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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>2009-11-06T22:15:12-05:00</dc:date>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.105004">
    <title>Fundamental length in quantum theories with PT-symmetric Hamiltonians. II. The case of quantum graphs</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.105004</link>
    <description>Author(s): Miloslav Znojil&lt;br/&gt;PT-symmetrization of quantum graphs is proposed as an innovation where an adjustable, tunable nonlocality is admitted. The proposal generalizes the PT-symmetric square-well models of Ref.&#160;[M. Znojil, Phys. Rev. D 80, 045022 (2009).] (with real spectrum and with a variable fundamental length &#952;) whi...&lt;br/&gt;[Phys. Rev. D 80, 105004] Published Fri Nov 06, 2009</description>
    <dc:creator>Miloslav Znojil</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.105004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 105004</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.105003">
    <title>Fermionic Casimir effect for parallel plates in the presence of compact dimensions with applications to nanotubes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.105003</link>
    <description>Author(s): S. Bellucci and A. A. Saharian&lt;br/&gt;We evaluate the Casimir energy and force for a massive fermionic field in the geometry of two parallel plates on background of Minkowski spacetime with an arbitrary number of toroidally compactified spatial dimensions. The bag boundary conditions are imposed on the plates and periodicity conditions ...&lt;br/&gt;[Phys. Rev. D 80, 105003] Published Fri Nov 06, 2009</description>
    <dc:creator>S. Bellucci and A. A. Saharian</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.105003</dc:identifier>
    <dc:source>Phys. Rev. D 80, 105003</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104007">
    <title>Interaction of the Barbero-Immirzi field with matter and pseudoscalar perturbations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104007</link>
    <description>Author(s): Simone Mercuri and Victor Taveras&lt;br/&gt;In loop quantum gravity the classical point of departure is the Einstein-Hilbert action modified by the addition of the so-called Holst term. Classically, this term does not affect the equations of motion, but it induces a well-known quantization ambiguity in the quantum theory, parametrized by the ...&lt;br/&gt;[Phys. Rev. D 80, 104007] Published Fri Nov 06, 2009</description>
    <dc:creator>Simone Mercuri and Victor Taveras</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104007</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104007</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104006">
    <title>Large-scale structure in brane-induced gravity. I. Perturbation theory</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104006</link>
    <description>Author(s): Rom&#225;n Scoccimarro&lt;br/&gt;We study the growth of subhorizon perturbations in brane-induced gravity using perturbation theory. We solve for the linear evolution of perturbations taking advantage of the symmetry under gauge transformations along the extra-dimension to decouple the bulk equations in the quasistatic approximatio...&lt;br/&gt;[Phys. Rev. D 80, 104006] Published Fri Nov 06, 2009</description>
    <dc:creator>Rom&#225;n Scoccimarro</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104006</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104006</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104005">
    <title>Large-scale structure in brane-induced gravity. II. Numerical simulations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104005</link>
    <description>Author(s): Kwan Chuen Chan and Rom&#225;n Scoccimarro&lt;br/&gt;We use N-body simulations to study the nonlinear structure formation in brane-induced gravity, developing a new method that requires alternate use of Fast Fourier Transforms and relaxation. This enables us to compute the nonlinear matter power spectrum and bispectrum, the halo mass function, and the...&lt;br/&gt;[Phys. Rev. D 80, 104005] Published Fri Nov 06, 2009</description>
    <dc:creator>Kwan Chuen Chan and Rom&#225;n Scoccimarro</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104005</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104005</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103507">
    <title>Gauge-invariant construction of quantum cosmology</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103507</link>
    <description>Author(s): Fumitoshi Amemiya and Tatsuhiko Koike&lt;br/&gt;We present and analyze a gauge-invariant quantum theory of the Friedmann-Robertson-Walker universe with dust. We construct the reduced phase space spanned by gauge-invariant quantities by using the so-called relational formalism at the classical level. The reduced phase space thereby obtained can be...&lt;br/&gt;[Phys. Rev. D 80, 103507] Published Fri Nov 06, 2009</description>
    <dc:creator>Fumitoshi Amemiya and Tatsuhiko Koike</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103507</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103507</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103506">
    <title>Incompatibility of rotation curves with gravitational lensing for TeVeS theory</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103506</link>
    <description>Author(s): Ignacio Ferreras, Nick E. Mavromatos, Mairi Sakellariadou, and Muhammad Furqaan Yusaf&lt;br/&gt;We constrain the one-parameter (&#945;) class of TeVeS models by testing the theory against both rotation curve and strong gravitational lensing data on galactic scales, remaining fully relativistic in our formalism. The upshot of our analysis is that&#8212;at least in its simplest original form, which is t...&lt;br/&gt;[Phys. Rev. D 80, 103506] Published Fri Nov 06, 2009</description>
    <dc:creator>Ignacio Ferreras, Nick E. Mavromatos, Mairi Sakellariadou, and Muhammad Furqaan Yusaf</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103506</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103506</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103004">
    <title>Present and future gamma-ray probes of the Cygnus OB2 environment</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103004</link>
    <description>Author(s): Luis A. Anchordoqui, Haim Goldberg, Russell D. Moore, Sergio Palomares-Ruiz, Diego F. Torres, and Thomas J. Weiler&lt;br/&gt;The MAGIC Collaboration has provided new observational data pertaining to the TeV J2032+4130 gamma-ray source (within the Cygnus OB2 region), for energies E_{&#947;} &gt;400&#8201;&#8201;GeV. It is then appropriate to update the impact of these data on gamma-ray production mechanisms in stellar associations. We con...&lt;br/&gt;[Phys. Rev. D 80, 103004] Published Fri Nov 06, 2009</description>
    <dc:creator>Luis A. Anchordoqui, Haim Goldberg, Russell D. Moore, Sergio Palomares-Ruiz, Diego F. Torres, and Thomas J. Weiler</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103004</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.095007">
    <title>Rapidity gap events in squark pair production at the LHC</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.095007</link>
    <description>Author(s): Sascha Bornhauser, Manuel Drees, Herbert K. Dreiner, and Jong Soo Kim&lt;br/&gt;The exchange of electroweak gauginos in the t or u channel allows squark pair production at hadron colliders without color exchange between the squarks. This can give rise to events where little or no energy is deposited in the detector between the squark decay products. We discuss the potential for...&lt;br/&gt;[Phys. Rev. D 80, 095007] Published Fri Nov 06, 2009</description>
    <dc:creator>Sascha Bornhauser, Manuel Drees, Herbert K. Dreiner, and Jong Soo Kim</dc:creator>
    <dc:date>2009-11-06T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.095007</dc:identifier>
    <dc:source>Phys. Rev. D 80, 095007</dc:source>
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    <dc:subject>D1</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.105002">
    <title>Amelioration of the little hierarchy problem in SU(4)_{c} &#215;SU(2)_{L} &#215;SU(2)_{R}</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.105002</link>
    <description>Author(s): Ilia Gogoladze, Mansoor Ur Rehman, and Qaisar Shafi&lt;br/&gt;The little hierarchy problem encountered in the constrained minimal supersymmetric model can be ameliorated in supersymmetric models based on the gauge symmetry G_{422} &#8801;SU(4)_{c} &#215;SU(2)_{L} &#215;SU(2)_{R} . The standard assumption in the constrained minimal supersymmetric model [and in SU(5) and SO...&lt;br/&gt;[Phys. Rev. D 80, 105002] Published Thu Nov 05, 2009</description>
    <dc:creator>Ilia Gogoladze, Mansoor Ur Rehman, and Qaisar Shafi</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.105002</dc:identifier>
    <dc:source>Phys. Rev. D 80, 105002</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>105002</prism:startingPage>
    <dc:subject>D15</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104004">
    <title>Smooth lattice construction of the Oppenheimer-Snyder spacetime</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104004</link>
    <description>Author(s): Leo Brewin and Jules Kajtar&lt;br/&gt;We present test results for the smooth lattice method using an Oppenheimer-Snyder spacetime. The results are in excellent agreement with theory and numerical results from other authors.&lt;br/&gt;[Phys. Rev. D 80, 104004] Published Thu Nov 05, 2009</description>
    <dc:creator>Leo Brewin and Jules Kajtar</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104004</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review D</prism:publicationName>
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    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104004</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104003">
    <title>Asymptotically free scalar curvature-ghost coupling in quantum Einstein gravity</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104003</link>
    <description>Author(s): Astrid Eichhorn, Holger Gies, and Michael M. Scherer&lt;br/&gt;We consider the asymptotic-safety scenario for quantum gravity which constructs a nonperturbatively renormalizable quantum gravity theory with the help of the functional renormalization group (RG). We verify the existence of a non-Gaussian fixed point and include a running curvature-ghost coupling a...&lt;br/&gt;[Phys. Rev. D 80, 104003] Published Thu Nov 05, 2009</description>
    <dc:creator>Astrid Eichhorn, Holger Gies, and Michael M. Scherer</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104003</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104003</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>104003</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.80.104002">
    <title>Equivalence principle implications of modified gravity models</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104002</link>
    <description>Author(s): Lam Hui, Alberto Nicolis, and Christopher W. Stubbs&lt;br/&gt;Theories that attempt to explain the observed cosmic acceleration by modifying general relativity all introduce a new scalar degree of freedom that is active on large scales, but is screened on small scales to match experiments. We demonstrate that if such screening occurs via the chameleon mechanis...&lt;br/&gt;[Phys. Rev. D 80, 104002] Published Thu Nov 05, 2009</description>
    <dc:creator>Lam Hui, Alberto Nicolis, and Christopher W. Stubbs</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104002</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104002</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104002</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103505">
    <title>Exact cosmological solutions with nonminimal derivative coupling</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103505</link>
    <description>Author(s): Sergey V. Sushkov&lt;br/&gt;We consider a gravitational theory of a scalar field &#981; with nonminimal derivative coupling to curvature. The coupling terms have the form &#954;_{1} R&#981;_{,&#956;} &#981;^{,&#956;} and &#954;_{2} R_{&#956;&#957;} &#981;^{,&#956;} &#981;^{,&#957;} , where &#954;_{1} and &#954;_{2} are coupling parameters with dimensions of length squared. In general, ...&lt;br/&gt;[Phys. Rev. D 80, 103505] Published Thu Nov 05, 2009</description>
    <dc:creator>Sergey V. Sushkov</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103505</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103505</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103505</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103504">
    <title>Inflation, baryogenesis, and gravitino dark matter at ultralow reheat temperatures</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103504</link>
    <description>Author(s): Kazunori Kohri, Anupam Mazumdar, and Narendra Sahu&lt;br/&gt;It is quite possible that the reheat temperature of the Universe is extremely low close to the scale of big bang nucleosynthesis, i.e. T_{R} &#8764;1&#8211;10&#8201;&#8201;MeV. At such low reheat temperatures generating matter, antimatter asymmetry and synthesizing dark matter particles are challenging issues which...&lt;br/&gt;[Phys. Rev. D 80, 103504] Published Thu Nov 05, 2009</description>
    <dc:creator>Kazunori Kohri, Anupam Mazumdar, and Narendra Sahu</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103504</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103504</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103504</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103503">
    <title>Archipelagian cosmology: Dynamics and observables in a universe with discretized matter content</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103503</link>
    <description>Author(s): Timothy Clifton and Pedro G. Ferreira&lt;br/&gt;We consider a model of the Universe in which the matter content is in the form of discrete islands, rather than a continuous fluid. In the appropriate limits the resulting large-scale dynamics approach those of a Friedmann-Robertson-Walker (FRW) universe. The optical properties of such a space-time,...&lt;br/&gt;[Phys. Rev. D 80, 103503] Published Thu Nov 05, 2009</description>
    <dc:creator>Timothy Clifton and Pedro G. Ferreira</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103503</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103503</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103503</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103003">
    <title>Reconstructing the neutron-star equation of state from astrophysical measurements</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103003</link>
    <description>Author(s): Feryal &#214;zel and Dimitrios Psaltis&lt;br/&gt;The properties of matter at ultrahigh densities, low temperatures, and with a significant asymmetry between protons and neutrons can be studied exclusively through astrophysical observations of neutron stars. We show that measurements of the masses and radii of neutron stars can lead to tight constr...&lt;br/&gt;[Phys. Rev. D 80, 103003] Published Thu Nov 05, 2009</description>
    <dc:creator>Feryal &#214;zel and Dimitrios Psaltis</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103003</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103003</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103003</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103002">
    <title>The G&#246;del universe: Exact geometrical optics and analytical investigations on motion</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103002</link>
    <description>Author(s): Frank Grave, Michael Buser, Thomas M&#252;ller, G&#252;nter Wunner, and Wolfgang P. Schleich&lt;br/&gt;In this work we derive the analytical solution of the geodesic equations of G&#246;del&#8217;s universe for both particles and light in a special set of coordinates, which reveals the physical properties of this spacetime in a very transparent way. We also recapitulate the equations of isometric transport f...&lt;br/&gt;[Phys. Rev. D 80, 103002] Published Thu Nov 05, 2009</description>
    <dc:creator>Frank Grave, Michael Buser, Thomas M&#252;ller, G&#252;nter Wunner, and Wolfgang P. Schleich</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103002</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103002</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103002</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.096002">
    <title>N_{f}^{3} g^{6}  term in the pressure of hot QCD</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.096002</link>
    <description>Author(s): A. Gynther, A. Kurkela, and A. Vuorinen&lt;br/&gt;We determine the first independent part of the g^{6} coefficient in the weak coupling expansion of the QCD pressure at high temperatures, the one proportional to the maximal power of the number of quark flavors N_{f} . In addition to introducing and developing computational methods that can be used ...&lt;br/&gt;[Phys. Rev. D 80, 096002] Published Thu Nov 05, 2009</description>
    <dc:creator>A. Gynther, A. Kurkela, and A. Vuorinen</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.096002</dc:identifier>
    <dc:source>Phys. Rev. D 80, 096002</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>096002</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.095006">
    <title>Protecting unparticles from the MSSM Higgs sector</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.095006</link>
    <description>Author(s): Ann E. Nelson, Maurizio Piai, and Christopher Spitzer&lt;br/&gt;We construct a model of an unparticle sector consisting of a supersymmetric SU(N) gauge theory with the number of flavors in the Seiberg conformal window. We couple this sector to the minimal supersymmetric standard model via heavy messengers. The resulting low energy theory has a Higgs coupling to ...&lt;br/&gt;[Phys. Rev. D 80, 095006] Published Thu Nov 05, 2009</description>
    <dc:creator>Ann E. Nelson, Maurizio Piai, and Christopher Spitzer</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.095006</dc:identifier>
    <dc:source>Phys. Rev. D 80, 095006</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>095006</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.095005">
    <title>Correlation between direct dark matter detection and Br(B_{s} &#8594;&#956;&#956;) with a large phase of B_{s} -B [over &#175;] _{s}  mixing</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.095005</link>
    <description>Author(s): Bhaskar Dutta, Yukihiro Mimura, and Yudi Santoso&lt;br/&gt;We combine the analyses for flavor changing neutral current processes and dark matter solutions in minimal-type supersymmetric grand unified theory models, SO(10) and SU(5), with a large B_{s} -B [over &#175;] _{s} mixing phase and large tan&#8289;&#946;. For large tan&#8289;&#946;, the double-penguin diagram dominates...&lt;br/&gt;[Phys. Rev. D 80, 095005] Published Thu Nov 05, 2009</description>
    <dc:creator>Bhaskar Dutta, Yukihiro Mimura, and Yudi Santoso</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.095005</dc:identifier>
    <dc:source>Phys. Rev. D 80, 095005</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>095005</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.095004">
    <title>Soft gluon resummation for the production of gluino-gluino and squark-antisquark pairs at the LHC</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.095004</link>
    <description>Author(s): A. Kulesza and L. Motyka&lt;br/&gt;We study the effect of soft gluon emission in the hadroproduction of gluino-gluino and squark-antisquark pairs at the next-to-leading logarithmic accuracy within the framework of the minimal supersymmetric model. We present the calculation of the one-loop soft anomalous dimension matrices controllin...&lt;br/&gt;[Phys. Rev. D 80, 095004] Published Thu Nov 05, 2009</description>
    <dc:creator>A. Kulesza and L. Motyka</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.095004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 095004</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>095004</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.094004">
    <title>Parton distribution function nuclear corrections for charged lepton and neutrino deep inelastic scattering processes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.094004</link>
    <description>Author(s): I. Schienbein, J. Y. Yu, K. Kova&#345;&#237;k, C. Keppel, J. G. Morf&#237;n, F. I. Olness, and J. F. Owens&lt;br/&gt;We perform a &#967;^{2} analysis of nuclear parton distribution functions (NPDFs) using neutral current charged-lepton (&#8467;^{&#177;} A) deeply inelastic scattering (DIS), and Drell-Yan data for several nuclear targets. The nuclear A dependence of the NPDFs is extracted in a next-to-leading order fit. We com...&lt;br/&gt;[Phys. Rev. D 80, 094004] Published Thu Nov 05, 2009</description>
    <dc:creator>I. Schienbein, J. Y. Yu, K. Kova&#345;&#237;k, C. Keppel, J. G. Morf&#237;n, F. I. Olness, and J. F. Owens</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.094004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 094004</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>094004</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.092002">
    <title>Prospects for the measurement of the unitarity triangle angle &#947; from B^{0} &#8594;DK^{+} &#960;^{-}  decays</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.092002</link>
    <description>Author(s): Tim Gershon and Mike Williams&lt;br/&gt;The potential for a precise measurement of the unitarity triangle angle &#947; in future experiments from the decay B^{0} &#8594;DK^{*0} is well known. It has recently been suggested that the sensitivity can be significantly enhanced by analyzing the B^{0} &#8594;DK^{+} &#960;^{-} Dalitz plot to extract amplitudes ...&lt;br/&gt;[Phys. Rev. D 80, 092002] Published Thu Nov 05, 2009</description>
    <dc:creator>Tim Gershon and Mike Williams</dc:creator>
    <dc:date>2009-11-05T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.092002</dc:identifier>
    <dc:source>Phys. Rev. D 80, 092002</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-05T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>092002</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104001">
    <title>Turning big bang into big bounce. I. Classical dynamics</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104001</link>
    <description>Author(s): Piotr Dzier&#380;ak, Przemys&#322;aw Ma&#322;kiewicz, and W&#322;odzimierz Piechocki&lt;br/&gt;The big bounce (BB) transition within a flat Friedmann-Robertson-Walker model is analyzed in the setting of loop geometry underlying the loop cosmology. We solve the constraint of the theory at the classical level to identify physical phase space and find the Lie algebra of the Dirac observables. We...&lt;br/&gt;[Phys. Rev. D 80, 104001] Published Wed Nov 04, 2009</description>
    <dc:creator>Piotr Dzier&#380;ak, Przemys&#322;aw Ma&#322;kiewicz, and W&#322;odzimierz Piechocki</dc:creator>
    <dc:date>2009-11-04T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104001</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104001</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-04T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104001</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103502">
    <title>Nonthermal production of WIMPs, cosmic e^{&#177;}  excesses, and &#947; rays from the Galactic Center</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103502</link>
    <description>Author(s): Xiao-Jun Bi, Robert Brandenberger, Paolo Gondolo, Tianjun Li, Qiang Yuan, and Xinmin Zhang&lt;br/&gt;In this paper we propose a dark matter model and study aspects of its phenomenology. Our model is based on a new dark matter sector with a U(1)^{&#8242;} gauge symmetry plus a discrete symmetry added to the standard model of particle physics. The new fields of the dark matter sector have no hadronic cha...&lt;br/&gt;[Phys. Rev. D 80, 103502] Published Wed Nov 04, 2009</description>
    <dc:creator>Xiao-Jun Bi, Robert Brandenberger, Paolo Gondolo, Tianjun Li, Qiang Yuan, and Xinmin Zhang</dc:creator>
    <dc:date>2009-11-04T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103502</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103502</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>10</prism:issueIdentifier>
    <prism:publicationDate>2009-11-04T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103502</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.096001">
    <title>Positivity issues for the pinch-technique gluon propagator and their resolution</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.096001</link>
    <description>Author(s): John M. Cornwall&lt;br/&gt;Although gauge-boson propagators in asymptotically-free gauge theories satisfy a dispersion relation, they do not satisfy the K&#228;llen-Lehmann (KL) representation because the spectral function changes sign. We argue that this is a simple consequence of asymptotic freedom. On the basis of the QED-like...&lt;br/&gt;[Phys. Rev. D 80, 096001] Published Wed Nov 04, 2009</description>
    <dc:creator>John M. Cornwall</dc:creator>
    <dc:date>2009-11-04T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.096001</dc:identifier>
    <dc:source>Phys. Rev. D 80, 096001</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-04T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>096001</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.094003">
    <title>Cosmic ray interaction event generator SIBYLL 2.1</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.094003</link>
    <description>Author(s): Eun-Joo Ahn, Ralph Engel, Thomas K. Gaisser, Paolo Lipari, and Todor Stanev&lt;br/&gt;The cosmic ray interaction event generator Sibyll is widely used in extensive air shower simulations. We describe in detail the properties of Sibyll&#160;2.1 and the differences with the original version 1.7. The major structural improvements are the possibility to have multiple soft interactions, intro...&lt;br/&gt;[Phys. Rev. D 80, 094003] Published Wed Nov 04, 2009</description>
    <dc:creator>Eun-Joo Ahn, Ralph Engel, Thomas K. Gaisser, Paolo Lipari, and Todor Stanev</dc:creator>
    <dc:date>2009-11-04T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.094003</dc:identifier>
    <dc:source>Phys. Rev. D 80, 094003</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-04T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>094003</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.094002">
    <title>W+3 jet production at the Tevatron</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.094002</link>
    <description>Author(s): R. Keith Ellis, Kirill Melnikov, and Giulia Zanderighi&lt;br/&gt;We compute the next-to-leading order QCD corrections to the production of W bosons in association with three jets at the Tevatron in the leading color approximation, which we define by considering the number of colors and the number of light flavors as being of the same order of magnitude. The theor...&lt;br/&gt;[Phys. Rev. D 80, 094002] Published Wed Nov 04, 2009</description>
    <dc:creator>R. Keith Ellis, Kirill Melnikov, and Giulia Zanderighi</dc:creator>
    <dc:date>2009-11-04T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.094002</dc:identifier>
    <dc:source>Phys. Rev. D 80, 094002</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-04T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>094002</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.094001">
    <title>Charm changing weak hadronic decays of triplet (C=1) baryons emitting axial-vector mesons including factorizable and pole contributions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.094001</link>
    <description>Author(s): Arvind Sharma and R. C. Verma&lt;br/&gt;We investigate the weak nonleptonic decays of &#923;_{c}^{+} , &#926;_{c}^{+} , and &#926;_{c}^{0} into the octet baryons (J^{P} =1/2^{+} ) and axial-vector mesons (J^{P} =1^{+} ) employing the factorization scheme for W-emission diagrams and the pole model for W-exchange contributions. Determining the baryon-b...&lt;br/&gt;[Phys. Rev. D 80, 094001] Published Wed Nov 04, 2009</description>
    <dc:creator>Arvind Sharma and R. C. Verma</dc:creator>
    <dc:date>2009-11-04T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.094001</dc:identifier>
    <dc:source>Phys. Rev. D 80, 094001</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>80</prism:volume>
    <prism:issueIdentifier>9</prism:issueIdentifier>
    <prism:publicationDate>2009-11-04T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>094001</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
</rdf:RDF>
