<?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">WJCMP</journal-id><journal-title-group><journal-title>World Journal of Condensed Matter Physics</journal-title></journal-title-group><issn pub-type="epub">2160-6919</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjcmp.2012.23024</article-id><article-id pub-id-type="publisher-id">WJCMP-22145</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Effect of Different Calcination Process and Gd&lt;sub&gt;2&lt;/sub&gt;O&lt;sub&gt;3&lt;/sub&gt; as Impurities on the Different Phases of Bi-Based Superconductor
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>hmad</surname><given-names>Amirabadizadeh</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sara</surname><given-names>Memarzadeh</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>Naser</surname><given-names>Tajabor</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>Hadi</surname><given-names>Arabi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Physics, Faculty of Science, University of Birjand, Birjand, Iran</addr-line></aff><aff id="aff2"><addr-line>Department of Physics, Faculty of Science, Fer-dowsi University of Mashhad, Mashhad, Iran</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>ahmadamirabadi@yahoo.com(HA)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>31</day><month>08</month><year>2012</year></pub-date><volume>02</volume><issue>03</issue><fpage>148</fpage><lpage>152</lpage><history><date date-type="received"><day>February</day>	<month>18th,</month>	<year>2012</year></date><date date-type="rev-recd"><day>March</day>	<month>25th,</month>	<year>2012</year>	</date><date date-type="accepted"><day>April</day>	<month>3rd,</month>	<year>2012</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>
 
 
  In this research two samples of a nominal composition Bi
  <sub>1.6</sub>Pb
  <sub>0.4</sub>Sr
  <sub>2</sub>Ca
  <sub>2</sub>Cu
  <sub>3</sub>O
  <sub>x</sub> were prepared by the solid state reaction method, using two different routes. Codes A and B are used to refer to the two samples. In preparing sample A, the standard method for calcination was used, while for sample B, the SrCO
  <sub>3</sub> and CaCO
  <sub>3</sub> were calcinated at 1100℃ for 3 h. Calcination was done separately on SrCO
  <sub>3</sub> and CaCO
  <sub>3</sub> in order to eliminate CO
  <sub>2</sub>. Then after mixing and grinding, the powder mixtures of Bi
  <sub>2</sub>O
  <sub>3</sub>, CuO, PbO, SrO and CaO were calcinated at 840℃ for 70 h. Also, the samples (samples C) of nominal compositions Bi
  <sub>1.6</sub>Pb
  <sub>0.4</sub>Sr
  <sub>2</sub>Ca
  <sub>2</sub>Cu
  <sub>3</sub>O
  <sub>x</sub>+ % x Gd
  <sub>2</sub>O
  <sub>3</sub> (% x = 0, 3, 5, 7 and 9) have been synthesized by this method. The XRD and SEM results show that addition of Gd
  <sub>2</sub>O
  <sub>3</sub> helps to increase the amount of Bi-2212 phase, while alternative calcination process improves the formation of the Bi-2223 phase. In addition, the AC susceptibility measurements confirm the XRD and SEM results.
 
</p></abstract><kwd-group><kwd>Bi-Pb-Sr-Ca-Cu-O System; X-Ray Diffraction; Scanning Electron Microscopy; AC Susceptibility</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The Bi-Pb-Sr-Ca-Cu-O system exhibits three different superconducting phases of (Bi-Pb)<sub>2</sub>Sr<sub>2</sub>CuO<sub>x</sub> (Bi-2201), (Bi-Pb)<sub>2</sub>Sr<sub>2</sub>CaCu<sub>2</sub>O<sub>x</sub> (Bi-2212) and (Bi-Pb)<sub>2</sub>Sr<sub>2</sub>Ca<sub>2</sub>Cu<sub>3</sub>O<sub>x</sub> (Bi-2223), which show critical temperatures (T<sub>c</sub>) of about 10, 80 and 110 K, respectively [1-3]. In the BSCCO system, the Bi-2212 phase is thermodynamically stable over a wide temperature range and among the three members of the BSCCO family the Bi-2212 and Bi-2223 phases have been the most extensively studied to date. In contrast to the Bi-2212 phase, the Bi-2223 phase is stable only in an extremely narrow temperature range and thus it is difficult to prepare single phase Bi-2223 ceramics [<xref ref-type="bibr" rid="scirp.22145-ref4">4</xref>]. Usually, in polycrystalline Bi-based superconducting preparations, these two phases tend to co-exist. The calcination process used in this research for Bi-based materials helps to increase the amount of the Bi-2223 phase relative to the amount of the Bi-2212 phase.</p><p>Effect of rare earth and some oxide as impurities or substitution of them for Bi and Sr in polycrystalline Bibased superconductor’s properties such as T<sub>c</sub> and J<sub>c</sub> have been investigated by several researchers [5-15]. Here we have studied the effect of Gd<sub>2</sub>O<sub>3</sub> as impurities on the general formula of Bi<sub>1.6</sub>Pb<sub>0.4</sub>Sr<sub>2</sub>Ca<sub>2</sub>Cu<sub>3</sub>O<sub>x</sub> + Gd<sub>2</sub>O<sub>3 </sub>composites and investigated the addition of these impurities on different phases of Bi-Based superconductor.</p></sec><sec id="s2"><title>2. Experimental</title><sec id="s2_1"><title>2.1. Different Calcination Process</title><p>In the usual solid state reaction method for producing Bi-based superconductors, calcination stage is used to eliminate the carbonates and to produce an oxide with a nominal composition (Bi-Pb)<sub>2</sub>Sr<sub>2</sub>Ca<sub>n-1</sub>Cu<sub>n</sub>O<sub>x</sub> [<xref ref-type="bibr" rid="scirp.22145-ref7">7</xref>]. Calcination of powder mixtures of Bi<sub>2</sub>O<sub>3</sub>, CuO, PbO, SrCO<sub>3</sub> and CaCO<sub>3</sub> is performed at temperatures less than or equal to 900˚C. The decomposition temperatures for CaCO<sub>3</sub> and SrCO<sub>3</sub> are 900˚C and 1290˚C, respectively [<xref ref-type="bibr" rid="scirp.22145-ref16">16</xref>]. Therefore, elimination of CO<sub>2</sub>, at 850˚C, from this mixture, can take a long time; but if the calcination temperature is increased, the mixture could melt.</p><p>In this research, two samples of nominal compositions Bi<sub>1.6</sub>Pb<sub>0.4</sub>Sr<sub>2</sub>Ca<sub>2</sub>Cu<sub>3</sub>O<sub>x</sub> were prepared by the standard solidstate reaction method and by using two different routes. Codes A and B are used to refer to the samples. In preparing sample A, the oxide powders (Bi<sub>2</sub>O<sub>3</sub>, PbO, SrCO<sub>3</sub>, CaCO<sub>3</sub> and CuO), taken in stoichiometric proportions, were ground and calcinated at 840˚C for 70 h. The powders were well mixed and ground in an agate mortar and pestle and pressed into pellets (15 mm in diameter and 2 mm in thickness) and sintered at 850˚C for 230 h with four intermediate grinding processes. The chosen rate of temperature increase and decrease was 2˚C-min<sup>−1</sup>. For sample B, the SrCO<sub>3</sub> and CaCO<sub>3</sub> were calcinated at 1100˚C for 3 h. The calcination was done in order to eliminate CO<sub>2</sub> separately for SrCO<sub>3</sub> and CaCO<sub>3.</sub> Then after mixing and grinding, the powder mixtures of Bi<sub>2</sub>O<sub>3</sub>, CuO, PbO, SrO and CaO were calcined at 840˚C for 70 h. The conditions for the second stage of calcination and sintering were similar to those for sample A.</p><p>The amount of residual of CO<sub>2</sub> can be measured by the LOI (loss on ignition) coefficient. Loss on ignition is a test used in inorganic analytical chemistry, particularly in the analysis of minerals. It consists of strongly heating (igniting) a sample of the material at a specified temperature, allowing volatile substances to escape until its mass ceases to change. The process may be repeated to show that mass-change is complete. LOI is defined as [<xref ref-type="bibr" rid="scirp.22145-ref17">17</xref>]:</p><p><img src="6-4800093\c0a07a8f-3944-42a1-9fb4-42da9460eae6.jpg" /></p><p>where W and <img src="6-4800093\10f18d38-f111-4bd2-9d30-3e11c7382a59.jpg" /> are the weight of the sample before heat treatment and the weight of the sample after heat treatment, respectively. Hence</p><p><img src="6-4800093\f3d883aa-3092-44e5-a665-c32ecf8e7e6c.jpg" /></p><p><img src="6-4800093\14571c03-8899-4bf6-ae51-a19af5d26050.jpg" /></p><p><img src="6-4800093\50f772b7-78c0-404a-a87f-9da4de68e242.jpg" /></p><p>and</p><p><img src="6-4800093\40f904ab-f4b0-41b6-86c8-956d0e2492a6.jpg" /></p><p><img src="6-4800093\728cd49f-7a09-499f-8b1a-deaa30f4087f.jpg" /></p><p>where x in the above equations is used to denote the mol number of the indicated materials and the coefficient LOI is constant for each desired amount of the composition. The samples A and B are compared to determine the effect of further calcination stage in B sample on the formation of the Bi-2223 phase.</p>• 2.2. Addition of Gd<sub>2</sub>O<sub>3</sub> as Impurities<p>• The Bi<sub>1.6</sub>Pb<sub>0.4</sub>Sr<sub>2</sub>Ca<sub>2</sub>Cu<sub>3</sub>O<sub>x</sub> + % x Gd<sub>2</sub>O<sub>3</sub> (% x = 0, 3, 5, 7 and 9) composites were papered by two steps. First, the (Bi-Pb)<sub>2</sub>Sr<sub>2</sub>Ca<sub>2</sub>Cu<sub>3</sub>O<sub>x</sub> was synthesized by conventional solid-state reaction method. High purity (99.5%), Bi<sub>2</sub>O<sub>3</sub>, PbO, SrCO<sub>3</sub>, CaCO<sub>3</sub> and CuO powders were mixed in the appropriate stoichiometric ratio and grinding in an agate mortar. The well-mixed powders were calcined at 840˚C for 70 h. Finally, after regrinding the (Bi-Pb)<sub>2</sub>Sr<sub>2</sub>Ca<sub>2</sub>Cu<sub>3</sub>O<sub>x</sub> and Gd<sub>2</sub>O<sub>3</sub> powders, the appropriate amounts of these powders were mixed and a homogenous powders were pressed in pellets and sintered at 850˚C for 230 h. Sample codes (C<sub>000</sub>, C<sub>003</sub>, C<sub>005</sub>, C<sub>007 </sub>and C<sub>009</sub>) are used to refer to the samples.</p><p>• The X-ray diffraction (XRD) studies were preformed with Cu-Kα radiation. The surface morphology of samples, which is an important surface property and very useful for understanding their defect structure, grain size, voids, etc., was studied by scanning electron microscopy (SEM). Finally, cylindrical specimens were cut from the sintered samples and used for AC susceptibility measurements. The real part of the AC susceptibility was measured with a Lake Shore Model 7000 AC susceptometer. The measurements were performed at a frequency of 333.3 Hz as a function of temperature at fixed AC magnetic field amplitude of 500 A/m. The AC field was applied parallel to the cylindrical axis.</p></sec></sec><sec id="s3"><title>3. Results and Discussions</title><sec id="s3_1"><title>3.1. Effect of Different Calcination Process</title><sec id="s3_1_1"><title>3.1.1. X-Ray Diffraction</title><p><xref ref-type="fig" rid="fig1">Figure 1</xref> shows the indexed X-ray diffraction patterns for samples A and B. The majority of the diffraction lines correspond mainly to Bi-2223 and Bi-2212 and the unit cells are orthorhombic for both samples. Due to the coexistence of Bi-2212 phase with Bi-2223 phase, a quantitative analysis is often required to estimate the amount of Bi-2212 and Bi-2223. XRD is the most widely used method for this kind of quantitative phase analysis. The volume fraction of Bi-2223 and Bi-2212 phases can be estimated using various methods. Some workers [18-20] have used (002) and (115) or (0010) and (008) peaks of Bi-2223 and Bi-2212 phases, respectively, and others [<xref ref-type="bibr" rid="scirp.22145-ref21">21</xref>] used all the peaks of the Bi-2223 and Bi-2212 phases for the estimation of the volume fraction. Here the (0010) and (008) peaks of Bi-2223 and Bi-2212 phases are used to estimate the volume fraction of the phases present. The fractional amount of the Bi-2223 phase relative to the Bi-2212 phase could be estimated from the intensities according to:</p><p><img src="6-4800093\c241dabc-c076-4bf1-9a28-b1815dd8750e.jpg" /></p><p><img src="6-4800093\54fc1db5-d0b7-4406-a1d7-427a2cbf89d6.jpg" /></p><p>where I is the intensity of peaks corresponding to the phases present. The volume fractions of the Bi-2223 and Bi-2212 in sample B are 40% and 31%; in sample A the</p><p>corresponding volume fractions are 21% and 39%, respectively. This shows that further calcination favors the formation of Bi-2223 phase.</p></sec><sec id="s3_1_2"><title>3.1.2. SEM Studies</title><p>The scanning electron micrographs of the samples after the final sintering step are shown in Figures 2(a) and (b). It is clear from these figures that the superconducting grains seem to be connected with each other while there are some unfilled spaces among them. The grain size and the distribution of grains on the surface of the samples are quite different. The surface of sample A is smoother and denser, while that of sample B has larger grains and more voids. Khalil [22,23] reported that the decrease of porosity might be related to an increase in (a) grain coupling strength and (b) degree of grain orientation of the BSCCO samples. On the other hand, Tampieri et al. [<xref ref-type="bibr" rid="scirp.22145-ref24">24</xref>] reported that the Bi-2212 phase has higher crystallographic density and stronger intergranular links than the Bi-2223 phase. Characteristic flaky grains of (Bi,Pb)-2212 and plate-like grains which are the typical grain structure of (Bi,Pb)-2223 are visible in both samples. Here the layered structure is only partially maintained with reduction in grain size and texture. In the XRD patterns of the samples, it is seen that sample B contains more Bi-2223 phase than sample A. Therefore, the highest density value would be expected for sample A. Here, the grains become more compressed and closely packed leaving a large number of inter-grain voids. These results agree with those obtained by XRD. The average grain size at different spots of the samples is between 1 and 9 &#181;m. The size of the largest particle in sample B is almost twice as large as in sample A.</p></sec><sec id="s3_1_3"><title>3.1.3. AC Susceptibility Studies</title><p>Positioning For the superconducting samples, the real part of the AC susceptibility <img src="6-4800093\770d89bf-b0bc-4ddc-8feb-a6e0cb835e55.jpg" /> was measured after the final sintering step. The real part of the AC susceptibility versus temperature for samples A and B is shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>. The superconducting transition temperature was determined from the onset of the diamagnetic signal. The diamagnetic transition in the real part of the AC susceptibility occurs sharply at T<sub>c</sub> (onset). The onset temperature of both samples lies between 108 and 110 &#177; 1 K. Curves A and B show that initially both phases of Bi-2223 and Bi-2212 are present in the samples. The sharper transition observed in sample B suggests that this sample present a higher superconducting fraction of 2223 than sample A. But the actual estimate of superconducting volume fraction is not possible by this experiment [5,11].</p></sec></sec><sec id="s3_2"><title>3.2. Effect of Gd<sub>2</sub>O<sub>3</sub> as Impurities</title><sec id="s3_2_1"><title>3.2.1. X-Ray Diffraction</title><p><xref ref-type="fig" rid="fig4">Figure 4</xref> shows the X-ray diffraction patterns for C<sub>000,</sub> C<sub>003, </sub>C<sub>005, </sub>C<sub>007 </sub>and C<sub>009 </sub>samples. The Bi-2223 and Bi-2212 phases co-exist in the composites. 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