<?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">AMPC</journal-id><journal-title-group><journal-title>Advances in Materials Physics and Chemistry</journal-title></journal-title-group><issn pub-type="epub">2162-531X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ampc.2015.510043</article-id><article-id pub-id-type="publisher-id">AMPC-60668</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> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Flux Pinning in Y- and Ag-Doped MgB&lt;sub&gt;2&lt;/sub&gt;
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ack</surname><given-names>Dyson</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Daniele</surname><given-names>Rinaldi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Gianni</surname><given-names>Barucca</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Gianni</surname><given-names>Albertini</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Simone</surname><given-names>Sprio</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Anna</surname><given-names>Tampieri</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>SIMAU, Università Politecnica delle Marche, Ancona, Italy</addr-line></aff><aff id="aff2"><addr-line>Institute of Science and Technology for Ceramics, National Research Council, Faenza, Italy</addr-line></aff><pub-date pub-type="epub"><day>30</day><month>09</month><year>2015</year></pub-date><volume>05</volume><issue>10</issue><fpage>426</fpage><lpage>438</lpage><history><date date-type="received"><day>24</day>	<month>August</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>25</month>	<year>October</year>	</date><date date-type="accepted"><day>28</day>	<month>October</month>	<year>2015</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>
 
 
  High temperature superconductor research is presently concentrated upon the flux pinning properties of the Abrikosov lattice of the mixed-mode superconducting phase. The temperature thermal fluctuations, current and magnetic field unpin the flux vortices and so cause electromagnetic resistivity in high temperature superconductors. Materials with higher vortex pinning exhibit less resistivity and are more attractive for industrial uses. In the present article, we measured and correlated the pinning flux energy barrier, determined by AC magnetic measurements, and transmission electron microscopy measurements to the critical current 
  J<sub>c</sub> in Yttrium- and Silver-doped MgB
  <sub>2</sub> superconductors. The energy of the flux vortex was evaluated as a function of the magnetic field. The energy barrier curves suggest an optimal doping level to occur in doped materials. This result only depends on the optimal size and distribution of precipitates, and not on their chemical composition. The energy barriers have been compared with that of undoped MgB
  <sub>2</sub> in literature.
 
</p></abstract><kwd-group><kwd>Flux Pinning</kwd><kwd> AC Magnetic Measurements</kwd><kwd> Critical Current</kwd><kwd> Yttrium-Doping</kwd><kwd> Silver-Doping</kwd><kwd> MgB&lt;sub&gt;2&lt;/sub&gt; Superconductors</kwd><kwd> Transmission Electron Microscopy</kwd><kwd> X-Ray Diffraction</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Magnesium diboride MgB<sub>2</sub> BCS-type superconductors (SCs) are widely used in sensors, electric power appli- cations and electronic devices. In fact, even though their critical temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x6.png" xlink:type="simple"/></inline-formula> is lower than in tra- ditional cuprate SCs, their upper critical field <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x7.png" xlink:type="simple"/></inline-formula> is actually higher while an operating temperature of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x8.png" xlink:type="simple"/></inline-formula> is relatively easy to reach using liquid hydrogen or cryocoolers. The absence of weak links in the matrix (no inter-granular obstacles impede current flow) as well as a strong coupling between grains makes MgB<sub>2</sub> very useful in technological applications [<xref ref-type="bibr" rid="scirp.60668-ref1">1</xref>] . The possible enhancement of the critical temperature and the improvement of the existing high levels of transport current are therefore important topics for this material. On the other hand, the low density of the pure compound and the relative scarcity of pinning centres, actually reduce the sustainable current density in high magnetic fields.</p><p>The metal-like structure of MgB<sub>2</sub> at room temperature makes it ideal for applications in engineering contexts unlike the cuprate SCs, which exhibits a non-metallic behaviour at room temperature. The latter fact limits the technological applications of cuprate due to difficulties associated with the material processing. As an example, MgB<sub>2</sub> can be readily transformed into wires and tapes whereas the well-known cuprate YBCO needs to be deposited onto wires through specifically settled processes.</p><p>Superconductivity in MgB<sub>2</sub> is based on two differing mechanisms due to its electronic structure. MgB<sub>2</sub> has strong <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x9.png" xlink:type="simple"/></inline-formula> bonds in the B planes and weak <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x10.png" xlink:type="simple"/></inline-formula> bonds in between them. Phonon modes in the Boron planes have a dominant effect due to strong electron-phonon <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x11.png" xlink:type="simple"/></inline-formula> coupling [<xref ref-type="bibr" rid="scirp.60668-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref3">3</xref>] , which results in the formation of strong electron pairs confined to the planes. It is related to a complicated Fermi surface, with two superconduct- ing bands, which induces a strongly anisotropic conductivity in the lattice structure. The two bands produce different levels of superconductivity, the intra-planar variant being the weaker, leaving a particularly large conductivity in the Boron ab-plane. The high critical temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x12.png" xlink:type="simple"/></inline-formula> of MgB<sub>2</sub> is due to the electron-phonon coupling in the plane [<xref ref-type="bibr" rid="scirp.60668-ref4">4</xref>] where the inter- and intra-band scattering effects tend to reduce the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x13.png" xlink:type="simple"/></inline-formula> value [<xref ref-type="bibr" rid="scirp.60668-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref5">5</xref>] .</p><p>The complicated dual band superconductivity structure of MgB<sub>2</sub> affects the main superconducting parameters like the irreversibility field, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x14.png" xlink:type="simple"/></inline-formula>, the upper critical field<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x15.png" xlink:type="simple"/></inline-formula>, the critical superconducting temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x16.png" xlink:type="simple"/></inline-formula> and, importantly, also the critical current <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x17.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.60668-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref7">7</xref>] . In order to increase the values of the last two parameters, the introduction of controlled amounts of doping agents is an interesting procedure: in past experiments, the critical superconducting field was observed to rise but the critical temperature remained idle [<xref ref-type="bibr" rid="scirp.60668-ref7">7</xref>] . To the best of our knowledge, increase of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x18.png" xlink:type="simple"/></inline-formula> induced by doping MgB<sub>2</sub> was only reported in the high field case of nano-C doped MgB<sub>2</sub> [<xref ref-type="bibr" rid="scirp.60668-ref8">8</xref>] .</p><p>Conversely, it was found that the critical current could be modified through doping. Indeed, in MgB<sub>2</sub> the current flow is not governed by the weak link mechanism and hence the vortex dynamics alone determines the value of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x19.png" xlink:type="simple"/></inline-formula>. Compounds like Nb<sub>3</sub>Sn support a higher <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x20.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.60668-ref9">9</xref>] because factors like mass density, packing fraction and connectivity as well as impurities like MgO play a major enhancing role in the material. In type II SCs, operating in the mixed regime, the Abrikosov flux lattice can be driven by the electric field, which induces a backward electromotance, dissipating power as the flux changes through the circuit. In such complicated scenarios, thermally activated flux flow (TAFF) and flux creep have been observed [<xref ref-type="bibr" rid="scirp.60668-ref10">10</xref>] . The remedy to this is the introduction of pinning centres locking the flux vortices with a potential thus allowing the critical current to increase. Different types of pinning centres can be introduced, e.g. grain boundaries, point defects as well as impurities and lattice variations brought on by doping [<xref ref-type="bibr" rid="scirp.60668-ref8">8</xref>] .</p><p>In order to make the formation of pinning centres effective to increase<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x21.png" xlink:type="simple"/></inline-formula>, they should exhibit sizes as large as the coherence length [<xref ref-type="bibr" rid="scirp.60668-ref8">8</xref>] . In MgB<sub>2</sub> it is valued in the range between 2 and 10 nm [<xref ref-type="bibr" rid="scirp.60668-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref11">11</xref>] . Zehetmayer et al. [<xref ref-type="bibr" rid="scirp.60668-ref7">7</xref>] report that neutron radiation induces defects of about 5 - 10 nm in size, thus creating pinning centres that in- fluence mainly the intra-band <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x22.png" xlink:type="simple"/></inline-formula> scattering. Compared to the alternative Carbon doping, neutron irradia- tion seems an efficient method for adding pinning centres into the material. Since grain boundaries also act as pinning centres, the decreasing grain dimensions improve the critical current. Beside the pinning centres, the densification of the compound in general enhances the superconducting state.</p><p>For MgB<sub>2</sub> in particular, good results in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x23.png" xlink:type="simple"/></inline-formula> enhancement have been obtained by the use of doping agents. Different elements have been used so far, spanning from rare-earths to magnetic elements as well as Silicon [<xref ref-type="bibr" rid="scirp.60668-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref13">13</xref>] . The best results are obtained when Carbon substitutes Boron. Carbon is an electron donor that can influence the Fermi surface of the MgB<sub>2</sub> lattice. The result is a significant enhancement of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x24.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x25.png" xlink:type="simple"/></inline-formula> through enhanced intra-band scattering [<xref ref-type="bibr" rid="scirp.60668-ref7">7</xref>] . The Carbon substitution in the Boron layer causes an in-plane lattice distortion, tending to reduce the coherence length. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x26.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x27.png" xlink:type="simple"/></inline-formula> actually increase owing to the extra intra- band scattering in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x28.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x29.png" xlink:type="simple"/></inline-formula> orbitals. This improves the flux pinning in high fields and in turn <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x30.png" xlink:type="simple"/></inline-formula> when the doping levels are optimal [<xref ref-type="bibr" rid="scirp.60668-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref14">14</xref>] . Unfortunately, these gains were accompanied by a lowering of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x31.png" xlink:type="simple"/></inline-formula>.</p><p>Alternatively, SiC doping causes lattice distortion as well dislocation, which in turn acts as pinning centres [<xref ref-type="bibr" rid="scirp.60668-ref15">15</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref16">16</xref>] . Good results have been obtained also by means of graphene doping [<xref ref-type="bibr" rid="scirp.60668-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref17">17</xref>] .</p><p>Improvement of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x32.png" xlink:type="simple"/></inline-formula> can also occur without ion substitution in the MgB<sub>2</sub> lattice. In this respect, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x33.png" xlink:type="simple"/></inline-formula>values higher than in pure sample were found in Cu-doped samples, due to the formation of an additional MgCu<sub>2</sub> phase that acted as pinning centres [<xref ref-type="bibr" rid="scirp.60668-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref19">19</xref>] . If, on the contrary, substitution of Magnesium with Copper occurs, a hole-donor compound is obtained, which produced an unexpected reduction in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x34.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.60668-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref21">21</xref>] . Also Silver doping in MgB<sub>2</sub> yielded an increase of the critical current, due to the formation of MgAg nanoparticles that acted as pinning centres [<xref ref-type="bibr" rid="scirp.60668-ref22">22</xref>] - [<xref ref-type="bibr" rid="scirp.60668-ref24">24</xref>] .</p><p>On the basis of these previous investigations, it can be concluded that, since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x35.png" xlink:type="simple"/></inline-formula> depends on the vortex dynamics, a high flux pinning efficiency is fundamental in sustaining high levels of critical current.</p><p>This paper studies the behaviour of the vortex pinning potential (barrier) in Magnesium diboride doped with Silver or Yttrium, a hole and an electron donor, respectively. Samples are prepared by means of hot isostatic pressing (HIP) or uniaxial hot pressing (UHP) techniques, respectively. The correlation between structural properties and performance, in terms of critical current, was analysed in order to elucidate the importance of pinning centres in doped MgB<sub>2</sub>. In particular, scope of this work is to clarify the influence of Silver and Yttrium doping agents (at our best knowledge the latter was rarely studied) on the height of the vortex energy barrier. This last is a fundamental property for improving the superconducting critical current in the presence of external magnetic fields. Moreover, the model used to evaluate the flux energy barrier proved to be a convenient tool for the analysis and the comprehension of the J<sub>c</sub> magnitude in relation with structural parameters. In fact, non linear and complex phenomena involved in the depinning mechanism need special care in the data analysis.</p><p>In a previous study of MgB<sub>2</sub> [<xref ref-type="bibr" rid="scirp.60668-ref23">23</xref>] , it was discussed that the sample purity and density were not directly related to the superconducting properties, while the pinning centres were suggested to play a fundamental role. Interest- ing results in this sense were obtained with small amounts of Ag and Y doping. In order to make this last point clear, our results are compared with those reported in literature in the case of undoped MgB<sub>2</sub> samples, either synthesized as bulk or as film.</p></sec><sec id="s2"><title>2. Experimental</title><p>UHP (Y-doped) and HIP (Ag-doped) techniques have been used to obtain consolidated MgB<sub>2</sub> bulk samples. The UHP (Uniaxial Hot Pressing) samples were prepared as follow, magnesium, boron and yttrium powders in the composition Mg<sub>1</sub><sub>−</sub><sub>x</sub>Y<sub>x</sub>B<sub>2</sub>, have been heated in vacuum at a rate of ~25 K/min up to the sintering temperature of 1373 K. At T = 773 K, a pressure of 30 MPa was applied and kept constant. The sample was kept at the final temperature for 20 min and then spontaneously cooled up to ambient temperature under vacuum. No pressure is applied during the cooling. The HIP (Hot Isostatic Pressing) samples were prepared starting from the composition Mg<sub>1</sub><sub>−</sub><sub>x</sub>Ag<sub>x</sub>B<sub>2</sub>. At first, a pressure of 150 MPa in inert atmosphere was applied, followed by a cold isostatic pressing at 300 MPa. The pellets were then encapsulated under vacuum prior pressure-heating treatments. Pressure and temperature were increased to reach the final value simultaneously (150 MPa and 1073 K, for 1 hour). Then the samples spontaneously cool under high pressure until the temperature of 373 K, then the pressure was lowered up to atmospheric pressure.</p><p>These complex preparation techniques are explained in detail in Ref. [<xref ref-type="bibr" rid="scirp.60668-ref23">23</xref>] . The samples are listed in <xref ref-type="table" rid="table1">Table 1</xref>. Once manufactured, the samples were structurally characterized by X-ray diffraction (XRD) using a Bruker D8 Advance diffractometer (operating with a Cu-Kα radiation source) together with transmission electron micro- scopy (TEM), carried out on a Philips CM200 electron microscope operating at 200 kV. For TEM observations, the samples were prepared by scraping small amounts of powder from each pellet over carbon coated copper grids.</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Studied samples with molar composition and preparation technique</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Sample</th><th align="center" valign="middle" >Technique</th></tr></thead><tr><td align="center" valign="middle" >AG1: 1Mg + 2B + 0.01Ag</td><td align="center" valign="middle" >HIP</td></tr><tr><td align="center" valign="middle" >AG5: 1Mg + 2B + 0.05Ag</td><td align="center" valign="middle" >HIP</td></tr><tr><td align="center" valign="middle" >AG20: 1Mg + 2B + 0.2Ag</td><td align="center" valign="middle" >HIP</td></tr><tr><td align="center" valign="middle" >Y05: 1Mg + 2B + 0.005Y</td><td align="center" valign="middle" >UHP</td></tr><tr><td align="center" valign="middle" >Y10: 1Mg + 2B + 0.010Y</td><td align="center" valign="middle" >UHP</td></tr><tr><td align="center" valign="middle" >Y15: 1Mg + 2B + 0.015Y</td><td align="center" valign="middle" >UHP</td></tr></tbody></table></table-wrap><p>The AC magnetic measurements were carried out on a Quantum Design PPMS system. Complex magnetic susceptibility data were collected as a function of temperature by applying a static field (varying from 1.5 to 7.0 T), being the AC field fixed at 1 Oersted, with frequency (f) varying from 100 Hz to 10 KHz for each applied static field. The nonlinear complex susceptibility has been measured up to the third harmonic for each measuring frequency. These experimental measurements are fitted using nonlinear numerical analysis (see appendix) and values for the flux pinning potential (energy barrier) calculated in each case [<xref ref-type="bibr" rid="scirp.60668-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref25">25</xref>] - [<xref ref-type="bibr" rid="scirp.60668-ref28">28</xref>] . These were grouped according to the applied field for each case of Y and Ag doping.</p></sec><sec id="s3"><title>3. Results and Discussion</title><p>X-ray patterns recorded for the Ag- and Y-doped MgB<sub>2</sub> samples are reported in <xref ref-type="fig" rid="fig1">Figure 1</xref>. In the whole range of investigation, no significant change of MgB<sub>2</sub> lattice parameters was found, within experimental error. Thus we concluded that no substitutions occurred in the MgB<sub>2</sub> unit cell.</p><fig-group id="fig1"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> X-ray patterns of Ag-doped (a) and Y-doped (b) MgB<sub>2</sub> samples. A re- ference scan from an undoped MgB<sub>2</sub> sample (prepared by HIP) is also reported.</title></caption><fig id ="fig1_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x36.png"/></fig><fig id ="fig1_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x37.png"/></fig></fig-group><p>All the diffraction peaks of the undoped sample are attributed to pure MgB<sub>2</sub> and MgO compounds while addi- tional peaks are observed in the doped samples.</p><p>For the Ag-doped samples, the increase in Ag concentration caused the Mg peaks to disappear while the phase Ag-Mg, presents as ε’-Ag<sub>0.24</sub>Mg<sub>0.76</sub> (ICDD card number 39-0992) in the AG1 sample, as ε’-Ag<sub>0.24</sub>Mg<sub>0.76</sub> and ε-AgMg<sub>3</sub> (ICDD card number 39-0991) in AG5, becomes AgMg<sub>3</sub> (ICDD card number 01-1170) in the AG20 sample. Furthermore, the presence of metallic Ag was found to increase with the amount of Ag intro- duced in the MgB<sub>2</sub> matrix. The mean dimension of the Ag-Mg grains evaluated through the Scherrer formula was 9 &#177; 1 nm for the AG1 sample, 10 &#177; 1 nm for AG5 and 13 &#177; 1 nm for AG20.</p><p>In the Y-doped samples, X-ray measurements showed the presence of MgB<sub>4</sub> (ICDD card number 73-1014) and YB<sub>4</sub> (ICDD card number 79-1992) phases in addition to MgB<sub>2</sub> and MgO. The intensity of MgB<sub>4</sub> peaks remained unchanged with the Yttrium content, whereas those belonging to YB<sub>4</sub> increased. The evaluated average grain size of MgB<sub>4</sub> was the same for both Y05 and Y15 samples: d = 54 &#177; 1 nm. The average grain size of YB<sub>4</sub> was 13 &#177; 3 nm for Y05 and 38 &#177; 2 nm for Y15.</p><p>Better results in XRD analysis with respect to a previous work [<xref ref-type="bibr" rid="scirp.60668-ref23">23</xref>] are due to the improved instrument re- solution. The sample Y10 could not be analysed by XRD but this deficiency does not invalidate the conclusions of the present work, as highlighted in the following discussion.</p><p>Transmission Electron Microscopy (TEM) analyses of Ag- and Y-doped samples confirmed the results of X-ray analysis and show the presence of precipitates outside the MgB<sub>2</sub> grains. In particular two bright field images for sample AG5 are given in <xref ref-type="fig" rid="fig2">Figure 2</xref>. Small dark precipitates of size ranging from 10 nm to 20 nm are also easily visible. The corresponding electron diffraction patterns are shown in the insets. Diffraction spots and rings can be attributed to the presence of the MgB<sub>2</sub> lattice and Magnesium-Silver phases (it was not actually possible to distinguish between Ag or Mg<sub>3−x</sub>Ag<sub>x</sub> by TEM diffraction analyses).</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> shows two bright field images of the Y-doped sample Y15. Small dark precipitates having sizes ranging from few nanometres to a few tens of nanometres are visible. The diffraction images related to these areas indicate the presence of MgB<sub>4</sub> and YB<sub>4</sub> phases (it was not possible to distinguish between the two phases).</p><p>The values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x38.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x39.png" xlink:type="simple"/></inline-formula> were measured through the AC complex magnetic susceptibility [<xref ref-type="bibr" rid="scirp.60668-ref23">23</xref>] . From these parameters the ability of the material to support the superconducting state can be inferred. A measure of the quality of a superconductor is the transition ratio, TR (defined as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x40.png" xlink:type="simple"/></inline-formula> where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x41.png" xlink:type="simple"/></inline-formula> is the transition width, for more details see Ref. [<xref ref-type="bibr" rid="scirp.60668-ref21">21</xref>] ). A further parameter is the ratio<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x42.png" xlink:type="simple"/></inline-formula>, with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x43.png" xlink:type="simple"/></inline-formula>.</p><p>According to <xref ref-type="table" rid="table2">Table 2</xref>, the Ag- and Y-doped samples have relatively good performances as superconductors</p><fig-group id="fig2"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> (a) Sample AG5 seen as a TEM image and as a diffraction pattern (inset). (b) Sample AG5 seen as a TEM image and as a diffraction pattern (inset) at around twice the magnification of image (a).</title></caption><fig id ="fig2_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x44.png"/></fig></fig-group><fig-group id="fig3"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> (a) Sample Y15 seen as a TEM image and as a diffraction pattern (inset); (b) Sample Y15 seen as a TEM image and as a diffraction pattern (inset) at around thrice the magnification of image (a).</title></caption><fig id ="fig3_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x45.png"/></fig></fig-group><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Superconductor behaviour parameterised according to the T<sub>c</sub>, TR and ΔT<sub>200</sub> indices</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Sample</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x46.png" xlink:type="simple"/></inline-formula>(&#177;0.25%)</th><th align="center" valign="middle" >TR (&#177;8%)</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x47.png" xlink:type="simple"/></inline-formula>(&#177;8%)</th></tr></thead><tr><td align="center" valign="middle" >AG1</td><td align="center" valign="middle" >38.45</td><td align="center" valign="middle" >0.0036</td><td align="center" valign="middle" >0.62</td></tr><tr><td align="center" valign="middle" >AG5</td><td align="center" valign="middle" >38.53</td><td align="center" valign="middle" >0.0057</td><td align="center" valign="middle" >0.70</td></tr><tr><td align="center" valign="middle" >AG20</td><td align="center" valign="middle" >38.38</td><td align="center" valign="middle" >0.0078</td><td align="center" valign="middle" >1.04</td></tr><tr><td align="center" valign="middle" >Y05</td><td align="center" valign="middle" >38.85</td><td align="center" valign="middle" >0.0154</td><td align="center" valign="middle" >0.59</td></tr><tr><td align="center" valign="middle" >Y10</td><td align="center" valign="middle" >38.85</td><td align="center" valign="middle" >0.0129</td><td align="center" valign="middle" >0.72</td></tr><tr><td align="center" valign="middle" >Y15</td><td align="center" valign="middle" >38.81</td><td align="center" valign="middle" >0.0173</td><td align="center" valign="middle" >0.67</td></tr></tbody></table></table-wrap><p>and the two groups show similar behaviour albeit at different levels. In particular, the critical temperature is comparable to those reported in literature for MgB<sub>2</sub> superconductors.</p><p>The critical current was valued by means of AC magnetic susceptibility as a function of temperature in a range just below the critical temperature in absence of a DC applied field. Overall trends in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x48.png" xlink:type="simple"/></inline-formula> for various samples are shown in <xref ref-type="fig" rid="fig4">Figure 4</xref>. In terms of the absolute temperature, the Y-doped group obtained better perfor- mance. No major difference in absolute current has been detected among the Y-doped samples but degradation is evident in the AG20 sample among the Ag-doped samples.</p><p>For a deeper understanding of the critical current behaviour, we consider the pinning mechanism in the super- conducting regime and compute the energy barrier for the pinning, especially when an external field is applied. In this framework the higher the flux pinning barrier, the higher the maximum current the sample will support. In fact, when the magnetic flux detaches, the Lorentz forces induce a finite resistivity, which destroys the super- conducting state. In this context different models based on the complex magnetic AC susceptibility measure- ments in presence of applied external fields have been proposed. Zazo et al. valued the activation energy for the flux by applying the Arrhenius law [<xref ref-type="bibr" rid="scirp.60668-ref26">26</xref>] . For a YBaCuO polycrystalline sample, they reported an activation energy varying from 3.41 to 1.41 eV; in this respect the Arrhenius law turned out to be too simple to correctly interpret the complex flux dynamics of the system in our case.</p><p>In order to improve the analysis, Qin et al. [<xref ref-type="bibr" rid="scirp.60668-ref27">27</xref>] suggested that the dependence of the flux creep activation</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> The critical current derived from AC susceptibility measurements plotted as a function of the temperature</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x49.png"/></fig><p>energy upon applied magnetic field follows a power law and proposed the following mathematical model:</p><disp-formula id="scirp.60668-formula1333"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-1510418x50.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x51.png" xlink:type="simple"/></inline-formula> is the flux pinning energy barrier, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x52.png" xlink:type="simple"/></inline-formula>is the applied magnetic induction,</p><disp-formula id="scirp.60668-formula1334"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-1510418x53.png"  xlink:type="simple"/></disp-formula><p>is the critical current evaluation according to the Bean critical state model [<xref ref-type="bibr" rid="scirp.60668-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref29">29</xref>] , <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x54.png" xlink:type="simple"/></inline-formula>is the measuring field, d is the sample half-thickness, U(T) is a temperature scaling function</p><disp-formula id="scirp.60668-formula1335"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-1510418x55.png"  xlink:type="simple"/></disp-formula><p>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x56.png" xlink:type="simple"/></inline-formula> is the irreversibility temperature to be determined from the data.</p><p>On the left hand side of Equation (1), f is the measurement frequency and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x57.png" xlink:type="simple"/></inline-formula> is the inverse of the cha- racteristic time scale.</p><p>Amalgamating these expressions gives the experimental relationship:</p><disp-formula id="scirp.60668-formula1336"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-1510418x58.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x59.png" xlink:type="simple"/></inline-formula> and</p><disp-formula id="scirp.60668-formula1337"><graphic  xlink:href="http://html.scirp.org/file/4-1510418x60.png"  xlink:type="simple"/></disp-formula><p>T is set to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x61.png" xlink:type="simple"/></inline-formula>, the temperature at which the maximum in the imaginary part of the complex susceptibility occurs [<xref ref-type="bibr" rid="scirp.60668-ref27">27</xref>] . In fact at this temperature the complete flux penetration is established for every tuple <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x62.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.60668-ref29">29</xref>] . At this point it is sufficient to set the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x63.png" xlink:type="simple"/></inline-formula> to the onset temperature of third susceptibility harmonic valued at the higher frequency [<xref ref-type="bibr" rid="scirp.60668-ref28">28</xref>] . Equation (4) is linear with respect to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x64.png" xlink:type="simple"/></inline-formula>, plotting it in the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x65.png" xlink:type="simple"/></inline-formula> plane at constant<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x66.png" xlink:type="simple"/></inline-formula>. Unfortunately, using Equation (4), as a model with the present data, does not satisfactorily produce the expected straight line with slope <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x67.png" xlink:type="simple"/></inline-formula> and intercept<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x67.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x68.png" xlink:type="simple"/></inline-formula>.</p><p>Ghigo et al. [<xref ref-type="bibr" rid="scirp.60668-ref28">28</xref>] suggested the modified equation which we adopt here:</p><disp-formula id="scirp.60668-formula1338"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-1510418x69.png"  xlink:type="simple"/></disp-formula><p>Setting <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x70.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x71.png" xlink:type="simple"/></inline-formula> we obtain:</p><disp-formula id="scirp.60668-formula1339"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-1510418x72.png"  xlink:type="simple"/></disp-formula><p>The experimental x values are calculated with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x73.png" xlink:type="simple"/></inline-formula> as above. The equation above is fitted using a non- linear algorithm to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x74.png" xlink:type="simple"/></inline-formula> data to get values for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x75.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x76.png" xlink:type="simple"/></inline-formula> (see Appendix). Applying this model a satis- factory fit is obtained: the graph in <xref ref-type="fig" rid="fig5">Figure 5</xref> is a plot of this fitted curve for different field levels for the 20% Ag doping.</p><p>In <xref ref-type="fig" rid="fig6">Figure 6</xref> the valued <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x77.png" xlink:type="simple"/></inline-formula> are plotted as a function of applied field.</p><p>The phenomenological data analysis procedure described above gives the simplest, most reliable impression of how doping influences the energy barrier variation supported by the data.</p><p>Both for Yttrium and Silver a decrease of U<sub>0</sub> barrier is observed at increasing applied magnetic field. At a fixed field, the U<sub>0</sub> values do not always increase with increasing concentration of dopant, thus indicating that</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> The frequency logarithm (ln f) of the measurement AC magnetic field plotted against x (as defined in the text). The power law (7) is fitted to x valued from the experimental data. The fit concerns the 20% Ag doped MgB<sub>2</sub> sample at different DC field: B<sub>DC</sub> field is expressed in Tesla</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x78.png"/></fig><fig-group id="fig6"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> The energy barrier variation U<sub>0</sub> with applied DC field across each doping series (the zero field point omitted due to low confidence). (a) Ag series. (b) Y series.</title></caption><fig id ="fig6_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x79.png"/></fig><fig id ="fig6_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x80.png"/></fig></fig-group><p>optimal concentrations for obtaining high barriers occurs.</p><p>The data in <xref ref-type="fig" rid="fig6">Figure 6</xref> resemble a power law: however, at high field values the samples exhibit the same behaviour regardless of doping content.</p><p>These experiments suggest the occurrence of a maximum doping level in a type II superconductor for the optimal flux pinning properties―a possible consequence of which is the maximum sustainable <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x81.png" xlink:type="simple"/></inline-formula> for the material.</p><p>No significant improvements have been detected in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x82.png" xlink:type="simple"/></inline-formula> although the doped samples exhibit high <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x83.png" xlink:type="simple"/></inline-formula> (rang- ing from 38.85 K to 38.38 K). As outlined in the introduction, the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x84.png" xlink:type="simple"/></inline-formula> depends on the electron-phonon coupling as well as the intra- and inter-band scattering and electron density.</p><p>The values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x85.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x86.png" xlink:type="simple"/></inline-formula> could change in principle when Y substitutes for Mg because Y is an electron donor. In our case, although there is no experimental evidence for Mg substitution in the crystalline structure, the critical current is affected by the introduction of Ag or Y. This can be explained in terms of the formation of pinning centres. In fact both the X-ray and TEM analyses demonstrated the existence of non-superconducting precipitates, with dimensions in the range 2 to 10 nm; exactly those required to act as efficient pinning centres [<xref ref-type="bibr" rid="scirp.60668-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.60668-ref8">8</xref>] . In the Y-doped samples, among the other precipitates with higher dimensions, the mean radius for the YB<sub>4</sub> is 13 &#177; 3 nm for the sample at 0.5% doping, increasing up to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x87.png" xlink:type="simple"/></inline-formula> nm for 1.5% doping.</p><p>In the Ag-doped samples we detected in MgB<sub>2</sub> doped at 1% Ag nanometric precipitates of MgO and Ag<sub>x</sub>Mg<sub>3</sub><sub>−</sub><sub>x</sub>. These precipitates, having a mean radius of 9 &#177; 1 nm, tend to become larger with Ag concentration (D = 10 &#177; 1 nm in AG5 and d = 13 &#177; 1 nm in AG20) and moreover will transform into the AgMg<sub>3</sub> phase. The precipitate size increases with the dopant concentration for both types of dopant.</p><p>The behaviour of the calculated energy barrier is in agreement with the hypothesis concerning the role played by pinning centres. The Y doping is more effective than Ag at very low dopant concentration and low fields. In all cases the pinning barrier decreases rapidly with the field.</p><p>The MgB<sub>2</sub> doped at 0.5% Y has a possible YO<sub>x</sub> phase as well as a better distribution of pinning centres compared with the sample doped at 1.5% Y which has larger YB<sub>4</sub> precipitates. Both of these contain MgO and MgB<sub>4</sub>.</p><p>In the case of the Ag-doped samples, increasing concentration of Ag increases the number of precipitates such as Ag-Mg of appropriate size to act as pinning centres. By exceeding a certain value of the concentration of Ag, precipitates tend to grow (in size, but probably also in density) losing their effectiveness as pinning centres. The energy barrier variation for both types of doping follows a similar trend.</p><p>The effectiveness of doping to increase the energy barrier is deduced after comparing these experimental data with those obtained from undoped MgB<sub>2</sub> samples reported in literature. In MgB<sub>2</sub> film [<xref ref-type="bibr" rid="scirp.60668-ref30">30</xref>] , U<sub>0</sub> is about 0.9 eV for magnetic field in the range 0 - 1 T, decreasing down to 0.08 at about 7 T. The data have been valued by fitting r to the Arrhenius law. In bulk MgB<sub>2</sub> Jin et al. valued U<sub>0</sub> ranging from 0.6 eV to 0.25 eV at 0.5 and 1 T respectively, by means of current measurements [<xref ref-type="bibr" rid="scirp.60668-ref31">31</xref>] . Senatore et al. compared the experimental results of AC measurements in Bulk MgB<sub>2</sub>, with susceptibility curves obtained by numerical calculations, assuming a non- linear diffusion equation for the magnetic field. They obtained good results fitting with U<sub>0</sub> = 0.7 eV at 0.02 T [<xref ref-type="bibr" rid="scirp.60668-ref32">32</xref>] . Although the reported data are obtained from different samples and different techniques, they confirm that the doping strongly modifies the barrier height. Moreover, at high field (7 - 9 T) Patnaik et al. found U<sub>0</sub> about 0.17 eV [<xref ref-type="bibr" rid="scirp.60668-ref33">33</xref>] , in textured film which is comparable to the values presented in this work, thus confirming that at high field the studied pinning centres are less effective (see also above and Ref. [<xref ref-type="bibr" rid="scirp.60668-ref30">30</xref>] ).</p><p>Our data indicate a strong increase of the energy barrier in doped samples with respect to all these values obtained in the undoped samples, at least at low fields (less than about 5 T).</p><p>The obtained U<sub>0</sub> values indicate an optimal doping level for both the dopants (about 5% for Ag and 0.5% for Y doping). The dopant excess degrades the samples and introduces disorder.</p></sec><sec id="s4"><title>4. Conclusions</title><p>The Y and Ag doped MgB<sub>2</sub> superconductors have been studied by means of magnetic, XRD and TEM measure- ments. The flux pinning energy barrier U<sub>0</sub> has been evaluated and compared among the different samples. The energy barrier height U<sub>0</sub> ranges from 3.5 to 6 eV for the Ag and Y doped samples respectively at low field and fast decreases with the applied magnetic field. The U<sub>0</sub> values of undoped samples shown in the literature (lower then 1 eV at 1 T ) are lower with respect to the doped samples here reported (higher then about 2 eV at 1 T), thus putting in evidence the efficiency of doping, at least at low magnetic field (about 5 T), as explained in the discussion. Better performance levels were achieved in cases where doping was low. As the doping agents do not substitute Mg, the reported results can be considered a clue that efficiency of the pinning centres depends on their size and distribution. The detection of optimal doping levels can be related to the occurrence of optimal dimensions and distributions of the precipitates.</p><p>As Y-doping is rarely studied, this paper also reports useful information on that electron donor dopant.</p></sec><sec id="s5"><title>Cite this paper</title><p>JackDyson,DanieleRinaldi,GianniBarucca,GianniAlbertini,SimoneSprio,AnnaTampieri, (2015) Flux Pinning in Y- and Ag-Doped MgB<sub>2</sub>. Advances in Materials Physics and Chemistry,05,426-438. doi: 10.4236/ampc.2015.510043</p></sec><sec id="s6"><title>Appendix</title><p>The quadruple <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x88.png" xlink:type="simple"/></inline-formula> are to be considered as fitting parameters. The equation is forward sensitive to the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x89.png" xlink:type="simple"/></inline-formula> parameter and is better fitted using a backward optimisation algorithm with respect to this variable. Here again it is sufficient to set the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x90.png" xlink:type="simple"/></inline-formula> to the onset temperature of third susceptibility harmonic valued at the higher frequency [<xref ref-type="bibr" rid="scirp.60668-ref28">28</xref>] ―removing one of the unknowns, leaving the triplet <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x91.png" xlink:type="simple"/></inline-formula> to determine for every data line. Choosing a particular data line, the second and third parameters are determined through “standard” nonlinear fit, while <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x92.png" xlink:type="simple"/></inline-formula> is seeded through a few preliminary tests (Equation (8) below indicates that in most cases the correct<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x93.png" xlink:type="simple"/></inline-formula>).</p><p>The value of the fitted <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x94.png" xlink:type="simple"/></inline-formula> coefficient is then computed for the fit and tabulated. The operation is then repeated for other values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x95.png" xlink:type="simple"/></inline-formula> until a maximum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x96.png" xlink:type="simple"/></inline-formula> case can be identified. That is taken to be the best fit for the data under consideration. There are sufficient data at every field and temperature value and this together with physical regularization permits a more than reasonable degree of confidence in this fitting system. In fact, for every line, {8, 32, 64, 128, 256} respective <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x97.png" xlink:type="simple"/></inline-formula> values are sampled to extract the best value. The answer always converges to a stable limit in every case.</p><p>Practically, there are two areas where problems can occur. The first is the intrinsic mathematical form. In practice the observed curvature, C, of the data points with respect to Equation (5) is small which implies that in Equation (6) one can perturb<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x98.png" xlink:type="simple"/></inline-formula>, and set:</p><disp-formula id="scirp.60668-formula1340"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-1510418x99.png"  xlink:type="simple"/></disp-formula><p>and expand the curvature function as a series:</p><disp-formula id="scirp.60668-formula1341"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/4-1510418x100.png"  xlink:type="simple"/></disp-formula><p>For <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x101.png" xlink:type="simple"/></inline-formula> and small <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x102.png" xlink:type="simple"/></inline-formula> the curvature: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x103.png" xlink:type="simple"/></inline-formula>and varies directly as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x104.png" xlink:type="simple"/></inline-formula> which is small</p><p>and approximately constant (for a given curve) in this temperature range. This range is exactly where the measurements are assumed to be taken and the low curvature exhibited by the data sets in turn limit the range for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x105.png" xlink:type="simple"/></inline-formula> to small numbers. In fact a few numerical tests show that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x105.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x106.png" xlink:type="simple"/></inline-formula> for every curve in the experi- ment.</p><p>These curves tend also to be a good guide to the reliability of the data itself. When for a data series the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x107.png" xlink:type="simple"/></inline-formula> values are closely grouped the data set shows a higher continuity and greater physical plausibility. If an <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x107.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x108.png" xlink:type="simple"/></inline-formula></p><fig-group id="fig7"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> An example of the α parameter backward optimisation process: the nonlinear fit residual R<sup>2</sup> is maximised in every applied field case. (a) The α line grouping MgB<sub>2</sub> doped with Ag at 20%―note that the α grouping is close for every applied field case; (b) The α line grouping MgB<sub>2</sub> doped with Y at 0.5%―the anomaly in the set is the α value to the far right, not surprising as it is the line for zero applied field at this Y doping percentage.</title></caption><fig id ="fig7_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x110.png"/></fig><fig id ="fig7_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/4-1510418x109.png"/></fig></fig-group><p>value lies far outside the group then that data point would be an outlier and a value for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x111.png" xlink:type="simple"/></inline-formula> developed from it might better be discarded or viewed at least with a certain degree of suspicion. In fact this situation happens for almost all the data series for the zero DC field plots (see <xref ref-type="fig" rid="fig7">Figure 7</xref>(b)).</p><p>Mathematically, that confirms the intuition that the three parameter nonlinear fit is a perturbation of Equation (5) in the irreversible temperature region and the relatively small values of y and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/4-1510418x112.png" xlink:type="simple"/></inline-formula> probably mean that it is not too far from a convex optimisation problem. This hypothesis is supported by <xref ref-type="fig" rid="fig7">Figure 7</xref>. In fact as already stated, working with the data using this model it is possible to obtain good fits with consistent values for all the pa- rameters―if there are anomalies then they occur due to experimental issues as opposed to data analysis/extrac- tion.</p></sec><sec id="s7"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.60668-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Chandrashekar, R.G., Tiwari, R.S., Srivastava, O.N. and Malik, S.K. (2007) Enhancement of Flux Pinning and High Critical Current Density in Graphite Doped MgB2 Superconductor. Journal of Applied Physics, 101, Article ID: 043906.</mixed-citation></ref><ref id="scirp.60668-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Buzea, C. and Yamashita, T. (2001) Review of the Superconducting Properties of MgB2. 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