000 ppm (peak-to-valley) in the decay rates of 8 radionuclides over a 20-year span, including beta decay (weak interaction) and alpha decay (strong interaction). All decay rates peaked in January-February and minimized in July-August without any candidate cause suggested. We confirmed that Planck’s constant was the cause by verifying similar variations in Esaki tunnel diode current, which is purely electromagnetic. The combined data from previous strong and weak decays plus our own E &amp; M tunnel data showed similar magnitude and time phasing for strong, weak and E &amp; M interactions, except that the tunnel diode temporal variations were 180 deg out of phase—as we predicted. The logic for this 180 deg phase shift was straight forward. Radioactive decay and electron tunneling both have h in the denominator of the tunneling exponent, but tunnel diodes also have h
  <sup>2</sup> in the numerator of the exponent due to the size of atoms being proportional to h
  <sup>2</sup>. This extra h
  <sup>2</sup> makes the exponent proportional to h for electron tunneling instead of proportional to 1/h for strong and weak decay—shifting the annual oscillation for E &amp; M tunnel current by 180 deg. Radioactive decay had a maximum around January-February of each year and a minimum around July-August of each year. Tunnel current (the equivalent to radioactive decay rate) had the opposite—a minimum around January of each year and a maximum around July of each year. This predicted and observed sign flip in the temporal variations between radioactive decay and electron tunneling provides strong evidence that h variations across the Earth’s orbit are the cause of these annual cycles. In this paper we take the next step by verifying whether the Sun and a potential more distant cosmic source radiate the vacuum E &amp; M field, just as all stars generate massive amounts of regular E &amp; M radiation. We reprocessed two years of data, 6 million data points, from our tunnel diode experiment to search for day-night oscillations in tunnel current. Here we assume that the Earth would block the radiated vacuum field half of each day. Sun-locked signals have 365 cycles per year and cosmos locked signals have 366 cycles per year. With our two years of data, these two signals are separated by a null-signal, which is not locked to the Earth or to the cosmos—allowing us to clearly distinguish the solar and cosmic sources. 1) We found sun-locked variations in the vacuum field, peaking around local noon with 10
  <sup>-13</sup> probability of false alarm. Other potential causes are carefully examined and ruled out. 2) We also found cosmos-locked variations in the vacuum field, peaking at the right ascension of the red super-giant star Betelgeuse with 10
  <sup>-7</sup> probability of false alarm. Cosmos locked sources are easily distinguished from the solar source because they have one extra cycle per year, two extra cycles during the two years of the experiment. They are thus independent Fourier components, easily separated by a Fourier transform. Both of these high probability detections support that the vacuum field spectrum may vary in space and time and be enhanced by stellar sources.
 
</p></abstract><kwd-group><kwd>Planck’s Constant</kwd><kwd> Variable Radioactive Decay Rate</kwd><kwd> Variable Plank’s Constant</kwd><kwd> Solar Radiation</kwd><kwd> Casimir Radiation</kwd><kwd> Cosmic Red Shift</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>This paper explores the nature of the Vacuum Field, which has been a mystery for 100 years. In first half of the 20<sup>th</sup> century, many scientists thought the ground state energy of the E &amp; M field (called the vacuum state) was a mathematical result without physical meaning until Hendrik Casimir proposed an experimental test in 1948. This experimental work verified the existence of the vacuum field at power levels equal to the entire power generation of our Earth civilization in every square inch. The observed pressure in the Casimir experiments matched the terawatts/cm<sup>2</sup> of predicted E &amp; M power, but nothing was heated. The vacuum field is currently regarded to be a vastly intense form of E &amp; M radiation that creates pressure without heat.</p><p>In these Casimir experiments, the observed radiation pressure of 19 psi occurred because the intensity of the vacuum field varied more than 10:1 between the two plates compared to outside the plates. If the vacuum field can vary hugely in our labs, one might expect the vacuum field could also vary in space and time across the universe, and this research detects and reports such variations in our solar system and beyond.</p><p>Past research papers from three national labs and other groups showed annual variations in strong and weak radioactive decay rates without proposing a cause [<xref ref-type="bibr" rid="scirp.94989-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.94989-ref10">10</xref>] . Our contribution was first to hypothesize that Planck’s constant was the link between strong and weak interactions, suggesting that variations in h might be responsible. We then tested this hypothesis using tunnel diodes—purely an E &amp; M phenomenon—and found the same annual oscillation of similar magnitude except180 deg out of phase—as predicted and discussed below. A short summary of the data is given here, with the details in [<xref ref-type="bibr" rid="scirp.94989-ref11">11</xref>] and pictures of the hardware in Appendix, showing the design of the tunnel diode experiment.</p><p>Two cosmological studies are also referenced [<xref ref-type="bibr" rid="scirp.94989-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.94989-ref13">13</xref>] , which show 3.6 and 4.2 sigma variations of the fine structure constant α with cosmic distance in a dipole mode with angle. Since the fine structure constant includes h in its denominator, these data also support spatial variations in h across the cosmos.</p><p>The ability for the vacuum field to vary in time and space by factors of 10 or more has been verified in our laboratories by many published experiments, all derived from Casimir’s original paper in 1948 [<xref ref-type="bibr" rid="scirp.94989-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.94989-ref15">15</xref>] . The pressure created by the well-accepted variations in the vacuum field intensity has been refined to the point where this variable vacuum field even drives micro-machines [<xref ref-type="bibr" rid="scirp.94989-ref15">15</xref>] . Thus this research was trying to determine if the variations in the vacuum field we see in our labs are also present in space, and if so, to identify the sources of those variations.</p><p>In searching for potential sources of the vacuum field, we analyzed the previous tunnel diode data to look for potential vacuum field radiation coming from our Sun. We found a daily tunnel signal consistent with increased h that peaked at noon each day. The probability of false alarm was about 10<sup>−13</sup>.</p><p>In addition, the same analysis found a radiation signal locked to the distant cosmos with a 10<sup>−7</sup> probability of false alarm aligned in the direction of Betelgeuse, a red super-giant as bright as 55,000 suns. This star is predicted by astronomers to go supernova in about one million years.</p><p>We begin with a short summary of the previously reported time-varying radioactive decay and annual tunnel diode variations, and the logic that leads to the conclusion that variations in h are responsible.</p><p>Then the new data is presented along with its more detailed analysis, showing high probability detection of radiation from the sun and a separate cosmic source. In respect for Hendrik Casimir, who started the exploration of the vacuum field in 1948, we have called this new form of radiation, Casimir Radiation.</p><p>1) Time Varying Radioactive Decay Rate.</p><p>Annual variations of 1000 - 3000 ppm (peak-to-valley) have been observed in the decay rates of 8 radionuclides over a 20-year span by six organizations on three continents, including German, Russian and US national labs [<xref ref-type="bibr" rid="scirp.94989-ref1">1</xref>] - [<xref ref-type="bibr" rid="scirp.94989-ref10">10</xref>] . The decay modes affected included beta decay (weak interaction) and alpha decay (strong interaction). <xref ref-type="table" rid="table1">Table 1</xref> summarizes the results and <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref> and <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref> show some of the experimental results.</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Summary of various tests for time varying nuclear decay including alpha decay, beta minus decay and beta capture. The date of peak decay was somewhat variable with year from about Dec 15 to March 1 even for 10 year continuous experiments of the same radionuclide. The peak-to-valley of the annual modulation varied from 0.0007 - 0.0037 of the time average radioactive decay rate</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >ID #</th><th align="center" valign="middle" >Nuclide</th><th align="center" valign="middle" >Half-life (yr)</th><th align="center" valign="middle" >Decay Mode</th><th align="center" valign="middle" >Variation</th><th align="center" valign="middle" >Technique</th><th align="center" valign="middle" >Mag of Modul</th><th align="center" valign="middle" >Peak Day</th><th align="center" valign="middle" >Author</th><th align="center" valign="middle" >Organization</th></tr></thead><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >226Ra</td><td align="center" valign="middle" >1600</td><td align="center" valign="middle" >alpha decay</td><td align="center" valign="middle" >Annual</td><td align="center" valign="middle" >ABSOLUTE</td><td align="center" valign="middle" >~1.5E−3</td><td align="center" valign="middle" >30</td><td align="center" valign="middle" >Siegert [<xref ref-type="bibr" rid="scirp.94989-ref1">1</xref>]</td><td align="center" valign="middle" >PTB</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >154Eu</td><td align="center" valign="middle" >8.59</td><td align="center" valign="middle" >beta minus decay</td><td align="center" valign="middle" >Annual</td><td align="center" valign="middle" >ABSOLUTE</td><td align="center" valign="middle" >~1.5E−3</td><td align="center" valign="middle" >30</td><td align="center" valign="middle" >Siegert [<xref ref-type="bibr" rid="scirp.94989-ref1">1</xref>]</td><td align="center" valign="middle" >PTB</td></tr><tr><td align="center" valign="middle" >1-2</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >NO</td><td align="center" valign="middle" >RATIO 1:2</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >NA</td><td align="center" valign="middle" >Siegert [<xref ref-type="bibr" rid="scirp.94989-ref1">1</xref>]</td><td align="center" valign="middle" >PTB</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >238Pu</td><td align="center" valign="middle" >78.74</td><td align="center" valign="middle" >alpha decay</td><td align="center" valign="middle" >Annual</td><td align="center" valign="middle" >ABSOLUTE</td><td align="center" valign="middle" >~2E−3</td><td align="center" valign="middle" >−15</td><td align="center" valign="middle" >Ellis [<xref ref-type="bibr" rid="scirp.94989-ref2">2</xref>]</td><td align="center" valign="middle" >Baylor College</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >3H</td><td align="center" valign="middle" >12.3</td><td align="center" valign="middle" >beta minus decay</td><td align="center" valign="middle" >Annual</td><td align="center" valign="middle" >ABSOLUTE</td><td align="center" valign="middle" >3.7E−3</td><td align="center" valign="middle" >45</td><td align="center" valign="middle" >Falkenberg [<xref ref-type="bibr" rid="scirp.94989-ref3">3</xref>]</td><td align="center" valign="middle" >Unknown</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >32Si</td><td align="center" valign="middle" >170</td><td align="center" valign="middle" >beta minus decay</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Alburger [<xref ref-type="bibr" rid="scirp.94989-ref4">4</xref>]</td><td align="center" valign="middle" >Brookhaven</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >36Cl</td><td align="center" valign="middle" >3.01E+05</td><td align="center" valign="middle" >beta minus decay</td><td align="center" valign="middle" >Annual</td><td align="center" valign="middle" >RATIO 5:6</td><td align="center" valign="middle" >0.7E−3</td><td align="center" valign="middle" >40</td><td align="center" valign="middle" >Alburger [<xref ref-type="bibr" rid="scirp.94989-ref4">4</xref>]</td><td align="center" valign="middle" >Brookhaven</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >54Mn</td><td align="center" valign="middle" >312d</td><td align="center" valign="middle" >beta capture</td><td align="center" valign="middle" >Annual</td><td align="center" valign="middle" >ABSOLUTE</td><td align="center" valign="middle" >~1E−3</td><td align="center" valign="middle" >NA</td><td align="center" valign="middle" >Jenkins [<xref ref-type="bibr" rid="scirp.94989-ref5">5</xref>]</td><td align="center" valign="middle" >Purdue</td></tr><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >60Co</td><td align="center" valign="middle" >5.27</td><td align="center" valign="middle" >beta minus decay</td><td align="center" valign="middle" >Annual</td><td align="center" valign="middle" >ABSOLUTE</td><td align="center" valign="middle" >~1.5E−3</td><td align="center" valign="middle" >~90</td><td align="center" valign="middle" >Parkhomov [<xref ref-type="bibr" rid="scirp.94989-ref6">6</xref>]</td><td align="center" valign="middle" >Moscow State</td></tr><tr><td align="center" valign="middle" >9</td><td align="center" valign="middle" >90Sr</td><td align="center" valign="middle" >28.9</td><td align="center" valign="middle" >beta minus decay</td><td align="center" valign="middle" >Annual</td><td align="center" valign="middle" >ABSOLUTE</td><td align="center" valign="middle" >~1.5E−3</td><td align="center" valign="middle" >~60</td><td align="center" valign="middle" >Parkhomov [<xref ref-type="bibr" rid="scirp.94989-ref6">6</xref>]</td><td align="center" valign="middle" >Moscow State</td></tr></tbody></table></table-wrap><p>2) Hypothesis that only Planck’s constant h is in common with strong and weak interactions, and thus might be responsible. Confirm that E &amp; M tunneling sees an annual variation consistent with h varying across the Earth orbit.</p><p>There is very little in common between strong and weak interactions except Planck’s constant, so we hypothesized that small variations in Planck's constant might account for the observed synchronized variations in strong and weak decays. If so, then h would be a maximum on Earth around January-February of each year and a minimum around July-August of each year based on the 20 years of radioactive decay data.</p><p>To test the hypothesis that h was varying across Earth’s orbit, a purely electromagnetic experiment was set up to search for the same annual variations. From Jun 14, 2011 to Jan 29, 2014 (941 days), annual variations in tunneling voltage through 5 parallel Esaki tunnel diodes were recorded. Since electron tunneling has both h in the denominator of the exponent due to tunneling as well as h<sup>2</sup> in the numerator due to the size of atoms being proportional to h<sup>2</sup>, we set up the experiment with fixed tunnel current and measured the voltage shifts. This had the effect of shifting the temporal variations by 180 degrees compared to current variations at fixed voltage, allowed us to compare our data directly with the radioactive decay plots.</p><p>These tunneling variations were similar in magnitude and phase to the radioactive decay variations and supported the hypothesis that there is a gradient in h across the Earth’s orbit. <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref> shows the full 2<sup>1/2</sup> years of data. It found annual variations of 826 ppm peak-to-valley peaking around Jan 1.</p><p>We next did a best-least-squares fit to the Esaki voltage data with a sine wave to get the following results—an annual 850.5 ppm variation in the tunnel diode current.</p><p>Mean Value = 14.97 mV, Peak to Valley Sine = 0.01273 mV.</p><p>Peak to Valley/Mean = 850.5 ppm, CosPhase = −1.273 deg = Dec 31 peak.</p><p>Using the estimated h gain for this tunnel diode of 40.85, we get an estimated annual variation in Planck’s parameter h of 20.8 ppm peak-to-valley.</p><p>Please refer to the original paper for more details [<xref ref-type="bibr" rid="scirp.94989-ref11">11</xref>] .</p><p>3) Why did a recent NIST measurement of h not show variations? [<xref ref-type="bibr" rid="scirp.94989-ref16">16</xref>]</p><p>NIST recently did an experiment to measure time variations in h and found none of significance. However, their experiment was linear, which guarantees that they cannot detect variations in h. The logic is simple. Basically, h controls the time rates of all phenomena. Thus, all their clocks also run slower or faster with h—cancelling out any real variation for a linear process. You must have a nonlinear detection process (such as tunneling or radioactive decay) to measure h variations.</p><p>4) High probability detection of radiation from the sun in the E &amp; M Planck experiment, creating oscillations in tunnel current locked to day/night (Newly reported here).</p><p>In <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref> we show blow-ups of the annual and daily peaks over a 2 year period. We note that by choosing 365 &#215; 2 days in this Fourier analysis, 365 cycles per year is exactly one cycle per solar day. We also observed a cosmos-locked variation with 366 cycles/year. As is well known, the Earth completes an extra cycle of rotation relative to the outside universe every 365 days. Mathematically there is no cross-coupling between the two Fourier components, which thus represent independent sources of radiation.</p><p>Eliminating Temperature Variations as an Explanation: Given that there are daily temperature variations in any lab, we wondered whether those could</p><p>create a daily tunnel signal that had not been properly corrected for those temperature variations. Our tunnel diodes were thermally bonded to a thick copper plate that was maintained at 40 +/− 0.1 deg C for the full 2<sup>1/2</sup> years, and the actual plate temperature was recorded every 10 seconds (3 million times a year). We had experimentally calibrated the effect of plate temperature prior to beginning the experiment and removed that small effect in the processing.</p><p>Since almost everything happens on the thick Esaki copper plate, which includes the tunnel diodes, temperature sensor and the precision current measurement resistor all bonded to it, we looked carefully at that temperature calibration coefficient which measured the impact of plate temperature on tunnel current. In searching for a more optimal temperature calibration coefficient, we reasoned that uncorrected temperature variations should cause a general increase in the background noise level as well as possibly a one cycle per day signal.</p><p>We had experimentally measured the temperature coupling after we set up the experiment prior to gathering annual data, but we knew that there were signs of a slow drift over a few months (Those early months were discarded from the data used in the analysis reported here). Dropping the temperature coupling coefficient by 19% minimized the noise floor from 91.70 ppm<sup>2</sup> to 40.44 ppm<sup>2</sup> and reduced the daily oscillation from about 10 ppm to 2.430 ppm. This was obviously a significant coupling, now optimized and removed. Dropping the small quadratic temperature term entirely reduced the noise floor to 40.32 ppm<sup>2</sup>—almost no effect, and dropped the daily oscillation by 2% to 2.388 ppm. Dropping the temperature coefficient for the current by 4% decreased the noise floor to its minimal value of 40.31 ppm<sup>2</sup>—almost no effect. With all this optimization of temperature correction, the daily oscillation dropped to 2.3138 ppm—our final value. This process of trying to adjust our temperature coupling coefficient to minimize the annual signal convinced us that at most a small part of the remaining 24 hour oscillation came from uncorrected temperature variations.</p><p>The original temperature correction coefficient was measured when the hardware was first turned on, and we know there was at least a 30-day initial burn in transient before stable operation was seen, so it is reasonable that the effective temperature sensitivity could be reduced 19% from what was first measured. No other temperature coefficients appear to reduce the noise floor significantly. This makes sense because all the key physics happens on the temperature stabilized and temperature monitored Esaki copper plate—which is why we designed it that way.</p><p>After all these small corrections for temperature, we got the data shown above in <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>, showing both sun-locked and cosmos-locked oscillations. We note that the cosmos locked signals are asynchronous with day-night variations and thus represent a completely different and orthogonal signal—as is normal for different Fourier components.</p></sec><sec id="s2"><title>2. Probability of False Alarm</title><p>With a complex Gaussian random noise floor, the magnitude<sup>2</sup> has an exponential distribution with the probability of the noise exceeding a value μ equal to exp(−μ/σ). To estimate the rms noise floor σ of the magnitude squared we measure the mean and standard deviation of the magnitude<sup>2</sup> of the complex Fourier transform in regions above and below the signal region, at Fourier components 730 and 732 day. The standard deviations are almost exactly equal, and the means are about 9% apart.</p><p>In <xref ref-type="fig" rid="fig5"><xref ref-type="fig" rid="fig">Figure </xref>5</xref> we examine the mean value and standard deviation for the squared-magnitude of the signals below and above the yearly peaks. For Complex Gaussian noise, the means and standard deviations should be equal, and this data is close to that. The two portions had similar statistics to about 8% on the mean value and 3% on the standard deviation. We took the geometric mean of the two standard deviations—although they were so close to equal that their average gave almost the same value.</p><p>Using the familiar exponential model for mean-square complex Gaussian noise, we get a simple exponential probability function as shown in <xref ref-type="fig" rid="fig6"><xref ref-type="fig" rid="fig">Figure </xref>6</xref>. The probability that the sun-locked signal came from random noise is about 10<sup>−13</sup>, and the probability that the cosmos locked signal came from random noise is about 10<sup>−7</sup>.</p></sec><sec id="s3"><title>3. Checking the Shape of the Sun-Locked Signal</title><p>To look at the daily response in more detail, we averaged the tunnel data over 365 &#215; 2 = 730 days of 24 hours each. The average is shown in the plot below, <xref ref-type="fig" rid="fig7"><xref ref-type="fig" rid="fig">Figure </xref>7</xref>. This is the voltage required to maintain the constant tunnel current. We note that this residual voltage signal is quite opposite in shape to the effect of lab temperature variations, which tend to be coolest in the morning and warmest in the afternoon, producing more tunneling in the afternoon and thus a lower voltage in our constant current design—the opposite of what we see here.</p></sec><sec id="s4"><title>4. Checking the Shape of the Cosmos-Locked Signal</title><p>To look at the daily response locked to the cosmos, we averaged tunnel data over 366 &#215; 2 = 732 days shifting the start of the day by 24 hrs/366 days every day. The average is shown in <xref ref-type="fig" rid="fig8"><xref ref-type="fig" rid="fig">Figure </xref>8</xref>, looking rather different than the daily average since it is an independent Fourier component with no coupling to the sun-locked Fourier component. Here the hours match the orientation of the Earth when the data collection began on 10/1/2011.</p></sec><sec id="s5"><title>5. Discussion</title><p>70 years ago, the vacuum field had been considered to be a simple result of the non-zero ground state energy in quantum mechanics. A large number of experiments, beginning with Casimir [<xref ref-type="bibr" rid="scirp.94989-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.94989-ref15">15</xref>] , have confirmed that the vacuum E &amp; M fields exist in terawatt/cm<sup>2</sup> intensity, creating up to 19 pounds/inch<sup>2</sup> pressure on two closely spaced reflective plates. The fields measured are experimentally real and intense.</p><p>When annual oscillations in radioactive decay rates were reported by three national labs (US, Russian and German), variations in Planck’s constant became a candidate, confirmed in an independent electron tunneling experiment [<xref ref-type="bibr" rid="scirp.94989-ref11">11</xref>] . In addition, that same tunneling experiment with additional analysis showed high confidence detections of Planck radiation coming both from the direction of the Sun and from a direction outside our solar system aligned in right ascension with the red super giant star Betelgeuse.</p><p>This research combined with earlier time varying radioactive decay concludes:</p><p>1) The vacuum field is a spectrum of radiation that can vary temporally and spatially to create observable time varying effects when forms of detection are used which are nonlinear in h (Such as radioactive decay and tunneling).</p><p>2) The Sun, and by generalization all stars, is shown to emit a local spectrum of vacuum radiation which adds to the vacuum field from the surrounding universe.</p></sec><sec id="s6"><title>6. Conclusions</title><p>1) h is a spectrum of radiation, we call Casimir radiation, that has been shown to vary in intensity and frequency in our laboratories in over 50 experiments.</p><p>2) Annual variations in strong decay, weak decay and electromagnetic tunneling are all consistent with h varying around the orbit of the Earth—peaking in January and minimizing in July. No other cause has been identified.</p><p>3) The annual variations of electromagnetic tunnel current were 180 degrees out of phase with strong and weak decay rates, since electromagnetic tunneling has an additional factor of h<sup>2</sup> in the numerator of the tunneling exponent due to the size of the atoms changing proportional to h<sup>2</sup>. This was predicted and confirmed experimentally by the author, supporting h as the causal factor.</p><p>4) The E &amp; M tunnel diode data (reported here) detected sun-locked and cosmos-locked variations in tunnel current at 13 sigma and 7 sigma confidence, providing strong evidence that the Sun as well as more distant cosmic sources is generating Casimir radiation.</p><p>5) The model that emerges from the above research is that the vacuum field is much more complex and much more interactive than commonly believed. The vacuum field has been proven in 50 years of Casimir lab experiments to vary spatially, temporally and spectrally in our labs. These new data show Casimir radiation also varying across the Earth’s orbit, and our own Sun seems to be emitting it as well as a more distant cosmic source.</p><p>Future Research: Our conclusion is that the vacuum field is not a single invariant spectrum but is a general background with many local variations, likely with every star emitting it. Such Casimir emissions would tend to increase the value of h over time, making the time rate of the universe speed up with age. For this reason, this process of emitting Casimir radiation from stars may contribute to the observed red shift in the universe—not from a Doppler shift, but simply because time is flowing more slowly in the past with its lower level of Casimir radiation (the vacuum field). Quantitative models for the emission of Casimir radiation would allow evaluation of this option, perhaps also affecting the needs for dark energy and dark matter, which have so far eluded detection.</p></sec><sec id="s7"><title>Conflicts of Interest</title><p>The author declares no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s8"><title>Cite this paper</title><p>Hutchin, R.A. (2019) Detection of Casimir Radiation from Our Sun. Optics and Photonics Journal, 9, 141-154. https://doi.org/10.4236/opj.2019.99013</p></sec><sec id="s9"><title>Appendix—Experimental Hardware Design</title><p>The heart of the experiment is 5 Schottky tunnel diodes wired in parallel and bonded to a 1 cm thick temperature controlled copper plate, as shown in <xref ref-type="fig" rid="fig">Figure </xref>A1. Heavy duty resistors are bonded to the under-side of the copper plate to control the temperature, which was set to 40 deg C—much higher than the room temperature. A PID thermal controller was setup to maintain the temperature +/− 0.1 deg C. All temperatures, currents, and voltages were monitored every 10 seconds for 2<sup>1/2</sup> years—all of them with 10 digit accuracy except for the internal temperature of the voltage and current meters, which were recorded to 0.1˚C as shown in <xref ref-type="fig" rid="fig">Figure </xref>A2.</p><p>The sensors head and all the electronics were kept in separate Faraday cages to shield them from any local microwave effects, as shown in <xref ref-type="fig" rid="fig">Figure </xref>A3. This additional isolation plus the shielded boxes in which the tunnel diodes were mounted should have isolated these tunnel junctions from all local effects except for the Casimir radiation itself, which we measured.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.94989-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Siegert, H., Schrader, H. and Sch&amp;#246;tzig, U. 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