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    <title>Recent Articles in Phys. Rev. D</title>
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    <description>Recent articles in  Physical Review D</description>
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    <dc:rights>Copyright (c) 2009 The American Physical Society</dc:rights>
    <dc:date>2009-07-03T20:15:13-04:00</dc:date>
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    <title>Publisher&#8217;s Note: Trispectrum versus bispectrum in single-field inflation [Phys. Rev. D 79, 103530 (2009)]</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.029901</link>
    <description>Author(s): Kevin T. Engel, Keith S. Lee, and Mark B. Wise&lt;br/&gt;[Phys. Rev. D 80, 029901] Published Thu Jul 02, 2009</description>
    <dc:creator>Kevin T. Engel, Keith S. Lee, and Mark B. Wise</dc:creator>
    <dc:date>2009-07-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.029901</dc:identifier>
    <dc:source>Phys. Rev. D 80, 029901</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.024002">
    <title>Post-Newtonian corrections to the gravitational-wave memory for quasicircular, inspiralling compact binaries</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.024002</link>
    <description>Author(s): Marc Favata&lt;br/&gt;The Christodoulou memory is a nonlinear contribution to the gravitational-wave field that is sourced by the gravitational-wave stress-energy tensor. For quasicircular, inspiralling binaries, the Christodoulou memory produces a growing, nonoscillatory change in the gravitational-wave &#8220;plus&#8221; polar...&lt;br/&gt;[Phys. Rev. D 80, 024002] Published Thu Jul 02, 2009</description>
    <dc:creator>Marc Favata</dc:creator>
    <dc:date>2009-07-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.024002</dc:identifier>
    <dc:source>Phys. Rev. D 80, 024002</dc:source>
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    <title>Asymptotic behavior of dynamical variables and naked singularity formation in spherically symmetric gravitational collapse</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.024001</link>
    <description>Author(s): Hayato Kawakami, Eiji Mitsuda, Yasusada Nambu, and Akira Tomimatsu&lt;br/&gt;In considering the gravitational collapse of matter, it is an important problem to clarify what kind of conditions leads to the formation of naked singularity. For this purpose, we apply the 1+3 orthonormal frame formalism introduced by Uggla et&#160;al. to the spherically symmetric gravitational collap...&lt;br/&gt;[Phys. Rev. D 80, 024001] Published Thu Jul 02, 2009</description>
    <dc:creator>Hayato Kawakami, Eiji Mitsuda, Yasusada Nambu, and Akira Tomimatsu</dc:creator>
    <dc:date>2009-07-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.024001</dc:identifier>
    <dc:source>Phys. Rev. D 80, 024001</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.023502">
    <title>Negative vacuum energy densities and the causal diamond measure</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.023502</link>
    <description>Author(s): Michael P. Salem&lt;br/&gt;Arguably a major success of the landscape picture is the prediction of a small, nonzero vacuum energy density. The details of this prediction depend in part on how the diverging spacetime volume of the multiverse is regulated, a question that remains unresolved. One proposal, the causal diamond meas...&lt;br/&gt;[Phys. Rev. D 80, 023502] Published Thu Jul 02, 2009</description>
    <dc:creator>Michael P. Salem</dc:creator>
    <dc:date>2009-07-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.023502</dc:identifier>
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    <title>Cosmological BCS mechanism and the big bang singularity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.023501</link>
    <description>Author(s): Stephon Alexander and Tirthabir Biswas&lt;br/&gt;We provide a novel mechanism that resolves the big bang singularity present in Friedman-Lemaitre-Robertson-Walker space-times without the need for ghost fields. Building on the fact that a four-fermion interaction arises in general relativity when fermions are covariantly coupled, we show that at ea...&lt;br/&gt;[Phys. Rev. D 80, 023501] Published Thu Jul 02, 2009</description>
    <dc:creator>Stephon Alexander and Tirthabir Biswas</dc:creator>
    <dc:date>2009-07-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.023501</dc:identifier>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.016001">
    <title>Simple flavor protection for the Randall-Sundrum model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.016001</link>
    <description>Author(s): Csaba Cs&#225;ki, Adam Falkowski, and Andreas Weiler&lt;br/&gt;We present a simple variation of warped flavor models where the hierarchies of fermion masses and mixings are still explained but dangerous flavor-violating effects in the Kaon sector are greatly reduced. The key new ingredients are two horizontal U(1) symmetries. These symmetries forbid flavor viol...&lt;br/&gt;[Phys. Rev. D 80, 016001] Published Thu Jul 02, 2009</description>
    <dc:creator>Csaba Cs&#225;ki, Adam Falkowski, and Andreas Weiler</dc:creator>
    <dc:date>2009-07-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.016001</dc:identifier>
    <dc:source>Phys. Rev. D 80, 016001</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.013001">
    <title>kg-mass prototype demonstrator for dual gravitational wave detector: Optomechanical excitation and cooling</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.013001</link>
    <description>Author(s): M. Anderlini, F. Marino, and F. Marin&lt;br/&gt;The next generation of gravitational wave (gw) detectors is expected to fully enter into the quantum regime of force and displacement detection. With this aim, it is important to scale up the experiments on opto-mechanical effects from the microscopic regime to large mass systems and test the scheme...&lt;br/&gt;[Phys. Rev. D 80, 013001] Published Thu Jul 02, 2009</description>
    <dc:creator>M. Anderlini, F. Marino, and F. Marin</dc:creator>
    <dc:date>2009-07-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.013001</dc:identifier>
    <dc:source>Phys. Rev. D 80, 013001</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.125030">
    <title>Discrete symmetry breaking and baryon currents in U(N) and SU(N) gauge theories</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.125030</link>
    <description>Author(s): B. Lucini and A. Patella&lt;br/&gt;In SU(N) gauge theories with fermions in the fundamental or in a two-index (either symmetric or antisymmetric) representation formulated on a manifold with at least one compact dimension with nontrivial holonomy the discrete symmetries C, P, and T are broken at small enough size of the compact direc...&lt;br/&gt;[Phys. Rev. D 79, 125030] Published Tue Jun 30, 2009</description>
    <dc:creator>B. Lucini and A. Patella</dc:creator>
    <dc:date>2009-06-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.125030</dc:identifier>
    <dc:source>Phys. Rev. D 79, 125030</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:startingPage>125030</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.124048">
    <title>Relativistic static thin dust disks with an inner edge: An infinite family of new exact solutions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.124048</link>
    <description>Author(s): Guillermo A. Gonz&#225;lez, Antonio C. Guti&#233;rrez-Pi&#241;eres, and Viviana M. Vi&#241;a-Cervantes&lt;br/&gt;An infinite family of new exact solutions of the vacuum Einstein equations is presented. The solutions are static and axially symmetric and correspond to an infinite family of thin dust disks with a central inner edge. The metric functions of all the solutions can be explicitly computed, and can be ...&lt;br/&gt;[Phys. Rev. D 79, 124048] Published Tue Jun 30, 2009</description>
    <dc:creator>Guillermo A. Gonz&#225;lez, Antonio C. Guti&#233;rrez-Pi&#241;eres, and Viviana M. Vi&#241;a-Cervantes</dc:creator>
    <dc:date>2009-06-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.124048</dc:identifier>
    <dc:source>Phys. Rev. D 79, 124048</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:startingPage>124048</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.124047">
    <title>Energy-momentum diffusion from spacetime discreteness</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.124047</link>
    <description>Author(s): Lydia Philpott, Fay Dowker, and Rafael D. Sorkin&lt;br/&gt;We study potentially observable consequences of spatiotemporal discreteness for the motion of massive and massless particles. First we describe some simple models for the motion of a massive point particle in a fixed causal set background. If the causal set is faithfully embeddable in Minkoswki spac...&lt;br/&gt;[Phys. Rev. D 79, 124047] Published Tue Jun 30, 2009</description>
    <dc:creator>Lydia Philpott, Fay Dowker, and Rafael D. Sorkin</dc:creator>
    <dc:date>2009-06-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.124047</dc:identifier>
    <dc:source>Phys. Rev. D 79, 124047</dc:source>
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    <prism:startingPage>124047</prism:startingPage>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.124046">
    <title>Fate of black branes in Einstein-Gauss-Bonnet gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.124046</link>
    <description>Author(s): P. Suranyi, C. Vaz, and L. C. Wijewardhana&lt;br/&gt;Black branes are studied in Einstein-Gauss-Bonnet gravity. Evaporation drives black branes toward one of two singularities depending on the sign of &#945;, the Gauss-Bonnet coupling. For positive &#945; and sufficiently large ratio sqrt[&#945;] /L, where L/2&#960; is the radius of compactification, black branes avo...&lt;br/&gt;[Phys. Rev. D 79, 124046] Published Tue Jun 30, 2009</description>
    <dc:creator>P. Suranyi, C. Vaz, and L. C. Wijewardhana</dc:creator>
    <dc:date>2009-06-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.124046</dc:identifier>
    <dc:source>Phys. Rev. D 79, 124046</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:startingPage>124046</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.123528">
    <title>Stringy WIMP detection and annihilation</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.123528</link>
    <description>Author(s): James A. Maxin, Van E. Mayes, and Dimitri V. Nanopoulos&lt;br/&gt;We calculate the direct dark matter detection spin-independent and proton spin-dependent cross sections for a semirealistic intersecting D6-brane model. The cross sections are compared to the latest constraints of the current dark matter direct detection experiments, as well as the projected results...&lt;br/&gt;[Phys. Rev. D 79, 123528] Published Tue Jun 30, 2009</description>
    <dc:creator>James A. Maxin, Van E. Mayes, and Dimitri V. Nanopoulos</dc:creator>
    <dc:date>2009-06-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.123528</dc:identifier>
    <dc:source>Phys. Rev. D 79, 123528</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:startingPage>123528</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.115024">
    <title>Electroweak phase transition, critical bubbles, and sphaleron decoupling condition in the MSSM</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.115024</link>
    <description>Author(s): Koichi Funakubo and Eibun Senaha&lt;br/&gt;The electroweak phase transition and the sphaleron decoupling condition in the minimal supersymmetric standard model are revisited taking the latest experimental data into account. The light Higgs boson scenario and the ordinary decoupling limit, which are classified by the relative size between the...&lt;br/&gt;[Phys. Rev. D 79, 115024] Published Tue Jun 30, 2009</description>
    <dc:creator>Koichi Funakubo and Eibun Senaha</dc:creator>
    <dc:date>2009-06-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.115024</dc:identifier>
    <dc:source>Phys. Rev. D 79, 115024</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2009-06-30T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>115024</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.125029">
    <title>Dirac quantization condition for monopole in noncommutative space-time</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.125029</link>
    <description>Author(s): Masud Chaichian, Subir Ghosh, Miklos L&#229;ngvik, and Anca Tureanu&lt;br/&gt;Since the structure of space-time at very short distances is believed to get modified possibly due to noncommutativity effects and as the Dirac quantization condition, &#956;e=N/2&#8463;c, probes the magnetic field point singularity, a natural question arises whether the same condition will still survive. W...&lt;br/&gt;[Phys. Rev. D 79, 125029] Published Mon Jun 29, 2009</description>
    <dc:creator>Masud Chaichian, Subir Ghosh, Miklos L&#229;ngvik, and Anca Tureanu</dc:creator>
    <dc:date>2009-06-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.125029</dc:identifier>
    <dc:source>Phys. Rev. D 79, 125029</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>125029</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.124045">
    <title>Mass inflation in Brans-Dicke gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.124045</link>
    <description>Author(s): P. P. Avelino, A. J. Hamilton, and C. A. Herdeiro&lt;br/&gt;A detailed nonlinear analysis of the internal structure of spherical, charged black holes that are accreting scalar matter is performed in the framework of the Brans-Dicke theory of gravity. We choose the lowest value of the Brans-Dicke parameter that is compatible with observational constraints. Fi...&lt;br/&gt;[Phys. Rev. D 79, 124045] Published Mon Jun 29, 2009</description>
    <dc:creator>P. P. Avelino, A. J. Hamilton, and C. A. Herdeiro</dc:creator>
    <dc:date>2009-06-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.124045</dc:identifier>
    <dc:source>Phys. Rev. D 79, 124045</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>124045</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.124044">
    <title>Pad&#233; approximants of the Green function in spherically symmetric spacetimes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.124044</link>
    <description>Author(s): Marc Casals, Sam Dolan, Adrian C. Ottewill, and Barry Wardell&lt;br/&gt;We investigate the scalar Green function for spherically symmetric spacetimes expressed as a coordinate series expansion in the separation of the points. We calculate the series expansion of the function V(x,x^{&#8242;} ) appearing in the Hadamard parametrix of the scalar Green function to very high ord...&lt;br/&gt;[Phys. Rev. D 79, 124044] Published Mon Jun 29, 2009</description>
    <dc:creator>Marc Casals, Sam Dolan, Adrian C. Ottewill, and Barry Wardell</dc:creator>
    <dc:date>2009-06-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.124044</dc:identifier>
    <dc:source>Phys. Rev. D 79, 124044</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>124044</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.124043">
    <title>Self-force calculations with matched expansions and quasinormal mode sums</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.124043</link>
    <description>Author(s): Marc Casals, Sam Dolan, Adrian C. Ottewill, and Barry Wardell&lt;br/&gt;Accurate modeling of gravitational wave emission by extreme-mass ratio inspirals is essential for their detection by the LISA mission. A leading perturbative approach involves the calculation of the self-force acting upon the smaller orbital body. In this work, we present the first application of th...&lt;br/&gt;[Phys. Rev. D 79, 124043] Published Mon Jun 29, 2009</description>
    <dc:creator>Marc Casals, Sam Dolan, Adrian C. Ottewill, and Barry Wardell</dc:creator>
    <dc:date>2009-06-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.124043</dc:identifier>
    <dc:source>Phys. Rev. D 79, 124043</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>124043</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.123527">
    <title>Consistent cosmological modifications to the Einstein equations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.123527</link>
    <description>Author(s): Constantinos Skordis&lt;br/&gt;General relativity is a phenomenologically successful theory that rests on firm foundations, but has not been tested on cosmological scales. The deep mystery of dark energy (and possibly even the requirement of cold dark matter), has increased the need for testing modifications to general relativity...&lt;br/&gt;[Phys. Rev. D 79, 123527] Published Mon Jun 29, 2009</description>
    <dc:creator>Constantinos Skordis</dc:creator>
    <dc:date>2009-06-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.123527</dc:identifier>
    <dc:source>Phys. Rev. D 79, 123527</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>123527</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.119903">
    <title>Publisher&#8217;s Note: Spin content of &#923; in QCD sum rules [Phys. Rev. D 79, 114028 (2009)]</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.119903</link>
    <description>Author(s): G&#252;ray Erkol and Makoto Oka&lt;br/&gt;[Phys. Rev. D 79, 119903] Published Mon Jun 29, 2009</description>
    <dc:creator>G&#252;ray Erkol and Makoto Oka</dc:creator>
    <dc:date>2009-06-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.119903</dc:identifier>
    <dc:source>Phys. Rev. D 79, 119903</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2009-06-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>119903</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.114505">
    <title>Nucleon form factors with 2+1 flavor dynamical domain-wall fermions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.114505</link>
    <description>Author(s): Takeshi Yamazaki, Yasumichi Aoki, Tom Blum, Huey-Wen Lin, Shigemi Ohta, Shoichi Sasaki, Robert Tweedie, and James Zanotti RBC and UKQCD Collaborations&lt;br/&gt;We report our numerical lattice QCD calculations of the isovector nucleon form factors for the vector and axial-vector currents: the vector, induced tensor, axial-vector, and induced pseudoscalar form factors. The calculation is carried out with the gauge configurations generated with N_{f} =2+1 dyn...&lt;br/&gt;[Phys. Rev. D 79, 114505] Published Mon Jun 29, 2009</description>
    <dc:creator>Takeshi Yamazaki, Yasumichi Aoki, Tom Blum, Huey-Wen Lin, Shigemi Ohta, Shoichi Sasaki, Robert Tweedie, and James Zanotti RBC and UKQCD Collaborations</dc:creator>
    <dc:date>2009-06-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.114505</dc:identifier>
    <dc:source>Phys. Rev. D 79, 114505</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2009-06-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>114505</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.114034">
    <title>Possible J^{PC} =0^{--}  exotic state</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.114034</link>
    <description>Author(s): Chun-Kun Jiao, Wei Chen, Hua-Xing Chen, and Shi-Lin Zhu&lt;br/&gt;In order to explore the possible existence of the exotic 0^{--} state, we have constructed the tetraquark interpolating operators systematically. As a byproduct, we notice the 0^{+-} tetraquark operators without derivatives do not exist. The special Lorentz structure of the 0^{--} currents forbids t...&lt;br/&gt;[Phys. Rev. D 79, 114034] Published Mon Jun 29, 2009</description>
    <dc:creator>Chun-Kun Jiao, Wei Chen, Hua-Xing Chen, and Shi-Lin Zhu</dc:creator>
    <dc:date>2009-06-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.114034</dc:identifier>
    <dc:source>Phys. Rev. D 79, 114034</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2009-06-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>114034</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.113015">
    <title>Oscillations of Dirac and Majorana neutrinos in matter and a magnetic field</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.113015</link>
    <description>Author(s): Maxim Dvornikov and Jukka Maalampi&lt;br/&gt;We study the evolution of massive mixed Dirac and Majorana neutrinos in matter under the influence of a transversal magnetic field. The analysis is based on relativistic quantum mechanics. We solve exactly the evolution equation for relativistic neutrinos, find the neutrino wave functions, and calcu...&lt;br/&gt;[Phys. Rev. D 79, 113015] Published Mon Jun 29, 2009</description>
    <dc:creator>Maxim Dvornikov and Jukka Maalampi</dc:creator>
    <dc:date>2009-06-29T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.113015</dc:identifier>
    <dc:source>Phys. Rev. D 79, 113015</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>11</prism:issueIdentifier>
    <prism:publicationDate>2009-06-29T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>113015</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.128301">
    <title>Comment on &#8220;Modeling galaxy halos using dark matter with pressure&#8221;</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.128301</link>
    <description>Author(s): Kung-Yi Su and Pisin Chen&lt;br/&gt;We comment on the calculational mistake in the paper &#8220;Modeling galaxy halos using dark matter with pressure&#8221; by Somnath Bharadwaj and Sayan Kar. The authors made a mistake while calculating the metric, which led to an overestimate of the deflection angle of light passing through the halos for -1&lt;w_{r} &lt;-0.5 and an underestimate of the deflection angle for -0.5&lt;w_{r} &lt;0. In addition, the solution for w_{r} &gt;...&lt;br/&gt;[Phys. Rev. D 79, 128301] Published Fri Jun 26, 2009</description>
    <dc:creator>Kung-Yi Su and Pisin Chen</dc:creator>
    <dc:date>2009-06-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.128301</dc:identifier>
    <dc:source>Phys. Rev. D 79, 128301</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>128301</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.125028">
    <title>One-loop self-energies in the electroweak model with a nonlinearly realized gauge group</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.125028</link>
    <description>Author(s): D. Bettinelli, R. Ferrari, and A. Quadri&lt;br/&gt;We evaluate at one loop the self-energies for the W, Z mesons in the electroweak model where the gauge group is nonlinearly realized. In this model the Higgs boson parameters are absent, while a second mass parameter appears together with a scale for the radiative corrections. We estimate these para...&lt;br/&gt;[Phys. Rev. D 79, 125028] Published Fri Jun 26, 2009</description>
    <dc:creator>D. Bettinelli, R. Ferrari, and A. Quadri</dc:creator>
    <dc:date>2009-06-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.125028</dc:identifier>
    <dc:source>Phys. Rev. D 79, 125028</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>125028</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.125027">
    <title>Unwinding in Hopfion vortex bunches</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.125027</link>
    <description>Author(s): Juha J&#228;ykk&#228; and Jarmo Hietarinta&lt;br/&gt;We investigate the behavior of parallel Faddeev-Hopf vortices under energy minimization in a system with physically relevant, but unusual boundary conditions. The homotopy classification is no longer provided by the Hopf invariant, but rather by the set of integer homotopy invariants proposed by Pon...&lt;br/&gt;[Phys. Rev. D 79, 125027] Published Fri Jun 26, 2009</description>
    <dc:creator>Juha J&#228;ykk&#228; and Jarmo Hietarinta</dc:creator>
    <dc:date>2009-06-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.125027</dc:identifier>
    <dc:source>Phys. Rev. D 79, 125027</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>125027</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.124042">
    <title>More on massive 3D gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.124042</link>
    <description>Author(s): Eric A. Bergshoeff, Olaf Hohm, and Paul K. Townsend&lt;br/&gt;We explore the space of static solutions of the recently discovered three-dimensional &#8220;new massive gravity&#8221; (NMG), allowing for either sign of the Einstein-Hilbert term and a cosmological term parametrized by a dimensionless constant &#955;. For &#955;=-1 we find black hole solutions asymptotic (but not...&lt;br/&gt;[Phys. Rev. D 79, 124042] Published Fri Jun 26, 2009</description>
    <dc:creator>Eric A. Bergshoeff, Olaf Hohm, and Paul K. Townsend</dc:creator>
    <dc:date>2009-06-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.124042</dc:identifier>
    <dc:source>Phys. Rev. D 79, 124042</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>124042</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.124041">
    <title>Even the Minkowski space is holed</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.124041</link>
    <description>Author(s): S. Krasnikov&lt;br/&gt;To cure the lack of predictive power of general relativity, Geroch proposed to complete the theory with an additional postulate that only &#8220;hole-free&#8221; spacetimes are permitted. This postulate (or, rather, that obtained from it by some disambiguating) seems physically well-founded and at the same ...&lt;br/&gt;[Phys. Rev. D 79, 124041] Published Fri Jun 26, 2009</description>
    <dc:creator>S. Krasnikov</dc:creator>
    <dc:date>2009-06-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.124041</dc:identifier>
    <dc:source>Phys. Rev. D 79, 124041</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>124041</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.123526">
    <title>Spikes in the mixmaster regime of G_{2}  cosmologies</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.123526</link>
    <description>Author(s): Woei Chet Lim, Lars Andersson, David Garfinkle, and Frans Pretorius&lt;br/&gt;We produce numerical evidence that spikes in the mixmaster regime of G_{2} cosmologies are transient and recurring, supporting the conjecture that the generalized mixmaster behavior is asymptotically nonlocal where spikes occur. Higher-order spike transitions are observed to split into separate firs...&lt;br/&gt;[Phys. Rev. D 79, 123526] Published Fri Jun 26, 2009</description>
    <dc:creator>Woei Chet Lim, Lars Andersson, David Garfinkle, and Frans Pretorius</dc:creator>
    <dc:date>2009-06-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.123526</dc:identifier>
    <dc:source>Phys. Rev. D 79, 123526</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>123526</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.123525">
    <title>Charged seven-dimensional spacetimes with spherically symmetric extra dimensions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.123525</link>
    <description>Author(s): Antonio De Felice and Christophe Ringeval&lt;br/&gt;We derive exact solutions of the seven-dimensional Einstein-Maxwell equations for a spacetime exhibiting Poincar&#233; invariance along four dimensions and spherical symmetry in the extra dimensions. Such topology generically arises in the context of braneworld models. Our solutions generalize previous ...&lt;br/&gt;[Phys. Rev. D 79, 123525] Published Fri Jun 26, 2009</description>
    <dc:creator>Antonio De Felice and Christophe Ringeval</dc:creator>
    <dc:date>2009-06-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.123525</dc:identifier>
    <dc:source>Phys. Rev. D 79, 123525</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>123525</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.79.123524">
    <title>Complementarity in the multiverse</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.79.123524</link>
    <description>Author(s): Raphael Bousso&lt;br/&gt;In the multiverse, as in AdS space, light cones relate bulk points to boundary scales. This holographic UV-IR connection defines a preferred global time cutoff that regulates the divergences of eternal inflation. An entirely different cutoff, the causal patch, arises in the holographic description o...&lt;br/&gt;[Phys. Rev. D 79, 123524] Published Fri Jun 26, 2009</description>
    <dc:creator>Raphael Bousso</dc:creator>
    <dc:date>2009-06-26T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.79.123524</dc:identifier>
    <dc:source>Phys. Rev. D 79, 123524</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>79</prism:volume>
    <prism:issueIdentifier>12</prism:issueIdentifier>
    <prism:publicationDate>2009-06-26T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>123524</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
</rdf:RDF>
