<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>0864-084X</journal-id>
<journal-title><![CDATA[Nucleus]]></journal-title>
<abbrev-journal-title><![CDATA[Nucleus]]></abbrev-journal-title>
<issn>0864-084X</issn>
<publisher>
<publisher-name><![CDATA[CUBAENERGIA]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0864-084X2007000100007</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Calculation of displacements per atom distributions in solid materials]]></article-title>
<article-title xml:lang="es"><![CDATA[Cálculo de distribuciones de desplazamientos atómicos en materiales sólidos]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Piñera Hernández]]></surname>
<given-names><![CDATA[Ibrahin]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Cruz Inclán]]></surname>
<given-names><![CDATA[Carlos M.]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Leyva Fabelo]]></surname>
<given-names><![CDATA[Antonio]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Abreu Alfonso]]></surname>
<given-names><![CDATA[Yamiel]]></given-names>
</name>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Centro de Aplicaciones Tecnológicas y Desarrollo Nuclear (CEADEN)  ]]></institution>
<addr-line><![CDATA[Ciudad de La Habana ]]></addr-line>
<country>Cuba</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>06</month>
<year>2007</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>06</month>
<year>2007</year>
</pub-date>
<numero>41</numero>
<fpage>39</fpage>
<lpage>44</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://scielo.sld.cu/scielo.php?script=sci_arttext&amp;pid=S0864-084X2007000100007&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.sld.cu/scielo.php?script=sci_abstract&amp;pid=S0864-084X2007000100007&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.sld.cu/scielo.php?script=sci_pdf&amp;pid=S0864-084X2007000100007&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[Se presentan los resultados de los cálculos de la distribución de desplazamientos atómicos en el superconductor <img src="http:/img/revistas/nuc/nuc41/images/e01074107.jpg" width="66" height="14"> y en láminas de hierro inducida por radiación gamma hasta 15 MeV. Se introdujo un procedimiento de cálculo para las secciones eficaces de desplazamiento y para las distribuciones de desplazamientos atómicos, basado en el uso de los valores de la distribución del flujo energético de los electrones secundarios, obtenidos con ayuda del código de cálculo MCNPX basado en el método de Monte Carlo. Se compararon los resultados de los cálculos de la distribución de desplazamientos atómicos con los perfiles de energía depositada, obteniéndose una correlación casi lineal entre ambos a diferentes profundidades en las muestras para un amplio intervalo de energías de la radiación gamma incidente.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[The results of the calculations of the displacements per atom distribution induced by the gamma irradiation on <img src="http:/img/revistas/nuc/nuc41/images/e01074107.jpg" width="66" height="14"> superconductor and Iron slabs up to 15 MeV are presented. Firstly, a calculation procedure for the displacements cross sections and the displacements per atom distributions was introduced, relaying on the application of the energy flux distribution values of secondary electrons, formerly calculated using the Monte Carlo methods based code system MCNPX. Finally, calculation results of displacements per atom distribution were compared with the corresponding energy deposition profiles, obtaining a nearly linear correlation among them at different depth positions for a wide range of Gamma Radiation incident energy.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Monte Carlo method]]></kwd>
<kwd lng="en"><![CDATA[atomic displacements]]></kwd>
<kwd lng="en"><![CDATA[gamma radiation]]></kwd>
<kwd lng="en"><![CDATA[simulation]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="left"><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>CIENCIAS    NUCLEARES</b></font></p>     <p align="right">&nbsp;</p>     <p><strong><font size="4" face="Verdana, Arial, Helvetica, sans-serif">Calculation    of displacements per atom distributions in solid materials</font></strong></p>     <p></p>     <p>&nbsp;</p>     <p><font size="3" face="Verdana, Arial, Helvetica, sans-serif">C&aacute;lculo    de distribuciones de desplazamientos at&oacute;micos en materiales s&oacute;lidos    </font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Ibrahin Pi&ntilde;era    Hern&aacute;ndez, Carlos M. Cruz Incl&aacute;n, Antonio Leyva Fabelo, Yamiel    Abreu Alfonso</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Centro de Aplicaciones    Tecnol&oacute;gicas y Desarrollo Nuclear (CEADEN)    <br>   Calle 30 No 502 e/ 5ta Ave. y 7ma. Playa, Ciudad de La Habana, Cuba    <br>   ipinera@ceaden.edu.cu</font></p> <hr>     ]]></body>
<body><![CDATA[<p><font size="2" face="Verdana, Arial, Helvetica, sans-serif"><b>RESUMEN</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Se presentan los    resultados de los c&aacute;lculos de la distribuci&oacute;n de desplazamientos    at&oacute;micos en el superconductor <img src="/img/revistas/nuc/n41/e01074107.jpg" width="32" height="32">.    y en l&aacute;minas de hierro inducida por radiaci&oacute;n gamma hasta 15 MeV.    Se introdujo un procedimiento de c&aacute;lculo para las secciones eficaces    de desplazamiento y para las distribuciones de desplazamientos at&oacute;micos,    basado en el uso de los valores de la distribuci&oacute;n del flujo energ&eacute;tico    de los electrones secundarios, obtenidos con ayuda del c&oacute;digo de c&aacute;lculo    MCNPX basado en el m&eacute;todo de Monte Carlo. Se compararon los resultados    de los c&aacute;lculos de la distribuci&oacute;n de desplazamientos at&oacute;micos    con los perfiles de energ&iacute;a depositada, obteni&eacute;ndose una correlaci&oacute;n    casi lineal entre ambos a diferentes profundidades en las muestras para un amplio    intervalo de energ&iacute;as de la radiaci&oacute;n gamma incidente.</font></p> <hr>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>ABSTRACT</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The results of    the calculations of the displacements per atom distribution induced by the gamma    irradiation on <img src="/img/revistas/nuc/n41/e01074107.jpg" width="32" height="32">    superconductor and Iron slabs up to 15 MeV are presented. Firstly, a calculation    procedure for the displacements cross sections and the displacements per atom    distributions was introduced, relaying on the application of the energy flux    distribution values of secondary electrons, formerly calculated using the Monte    Carlo methods based code system MCNPX. Finally, calculation results of displacements    per atom distribution were compared with the corresponding energy deposition    profiles, obtaining a nearly linear correlation among them at different depth    positions for a wide range of Gamma Radiation incident energy.</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Key words: Monte    Carlo method, atomic displacements, gamma radiation, simulation, superconductors,    iron, cross sections</font></p> <hr>     <p><font size="2" face="Verdana, Arial, Helvetica, sans-serif"><strong>INTRODUCTION</strong></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Nowadays, the damage    induced by the different types of radiations in advanced materials is broadly    studied. Mainly, those materials that get involved in experiments and development    of new technologies, like they are the high temperature superconducting materials    (HTSC), semiconductors, metals, on the base of which are essentially constituted    the radiation detectors, particle accelerators, nuclear reactors, etc. In this    sense, present investigation tries a study of two kinds of materials used with    these ends, the ceramic superconducting material <img src="/img/revistas/nuc/n41/e01074107.jpg" width="32" height="32">    and the metallic iron ones, through the mathematical simulation of the physical    processes that take place in these solid materials when being irradiated, in    a wide energy range that goes from some keV to 15 MeV. For it, the program MCNPX    [1] is used, with the help of which the physical necessary magnitudes are determined    to calculate the distribution of the Atom Displacements (AD) inside these materials,    by means of the implemented algorithm.    
<br>   Previous works involving AD determination on HTSC materials reported in [2-5]    for electron fluxes and in [6,7] for the Gamma Radiation, led to first attempts    for the overall estimation of its magnitude as a measurement of the potential    microscopic structural modifications induced by the Gamma Radiation Damage on    these materials.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">However, in spite    of the foregoing statement, the AD calculation approach presented by Belevtsev    et al. [7]; has a restricted character and meaning, since it follows the classical    AD calculation procedure introduced by Oen-Holmes [8] (see also [9]), which    does not take into account the shower and cross linked nature of gamma quanta    and secondary electron interactions arising at Gamma Radiation transport in    solids. This Gamma Radiation complex stochastic behavior can be nowadays, theoretically,    very well simulated and described by means of calculation codes based on the    Monte Carlo method, as for instance the MCNPX, EGSnrc [10];, GEANT4 [11], modeling    the transport of different types of radiations in the substance. An attempt    introducing a direct Monte Carlo methods based simulation of AD distribution    induced by the Gamma Radiation on Iron slabs has being reported by Sato et al.    [12].</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Then, it seems    to be justified the application of the standards outputs (tallies) of the available    Monte Carlo methods based simulation codes, cited before, as an alternative    way providing a posteriori realistic approach to the subject of Gamma Radiation    Damage calculations. Following this last idea, the present work tries a first    attempt to calculate AD rate distributions in solid materials involving Gamma    Radiation transport properties, an approach to Gamma Radiation Damage determination,    closer than previous reported works [7,13,14].</font></p>     ]]></body>
<body><![CDATA[<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Thus, a calculation    procedure was introduced, starting from the calculation code outputs of the    energy flux distribution values of secondary electrons, which are then processed    by the application of standard expressions describing the electron Primary Knock-on    interactions leading to AD events. This procedure was thus finally applied for    the calculation of AD distribution at different incident Gamma Radiation energies,    regarding the plane crystalline sites on the YBCO superconducting material and    the metallic iron ones.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Atom Displacements    Cross Sections</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The incident Gamma    Radiation produces secondary electrons in the material. These electrons can    remove an atom from the lattice through elastic scattering processes. The removed    atom is the so called Primary Knock-on Atom (PKA) and the corresponding cross    section, , was obtained starting from the McKinley-Feshbach approximation [15]    (see Eq.(2)). If any of these recoil atoms has a kinetic energy above the displacement    threshold energy Td, secondary atoms can be knocked-on by PKA and removed from    the lattice too. The number of secondary displaced atoms can be calculated introducing    the damage function . Then, the total number of displaced atoms per target atom    can be obtained writing the displacement per atom cross section as follow</font></p>     <p><img src="/img/revistas/nuc/n41/e02074107.jpg" width="753" height="613"></p>     
<p></p>     <p> </p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The number of atoms    displaced per electron was calculated following the expression proposed by     <br>   Oen-Holmes [8].</font></p>     <p>&nbsp;</p>     <p><img src="/img/revistas/nuc/n41/e03074107.jpg" width="732" height="337"></p>     
]]></body>
<body><![CDATA[<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">is the cutoff kinetic    energy of electrons in order to displace an atom from its crystalline site,    <img src="/img/revistas/nuc/n41/e06074107.jpg" width="22" height="21">    is the    
<br>   number of atoms in the unit of volume in the sample and (-dE dx) is the electron    stopping power,    <br>   calculated following the expression given by Bethe-Ashkin [16].</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><img src="/img/revistas/nuc/n41/e07074107.jpg" width="553" height="100">    
<br>   where <img src="/img/revistas/nuc/n41/e08074107.jpg" width="22" height="21">m    is the mean square atomic number of the sample material and is the mean excitation    potential    
<br>   of the atom. The classical macroscopic number of displaced atoms per electron,    <img src="/img/revistas/nuc/n41/e09074107.jpg" width="25" height="15">(E),    involves the    
<br>   calculation of AD events in a &uml;thick layer&uml; of thickness about the range    of electrons in the material. </font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The dependencies    of <img src="/img/revistas/nuc/n41/e04074107.jpg" width="34" height="14">    and <img src="/img/revistas/nuc/n41/e09074107.jpg" width="25" height="15">    on the electron kinetic energy are shown in figure 1, for the two studied materials.    As can be observed in this figure, cross sections vanishes down certain value    of electron kinetic energy, that in the case of oxygen atoms in YBCO, with <img src="/img/revistas/nuc/n41/e12074107.jpg" width="15" height="17">=    20 eV, takes a value above 130 keV. This means that electrons with energy lesser    to this value can not produce AD in the <img src="/img/revistas/nuc/n41/e11074107.jpg" width="36" height="13">    planar sites. For the copper atoms in YBCO that energy is about 745 keV and    for the iron atoms is near 626 keV.</font></p>     
<p><img src="/img/revistas/nuc/n41/f01074107.jpg" width="767" height="398"></p>     
]]></body>
<body><![CDATA[<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Simulation with    MCNPX code</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The sample geometries    and the irradiation conditions for calculations were similar as those used in    a previously reported work by Pi&ntilde;era [17,18], as follows: the ceramic    YBCO parallelepiped target was shaped with dimensions 2.8 mm x 16.0 mm x 1.5    mm (subdivided in voxells with 0.4 mm x 0.4 mm x 0.1 mm), on which impact 2    x <img src="/img/revistas/nuc/n41/e18074107.jpg" width="18" height="12">    photons at different selected incident energies (in the wide range from 662    keV to 15.0 MeV). The simulations were carried out under the same number of    independent histories for calculation purposes. In all the cases, the results    shown are normalized to the total number of histories (incident photons and    its secondary particles).</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Determination    of AD distribution</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Starting from the    integral expressions used to calculate AD rate for a continuous secondary electron    energy distribution, we propose the following expression to calculate the number    of displacement per atom (dpa) in the voxel volume,<img src="/img/revistas/nuc/n41/e13074107.jpg" width="29" height="16">    , as a sum extended over the calculated discrete electron flux values at a given    depth Z, generalized for any k-atom in the material</font></p>     
<p><img src="/img/revistas/nuc/n41/e14074107.jpg" width="264" height="62"></p>     
<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">where <img src="/img/revistas/nuc/n41/e19074107.jpg" width="17" height="17">is    the relative compositional weight of the k-atom in the material and <img src="/img/revistas/nuc/n41/e09074107.jpg" width="25" height="15">    arises from the evaluation of Eq.(5) for each one of these atoms.</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The previous expression    was applied to the studied materials. In the case of Fe, was applied to iron    atoms with <img src="/img/revistas/nuc/n41/e12074107.jpg" width="15" height="17">=    25 eV (= 1). In the case of YBCO, was applied to oxygen atoms with = <img src="/img/revistas/nuc/n41/e12074107.jpg" width="15" height="17">20    eV (nk= 4/7) and to copper atoms with <img src="/img/revistas/nuc/n41/e12074107.jpg" width="15" height="17">=    25 eV (nk= 2/3), both belonging to the <img src="/img/revistas/nuc/n41/e11074107.jpg" width="36" height="13">    planar cites.</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The calculation    results of total dpa values for both materials are shown in figure 2 for different    values of incident gamma energy <img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">Eg.    As can be observed, the number of dpa increases with the energy of incident    radiation. Note also that the difference between dpa values for each <img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">    increases more and more with depth, being strong this augment in the sample    thickness. This abrupt increase of dpa can be related with the production of    displacements in cascade, that takes place when increasing the electrons energy,    since atoms with more energy are taken out from its sites and these atoms in    turn, produce higher number of secondary atoms and consequently the cascade    of displaced atoms is bigger.</font></p>     
]]></body>
<body><![CDATA[<p><img src="/img/revistas/nuc/n41/f02074107.jpg" width="765" height="357"></p>     
<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">For energies <img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16"><img src="/img/revistas/nuc/n41/e20074107.jpg" width="10" height="11">1.25    MeV, the dpa distribution reaches its maximum inside the material (unimodal    distribution), as it has been observed in previous works [14,17,19]. Besides,    these dpa distribution shapes are similar to the observed in the obtained energy    deposition profiles at the same energies [18].</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The maximum dpa    values for each <img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">    are shown in table 1, for both materials, taken into account the contribution    of each atomic species.</font></p>     
<p><img src="/img/revistas/nuc/n41/t01074107.jpg" width="421" height="176"></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">From table 1 it    seem that in the case of YBCO the oxygen atoms have a bigger weight in the total    dpa values at low energies and, in contrast, the copper atoms at high energies.    This result is consistent with the evidences observed previously [2-4]. Note    also that the Fe material is more resistant to radiation damage at low energies    (<img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">&lt;    5.0 MeV) and YBCO at high irradiation energies.</font></p>     
<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>Comparison between    AD and energy deposition</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Starting from the    similarity between the dpa distributions and energy deposition profiles, a comparison    among them was performed, as it is showed below in figure 3. Due to the good    correspondence that was observed in this figure involving both magnitudes, a    linear fitting of this relationships was carried out for all incident energy.    The results of this fitting are given away in table 2, showing the slope parameter,    <img src="/img/revistas/nuc/n41/e17074107.jpg" width="8" height="12">(<img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">),    that represent the direct relation between dpa and energy deposition. The linear    regression coefficient R is shown too.</font></p>     
<p><img src="/img/revistas/nuc/n41/f03074107.jpg" width="754" height="443"></p>     
<p><img src="/img/revistas/nuc/n41/t02074107.jpg" width="429" height="191"></p>     
]]></body>
<body><![CDATA[<p></p>     <p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">It can be clearly    observed from figure 3 that AD depend linearly on the radiation energy deposition    in the material, and that this dependence is stronger when increasing <img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">.    This can be better distinguish in table 2, which shows how the values of <img src="/img/revistas/nuc/n41/e17074107.jpg" width="8" height="12"></font><font face="Verdana, Arial, Helvetica, sans-serif" size="2">(<img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">)    increase abruptly when increasing <img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">,    from approximately 30 dpa/eV for <img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">    = 0.662 MeV up to about 2 x 104 dpa/eV for <img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">    = 15.0 MeV. It can be also verify that the linear fitting is better (&gt; R)    at bigger <img src="/img/revistas/nuc/n41/e15074107.jpg" width="14" height="16">.</font></p>     
<p></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">These particular    behaviors can be expected, since secondary electrons plays an important and    decisive role on the general energy deposition mechanism and particularly on    the displacement of atoms from their crystalline sites arising at the gamma    quanta transport, which is extended over the whole target volume.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">These findings    seem to confirm partially the results reported by A. Leyva et al. [14], in which    the calculated energy depositions were taken as a measurement of the Gamma Radiation    Damage effects on the YBCO superconducting material.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>CONCLUSIONS</b></font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">The calculation    of AD rates induced by the Gamma Radiation to different energies in the YBCO    superconductor was carried out on the basis of a procedure relying on the use    of the standards tallies of the Monte Carlo method based simulation code MCNPX,    which are then applied to perform calculations through standard expressions    describing the electron Primary Knock-on interactions leading to Atom Displacements    events. This provides a realistic approach to the subject of Gamma Radiation    Damage calculations, where the imported secondary electrons energy profiles    emphasize the shower and cross linked nature of gamma quanta and secondary electron    interactions arising at Gamma Radiation transport in solids.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">A nearly position    independent linear correlations among AD rate and energy deposition were found,    which allows the application of an energy deposition scale for Gamma Radiation    Damage determination.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>ACKNOWLEDGEMENT</b></font></p>     ]]></body>
<body><![CDATA[<p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">This study was    supported by the Nuclear Energy and Advanced Technologies Agency of the Ministry    of Science, Technology and Environment of Cuba through the project PRN/7-2/9.</font></p>     <p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"><b>REFERENCES</b></font></p>     <!-- ref --><p><font face="Verdana, Arial, Helvetica, sans-serif" size="2">1. HENDRICKS JS,    MCKINNEY GW, TRELLUE HR, DURKEE JW, FINCH JP, FENSIN ML, JAMES MR, PELOWITZ    DB, WATERS LS, GALLMEIER FX, DAVID JC. MCNPXTM Version 2.6.B. Los Alamos National    Laboratory. June 2006. Report, LA-UR-06-3248.    <!-- ref --><br>   2. LEGRIS A, RULLIER-ALBENQUE F, RADEVA E, LEJAY P. J Phys I France. 1993;(    3): 1605.    <!-- ref --><br>   3. GIAPINTZAKIS J, GINSBERG DM, KIRK MA, OCKERS S. Phys Rev B 1994; 50 ( 21):    15967.    <!-- ref --><br>   4. JACKSON EM, WEAVER BD, SUMMERS GP, SHAPIRO P, BURKE EA. Phys Rev Lett 1995;    74 ( 15): 3033.    <!-- ref --><br>   5. BOURDILLON AJ, TAN NX. Supercond. Sci Tech. 1995;( 8): 507.    <!-- ref --><br>   6. YOSHIDA Y, KUBOZONO Y, URAKAWA T, MAEDA H, KASHINO S, MURAKAMI Y, OHTA T,    IZUMI F, YAMADA K, FURUKAWA Y. Solid State Commun. 1998; 105 ( 9): 557.    <!-- ref --><br>   7. BELEVTSEV BI, VOLCHOK IV, DALAKOVA ND, DOTSENKO VI, IVANCHENKO LG, KUZNICHENKO    AV. LAGVINOV II. Phys Stat Sol. (a) 2000;( 181): 437.    <!-- ref --><br>   8. OEN OS. HOLMES DK. J Appl Phys. 1959; 30 ( 8): 289.    <!-- ref --><br>   9. FUKUYA K. KIMURA I. J Nucl Sci Tech. 2003; 40 ( 6): 423-4.    <!-- ref --><br>   10. KAWRAKOW I, ROGERS DWO. The EGSnrc Code System: Monte Carlo Simulation of    Electron and Photon Transport. NRCC Report PIRS-701. Dec. Stanford Univ. California    (2003).    <!-- ref --><br>   11. AGOSTINELLI S, ALLISON J, AMAKO K. Nucl Instrum Meth A. 2003;( 506): 250.    <!-- ref --><br>   12. SATO O, TOBITA T, SUZUKI M. Proceedings of the Second International Workshop    on EGS. KEK Proceedings 2000; 193: 200-20.    <!-- ref --><br>   13. LEYVA A, ALFONSO O, CRUZ C. Rev Mex Fis. 2001; 47 ( 4): 76.    <!-- ref --><br>   14. LEYVA A, ALFONSO O, CRUZ C. Nucl Inst Meth B. 2002;( 174): 222-3.    <!-- ref --><br>   15. MCKINLEY WA, FESHBACH H. Phys Rev 1948;( 74): 1759.    <!-- ref --><br>   16. BETHE HA, ASHKIN J. Experimental Nuclear Physics. New York: John Wiley &amp;    Sons, Inc., 1953. vol. 1.    <!-- ref --><br>   17. PI&Ntilde;ERA I. Detailed energy balance and Atomic Displacements processes    induced by Gamma Radiation in YBCO ( Grade Thesis in Nucl. Phys.). Havana City,    Cuba. 2004 (in spanish).    <!-- ref --><br>   18. PI&Ntilde;ERA I. Study of Radiation Damage in solid materials by means of    the simulation of physical processes ( Master Thesis in Nucl. Phys.). Havana    City, Cuba. 2006 (in spanish).    <!-- ref --><br>   [19] PI&Ntilde;ERA I, CRUZ C, LEYVA A, ABREU Y. Phys Stat Sol (a). 2006. (accepted).</font><p><font face="Verdana, Arial, Helvetica, sans-serif" size="2"> </font><font face="Verdana, Arial, Helvetica, sans-serif" size="2">Centro    de Aplicaciones Tecnol&oacute;gicas y Desarrollo Nuclear (CEADEN)    <br>   Calle 30 No 502 e/ 5ta Ave. y 7ma. Playa, Ciudad de La Habana, Cuba     <br>   <a href="mailto:ipinera@ceaden.edu.cu">ipinera@ceaden.edu.cu</a></font></p>     <p> <font face="Verdana, Arial, Helvetica, sans-serif" size="2">   </font> </p>      ]]></body><back>
<ref-list>
<ref id="B1">
<label>1</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[HENDRICKS]]></surname>
<given-names><![CDATA[JS]]></given-names>
</name>
<name>
<surname><![CDATA[MCKINNEY]]></surname>
<given-names><![CDATA[GW]]></given-names>
</name>
<name>
<surname><![CDATA[TRELLUE]]></surname>
<given-names><![CDATA[HR]]></given-names>
</name>
<name>
<surname><![CDATA[DURKEE]]></surname>
<given-names><![CDATA[JW]]></given-names>
</name>
<name>
<surname><![CDATA[FINCH]]></surname>
<given-names><![CDATA[JP]]></given-names>
</name>
<name>
<surname><![CDATA[FENSIN]]></surname>
<given-names><![CDATA[ML]]></given-names>
</name>
<name>
<surname><![CDATA[JAMES]]></surname>
<given-names><![CDATA[MR]]></given-names>
</name>
<name>
<surname><![CDATA[PELOWITZ]]></surname>
<given-names><![CDATA[DB]]></given-names>
</name>
<name>
<surname><![CDATA[WATERS]]></surname>
<given-names><![CDATA[LS]]></given-names>
</name>
<name>
<surname><![CDATA[GALLMEIER]]></surname>
<given-names><![CDATA[FX]]></given-names>
</name>
<name>
<surname><![CDATA[DAVID]]></surname>
<given-names><![CDATA[JC]]></given-names>
</name>
</person-group>
<source><![CDATA[]]></source>
<year></year>
</nlm-citation>
</ref>
<ref id="B2">
<label>2</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[LEGRIS]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[RULLIER-ALBENQUE]]></surname>
<given-names><![CDATA[F]]></given-names>
</name>
<name>
<surname><![CDATA[RADEVA]]></surname>
<given-names><![CDATA[E]]></given-names>
</name>
<name>
<surname><![CDATA[LEJAY]]></surname>
<given-names><![CDATA[P]]></given-names>
</name>
</person-group>
<source><![CDATA[J Phys I France.]]></source>
<year>1993</year>
<numero>3</numero>
<issue>3</issue>
<page-range>1605</page-range></nlm-citation>
</ref>
<ref id="B3">
<label>3</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[GIAPINTZAKIS]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
<name>
<surname><![CDATA[GINSBERG]]></surname>
<given-names><![CDATA[DM]]></given-names>
</name>
<name>
<surname><![CDATA[KIRK]]></surname>
<given-names><![CDATA[MA]]></given-names>
</name>
<name>
<surname><![CDATA[OCKERS]]></surname>
<given-names><![CDATA[S]]></given-names>
</name>
</person-group>
<source><![CDATA[Phys Rev B]]></source>
<year>1994</year>
<volume>50</volume>
<numero>21</numero>
<issue>21</issue>
<page-range>15967</page-range></nlm-citation>
</ref>
<ref id="B4">
<label>4</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[JACKSON]]></surname>
<given-names><![CDATA[EM]]></given-names>
</name>
<name>
<surname><![CDATA[WEAVER]]></surname>
<given-names><![CDATA[BD]]></given-names>
</name>
<name>
<surname><![CDATA[SUMMERS]]></surname>
<given-names><![CDATA[GP]]></given-names>
</name>
<name>
<surname><![CDATA[SHAPIRO]]></surname>
<given-names><![CDATA[P]]></given-names>
</name>
<name>
<surname><![CDATA[BURKE]]></surname>
<given-names><![CDATA[EA]]></given-names>
</name>
</person-group>
<source><![CDATA[  Phys Rev Lett]]></source>
<year>1995</year>
<volume>74</volume>
<numero>15</numero>
<issue>15</issue>
<page-range>3033</page-range></nlm-citation>
</ref>
<ref id="B5">
<label>5</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[BOURDILLON]]></surname>
<given-names><![CDATA[AJ]]></given-names>
</name>
<name>
<surname><![CDATA[TAN]]></surname>
<given-names><![CDATA[NX]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Supercond]]></article-title>
<source><![CDATA[Sci Tech.]]></source>
<year>1995</year>
<numero>8</numero>
<issue>8</issue>
<page-range>507</page-range></nlm-citation>
</ref>
<ref id="B6">
<label>6</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[YOSHIDA]]></surname>
<given-names><![CDATA[Y]]></given-names>
</name>
<name>
<surname><![CDATA[KUBOZONO]]></surname>
<given-names><![CDATA[Y]]></given-names>
</name>
<name>
<surname><![CDATA[URAKAWA]]></surname>
<given-names><![CDATA[T]]></given-names>
</name>
<name>
<surname><![CDATA[MAEDA]]></surname>
<given-names><![CDATA[H]]></given-names>
</name>
<name>
<surname><![CDATA[KASHINO]]></surname>
<given-names><![CDATA[S]]></given-names>
</name>
<name>
<surname><![CDATA[MURAKAMI]]></surname>
<given-names><![CDATA[Y]]></given-names>
</name>
<name>
<surname><![CDATA[OHTA]]></surname>
<given-names><![CDATA[T]]></given-names>
</name>
<name>
<surname><![CDATA[IZUMI]]></surname>
<given-names><![CDATA[F]]></given-names>
</name>
<name>
<surname><![CDATA[YAMADA]]></surname>
<given-names><![CDATA[K]]></given-names>
</name>
<name>
<surname><![CDATA[FURUKAWA]]></surname>
<given-names><![CDATA[Y]]></given-names>
</name>
</person-group>
<source><![CDATA[Solid State Commun.]]></source>
<year>1998</year>
<volume>105</volume>
<numero>9</numero>
<issue>9</issue>
<page-range>557</page-range></nlm-citation>
</ref>
<ref id="B7">
<label>7</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[BELEVTSEV]]></surname>
<given-names><![CDATA[BI]]></given-names>
</name>
<name>
<surname><![CDATA[VOLCHOK]]></surname>
<given-names><![CDATA[IV]]></given-names>
</name>
<name>
<surname><![CDATA[DALAKOVA]]></surname>
<given-names><![CDATA[ND]]></given-names>
</name>
<name>
<surname><![CDATA[DOTSENKO]]></surname>
<given-names><![CDATA[VI]]></given-names>
</name>
<name>
<surname><![CDATA[IVANCHENKO]]></surname>
<given-names><![CDATA[LG]]></given-names>
</name>
<name>
<surname><![CDATA[KUZNICHENKO]]></surname>
<given-names><![CDATA[AV]]></given-names>
</name>
<name>
<surname><![CDATA[LAGVINOV]]></surname>
<given-names><![CDATA[II]]></given-names>
</name>
</person-group>
<source><![CDATA[(a)]]></source>
<year>2000</year>
<numero>181</numero>
<issue>181</issue>
<page-range>437</page-range></nlm-citation>
</ref>
<ref id="B8">
<label>8</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[OEN]]></surname>
<given-names><![CDATA[OS]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[HOLMES DK]]></article-title>
<source><![CDATA[J Appl Phys.]]></source>
<year>1959</year>
<volume>30</volume>
<numero>8</numero>
<issue>8</issue>
<page-range>289</page-range></nlm-citation>
</ref>
<ref id="B9">
<label>9</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[FUKUYA]]></surname>
<given-names><![CDATA[K]]></given-names>
</name>
<name>
<surname><![CDATA[KIMURA]]></surname>
<given-names><![CDATA[I]]></given-names>
</name>
</person-group>
<source><![CDATA[J Nucl Sci Tech.]]></source>
<year>2003</year>
<volume>40</volume>
<numero>6</numero>
<issue>6</issue>
<page-range>423-4</page-range></nlm-citation>
</ref>
<ref id="B10">
<label>10</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[KAWRAKOW]]></surname>
<given-names><![CDATA[I]]></given-names>
</name>
<name>
<surname><![CDATA[ROGERS]]></surname>
<given-names><![CDATA[DWO]]></given-names>
</name>
</person-group>
<source><![CDATA[The EGSnrc Code System: Monte Carlo Simulation of Electron and Photon Transport]]></source>
<year>2003</year>
<publisher-name><![CDATA[NRCC]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B11">
<label>11</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[AGOSTINELLI]]></surname>
<given-names><![CDATA[S]]></given-names>
</name>
<name>
<surname><![CDATA[ALLISON]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
<name>
<surname><![CDATA[AMAKO]]></surname>
<given-names><![CDATA[K]]></given-names>
</name>
</person-group>
<source><![CDATA[Nucl Instrum Meth A.]]></source>
<year>2003</year>
<numero>506</numero>
<issue>506</issue>
<page-range>250</page-range></nlm-citation>
</ref>
<ref id="B12">
<label>12</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[SATO]]></surname>
<given-names><![CDATA[O]]></given-names>
</name>
<name>
<surname><![CDATA[TOBITA]]></surname>
<given-names><![CDATA[T]]></given-names>
</name>
<name>
<surname><![CDATA[SUZUKI]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Proceedings of the Second International Workshop on EGS]]></article-title>
<source><![CDATA[KEK Proceedings]]></source>
<year>2000</year>
<volume>193</volume>
<page-range>200-20</page-range></nlm-citation>
</ref>
<ref id="B13">
<label>13</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[LEYVA]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[ALFONSO]]></surname>
<given-names><![CDATA[O]]></given-names>
</name>
<name>
<surname><![CDATA[CRUZ]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
</person-group>
<source><![CDATA[Rev Mex Fis.]]></source>
<year>2001</year>
<volume>47</volume>
<numero>4</numero>
<issue>4</issue>
<page-range>76</page-range></nlm-citation>
</ref>
<ref id="B14">
<label>14</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[LEYVA]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[ALFONSO]]></surname>
<given-names><![CDATA[O]]></given-names>
</name>
<name>
<surname><![CDATA[CRUZ]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
</person-group>
<source><![CDATA[Nucl Inst Meth B.]]></source>
<year>2002</year>
<numero>174</numero>
<issue>174</issue>
<page-range>222-3</page-range></nlm-citation>
</ref>
<ref id="B15">
<label>15</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[MCKINLEY]]></surname>
<given-names><![CDATA[WA]]></given-names>
</name>
<name>
<surname><![CDATA[FESHBACH]]></surname>
<given-names><![CDATA[H]]></given-names>
</name>
</person-group>
<source><![CDATA[Phys Rev]]></source>
<year>1948</year>
<numero>74</numero>
<issue>74</issue>
<page-range>1759</page-range></nlm-citation>
</ref>
<ref id="B16">
<label>16</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[BETHE]]></surname>
<given-names><![CDATA[HA]]></given-names>
</name>
<name>
<surname><![CDATA[ASHKIN]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
</person-group>
<source><![CDATA[Experimental Nuclear Physics]]></source>
<year>1953</year>
<publisher-loc><![CDATA[New York ]]></publisher-loc>
<publisher-name><![CDATA[John Wiley & Sons, Inc]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B17">
<label>17</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[PIÑERA]]></surname>
<given-names><![CDATA[I]]></given-names>
</name>
</person-group>
<source><![CDATA[Detailed energy balance and Atomic Displacements processes induced by Gamma Radiation in YBCO]]></source>
<year></year>
</nlm-citation>
</ref>
<ref id="B18">
<label>18</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[PIÑERA]]></surname>
<given-names><![CDATA[I]]></given-names>
</name>
</person-group>
<source><![CDATA[Study of Radiation Damage in solid materials by means of the simulation of physical processes]]></source>
<year></year>
</nlm-citation>
</ref>
<ref id="B19">
<label>19</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[PIÑERA]]></surname>
<given-names><![CDATA[I]]></given-names>
</name>
<name>
<surname><![CDATA[CRUZ]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
<name>
<surname><![CDATA[LEYVA]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[ABREU]]></surname>
<given-names><![CDATA[Y]]></given-names>
</name>
</person-group>
<source><![CDATA[Phys Stat Sol]]></source>
<year>2006</year>
</nlm-citation>
</ref>
</ref-list>
</back>
</article>
