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    <title>Recent Articles in Phys. Rev. C</title>
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    <description>Recent articles in Physical Review C</description>
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    <syn:updateBase>2013-05-17T21:06:12-04:00</syn:updateBase>
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    <dc:date>2013-05-17T21:06:12-04:00</dc:date>
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    <dc:rights>Copyright © 2013 the American Physical Society. Personal use only, all commercial or other reuse prohibited</dc:rights>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054320">
    <title>Spectroscopy of the proton drip-line nucleus ^{203}Fr</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054320</link>
    <description>Author(s): U. Jakobsson, S. Juutinen, J. Uusitalo, M. Leino, K. Auranen, T. Enqvist, P. T. Greenlees, K. Hauschild, P. Jones, R. Julin, S. Ketelhut, P. Kuusiniemi, M. Nyman, P. Peura, P. Rahkila, P. Ruotsalainen, J. Sarén, C. Scholey, and J. Sorri&lt;br/&gt;&lt;p&gt;The nucleus &lt;sup&gt;203&lt;/sup&gt;Fr has been studied through &lt;span style="font-style: italic;"&gt;γ&lt;/span&gt;-ray and electron spectroscopy, using the recoil-decay tagging technique. A 13/2&lt;sup&gt;+&lt;/sup&gt; state, with a half-life of 0.37(5) &lt;span style="font-style: italic;"&gt;μ&lt;/span&gt;s, has been observed in &lt;sup&gt;203&lt;/sup&gt;Fr. Both the &lt;span style="font-style: italic;"&gt;α&lt;/span&gt;-decay branch and the internal de-excitation of the 1/2&lt;sup&gt;+&lt;/sup&gt; isomer in &lt;sup&gt;203&lt;/sup&gt;Fr have been studied. Furth...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054320] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): U. Jakobsson, S. Juutinen, J. Uusitalo, M. Leino, K. Auranen, T. Enqvist, P. T. Greenlees, K. Hauschild, P. Jones, R. Julin, S. Ketelhut, P. Kuusiniemi, M. Nyman, P. Peura, P. Rahkila, P. Ruotsalainen, J. Sarén, C. Scholey, and J. Sorri</p><p> The nucleus <sup>203</sup>Fr has been studied through <span style="font-style: italic;">γ</span>-ray and electron spectroscopy, using the recoil-decay tagging technique. A 13/2<sup>+</sup> state, with a half-life of 0.37(5) <span style="font-style: italic;">μ</span>s, has been observed in <sup>203</sup>Fr. Both the <span style="font-style: italic;">α</span>-decay branch and the internal de-excitation of the 1/2<sup>+</sup> isomer in <sup>203</sup>Fr have been studied. Furth...</p><p>[Phys. Rev. C 87, 054320] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Spectroscopy of the proton drip-line nucleus ^{203}Fr</dc:title>
    <dc:creator>U. Jakobsson, S. Juutinen, J. Uusitalo, M. Leino, K. Auranen, T. Enqvist, P. T. Greenlees, K. Hauschild, P. Jones, R. Julin, S. Ketelhut, P. Kuusiniemi, M. Nyman, P. Peura, P. Rahkila, P. Ruotsalainen, J. Sarén, C. Scholey, and J. Sorri</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054320</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054320 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-17T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054320</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054320</prism:url>
    <prism:startingPage>054320</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054611">
    <title>Dispersive coupled-channels optical-model potential with soft-rotator couplings for Cr, Fe, and Ni isotopes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054611</link>
    <description>Author(s): Rui Li, Weili Sun, E. Sh. Soukhovitskiĩ, J. M. Quesada, and R. Capote&lt;br/&gt;&lt;p&gt;An approximate Lane-consistent dispersive coupled-channels optical potential is derived that describes nucleon-induced reactions on even iron isotopes. Realistic saturated couplings for &lt;sup&gt;54,56,58&lt;/sup&gt;Fe nuclei are built using nuclear wave functions of the soft-rotator model with the Hamiltonian parameters...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054611] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Rui Li, Weili Sun, E. Sh. Soukhovitskiĩ, J. M. Quesada, and R. Capote</p><p> An approximate Lane-consistent dispersive coupled-channels optical potential is derived that describes nucleon-induced reactions on even iron isotopes. Realistic saturated couplings for <sup>54,56,58</sup>Fe nuclei are built using nuclear wave functions of the soft-rotator model with the Hamiltonian parameters...</p><p>[Phys. Rev. C 87, 054611] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Dispersive coupled-channels optical-model potential with soft-rotator couplings for Cr, Fe, and Ni isotopes</dc:title>
    <dc:creator>Rui Li, Weili Sun, E. Sh. Soukhovitskiĩ, J. M. Quesada, and R. Capote</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054611</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054611 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-17T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054611</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054611</prism:url>
    <prism:startingPage>054611</prism:startingPage>
    <dc:subject>Nuclear Reactions</dc:subject>
    <prism:section>Nuclear Reactions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054907">
    <title>Direct photon production in d+Au collisions at sqrt[s_{NN}]=200 GeV</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054907</link>
    <description>Author(s): A. Adare et al. (PHENIX Collaboration)&lt;br/&gt;&lt;p&gt;Direct photons have been measured in √&lt;span style="border-top: 1px solid; padding-top: 0px;"&gt;&lt;span style="font-style: italic;"&gt;s&lt;/span&gt;&lt;sub&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;N&lt;/span&gt;&lt;span style="font-style: italic;"&gt;N&lt;/span&gt;&lt;/sub&gt;&lt;/sub&gt;&lt;/span&gt;=200 GeV &lt;span style="font-style: italic;"&gt;d&lt;/span&gt;+Au collisions at midrapidity. A wide &lt;span style="font-style: italic;"&gt;p&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;T&lt;/span&gt;&lt;/sub&gt; range is covered by measurements of nearly real virtual photons (1&amp;lt;&lt;span style="font-style: italic;"&gt;p&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;T&lt;/span&gt;&lt;/sub&gt;&amp;lt;6 GeV/&lt;span style="font-style: italic;"&gt;c&lt;/span&gt;) and real photons (5&amp;lt;&lt;span style="font-style: italic;"&gt;p&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;T&lt;/span&gt;&lt;/sub&gt;&amp;lt;16 GeV/&lt;span style="font-style: italic;"&gt;c&lt;/span&gt;). The invariant yield of the direct photons in &lt;span style="font-style: italic;"&gt;d&lt;/span&gt;+Au collisions over the scaled &lt;span style="font-style: italic;"&gt;p&lt;/span&gt;+&lt;span style="font-style: italic;"&gt;p&lt;/span&gt; cr...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054907] Published Fri May 17, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): A. Adare et al. (PHENIX Collaboration)</p><p> Direct photons have been measured in √<span style="border-top: 1px solid; padding-top: 0px;"><span style="font-style: italic;">s</span><sub><sub><span style="font-style: italic;">N</span><span style="font-style: italic;">N</span></sub></sub></span>=200 GeV <span style="font-style: italic;">d</span>+Au collisions at midrapidity. A wide <span style="font-style: italic;">p</span><sub><span style="font-style: italic;">T</span></sub> range is covered by measurements of nearly real virtual photons (1&lt;<span style="font-style: italic;">p</span><sub><span style="font-style: italic;">T</span></sub>&lt;6 GeV/<span style="font-style: italic;">c</span>) and real photons (5&lt;<span style="font-style: italic;">p</span><sub><span style="font-style: italic;">T</span></sub>&lt;16 GeV/<span style="font-style: italic;">c</span>). The invariant yield of the direct photons in <span style="font-style: italic;">d</span>+Au collisions over the scaled <span style="font-style: italic;">p</span>+<span style="font-style: italic;">p</span> cr...</p><p>[Phys. Rev. C 87, 054907] Published Fri May 17, 2013</p>]]></content:encoded>
    <dc:title>Direct photon production in d+Au collisions at sqrt[s_{NN}]=200 GeV</dc:title>
    <dc:creator>A. Adare et al. (PHENIX Collaboration)</dc:creator>
    <dc:date>2013-05-17T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054907</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054907 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-17T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054907</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054907</prism:url>
    <prism:startingPage>054907</prism:startingPage>
    <dc:subject>Relativistic Nuclear Collisions</dc:subject>
    <prism:section>Relativistic Nuclear Collisions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054318">
    <title>Properties of trapped neutrons interacting with realistic nuclear Hamiltonians</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054318</link>
    <description>Author(s): Pieter Maris, James P. Vary, S. Gandolfi, J. Carlson, and Steven C. Pieper&lt;br/&gt;&lt;p&gt;We calculate properties of neutron drops in external potentials using both quantum Monte Carlo and no-core full configuration techniques. The properties of the external wells are varied to examine different density profiles. We compare neutron drop results given by a selection of nuclear Hamiltonian...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054318] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Pieter Maris, James P. Vary, S. Gandolfi, J. Carlson, and Steven C. Pieper</p><p> We calculate properties of neutron drops in external potentials using both quantum Monte Carlo and no-core full configuration techniques. The properties of the external wells are varied to examine different density profiles. We compare neutron drop results given by a selection of nuclear Hamiltonian...</p><p>[Phys. Rev. C 87, 054318] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Properties of trapped neutrons interacting with realistic nuclear Hamiltonians</dc:title>
    <dc:creator>Pieter Maris, James P. Vary, S. Gandolfi, J. Carlson, and Steven C. Pieper</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054318</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054318 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054318</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054318</prism:url>
    <prism:startingPage>054318</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054319">
    <title>Influence of electron screening on α decay</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054319</link>
    <description>Author(s): F. F. Karpeshin&lt;br/&gt;&lt;p&gt;The effect of electron screening on the &lt;span style="font-style: italic;"&gt;α&lt;/span&gt; decay rate of typical nuclei is considered. To this end, the adiabatical approach is exploited, which consecutively takes into account the adiabaticity of the motion of the &lt;span style="font-style: italic;"&gt;α&lt;/span&gt; particle through the shells. The effect is found to be of the order of 0.1% to 0.01...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054319] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): F. F. Karpeshin</p><p> The effect of electron screening on the <span style="font-style: italic;">α</span> decay rate of typical nuclei is considered. To this end, the adiabatical approach is exploited, which consecutively takes into account the adiabaticity of the motion of the <span style="font-style: italic;">α</span> particle through the shells. The effect is found to be of the order of 0.1% to 0.01...</p><p>[Phys. Rev. C 87, 054319] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Influence of electron screening on α decay</dc:title>
    <dc:creator>F. F. Karpeshin</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054319</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054319 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054319</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054319</prism:url>
    <prism:startingPage>054319</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.059902">
    <title>Publisher's Note: Signature splitting inversion and backbending in ^{80}Rb [Phys. Rev. C 87, 034320 (2013)]</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.059902</link>
    <description>Author(s): Chuangye He, Shuifa Shen, Shuxian Wen, Lihua Zhu, Xiaoguang Wu, Guangsheng Li, Yue Zhao, Yupeng Yan, Zhijun Bai, Yican Wu, Yazhou Li, Gui Li, Shiwei Yan, M. Oshima, Y. Toh, A. Osa, M. Koizumi, Y. Hatsukawa, M. Matsuda, and T. Hayakawa&lt;br/&gt;[Phys. Rev. C 87, 059902] Published Thu May 16, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Chuangye He, Shuifa Shen, Shuxian Wen, Lihua Zhu, Xiaoguang Wu, Guangsheng Li, Yue Zhao, Yupeng Yan, Zhijun Bai, Yican Wu, Yazhou Li, Gui Li, Shiwei Yan, M. Oshima, Y. Toh, A. Osa, M. Koizumi, Y. Hatsukawa, M. Matsuda, and T. Hayakawa</p><p>[Phys. Rev. C 87, 059902] Published Thu May 16, 2013</p>]]></content:encoded>
    <dc:title>Publisher's Note: Signature splitting inversion and backbending in ^{80}Rb [Phys. Rev. C 87, 034320 (2013)]</dc:title>
    <dc:creator>Chuangye He, Shuifa Shen, Shuxian Wen, Lihua Zhu, Xiaoguang Wu, Guangsheng Li, Yue Zhao, Yupeng Yan, Zhijun Bai, Yican Wu, Yazhou Li, Gui Li, Shiwei Yan, M. Oshima, Y. Toh, A. Osa, M. Koizumi, Y. Hatsukawa, M. Matsuda, and T. Hayakawa</dc:creator>
    <dc:date>2013-05-16T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.059902</dc:identifier>
    <dc:source>Phys. Rev. C 87, 059902 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-16T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.059902</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.059902</prism:url>
    <prism:startingPage>059902</prism:startingPage>
    <dc:subject>Errata</dc:subject>
    <prism:section>Errata</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.051303">
    <title>Nuclear β^{+}/EC decays in covariant density functional theory and the impact of isoscalar proton-neutron pairing</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.051303</link>
    <description>Author(s): Z. M. Niu (牛中明), Y. F. Niu (牛一斐), Q. Liu (刘泉), H. Z. Liang (梁豪兆), and J. Y. Guo (郭建友)&lt;br/&gt;&lt;p&gt;Self-consistent proton-neutron quasiparticle random phase approximation based on the spherical nonlinear point-coupling relativistic Hartree-Bogoliubov theory is established and used to investigate the &lt;span style="font-style: italic;"&gt;β&lt;/span&gt;&lt;sup&gt;+&lt;/sup&gt;/electron-capture (EC)-decay half-lives of neutron-deficient Ar, Ca, Ti, Fe, Ni, Zn, Cd, and Sn ...&lt;/p&gt;&lt;br/&gt;&lt;img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt; &lt;br/&gt;[Phys. Rev. C 87, 051303] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Z. M. Niu (牛中明), Y. F. Niu (牛一斐), Q. Liu (刘泉), H. Z. Liang (梁豪兆), and J. Y. Guo (郭建友)</p><p><img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/>  Self-consistent proton-neutron quasiparticle random phase approximation based on the spherical nonlinear point-coupling relativistic Hartree-Bogoliubov theory is established and used to investigate the <span style="font-style: italic;">β</span><sup>+</sup>/electron-capture (EC)-decay half-lives of neutron-deficient Ar, Ca, Ti, Fe, Ni, Zn, Cd, and Sn ...</p><p>[Phys. Rev. C 87, 051303] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Nuclear β^{+}/EC decays in covariant density functional theory and the impact of isoscalar proton-neutron pairing</dc:title>
    <dc:creator>Z. M. Niu (牛中明), Y. F. Niu (牛一斐), Q. Liu (刘泉), H. Z. Liang (梁豪兆), and J. Y. Guo (郭建友)</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.051303</dc:identifier>
    <dc:source>Phys. Rev. C 87, 051303 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.051303</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.051303</prism:url>
    <prism:startingPage>051303</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.051304">
    <title>Decay pattern of the pygmy dipole resonance in ^{60}Ni</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.051304</link>
    <description>Author(s): M. Scheck, V. Yu. Ponomarev, T. Aumann, J. Beller, M. Fritzsche, J. Isaak, J. H. Kelley, E. Kwan, N. Pietralla, R. Raut, C. Romig, G. Rusev, D. Savran, K. Sonnabend, A. P. Tonchev, W. Tornow, H. R. Weller, and M. Zweidinger&lt;br/&gt;&lt;p&gt;Spin-1 states in &lt;sup&gt;60&lt;/sup&gt;Ni were excited with the (&lt;span style="font-style: italic;"&gt;γ&lt;/span&gt;⃗,&lt;span style="font-style: italic;"&gt;γ&lt;/span&gt;&lt;sup&gt;′&lt;/sup&gt;) reaction, exploiting the High Intensity &lt;span style="font-style: italic;"&gt;γ&lt;/span&gt;⃗-ray Source at Triangle University Nuclear Laboratory. This facility is capable of providing fully linearly polarized, quasimonochromatic, Compton-backscattered photons in the entrance channel of the reacti...&lt;/p&gt;&lt;br/&gt;&lt;img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt; &lt;br/&gt;[Phys. Rev. C 87, 051304] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): M. Scheck, V. Yu. Ponomarev, T. Aumann, J. Beller, M. Fritzsche, J. Isaak, J. H. Kelley, E. Kwan, N. Pietralla, R. Raut, C. Romig, G. Rusev, D. Savran, K. Sonnabend, A. P. Tonchev, W. Tornow, H. R. Weller, and M. Zweidinger</p><p><img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/>  Spin-1 states in <sup>60</sup>Ni were excited with the (<span style="font-style: italic;">γ</span>⃗,<span style="font-style: italic;">γ</span><sup>′</sup>) reaction, exploiting the High Intensity <span style="font-style: italic;">γ</span>⃗-ray Source at Triangle University Nuclear Laboratory. This facility is capable of providing fully linearly polarized, quasimonochromatic, Compton-backscattered photons in the entrance channel of the reacti...</p><p>[Phys. Rev. C 87, 051304] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Decay pattern of the pygmy dipole resonance in ^{60}Ni</dc:title>
    <dc:creator>M. Scheck, V. Yu. Ponomarev, T. Aumann, J. Beller, M. Fritzsche, J. Isaak, J. H. Kelley, E. Kwan, N. Pietralla, R. Raut, C. Romig, G. Rusev, D. Savran, K. Sonnabend, A. P. Tonchev, W. Tornow, H. R. Weller, and M. Zweidinger</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.051304</dc:identifier>
    <dc:source>Phys. Rev. C 87, 051304 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.051304</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.051304</prism:url>
    <prism:startingPage>051304</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054313">
    <title>Giant dipole resonance in ^{88}Mo from phonon damping model strength functions averaged over temperature and angular momentum distributions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054313</link>
    <description>Author(s): N. Dinh Dang, M. Ciemala, M. Kmiecik, and A. Maj&lt;br/&gt;&lt;p&gt;The line shapes of giant dipole resonance (GDR) in the decay of the compound nucleus &lt;sup&gt;88&lt;/sup&gt;Mo, which is formed after the fusion-evaporation reaction &lt;sup&gt;48&lt;/sup&gt;Ti + &lt;sup&gt;40&lt;/sup&gt;Ca at various excitation energies &lt;span style="font-style: italic;"&gt;E&lt;/span&gt;&lt;sup&gt;*&lt;/sup&gt; from 58 to 308 MeV, are generated by averaging the GDR strength functions predicted within the phonon damping...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054313] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): N. Dinh Dang, M. Ciemala, M. Kmiecik, and A. Maj</p><p> The line shapes of giant dipole resonance (GDR) in the decay of the compound nucleus <sup>88</sup>Mo, which is formed after the fusion-evaporation reaction <sup>48</sup>Ti + <sup>40</sup>Ca at various excitation energies <span style="font-style: italic;">E</span><sup>*</sup> from 58 to 308 MeV, are generated by averaging the GDR strength functions predicted within the phonon damping...</p><p>[Phys. Rev. C 87, 054313] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Giant dipole resonance in ^{88}Mo from phonon damping model strength functions averaged over temperature and angular momentum distributions</dc:title>
    <dc:creator>N. Dinh Dang, M. Ciemala, M. Kmiecik, and A. Maj</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054313</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054313 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054313</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054313</prism:url>
    <prism:startingPage>054313</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054314">
    <title>Nuclear superfluidity for antimagnetic rotation in ^{105}Cd and ^{106}Cd</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054314</link>
    <description>Author(s): Zhen-Hua Zhang (张振华), Peng-Wei Zhao (赵鹏巍), Jie Meng (孟杰), Jin-Yan Zeng (曾谨言), En-Guang Zhao (赵恩广), and Shan-Gui Zhou (周善贵)&lt;br/&gt;&lt;p&gt;The effects of nuclear superfluidity on antimagnetic rotation bands in &lt;sup&gt;105&lt;/sup&gt;Cd and &lt;sup&gt;106&lt;/sup&gt;Cd are investigated by the cranked shell model with the pairing correlations and blocking effects treated by a particle-number-conserving method. The experimental moments of inertia and the reduced &lt;span style="font-style: italic;"&gt;B&lt;/span&gt;(&lt;span style="font-style: italic;"&gt;E&lt;/span&gt;2) transition v...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054314] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Zhen-Hua Zhang (张振华), Peng-Wei Zhao (赵鹏巍), Jie Meng (孟杰), Jin-Yan Zeng (曾谨言), En-Guang Zhao (赵恩广), and Shan-Gui Zhou (周善贵)</p><p> The effects of nuclear superfluidity on antimagnetic rotation bands in <sup>105</sup>Cd and <sup>106</sup>Cd are investigated by the cranked shell model with the pairing correlations and blocking effects treated by a particle-number-conserving method. The experimental moments of inertia and the reduced <span style="font-style: italic;">B</span>(<span style="font-style: italic;">E</span>2) transition v...</p><p>[Phys. Rev. C 87, 054314] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Nuclear superfluidity for antimagnetic rotation in ^{105}Cd and ^{106}Cd</dc:title>
    <dc:creator>Zhen-Hua Zhang (张振华), Peng-Wei Zhao (赵鹏巍), Jie Meng (孟杰), Jin-Yan Zeng (曾谨言), En-Guang Zhao (赵恩广), and Shan-Gui Zhou (周善贵)</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054314</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054314 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054314</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054314</prism:url>
    <prism:startingPage>054314</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054315">
    <title>Comparison of 1n and 2n prescriptions for matter radii</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054315</link>
    <description>Author(s): H. T. Fortune and R. Sherr&lt;br/&gt;&lt;p&gt;We have computed the matter radius of &lt;sup&gt;17&lt;/sup&gt;N(g.s.), using both the 1&lt;span style="font-style: italic;"&gt;n&lt;/span&gt; and 2&lt;span style="font-style: italic;"&gt;n&lt;/span&gt; prescriptions. The two results differ by only 0.02 fm.&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054315] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): H. T. Fortune and R. Sherr</p><p> We have computed the matter radius of <sup>17</sup>N(g.s.), using both the 1<span style="font-style: italic;">n</span> and 2<span style="font-style: italic;">n</span> prescriptions. The two results differ by only 0.02 fm.</p><p>[Phys. Rev. C 87, 054315] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Comparison of 1n and 2n prescriptions for matter radii</dc:title>
    <dc:creator>H. T. Fortune and R. Sherr</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054315</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054315 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054315</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054315</prism:url>
    <prism:startingPage>054315</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054316">
    <title>High-spin structures of _{55}^{136}Cs_{81}</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054316</link>
    <description>Author(s): A. Astier, M.-G. Porquet, G. Duchêne, F. Azaiez, D. Curien, I. Deloncle, O. Dorvaux, B. J. P. Gall, M. Houry, R. Lucas, P. C. Srivastava, N. Redon, M. Rousseau, O. Stézowski, and Ch. Theisen&lt;br/&gt;&lt;p&gt;Odd-odd &lt;sup&gt;136&lt;/sup&gt;Cs nuclei have been produced in the &lt;sup&gt;18&lt;/sup&gt;O+&lt;sup&gt;208&lt;/sup&gt;Pb and &lt;sup&gt;12&lt;/sup&gt;C+&lt;sup&gt;238&lt;/sup&gt;U fusion-fission reactions and their &lt;span style="font-style: italic;"&gt;γ&lt;/span&gt; rays studied with the Euroball array. The high-spin level scheme was built up to ∼4.7 MeV excitation energy and spin &lt;span style="font-style: italic;"&gt;I&lt;/span&gt;∼16&lt;span style="font-style: italic;"&gt;ℏ&lt;/span&gt; from the triple &lt;span style="font-style: italic;"&gt;γ&lt;/span&gt;-ray coincidence data. The configurations of the thre...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054316] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): A. Astier, M.-G. Porquet, G. Duchêne, F. Azaiez, D. Curien, I. Deloncle, O. Dorvaux, B. J. P. Gall, M. Houry, R. Lucas, P. C. Srivastava, N. Redon, M. Rousseau, O. Stézowski, and Ch. Theisen</p><p> Odd-odd <sup>136</sup>Cs nuclei have been produced in the <sup>18</sup>O+<sup>208</sup>Pb and <sup>12</sup>C+<sup>238</sup>U fusion-fission reactions and their <span style="font-style: italic;">γ</span> rays studied with the Euroball array. The high-spin level scheme was built up to ∼4.7 MeV excitation energy and spin <span style="font-style: italic;">I</span>∼16<span style="font-style: italic;">ℏ</span> from the triple <span style="font-style: italic;">γ</span>-ray coincidence data. The configurations of the thre...</p><p>[Phys. Rev. C 87, 054316] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>High-spin structures of _{55}^{136}Cs_{81}</dc:title>
    <dc:creator>A. Astier, M.-G. Porquet, G. Duchêne, F. Azaiez, D. Curien, I. Deloncle, O. Dorvaux, B. J. P. Gall, M. Houry, R. Lucas, P. C. Srivastava, N. Redon, M. Rousseau, O. Stézowski, and Ch. Theisen</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054316</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054316 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054316</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054316</prism:url>
    <prism:startingPage>054316</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054904">
    <title>Early thermalization of quark-gluon matter with the elastic scattering of ggq and ggq[over ¯]</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054904</link>
    <description>Author(s): Xiao-Ming Xu, Zhen-Yu Shen, Zhi-Cheng Ye, and Wei-Jie Xu&lt;br/&gt;&lt;p&gt;Elastic gluon-gluon-quark (gluon-gluon-antiquark) scattering is studied in perturbative QCD with 123 Feynman diagrams at the tree level. Individually squared amplitudes and interference terms of the Feynman diagrams are derived. With the elastic gluon-gluon-quark scattering and the elastic gluon-glu...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054904] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Xiao-Ming Xu, Zhen-Yu Shen, Zhi-Cheng Ye, and Wei-Jie Xu</p><p> Elastic gluon-gluon-quark (gluon-gluon-antiquark) scattering is studied in perturbative QCD with 123 Feynman diagrams at the tree level. Individually squared amplitudes and interference terms of the Feynman diagrams are derived. With the elastic gluon-gluon-quark scattering and the elastic gluon-glu...</p><p>[Phys. Rev. C 87, 054904] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Early thermalization of quark-gluon matter with the elastic scattering of ggq and ggq[over ¯]</dc:title>
    <dc:creator>Xiao-Ming Xu, Zhen-Yu Shen, Zhi-Cheng Ye, and Wei-Jie Xu</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054904</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054904 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054904</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054904</prism:url>
    <prism:startingPage>054904</prism:startingPage>
    <dc:subject>Relativistic Nuclear Collisions</dc:subject>
    <prism:section>Relativistic Nuclear Collisions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054905">
    <title>Production of antinuclei and hypernuclei in a relativistic Hagedorn resonance gas model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054905</link>
    <description>Author(s): Subrata Pal and Walter Greiner&lt;br/&gt;&lt;p&gt;We study the production of light nuclei, hypernuclei, and their antiparticles in relativistic energy heavy ion collisions from sequential decay of massive resonance states within a Hagedorn resonance gas model. The production yield of these clusters and of the multistrange hypernuclear objects are p...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054905] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Subrata Pal and Walter Greiner</p><p> We study the production of light nuclei, hypernuclei, and their antiparticles in relativistic energy heavy ion collisions from sequential decay of massive resonance states within a Hagedorn resonance gas model. The production yield of these clusters and of the multistrange hypernuclear objects are p...</p><p>[Phys. Rev. C 87, 054905] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Production of antinuclei and hypernuclei in a relativistic Hagedorn resonance gas model</dc:title>
    <dc:creator>Subrata Pal and Walter Greiner</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054905</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054905 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054905</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054905</prism:url>
    <prism:startingPage>054905</prism:startingPage>
    <dc:subject>Relativistic Nuclear Collisions</dc:subject>
    <prism:section>Relativistic Nuclear Collisions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054906">
    <title>Universal centrality dependence of particle multiplicities in heavy-ion collisions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054906</link>
    <description>Author(s): H. J. Pirner, K. Reygers, and B. Z. Kopeliovich&lt;br/&gt;&lt;p&gt;Starting from the light-cone plasma (LCP) distribution of gluons produced in proton-proton collisions, we derive the invariant charged-particle yield &lt;span style="font-style: italic;"&gt;d&lt;/span&gt;&lt;span style="font-style: italic;"&gt;N&lt;/span&gt;/&lt;span style="font-style: italic;"&gt;d&lt;/span&gt;&lt;span style="font-style: italic;"&gt;y&lt;/span&gt; &lt;span style="font-style: italic;"&gt;d&lt;/span&gt;&lt;sup&gt;2&lt;/sup&gt;&lt;span style="font-style: italic;"&gt;p&lt;/span&gt;&lt;sub&gt;⊥&lt;/sub&gt; in heavy-ion collisions. Multiple scattering of partons in the other nucleus leads to &lt;span style="font-style: italic;"&gt;p&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;⊥&lt;/span&gt;&lt;/sub&gt; broadening, which depends on the centrality of the...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054906] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): H. J. Pirner, K. Reygers, and B. Z. Kopeliovich</p><p> Starting from the light-cone plasma (LCP) distribution of gluons produced in proton-proton collisions, we derive the invariant charged-particle yield <span style="font-style: italic;">d</span><span style="font-style: italic;">N</span>/<span style="font-style: italic;">d</span><span style="font-style: italic;">y</span> <span style="font-style: italic;">d</span><sup>2</sup><span style="font-style: italic;">p</span><sub>⊥</sub> in heavy-ion collisions. Multiple scattering of partons in the other nucleus leads to <span style="font-style: italic;">p</span><sub><span style="font-style: italic;">⊥</span></sub> broadening, which depends on the centrality of the...</p><p>[Phys. Rev. C 87, 054906] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>Universal centrality dependence of particle multiplicities in heavy-ion collisions</dc:title>
    <dc:creator>H. J. Pirner, K. Reygers, and B. Z. Kopeliovich</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054906</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054906 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054906</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054906</prism:url>
    <prism:startingPage>054906</prism:startingPage>
    <dc:subject>Relativistic Nuclear Collisions</dc:subject>
    <prism:section>Relativistic Nuclear Collisions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.057304">
    <title>New features of the Garvey-Kelson mass relations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.057304</link>
    <description>Author(s): Z. He, M. Bao, Y. M. Zhao, and A. Arima&lt;br/&gt;&lt;p&gt;In this Brief Report we report systematic deviations of the Garvey-Kelson mass relations for different parity combinations of neutrons and protons. A simple argument of such deviations is presented in terms of the pairing interaction.&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 057304] Published Wed May 15, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Z. He, M. Bao, Y. M. Zhao, and A. Arima</p><p> In this Brief Report we report systematic deviations of the Garvey-Kelson mass relations for different parity combinations of neutrons and protons. A simple argument of such deviations is presented in terms of the pairing interaction.</p><p>[Phys. Rev. C 87, 057304] Published Wed May 15, 2013</p>]]></content:encoded>
    <dc:title>New features of the Garvey-Kelson mass relations</dc:title>
    <dc:creator>Z. He, M. Bao, Y. M. Zhao, and A. Arima</dc:creator>
    <dc:date>2013-05-15T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.057304</dc:identifier>
    <dc:source>Phys. Rev. C 87, 057304 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-15T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.057304</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.057304</prism:url>
    <prism:startingPage>057304</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054609">
    <title>Three-beam setup for coherently controlling nuclear-state population</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054609</link>
    <description>Author(s): Wen-Te Liao, Adriana Pálffy, and Christoph H. Keitel&lt;br/&gt;&lt;p&gt;The controlled transfer of nuclear state population using two x-ray laser pulses is investigated theoretically. The laser pulses drive two nuclear transitions in a nuclear three-level system facilitating coherent population transfer via the quantum optics technique of stimulated Raman adiabatic pass...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054609] Published Tue May 14, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Wen-Te Liao, Adriana Pálffy, and Christoph H. Keitel</p><p> The controlled transfer of nuclear state population using two x-ray laser pulses is investigated theoretically. The laser pulses drive two nuclear transitions in a nuclear three-level system facilitating coherent population transfer via the quantum optics technique of stimulated Raman adiabatic pass...</p><p>[Phys. Rev. C 87, 054609] Published Tue May 14, 2013</p>]]></content:encoded>
    <dc:title>Three-beam setup for coherently controlling nuclear-state population</dc:title>
    <dc:creator>Wen-Te Liao, Adriana Pálffy, and Christoph H. Keitel</dc:creator>
    <dc:date>2013-05-14T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054609</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054609 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-14T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054609</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054609</prism:url>
    <prism:startingPage>054609</prism:startingPage>
    <dc:subject>Nuclear Reactions</dc:subject>
    <prism:section>Nuclear Reactions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054610">
    <title>Fusion-evaporation residues and α-decay chains of the superheavy element Z=115 formed in the ^{243}Am + ^{48}Ca reaction using the dynamical cluster-decay model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054610</link>
    <description>Author(s): Raj Kumar, Kirandeep Sandhu, Manoj K. Sharma, and Raj K. Gupta&lt;br/&gt;&lt;p&gt;The decay of the &lt;span style="font-style: italic;"&gt;Z&lt;/span&gt;=115 superheavy nuclear system, formed in the &lt;sup&gt;243&lt;/sup&gt;Am+&lt;sup&gt;48&lt;/sup&gt;Ca reaction, is studied by using the dynamical cluster-decay model. The calculated excitation functions of 2&lt;span style="font-style: italic;"&gt;n&lt;/span&gt;-, 3&lt;span style="font-style: italic;"&gt;n&lt;/span&gt;-, and 4&lt;span style="font-style: italic;"&gt;n&lt;/span&gt;-evaporation channels, for the excitation energy range &lt;span style="font-style: italic;"&gt;E&lt;/span&gt;&lt;sub&gt;CN&lt;/sub&gt;&lt;sup&gt;*&lt;/sup&gt;=31–47 MeV, are compared with the recent exper...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054610] Published Tue May 14, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Raj Kumar, Kirandeep Sandhu, Manoj K. Sharma, and Raj K. Gupta</p><p> The decay of the <span style="font-style: italic;">Z</span>=115 superheavy nuclear system, formed in the <sup>243</sup>Am+<sup>48</sup>Ca reaction, is studied by using the dynamical cluster-decay model. The calculated excitation functions of 2<span style="font-style: italic;">n</span>-, 3<span style="font-style: italic;">n</span>-, and 4<span style="font-style: italic;">n</span>-evaporation channels, for the excitation energy range <span style="font-style: italic;">E</span><sub>CN</sub><sup>*</sup>=31–47 MeV, are compared with the recent exper...</p><p>[Phys. Rev. C 87, 054610] Published Tue May 14, 2013</p>]]></content:encoded>
    <dc:title>Fusion-evaporation residues and α-decay chains of the superheavy element Z=115 formed in the ^{243}Am + ^{48}Ca reaction using the dynamical cluster-decay model</dc:title>
    <dc:creator>Raj Kumar, Kirandeep Sandhu, Manoj K. Sharma, and Raj K. Gupta</dc:creator>
    <dc:date>2013-05-14T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054610</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054610 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-14T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054610</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054610</prism:url>
    <prism:startingPage>054610</prism:startingPage>
    <dc:subject>Nuclear Reactions</dc:subject>
    <prism:section>Nuclear Reactions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.055204">
    <title>Case in favor of the N^{*}(1700)(3/2^{−})</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.055204</link>
    <description>Author(s): E. J. Garzon, J. J. Xie, and E. Oset&lt;br/&gt;&lt;p&gt;Using an interaction extracted from the local hidden-gauge Lagrangians, which brings together vector and pseudoscalar mesons, and the coupled channels &lt;span style="font-style: italic;"&gt;ρ&lt;/span&gt;&lt;span style="font-style: italic;"&gt;N&lt;/span&gt; (&lt;span style="font-style: italic;"&gt;s&lt;/span&gt; wave), &lt;span style="font-style: italic;"&gt;π&lt;/span&gt;&lt;span style="font-style: italic;"&gt;N&lt;/span&gt; (&lt;span style="font-style: italic;"&gt;d&lt;/span&gt; wave), &lt;span style="font-style: italic;"&gt;π&lt;/span&gt;&lt;span style="font-style: italic;"&gt;Δ&lt;/span&gt; (&lt;span style="font-style: italic;"&gt;s&lt;/span&gt; wave), and &lt;span style="font-style: italic;"&gt;π&lt;/span&gt;&lt;span style="font-style: italic;"&gt;Δ&lt;/span&gt; (&lt;span style="font-style: italic;"&gt;d&lt;/span&gt; wave), we look in the region of √&lt;span style="border-top: 1px solid; padding-top: 0px;"&gt;&lt;span style="font-style: italic;"&gt;s&lt;/span&gt;&lt;/span&gt;=1400–1850 MeV and find two resonances dynamically generated by th...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 055204] Published Tue May 14, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): E. J. Garzon, J. J. Xie, and E. Oset</p><p> Using an interaction extracted from the local hidden-gauge Lagrangians, which brings together vector and pseudoscalar mesons, and the coupled channels <span style="font-style: italic;">ρ</span><span style="font-style: italic;">N</span> (<span style="font-style: italic;">s</span> wave), <span style="font-style: italic;">π</span><span style="font-style: italic;">N</span> (<span style="font-style: italic;">d</span> wave), <span style="font-style: italic;">π</span><span style="font-style: italic;">Δ</span> (<span style="font-style: italic;">s</span> wave), and <span style="font-style: italic;">π</span><span style="font-style: italic;">Δ</span> (<span style="font-style: italic;">d</span> wave), we look in the region of √<span style="border-top: 1px solid; padding-top: 0px;"><span style="font-style: italic;">s</span></span>=1400–1850 MeV and find two resonances dynamically generated by th...</p><p>[Phys. Rev. C 87, 055204] Published Tue May 14, 2013</p>]]></content:encoded>
    <dc:title>Case in favor of the N^{*}(1700)(3/2^{−})</dc:title>
    <dc:creator>E. J. Garzon, J. J. Xie, and E. Oset</dc:creator>
    <dc:date>2013-05-14T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.055204</dc:identifier>
    <dc:source>Phys. Rev. C 87, 055204 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-14T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.055204</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.055204</prism:url>
    <prism:startingPage>055204</prism:startingPage>
    <dc:subject>Hadronic Physics and QCD</dc:subject>
    <prism:section>Hadronic Physics and QCD</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.055805">
    <title>Time-dependent Hartree-Fock approach to nuclear “pasta” at finite temperature</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.055805</link>
    <description>Author(s): B. Schuetrumpf, M. A. Klatt, K. Iida, J. A. Maruhn, K. Mecke, and P.-G. Reinhard&lt;br/&gt;&lt;p&gt;We present simulations of neutron-rich matter at subnuclear densities, like supernova matter, with the time-dependent Hartree-Fock approximation at temperatures of several MeV. The initial state consists of &lt;span style="font-style: italic;"&gt;α&lt;/span&gt; particles randomly distributed in space that have a Maxwell-Boltzmann distribution in momen...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 055805] Published Tue May 14, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): B. Schuetrumpf, M. A. Klatt, K. Iida, J. A. Maruhn, K. Mecke, and P.-G. Reinhard</p><p> We present simulations of neutron-rich matter at subnuclear densities, like supernova matter, with the time-dependent Hartree-Fock approximation at temperatures of several MeV. The initial state consists of <span style="font-style: italic;">α</span> particles randomly distributed in space that have a Maxwell-Boltzmann distribution in momen...</p><p>[Phys. Rev. C 87, 055805] Published Tue May 14, 2013</p>]]></content:encoded>
    <dc:title>Time-dependent Hartree-Fock approach to nuclear “pasta” at finite temperature</dc:title>
    <dc:creator>B. Schuetrumpf, M. A. Klatt, K. Iida, J. A. Maruhn, K. Mecke, and P.-G. Reinhard</dc:creator>
    <dc:date>2013-05-14T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.055805</dc:identifier>
    <dc:source>Phys. Rev. C 87, 055805 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-14T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.055805</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.055805</prism:url>
    <prism:startingPage>055805</prism:startingPage>
    <dc:subject>Nuclear Astrophysics</dc:subject>
    <prism:section>Nuclear Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.051001">
    <title>Angular distributions of the vector A_{y} and tensor A_{yy}, A_{xx}, A_{xz} analyzing powers in the d[over ⃗]d→^{3}Hp reaction at 200 MeV</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.051001</link>
    <description>Author(s): A. K. Kurilkin, T. Saito, V. P. Ladygin, T. Uesaka, M. Hatano, A. Yu. Isupov, M. Janek, H. Kato, N. B. Ladygina, Y. Maeda, A. I. Malakhov, J. Nishikawa, T. Ohnishi, H. Okamura, S. G. Reznikov, H. Sakai, N. Sakamoto, S. Sakoda, Y. Satou, K. Sekiguchi, K. Suda, A. Tamii, N. Uchigashima, T. A. Vasiliev, and K. Yako&lt;br/&gt;&lt;p&gt;A complete set of analyzing powers for the &lt;span style="font-style: italic;"&gt;d&lt;/span&gt;⃗&lt;span style="font-style: italic;"&gt;d&lt;/span&gt;→&lt;sup&gt;3&lt;/sup&gt;H&lt;span style="font-style: italic;"&gt;p&lt;/span&gt; reaction at the kinetic beam energy of 200 MeV has been measured in the full angular range in the c.m. frame. The observed signs of the tensor analyzing powers &lt;span style="font-style: italic;"&gt;A&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;y&lt;/span&gt;&lt;span style="font-style: italic;"&gt;y&lt;/span&gt;&lt;/sub&gt;, &lt;span style="font-style: italic;"&gt;A&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;x&lt;/span&gt;&lt;span style="font-style: italic;"&gt;x&lt;/span&gt;&lt;/sub&gt;, and &lt;span style="font-style: italic;"&gt;A&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;x&lt;/span&gt;&lt;span style="font-style: italic;"&gt;z&lt;/span&gt;&lt;/sub&gt; at forward and backward directions have clearly demonstrated the sensit...&lt;/p&gt;&lt;br/&gt;&lt;img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt; &lt;br/&gt;[Phys. Rev. C 87, 051001] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): A. K. Kurilkin, T. Saito, V. P. Ladygin, T. Uesaka, M. Hatano, A. Yu. Isupov, M. Janek, H. Kato, N. B. Ladygina, Y. Maeda, A. I. Malakhov, J. Nishikawa, T. Ohnishi, H. Okamura, S. G. Reznikov, H. Sakai, N. Sakamoto, S. Sakoda, Y. Satou, K. Sekiguchi, K. Suda, A. Tamii, N. Uchigashima, T. A. Vasiliev, and K. Yako</p><p><img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/>  A complete set of analyzing powers for the <span style="font-style: italic;">d</span>⃗<span style="font-style: italic;">d</span>→<sup>3</sup>H<span style="font-style: italic;">p</span> reaction at the kinetic beam energy of 200 MeV has been measured in the full angular range in the c.m. frame. The observed signs of the tensor analyzing powers <span style="font-style: italic;">A</span><sub><span style="font-style: italic;">y</span><span style="font-style: italic;">y</span></sub>, <span style="font-style: italic;">A</span><sub><span style="font-style: italic;">x</span><span style="font-style: italic;">x</span></sub>, and <span style="font-style: italic;">A</span><sub><span style="font-style: italic;">x</span><span style="font-style: italic;">z</span></sub> at forward and backward directions have clearly demonstrated the sensit...</p><p>[Phys. Rev. C 87, 051001] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>Angular distributions of the vector A_{y} and tensor A_{yy}, A_{xx}, A_{xz} analyzing powers in the d[over ⃗]d→^{3}Hp reaction at 200 MeV</dc:title>
    <dc:creator>A. K. Kurilkin, T. Saito, V. P. Ladygin, T. Uesaka, M. Hatano, A. Yu. Isupov, M. Janek, H. Kato, N. B. Ladygina, Y. Maeda, A. I. Malakhov, J. Nishikawa, T. Ohnishi, H. Okamura, S. G. Reznikov, H. Sakai, N. Sakamoto, S. Sakoda, Y. Satou, K. Sekiguchi, K. Suda, A. Tamii, N. Uchigashima, T. A. Vasiliev, and K. Yako</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.051001</dc:identifier>
    <dc:source>Phys. Rev. C 87, 051001 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.051001</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.051001</prism:url>
    <prism:startingPage>051001</prism:startingPage>
    <dc:subject>Nucleon-Nucleon Interaction, Few-Body Systems</dc:subject>
    <prism:section>Nucleon-Nucleon Interaction, Few-Body Systems</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.051302">
    <title>Evolution of surface deformations of weakly bound nuclei in the continuum</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.051302</link>
    <description>Author(s): J. C. Pei, Y. N. Zhang, and F. R. Xu&lt;br/&gt;&lt;p&gt;We study weakly bound deformed nuclei based on the coordinate-space Skyrme Hartree-Fock-Bogoliubov (HFB) approach, in which a large box is employed for treating the continuum and large spatial extensions. When the limit of the core-halo deformation decoupling is approached, calculations found an exo...&lt;/p&gt;&lt;br/&gt;&lt;img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt; &lt;br/&gt;[Phys. Rev. C 87, 051302] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): J. C. Pei, Y. N. Zhang, and F. R. Xu</p><p><img src="http://publish.aps.org/images/icons/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/>  We study weakly bound deformed nuclei based on the coordinate-space Skyrme Hartree-Fock-Bogoliubov (HFB) approach, in which a large box is employed for treating the continuum and large spatial extensions. When the limit of the core-halo deformation decoupling is approached, calculations found an exo...</p><p>[Phys. Rev. C 87, 051302] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>Evolution of surface deformations of weakly bound nuclei in the continuum</dc:title>
    <dc:creator>J. C. Pei, Y. N. Zhang, and F. R. Xu</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.051302</dc:identifier>
    <dc:source>Phys. Rev. C 87, 051302 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.051302</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.051302</prism:url>
    <prism:startingPage>051302</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054310">
    <title>Feasibility of the finite-amplitude method in covariant density functional theory</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054310</link>
    <description>Author(s): Haozhao Liang (梁豪兆), Takashi Nakatsukasa (中務 孝), Zhongming Niu (牛中明), and Jie Meng (孟杰)&lt;br/&gt;&lt;p&gt;The self-consistent relativistic random-phase approximation (RPA) in the radial coordinate representation is established by using the finite-amplitude method (FAM). Taking the isoscalar giant monopole resonance in spherical nuclei as example, the feasibility of the FAM for the covariant density func...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054310] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Haozhao Liang (梁豪兆), Takashi Nakatsukasa (中務 孝), Zhongming Niu (牛中明), and Jie Meng (孟杰)</p><p> The self-consistent relativistic random-phase approximation (RPA) in the radial coordinate representation is established by using the finite-amplitude method (FAM). Taking the isoscalar giant monopole resonance in spherical nuclei as example, the feasibility of the FAM for the covariant density func...</p><p>[Phys. Rev. C 87, 054310] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>Feasibility of the finite-amplitude method in covariant density functional theory</dc:title>
    <dc:creator>Haozhao Liang (梁豪兆), Takashi Nakatsukasa (中務 孝), Zhongming Niu (牛中明), and Jie Meng (孟杰)</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054310</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054310 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054310</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054310</prism:url>
    <prism:startingPage>054310</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054311">
    <title>α-decay spectroscopy of the chain ^{179}Tl^{g}→^{175}Au^{g}→^{171}Ir^{g}→^{167}Re^{m}</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054311</link>
    <description>Author(s): A. N. Andreyev et al.&lt;br/&gt;&lt;p&gt;Detailed &lt;span style="font-style: italic;"&gt;α&lt;/span&gt;-decay studies of &lt;sup&gt;179&lt;/sup&gt;Tl&lt;sup&gt;&lt;span style="font-style: italic;"&gt;g&lt;/span&gt;&lt;/sup&gt; and its daughter products &lt;sup&gt;175&lt;/sup&gt;Au&lt;sup&gt;&lt;span style="font-style: italic;"&gt;g&lt;/span&gt;&lt;/sup&gt; and &lt;sup&gt;171&lt;/sup&gt;Ir&lt;sup&gt;&lt;span style="font-style: italic;"&gt;g&lt;/span&gt;&lt;/sup&gt; were carried out in two complementary experiments at the mass separator ISOLDE (CERN) and velocity filter SHIP (GSI). First unambiguous determination of the &lt;span style="font-style: italic;"&gt;α&lt;/span&gt;-decay properties of &lt;sup&gt;175&lt;/sup&gt;Au&lt;sup&gt;&lt;span style="font-style: italic;"&gt;g&lt;/span&gt;&lt;/sup&gt; was performed as follows: &lt;span style="font-style: italic;"&gt;E&lt;/span&gt;&lt;sub&gt;&lt;span style="font-style: italic;"&gt;α&lt;/span&gt;&lt;/sub&gt; = 6433...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054311] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): A. N. Andreyev et al.</p><p> Detailed <span style="font-style: italic;">α</span>-decay studies of <sup>179</sup>Tl<sup><span style="font-style: italic;">g</span></sup> and its daughter products <sup>175</sup>Au<sup><span style="font-style: italic;">g</span></sup> and <sup>171</sup>Ir<sup><span style="font-style: italic;">g</span></sup> were carried out in two complementary experiments at the mass separator ISOLDE (CERN) and velocity filter SHIP (GSI). First unambiguous determination of the <span style="font-style: italic;">α</span>-decay properties of <sup>175</sup>Au<sup><span style="font-style: italic;">g</span></sup> was performed as follows: <span style="font-style: italic;">E</span><sub><span style="font-style: italic;">α</span></sub> = 6433...</p><p>[Phys. Rev. C 87, 054311] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>α-decay spectroscopy of the chain ^{179}Tl^{g}→^{175}Au^{g}→^{171}Ir^{g}→^{167}Re^{m}</dc:title>
    <dc:creator>A. N. Andreyev et al.</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054311</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054311 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054311</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054311</prism:url>
    <prism:startingPage>054311</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054312">
    <title>Structure of p-shell nuclei using three-nucleon interactions evolved with the similarity renormalization group</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054312</link>
    <description>Author(s): E. D. Jurgenson, P. Maris, R. J. Furnstahl, P. Navrátil, W. E. Ormand, and J. P. Vary&lt;br/&gt;&lt;p&gt;The similarity renormalization group (SRG) is used to soften interactions for &lt;span style="font-style: italic;"&gt;ab initio&lt;/span&gt; nuclear structure calculations by decoupling low- and high-energy Hamiltonian matrix elements. The substantial contribution of both initial and SRG-induced three-nucleon forces requires their consistent evolution...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054312] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): E. D. Jurgenson, P. Maris, R. J. Furnstahl, P. Navrátil, W. E. Ormand, and J. P. Vary</p><p> The similarity renormalization group (SRG) is used to soften interactions for <span style="font-style: italic;">ab initio</span> nuclear structure calculations by decoupling low- and high-energy Hamiltonian matrix elements. The substantial contribution of both initial and SRG-induced three-nucleon forces requires their consistent evolution...</p><p>[Phys. Rev. C 87, 054312] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>Structure of p-shell nuclei using three-nucleon interactions evolved with the similarity renormalization group</dc:title>
    <dc:creator>E. D. Jurgenson, P. Maris, R. J. Furnstahl, P. Navrátil, W. E. Ormand, and J. P. Vary</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054312</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054312 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054312</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054312</prism:url>
    <prism:startingPage>054312</prism:startingPage>
    <dc:subject>Nuclear Structure</dc:subject>
    <prism:section>Nuclear Structure</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054607">
    <title>Isospin transport in ^{84}Kr+^{112,124}Sn collisions at Fermi energies</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054607</link>
    <description>Author(s): S. Barlini et al. (FAZIA Collaboration)&lt;br/&gt;&lt;p&gt;Isotopically resolved fragments with &lt;span style="font-style: italic;"&gt;Z&lt;/span&gt;≲20 have been studied with a high-resolution telescope in a test run for the FAZIA Collaboration. The fragments were produced by the collision of a &lt;sup&gt;84&lt;/sup&gt;Kr beam at 35 MeV/nucleon with a neutron-rich (&lt;sup&gt;124&lt;/sup&gt;Sn) and a neutron-poor (&lt;sup&gt;112&lt;/sup&gt;Sn) target. The fragments, detected...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054607] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): S. Barlini et al. (FAZIA Collaboration)</p><p> Isotopically resolved fragments with <span style="font-style: italic;">Z</span>≲20 have been studied with a high-resolution telescope in a test run for the FAZIA Collaboration. The fragments were produced by the collision of a <sup>84</sup>Kr beam at 35 MeV/nucleon with a neutron-rich (<sup>124</sup>Sn) and a neutron-poor (<sup>112</sup>Sn) target. The fragments, detected...</p><p>[Phys. Rev. C 87, 054607] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>Isospin transport in ^{84}Kr+^{112,124}Sn collisions at Fermi energies</dc:title>
    <dc:creator>S. Barlini et al. (FAZIA Collaboration)</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054607</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054607 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054607</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054607</prism:url>
    <prism:startingPage>054607</prism:startingPage>
    <dc:subject>Nuclear Reactions</dc:subject>
    <prism:section>Nuclear Reactions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054608">
    <title>Charmonium production in antiproton-nucleus reactions at low energies</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054608</link>
    <description>Author(s): A. B. Larionov, M. Bleicher, A. Gillitzer, and M. Strikman&lt;br/&gt;&lt;p&gt;The &lt;span style="font-style: italic;"&gt;J&lt;/span&gt;/&lt;span style="font-style: italic;"&gt;Ψ&lt;/span&gt;(1&lt;span style="font-style: italic;"&gt;S&lt;/span&gt;) and &lt;span style="font-style: italic;"&gt;Ψ&lt;/span&gt;&lt;sup&gt;′&lt;/sup&gt;(2&lt;span style="font-style: italic;"&gt;S&lt;/span&gt;) production near threshold in antiproton-nucleus reactions is calculated on the basis of the Glauber model. The model takes into account the antiproton (pre-)absorption, proton Fermi motion, and charmonium formation length. We confirm an earlier prediction that the charmonium p...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054608] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): A. B. Larionov, M. Bleicher, A. Gillitzer, and M. Strikman</p><p> The <span style="font-style: italic;">J</span>/<span style="font-style: italic;">Ψ</span>(1<span style="font-style: italic;">S</span>) and <span style="font-style: italic;">Ψ</span><sup>′</sup>(2<span style="font-style: italic;">S</span>) production near threshold in antiproton-nucleus reactions is calculated on the basis of the Glauber model. The model takes into account the antiproton (pre-)absorption, proton Fermi motion, and charmonium formation length. We confirm an earlier prediction that the charmonium p...</p><p>[Phys. Rev. C 87, 054608] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>Charmonium production in antiproton-nucleus reactions at low energies</dc:title>
    <dc:creator>A. B. Larionov, M. Bleicher, A. Gillitzer, and M. Strikman</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054608</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054608 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054608</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054608</prism:url>
    <prism:startingPage>054608</prism:startingPage>
    <dc:subject>Nuclear Reactions</dc:subject>
    <prism:section>Nuclear Reactions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.054903">
    <title>Spinodal density enhancements in simulations of relativistic nuclear collisions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.054903</link>
    <description>Author(s): Jan Steinheimer and Jørgen Randrup&lt;br/&gt;&lt;p&gt;We recently introduced a fluid-dynamical model for simulating relativistic nuclear collisions in the presence of a first-order phase transition and made explorative studies of head-on lead-lead collisions. We give here a more detailed account of this novel theoretical tool and carry out more exhaust...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 054903] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): Jan Steinheimer and Jørgen Randrup</p><p> We recently introduced a fluid-dynamical model for simulating relativistic nuclear collisions in the presence of a first-order phase transition and made explorative studies of head-on lead-lead collisions. We give here a more detailed account of this novel theoretical tool and carry out more exhaust...</p><p>[Phys. Rev. C 87, 054903] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>Spinodal density enhancements in simulations of relativistic nuclear collisions</dc:title>
    <dc:creator>Jan Steinheimer and Jørgen Randrup</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.054903</dc:identifier>
    <dc:source>Phys. Rev. C 87, 054903 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.054903</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.054903</prism:url>
    <prism:startingPage>054903</prism:startingPage>
    <dc:subject>Relativistic Nuclear Collisions</dc:subject>
    <prism:section>Relativistic Nuclear Collisions</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.055803">
    <title>Dynamics of the inner crust of neutron stars: Hydrodynamics, elasticity, and collective modes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.055803</link>
    <description>Author(s): D. Kobyakov and C. J. Pethick&lt;br/&gt;&lt;p&gt;We present calculations of the hydrodynamics of the inner crust of neutron stars, where a superfluid neutron liquid coexists with a lattice of neutron-rich nuclei. The long-wavelength collective oscillations are combinations of phonons in the lattice and phonons in the superfluid neutrons. Velocitie...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 055803] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): D. Kobyakov and C. J. Pethick</p><p> We present calculations of the hydrodynamics of the inner crust of neutron stars, where a superfluid neutron liquid coexists with a lattice of neutron-rich nuclei. The long-wavelength collective oscillations are combinations of phonons in the lattice and phonons in the superfluid neutrons. Velocitie...</p><p>[Phys. Rev. C 87, 055803] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>Dynamics of the inner crust of neutron stars: Hydrodynamics, elasticity, and collective modes</dc:title>
    <dc:creator>D. Kobyakov and C. J. Pethick</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.055803</dc:identifier>
    <dc:source>Phys. Rev. C 87, 055803 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.055803</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.055803</prism:url>
    <prism:startingPage>055803</prism:startingPage>
    <dc:subject>Nuclear Astrophysics</dc:subject>
    <prism:section>Nuclear Astrophysics</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.87.055804">
    <title>Three-body calculations of the triple-α reaction</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.87.055804</link>
    <description>Author(s): S. Ishikawa&lt;br/&gt;&lt;p&gt;Recently, the triple-&lt;span style="font-style: italic;"&gt;α&lt;/span&gt; (3&lt;span style="font-style: italic;"&gt;α&lt;/span&gt;) process, by which three &lt;sup&gt;4&lt;/sup&gt;He nuclei are fused into a &lt;sup&gt;12&lt;/sup&gt;C nucleus in stars, was studied by using different methods to solve the quantum mechanical three-body problem. The results for the thermonuclear reaction rate for the process differ by several orders at low stellar tem...&lt;/p&gt;&lt;br/&gt;[Phys. Rev. C 87, 055804] Published Mon May 13, 2013</description>
    <content:encoded><![CDATA[<p>Author(s): S. Ishikawa</p><p> Recently, the triple-<span style="font-style: italic;">α</span> (3<span style="font-style: italic;">α</span>) process, by which three <sup>4</sup>He nuclei are fused into a <sup>12</sup>C nucleus in stars, was studied by using different methods to solve the quantum mechanical three-body problem. The results for the thermonuclear reaction rate for the process differ by several orders at low stellar tem...</p><p>[Phys. Rev. C 87, 055804] Published Mon May 13, 2013</p>]]></content:encoded>
    <dc:title>Three-body calculations of the triple-α reaction</dc:title>
    <dc:creator>S. Ishikawa</dc:creator>
    <dc:date>2013-05-13T10:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>doi:10.1103/PhysRevC.87.055804</dc:identifier>
    <dc:source>Phys. Rev. C 87, 055804 (2013)</dc:source>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>87</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2013-05-13T10:00:00-04:00</prism:publicationDate>
    <prism:doi>10.1103/PhysRevC.87.055804</prism:doi>
    <prism:url>http://link.aps.org/doi/10.1103/PhysRevC.87.055804</prism:url>
    <prism:startingPage>055804</prism:startingPage>
    <dc:subject>Nuclear Astrophysics</dc:subject>
    <prism:section>Nuclear Astrophysics</prism:section>
  </item>
</rdf:RDF>
