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    <title>Spin response of a normal Fermi liquid with noncentral interactions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.055805</link>
    <description>Author(s): C. J. Pethick and A. Schwenk&lt;br/&gt;We consider the spin response of a normal Fermi liquid with noncentral interactions under conditions intermediate between the collisionless and hydrodynamic regimes. This problem is of importance for calculations of neutrino properties in dense matter. By expressing the deviation of the quasiparticl...&lt;br/&gt;[Phys. Rev. C 80, 055805] Published Fri Nov 20, 2009</description>
    <dc:creator>C. J. Pethick and A. Schwenk</dc:creator>
    <dc:date>2009-11-20T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.055805</dc:identifier>
    <dc:source>Phys. Rev. C 80, 055805</dc:source>
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    <prism:publicationDate>2009-11-20T00:00:00-05:00</prism:publicationDate>
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    <dc:subject>Nuclear Astrophysics</dc:subject>
    <prism:section>Nuclear Astrophysics</prism:section>
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    <title>High-precision (p,t) reaction measurement to determine  ^{18} Ne(&#945;,p) ^{21} Na reaction rates</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.055804</link>
    <description>Author(s): A. Matic et al.&lt;br/&gt;x-ray bursts are identified as thermonuclear explosions in the outer atmosphere of accreting neutron stars. The thermonuclear runaway is fueled by the &#945;p process that describes a sequence of (&#945;,p) reactions triggered by the ^{18} Ne(&#945;,p) ^{21} Na breakout reaction from the hot CNO cycles. We stud...&lt;br/&gt;[Phys. Rev. C 80, 055804] Published Mon Nov 16, 2009</description>
    <dc:creator>A. Matic et al.</dc:creator>
    <dc:date>2009-11-16T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.055804</dc:identifier>
    <dc:source>Phys. Rev. C 80, 055804</dc:source>
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    <prism:publicationDate>2009-11-16T00:00:00-05:00</prism:publicationDate>
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    <title>Photoexcitation of astrophysically important states in  ^{26} Mg</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.055803</link>
    <description>Author(s): R. Longland, C. Iliadis, G. Rusev, A. P. Tonchev, R. J. deBoer, J. G&#246;rres, and M. Wiescher&lt;br/&gt;We performed a nuclear resonance fluorescence experiment to determine the energy and quantum numbers of excited states in ^{26} Mg. Spin-parity ambiguities of excited states in ^{26} Mg, the compound nucleus for the s-process neutron source ^{22} Ne(&#945;,n) ^{25} Mg, result in large uncertainties in t...&lt;br/&gt;[Phys. Rev. C 80, 055803] Published Mon Nov 16, 2009</description>
    <dc:creator>R. Longland, C. Iliadis, G. Rusev, A. P. Tonchev, R. J. deBoer, J. G&#246;rres, and M. Wiescher</dc:creator>
    <dc:date>2009-11-16T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.055803</dc:identifier>
    <dc:source>Phys. Rev. C 80, 055803</dc:source>
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    <title>&#947;-ray spectroscopy study of states in  ^{27} Si relevant for the  ^{26} Al^{m} (p,&#947;) ^{27} Si reaction in novae and supernovae</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.055802</link>
    <description>Author(s): G. Lotay, P. J. Woods, D. Seweryniak, M. P. Carpenter, R. V. F. Janssens, and S. Zhu&lt;br/&gt;The heavy-ion, fusion-evaporation reaction ^{12} C( ^{16} O,n) was used to identify &#947;-decay transitions from excited states in ^{27} Si above the proton threshold. The precise level energy measurements, J^{&#960;} assignments, and lifetime measurements of astrophysically important ^{26} Al^{m} +p reson...&lt;br/&gt;[Phys. Rev. C 80, 055802] Published Fri Nov 13, 2009</description>
    <dc:creator>G. Lotay, P. J. Woods, D. Seweryniak, M. P. Carpenter, R. V. F. Janssens, and S. Zhu</dc:creator>
    <dc:date>2009-11-13T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.055802</dc:identifier>
    <dc:source>Phys. Rev. C 80, 055802</dc:source>
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    <prism:publicationName>Physical Review C</prism:publicationName>
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    <prism:publicationDate>2009-11-13T00:00:00-05:00</prism:publicationDate>
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    <title>Calculation of stellar electron-capture cross sections on nuclei based on microscopic Skyrme functionals</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.055801</link>
    <description>Author(s): N. Paar, G. Col&#242;, E. Khan, and D. Vretenar&lt;br/&gt;A fully self-consistent microscopic framework for the evaluation of nuclear weak-interaction rates at finite temperature is introduced, based on Skyrme functionals. The single-nucleon basis and the corresponding thermal occupation factors of the initial nuclear state are determined in the finite-tem...&lt;br/&gt;[Phys. Rev. C 80, 055801] Published Wed Nov 11, 2009</description>
    <dc:creator>N. Paar, G. Col&#242;, E. Khan, and D. Vretenar</dc:creator>
    <dc:date>2009-11-11T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.055801</dc:identifier>
    <dc:source>Phys. Rev. C 80, 055801</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review C</prism:publicationName>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.80.045809" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Calibration of a liquid xenon detector with  ^{83} Kr^{m}</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.045809</link>
    <description>Author(s): L. W. Kastens, S. B. Cahn, A. Manzur, and D. N. McKinsey&lt;br/&gt;We report the preparation of a ^{83} Kr^{m} source and its use in calibrating a liquid xenon detector. ^{83} Kr^{m} atoms were produced through the decay of ^{83} Rb and introduced into liquid xenon. Decaying ^{83} Kr^{m} nuclei were detected through liquid xenon scintillation. Conversion electrons ...&lt;br/&gt;[Phys. Rev. C 80, 045809] Published Fri Oct 30, 2009</description>
    <dc:creator>L. W. Kastens, S. B. Cahn, A. Manzur, and D. N. McKinsey</dc:creator>
    <dc:date>2009-10-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.045809</dc:identifier>
    <dc:source>Phys. Rev. C 80, 045809</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
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    <prism:publicationDate>2009-10-30T00:00:00-04:00</prism:publicationDate>
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    <dc:subject>Nuclear Astrophysics</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.80.045808" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Dynamical instabilities of warm npe matter: &#948; meson effects</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.045808</link>
    <description>Author(s): Helena Pais, Alexandre Santos, and Constan&#231;a Provid&#234;ncia&lt;br/&gt;The effects of &#948; mesons on the dynamical instabilities of cold and warm nuclear and stellar matter at subsaturation densities are studied in the framework of relativistic mean-field hadron models (NL3, NL&#961;, and NL&#961;&#948;) with the inclusion of the electromagnetic field. The distillation effect and th...&lt;br/&gt;[Phys. Rev. C 80, 045808] Published Thu Oct 29, 2009</description>
    <dc:creator>Helena Pais, Alexandre Santos, and Constan&#231;a Provid&#234;ncia</dc:creator>
    <dc:date>2009-10-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.045808</dc:identifier>
    <dc:source>Phys. Rev. C 80, 045808</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
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    <prism:publicationDate>2009-10-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>045808</prism:startingPage>
    <dc:subject>Nuclear Astrophysics</dc:subject>
    <prism:section>Nuclear Astrophysics</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.80.042801" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Measurement of the inelastic branch of the  ^{14} O(&#945;,p) ^{17} F reaction: Implications for explosive burning in novae and x-ray bursters</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.042801</link>
    <description>Author(s): J. J. He, P. J. Woods, T. Davinson, M. Aliotta, J. B&#252;scher, E. Clement, P. Delahaye, M. Hass, D. G. Jenkins, V. Kumar, A. St. J. Murphy, P. Neyskens, R. Raabe, A. P. Robinson, D. Voulot, J. van der Walle, N. Warr, and F. Wenander&lt;br/&gt;A measurement of the inelastic component of the key astrophysical resonance in the ^{14} O(&#945;,p) ^{17} F reaction for burning and breakout from hot carbon-nitrogen-oxygen (CNO) cycles is reported. The inelastic component is found to be comparable to the ground-state branch and will enhance the ^{14}...&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt;&lt;br/&gt;[Phys. Rev. C 80, 042801] Published Tue Oct 27, 2009</description>
    <dc:creator>J. J. He, P. J. Woods, T. Davinson, M. Aliotta, J. B&#252;scher, E. Clement, P. Delahaye, M. Hass, D. G. Jenkins, V. Kumar, A. St. J. Murphy, P. Neyskens, R. Raabe, A. P. Robinson, D. Voulot, J. van der Walle, N. Warr, and F. Wenander</dc:creator>
    <dc:date>2009-10-27T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.042801</dc:identifier>
    <dc:source>Phys. Rev. C 80, 042801</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review C</prism:publicationName>
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    <prism:publicationDate>2009-10-27T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>042801</prism:startingPage>
    <dc:subject>Nuclear Astrophysics</dc:subject>
    <prism:section>Nuclear Astrophysics</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevC.80.045807" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>High precision  ^{89} Y(&#945;,&#945;) ^{89} Y scattering at low energies</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.045807</link>
    <description>Author(s): G. G. Kiss, P. Mohr, Zs. F&#252;l&#246;p, D. Galaviz, Gy. Gy&#252;rky, Z. Elekes, E. Somorjai, A. Kretschmer, K. Sonnabend, A. Zilges, and M. Avrigeanu&lt;br/&gt;Elastic scattering cross sections of the ^{89} Y(&#945;,&#945;) ^{89} Y reaction have been measured at energies E_{c.m.} =15.51 and 18.63&#160;MeV. The high-precision data for the semimagic N=50 nucleus ^{89} Y are used to derive a local potential and to evaluate the predictions of global and regional &#945;-nucleu...&lt;br/&gt;[Phys. Rev. C 80, 045807] Published Fri Oct 23, 2009</description>
    <dc:creator>G. G. Kiss, P. Mohr, Zs. F&#252;l&#246;p, D. Galaviz, Gy. Gy&#252;rky, Z. Elekes, E. Somorjai, A. Kretschmer, K. Sonnabend, A. Zilges, and M. Avrigeanu</dc:creator>
    <dc:date>2009-10-23T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.045807</dc:identifier>
    <dc:source>Phys. Rev. C 80, 045807</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>4</prism:issueIdentifier>
    <prism:publicationDate>2009-10-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>045807</prism:startingPage>
    <dc:subject>Nuclear Astrophysics</dc:subject>
    <prism:section>Nuclear Astrophysics</prism:section>
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    <title>Density dependence of the nuclear symmetry energy: A microscopic perspective</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.045806</link>
    <description>Author(s): Isaac Vida&#241;a, Constan&#231;a Provid&#234;ncia, Artur Polls, and Arnau Rios&lt;br/&gt;We perform a systematic analysis of the density dependence of nuclear symmetry energy within the microscopic Brueckner-Hartree-Fock (BHF) approach using the realistic Argonne V18 nucleon-nucleon potential plus a phenomenological three-body force of Urbana type. Our results are compared thoroughly wi...&lt;br/&gt;[Phys. Rev. C 80, 045806] Published Fri Oct 23, 2009</description>
    <dc:creator>Isaac Vida&#241;a, Constan&#231;a Provid&#234;ncia, Artur Polls, and Arnau Rios</dc:creator>
    <dc:date>2009-10-23T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.045806</dc:identifier>
    <dc:source>Phys. Rev. C 80, 045806</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationDate>2009-10-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>045806</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.80.045805" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>^{14} C(&#945;,&#947;) reaction rate</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.045805</link>
    <description>Author(s): E. D. Johnson, G. V. Rogachev, J. Mitchell, L. Miller, and K. W. Kemper&lt;br/&gt;The ^{14} C(&#945;,&#947;) reaction rate at temperatures below 0.3&#160;GK depends on the properties of two near threshold resonances in ^{18} O, the 1^{-} at 6.198&#160;MeV and the 3^{-} at 6.404&#160;MeV. The &#945;+ ^{14} C asymptotic normalization coefficients for these resonances were determined using the &#945;-transfer ...&lt;br/&gt;[Phys. Rev. C 80, 045805] Published Thu Oct 22, 2009</description>
    <dc:creator>E. D. Johnson, G. V. Rogachev, J. Mitchell, L. Miller, and K. W. Kemper</dc:creator>
    <dc:date>2009-10-22T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.045805</dc:identifier>
    <dc:source>Phys. Rev. C 80, 045805</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>4</prism:issueIdentifier>
    <prism:publicationDate>2009-10-22T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>045805</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.80.045804" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Response of spin polarized neutron matter under the presence of a strong magnetic field with Skyrme interactions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.045804</link>
    <description>Author(s): M. &#193;ngeles P&#233;rez-Garc&#237;a&lt;br/&gt;The effects of a strong magnetic field in the dynamical response of a pure neutron system to a weak neutrino probe are studied within the framework of the Landau Fermi liquid theory in the nonrelativistic Hartree-Fock approximation at zero temperature. We use Skyrme forces to parametrize the partial...&lt;br/&gt;[Phys. Rev. C 80, 045804] Published Wed Oct 21, 2009</description>
    <dc:creator>M. &#193;ngeles P&#233;rez-Garc&#237;a</dc:creator>
    <dc:date>2009-10-21T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.045804</dc:identifier>
    <dc:source>Phys. Rev. C 80, 045804</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>4</prism:issueIdentifier>
    <prism:publicationDate>2009-10-21T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>045804</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.80.045803" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>&#946;-delayed &#945; decay of  ^{16} N</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.045803</link>
    <description>Author(s): L. Buchmann, G. Ruprecht, and C. Ruiz&lt;br/&gt;The &#946;-delayed &#945; decay of ^{16} N has been used to restrict the E1 fraction of the ground state &#947; transition in the astrophysically important ^{12} C(&#945;,&#947;) ^{16} O reaction in several experiments. A review of the published measurements is given, and GEANT4 simulations and R-matrix calculations ar...&lt;br/&gt;[Phys. Rev. C 80, 045803] Published Wed Oct 21, 2009</description>
    <dc:creator>L. Buchmann, G. Ruprecht, and C. Ruiz</dc:creator>
    <dc:date>2009-10-21T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.045803</dc:identifier>
    <dc:source>Phys. Rev. C 80, 045803</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>4</prism:issueIdentifier>
    <prism:publicationDate>2009-10-21T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>045803</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.80.045802" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Equation of state of low-density neutron matter, and the ^{1} S_{0}  pairing gap</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.045802</link>
    <description>Author(s): S. Gandolfi, A. Yu. Illarionov, F. Pederiva, K. E. Schmidt, and S. Fantoni&lt;br/&gt;We report results of the equation of state of neutron matter in the low-density regime, where the Fermi wave vector ranges from 0.4&#10877;k_{F} &#10877;1.0&#8194;fm^{-1} . Neutron matter in this regime is superfluid because of the strong and attractive interaction in the ^{1} S_{0} channel. The properties of thi...&lt;br/&gt;[Phys. Rev. C 80, 045802] Published Fri Oct 16, 2009</description>
    <dc:creator>S. Gandolfi, A. Yu. Illarionov, F. Pederiva, K. E. Schmidt, and S. Fantoni</dc:creator>
    <dc:date>2009-10-16T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.045802</dc:identifier>
    <dc:source>Phys. Rev. C 80, 045802</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>4</prism:issueIdentifier>
    <prism:publicationDate>2009-10-16T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>045802</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.80.045801" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Nuclear statistical equilibrium neutrino spectrum</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.045801</link>
    <description>Author(s): Andrzej Odrzywolek&lt;br/&gt;The spectral emission of neutrinos from a plasma in nuclear statistical equilibrium (NSE) is investigated. Particular attention is paid to the possible emission of high-energy (&gt;10 MeV) neutrinos or antineutrinos. A newly developed numerical approach for describing the abundances of nuclei in NSE is ...&lt;br/&gt;[Phys. Rev. C 80, 045801] Published Fri Oct 09, 2009</description>
    <dc:creator>Andrzej Odrzywolek</dc:creator>
    <dc:date>2009-10-09T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.045801</dc:identifier>
    <dc:source>Phys. Rev. C 80, 045801</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>4</prism:issueIdentifier>
    <prism:publicationDate>2009-10-09T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>045801</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.80.035806" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Toward an experimentally determined  ^{26} Al^{m} (p,&#947;) ^{27} Si reaction rate in ONe novae</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.035806</link>
    <description>Author(s): C. M. Deibel, J. A. Clark, R. Lewis, A. Parikh, P. D. Parker, and C. Wrede&lt;br/&gt;Strong evidence of the nucleosynthesis of Galactic ^{26} Al has been found through measurements involving excesses in ^{26} Mg from the decay of ^{26} Al in meteoritic inclusions and the 1.809-MeV &#947;-ray line detected by satellites such as CGRO and INTEGRAL. Several sites for the production of ^{26}...&lt;br/&gt;[Phys. Rev. C 80, 035806] Published Tue Sep 29, 2009</description>
    <dc:creator>C. M. Deibel, J. A. Clark, R. Lewis, A. Parikh, P. D. Parker, and C. Wrede</dc:creator>
    <dc:date>2009-09-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.035806</dc:identifier>
    <dc:source>Phys. Rev. C 80, 035806</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>3</prism:issueIdentifier>
    <prism:publicationDate>2009-09-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>035806</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.80.035805" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Penning trap mass measurements of  ^{99-109} Cd with the ISOLTRAP mass spectrometer, and implications for the rp process</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.035805</link>
    <description>Author(s): M. Breitenfeldt, G. Audi, D. Beck, K. Blaum, S. George, F. Herfurth, A. Herlert, A. Kellerbauer, H. -J. Kluge, M. Kowalska, D. Lunney, S. Naimi, D. Neidherr, H. Schatz, S. Schwarz, and L. Schweikhard&lt;br/&gt;Penning trap mass measurements of neutron-deficient Cd isotopes ^{99-109} Cd have been performed with the ISOLTRAP mass spectrometer at ISOLDE/CERN, all with relative mass uncertainties below 3&#183;10^{-8} . A new mass evaluation has been performed. The mass of ^{99} Cd has been determined for the firs...&lt;br/&gt;[Phys. Rev. C 80, 035805] Published Wed Sep 23, 2009</description>
    <dc:creator>M. Breitenfeldt, G. Audi, D. Beck, K. Blaum, S. George, F. Herfurth, A. Herlert, A. Kellerbauer, H. -J. Kluge, M. Kowalska, D. Lunney, S. Naimi, D. Neidherr, H. Schatz, S. Schwarz, and L. Schweikhard</dc:creator>
    <dc:date>2009-09-23T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.035805</dc:identifier>
    <dc:source>Phys. Rev. C 80, 035805</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>3</prism:issueIdentifier>
    <prism:publicationDate>2009-09-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>035805</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.80.032802" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Chiral effective field theory calculations of neutrino processes in dense matter</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.032802</link>
    <description>Author(s): S. Bacca, K. Hally, C. J. Pethick, and A. Schwenk&lt;br/&gt;We calculate neutrino processes involving two nucleons at subnuclear densities using chiral effective field theory. Shorter range noncentral forces reduce the neutrino rates significantly compared with the one-pion exchange approximation currently used in supernova simulations. For densities &#961;&lt;10^{14} &#8194;g&#8194;cm^{-3} , we find that neutrino rates are well constrained by nuclear interactions and nucleon-nucleon scattering data. As an application, we calculate the mean-square energy transfer in scattering of a neutrino from nucleons and find that collision processes and spin-dependent mean-field effects dominate over the energy transfer due to nucleon recoil.&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt;&lt;br/&gt;[Phys. Rev. C 80, 032802] Published Wed Sep 23, 2009</description>
    <dc:creator>S. Bacca, K. Hally, C. J. Pethick, and A. Schwenk</dc:creator>
    <dc:date>2009-09-23T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.032802</dc:identifier>
    <dc:source>Phys. Rev. C 80, 032802</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>3</prism:issueIdentifier>
    <prism:publicationDate>2009-09-23T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>032802</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.80.038801" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Analysis of  ^{25} Al energy levels observed in the  ^{28} Si(p,&#945;) ^{25} Al reaction</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.038801</link>
    <description>Author(s): S. T. Pittman, D. W. Bardayan, J. C. Blackmon, R. L. Kozub, and M. S. Smith&lt;br/&gt;The level structure of ^{25} Al has been studied at the ORNL Holifield Radioactive Ion Beam Facility by measuring the angular and energy distributions of &#945; particles from the ^{28} Si(p,&#945;) ^{25} Al reaction. Proton beams (~10&#8194;nA) at laboratory energies of 40 and 42 MeV were generated by the 25 M...&lt;br/&gt;[Phys. Rev. C 80, 038801] Published Thu Sep 17, 2009</description>
    <dc:creator>S. T. Pittman, D. W. Bardayan, J. C. Blackmon, R. L. Kozub, and M. S. Smith</dc:creator>
    <dc:date>2009-09-17T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.038801</dc:identifier>
    <dc:source>Phys. Rev. C 80, 038801</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>3</prism:issueIdentifier>
    <prism:publicationDate>2009-09-17T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>038801</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.80.035804" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Measurements of proton-induced reaction cross sections on  ^{120} Te for the astrophysical p process</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.035804</link>
    <description>Author(s): R. T. G&#252;ray, N. &#214;zkan, C. Yal&#231;&#305;n, A. Palumbo, R. deBoer, J. G&#246;rres, P. J. Leblanc, S. O'Brien, E. Strandberg, W. P. Tan, M. Wiescher, Zs. F&#252;l&#246;p, E. Somorjai, H. Y. Lee, and J. P. Greene&lt;br/&gt;The total cross sections for the ^{120} Te(p,&#947;) ^{121} I and ^{120} Te(p,n) ^{120} I reactions have been measured by the activation method in the effective center-of-mass energies 2.47&#160;MeV&#8194;&#10877;&#8194;E_{c.m.}^{eff} &#8194;&#10877;&#8194;7.93&#160;MeV and 6.44&#8194;MeV&#8194;&#10877;&#8194;E_{c.m.}^{eff} &#8194;&#10877;&#8194;7.93&#8194;MeV, respecti...&lt;br/&gt;[Phys. Rev. C 80, 035804] Published Tue Sep 15, 2009</description>
    <dc:creator>R. T. G&#252;ray, N. &#214;zkan, C. Yal&#231;&#305;n, A. Palumbo, R. deBoer, J. G&#246;rres, P. J. Leblanc, S. O'Brien, E. Strandberg, W. P. Tan, M. Wiescher, Zs. F&#252;l&#246;p, E. Somorjai, H. Y. Lee, and J. P. Greene</dc:creator>
    <dc:date>2009-09-15T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.035804</dc:identifier>
    <dc:source>Phys. Rev. C 80, 035804</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>3</prism:issueIdentifier>
    <prism:publicationDate>2009-09-15T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>035804</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.80.032801" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Chiral asymmetry of the Fermi surface in dense relativistic matter in a magnetic field</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.032801</link>
    <description>Author(s): E. V. Gorbar, V. A. Miransky, and I. A. Shovkovy&lt;br/&gt;It is revealed that in the normal phase of dense relativistic matter in a magnetic field, there exists a contribution to the axial current associated with a relative shift of the longitudinal momenta in the dispersion relations of opposite chirality fermions. Unlike the topological contribution in t...&lt;br/&gt;&lt;img src="http://prola.aps.org/graphics/rapid30x30.gif" width="30" height="30" alt="Rapid Communication"/&gt;&lt;br/&gt;[Phys. Rev. C 80, 032801] Published Tue Sep 15, 2009</description>
    <dc:creator>E. V. Gorbar, V. A. Miransky, and I. A. Shovkovy</dc:creator>
    <dc:date>2009-09-15T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.032801</dc:identifier>
    <dc:source>Phys. Rev. C 80, 032801</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>3</prism:issueIdentifier>
    <prism:publicationDate>2009-09-15T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>032801</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.80.035803" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Symmetry coefficients and incompressibility of clusterized supernova matter</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.035803</link>
    <description>Author(s): S. K. Samaddar, J. N. De, X. Vi&#241;as, and M. Centelles&lt;br/&gt;The symmetry energy coefficients, incompressibility, and single-particle and isovector potentials of clusterized dilute nuclear matter are calculated at different temperatures employing the S-matrix approach to the evaluation of the equation of state. Calculations have been extended to understand th...&lt;br/&gt;[Phys. Rev. C 80, 035803] Published Mon Sep 14, 2009</description>
    <dc:creator>S. K. Samaddar, J. N. De, X. Vi&#241;as, and M. Centelles</dc:creator>
    <dc:date>2009-09-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.035803</dc:identifier>
    <dc:source>Phys. Rev. C 80, 035803</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>3</prism:issueIdentifier>
    <prism:publicationDate>2009-09-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>035803</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.80.035802" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Neutrino deuteron reaction in the heating mechanism of core-collapse supernovae</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.035802</link>
    <description>Author(s): S. X. Nakamura, K. Sumiyoshi, and T. Sato&lt;br/&gt;We examine a potential role of the neutrino deuteron reactions in the mechanism of supernovae explosion by evaluating the energy transfer cross section for the neutrino heating. We calculate the energy loss rate due to the neutrino absorptions through the charged-current process as well as the neutr...&lt;br/&gt;[Phys. Rev. C 80, 035802] Published Tue Sep 08, 2009</description>
    <dc:creator>S. X. Nakamura, K. Sumiyoshi, and T. Sato</dc:creator>
    <dc:date>2009-09-08T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.035802</dc:identifier>
    <dc:source>Phys. Rev. C 80, 035802</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>3</prism:issueIdentifier>
    <prism:publicationDate>2009-09-08T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>035802</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.80.035801" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Suppression of the stellar enhancement factor and the reaction  ^{85} Rb(p,n) ^{85} Sr</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.035801</link>
    <description>Author(s): T. Rauscher, G. G. Kiss, Gy. Gy&#252;rky, A. Simon, Zs. F&#252;l&#246;p, and E. Somorjai&lt;br/&gt;It is shown that a Coulomb suppression of the stellar enhancement factor occurs in many endothermic reactions at and far from stability. Contrary to common assumptions, reaction measurements for astrophysics with minimal impact of stellar enhancement should be preferably performed for those reaction...&lt;br/&gt;[Phys. Rev. C 80, 035801] Published Thu Sep 03, 2009</description>
    <dc:creator>T. Rauscher, G. G. Kiss, Gy. Gy&#252;rky, A. Simon, Zs. F&#252;l&#246;p, and E. Somorjai</dc:creator>
    <dc:date>2009-09-03T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.035801</dc:identifier>
    <dc:source>Phys. Rev. C 80, 035801</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>3</prism:issueIdentifier>
    <prism:publicationDate>2009-09-03T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>035801</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.80.025807" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Effects of distortion of the intercluster motion in  ^{2} H,  ^{3} He,  ^{3} H,  ^{6} Li, and  ^{9} Be on Trojan horse applications</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.025807</link>
    <description>Author(s): R. G. Pizzone, C. Spitaleri, A. M. Mukhamedzhanov, L. D. Blokhintsev, C. A. Bertulani, B. F. Irgaziev, M. La Cognata, L. Lamia, and S. Romano&lt;br/&gt;Deuteron induced quasifree scattering and reactions have been extensively investigated in the past few decades as well as ^{6} Li, ^{3} H, ^{3} He, and ^{9} Be induced reactions. This was done not only for the investigation of nuclear structure and reaction mechanisms but also for important astrophy...&lt;br/&gt;[Phys. Rev. C 80, 025807] Published Mon Aug 31, 2009</description>
    <dc:creator>R. G. Pizzone, C. Spitaleri, A. M. Mukhamedzhanov, L. D. Blokhintsev, C. A. Bertulani, B. F. Irgaziev, M. La Cognata, L. Lamia, and S. Romano</dc:creator>
    <dc:date>2009-08-31T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.025807</dc:identifier>
    <dc:source>Phys. Rev. C 80, 025807</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>2</prism:issueIdentifier>
    <prism:publicationDate>2009-08-31T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>025807</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.80.025806" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Effect of the &#948; meson on the instabilities of nuclear matter under strong magnetic fields</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.025806</link>
    <description>Author(s): A. Rabhi, C. Provid&#234;ncia, and J. Da Provid&#234;ncia&lt;br/&gt;We study the influence of the isovector-scalar meson on the spinodal instabilities and the distillation effect in asymmetric nonhomogenous nuclear matter under strong magnetic fields of the order of 10^{18} -10^{19} G. Relativistic nuclear models both with constant couplings (NLW) and with density-d...&lt;br/&gt;[Phys. Rev. C 80, 025806] Published Mon Aug 31, 2009</description>
    <dc:creator>A. Rabhi, C. Provid&#234;ncia, and J. Da Provid&#234;ncia</dc:creator>
    <dc:date>2009-08-31T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.025806</dc:identifier>
    <dc:source>Phys. Rev. C 80, 025806</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>2</prism:issueIdentifier>
    <prism:publicationDate>2009-08-31T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>025806</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.80.025805" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Cross-section measurement of the  ^{18} F(&#945;,p) ^{21} Ne reaction and possible implication for neutron production in explosive helium burning</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.025805</link>
    <description>Author(s): H. Y. Lee, M. Couder, A. Couture, S. Falahat, J. G&#246;rres, L. Lamm, P. J. LeBlanc, S. O'Brien, A. Palumbo, E. Stech, E. Strandberg, W. Tan, C. Ugalde, and M. Wiescher&lt;br/&gt;At the high temperature and density conditions of hot or explosive helium burning, the ^{18} F(&#945;,p) ^{21} Ne reaction may compete successfully with the ^{18} F(&#946;^{+} &#957;) decay. This suggests ^{21} Ne(&#945;,n) as an alternative neutron source in the r-process. We have determined the total cross sectio...&lt;br/&gt;[Phys. Rev. C 80, 025805] Published Tue Aug 25, 2009</description>
    <dc:creator>H. Y. Lee, M. Couder, A. Couture, S. Falahat, J. G&#246;rres, L. Lamm, P. J. LeBlanc, S. O'Brien, A. Palumbo, E. Stech, E. Strandberg, W. Tan, C. Ugalde, and M. Wiescher</dc:creator>
    <dc:date>2009-08-25T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.025805</dc:identifier>
    <dc:source>Phys. Rev. C 80, 025805</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>2</prism:issueIdentifier>
    <prism:publicationDate>2009-08-25T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>025805</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.80.025804" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Neutron capture cross sections of  ^{184} W and  ^{186} W</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.025804</link>
    <description>Author(s): J. Marganiec, I. Dillmann, C. Domingo Pardo, and F. K&#228;ppeler&lt;br/&gt;The neutron capture cross sections of ^{184} W and ^{186} W have been determined by means of the activation technique. The measurements were carried out at the Karlsruhe 3.75-MV Van de Graaff accelerator using the ^{7} Li(p,n) ^{7} Be reaction for neutron production. Samples of natural composition w...&lt;br/&gt;[Phys. Rev. C 80, 025804] Published Mon Aug 24, 2009</description>
    <dc:creator>J. Marganiec, I. Dillmann, C. Domingo Pardo, and F. K&#228;ppeler</dc:creator>
    <dc:date>2009-08-24T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.025804</dc:identifier>
    <dc:source>Phys. Rev. C 80, 025804</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>2</prism:issueIdentifier>
    <prism:publicationDate>2009-08-24T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>025804</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.80.025803" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Thermodynamic properties of nuclear matter with three-body forces</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.025803</link>
    <description>Author(s): V. Som&#224; and P. Bo&#380;ek&lt;br/&gt;We calculate thermodynamic quantities in symmetric nuclear matter within the self-consistent Green's functions method including three-body forces. The thermodynamic potential is computed directly from a diagrammatic expansion, implemented with the CD-Bonn and Nijmegen nucleon-nucleon potentials and ...&lt;br/&gt;[Phys. Rev. C 80, 025803] Published Thu Aug 13, 2009</description>
    <dc:creator>V. Som&#224; and P. Bo&#380;ek</dc:creator>
    <dc:date>2009-08-13T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.025803</dc:identifier>
    <dc:source>Phys. Rev. C 80, 025803</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>2</prism:issueIdentifier>
    <prism:publicationDate>2009-08-13T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>025803</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.80.025802" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:prism="http://prismstandard.org/namespaces/1.2/basic/" xmlns:dc="http://purl.org/dc/elements/1.1/">
    <title>Neutron Fermi liquids under the presence of a strong magnetic field with effective nuclear forces</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevC.80.025802</link>
    <description>Author(s): M. &#193;ngeles P&#233;rez-Garc&#237;a, J. Navarro, and A. Polls&lt;br/&gt;Landau's Fermi liquid parameters are calculated for non-superfluid pure neutron matter in the presence of a strong magnetic field at zero temperature. The particle-hole interactions in the system, where a net magnetization may be present, are characterized by these parameters in the framework of a m...&lt;br/&gt;[Phys. Rev. C 80, 025802] Published Wed Aug 12, 2009</description>
    <dc:creator>M. &#193;ngeles P&#233;rez-Garc&#237;a, J. Navarro, and A. Polls</dc:creator>
    <dc:date>2009-08-12T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevC.80.025802</dc:identifier>
    <dc:source>Phys. Rev. C 80, 025802</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review C</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>2</prism:issueIdentifier>
    <prism:publicationDate>2009-08-12T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>025802</prism:startingPage>
    <dc:subject>Nuclear Astrophysics</dc:subject>
    <prism:section>Nuclear Astrophysics</prism:section>
  </item>
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