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    <title>Recent Articles in Phys. Rev. D</title>
    <link>http://prd.aps.org/</link>
    <description>Recent articles in  Physical Review D</description>
    <dc:language>en-us</dc:language>
    <dc:rights>Copyright (c) 2009 The American Physical Society</dc:rights>
    <dc:date>2009-11-20T22:15:16-05:00</dc:date>
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    <title>Exact null tachyons from renormalization group flows</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.106005</link>
    <description>Author(s): Allan Adams, Albion Lawrence, and Ian Swanson&lt;br/&gt;We construct exact two-dimensional conformal field theories, corresponding to closed string tachyon and metric profiles invariant under shifts in a null coordinate, which can be constructed from any two-dimensional renormalization group flow. These solutions satisfy first order equations of motion i...&lt;br/&gt;[Phys. Rev. D 80, 106005] Published Fri Nov 20, 2009</description>
    <dc:creator>Allan Adams, Albion Lawrence, and Ian Swanson</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/PhysRevD.80.106005</dc:identifier>
    <dc:source>Phys. Rev. D 80, 106005</dc:source>
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    <title>Supersymmetry preserving mass deformation of N=1 super Yang-Mills theory in D=2+1 dimensions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.105020</link>
    <description>Author(s): Abhishek Agarwal&lt;br/&gt;We construct a massive non-Abelian N=1 supersymmetric Yang-Mills theory on R^{3} . This is achieved by using a nonlocal gauge and a Poincare invariant mass term for gluons due to Nair. The underlying supersymmetry algebra is shown to be a noncentral extension of the Poincare algebra by the spacetime...&lt;br/&gt;[Phys. Rev. D 80, 105020] Published Fri Nov 20, 2009</description>
    <dc:creator>Abhishek Agarwal</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/PhysRevD.80.105020</dc:identifier>
    <dc:source>Phys. Rev. D 80, 105020</dc:source>
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    <title>Noether symmetry approach in phantom quintessence cosmology</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104030</link>
    <description>Author(s): S. Capozziello, E. Piedipalumbo, C. Rubano, and P. Scudellaro&lt;br/&gt;In the framework of phantom quintessence cosmology, we use the Noether Symmetry Approach to obtain general exact solutions for the cosmological equations. This result is achieved by the quintessential (phantom) potential determined by the existence of the symmetry itself. A comparison between the th...&lt;br/&gt;[Phys. Rev. D 80, 104030] Published Fri Nov 20, 2009</description>
    <dc:creator>S. Capozziello, E. Piedipalumbo, C. Rubano, and P. Scudellaro</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/PhysRevD.80.104030</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104030</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104029">
    <title>Lifshitz black hole in three dimensions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104029</link>
    <description>Author(s): Eloy Ay&#243;n-Beato, Alan Garbarz, Gaston Giribet, and Mokhtar Hassa&#239;ne&lt;br/&gt;We show that three-dimensional massive gravity admits Lifshitz metrics with generic values of the dynamical exponent z as exact solutions. At the point z=3, exact black hole solutions that are asymptotically Lifshitz arise. These spacetimes are three-dimensional analogues of those that were recently...&lt;br/&gt;[Phys. Rev. D 80, 104029] Published Fri Nov 20, 2009</description>
    <dc:creator>Eloy Ay&#243;n-Beato, Alan Garbarz, Gaston Giribet, and Mokhtar Hassa&#239;ne</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/PhysRevD.80.104029</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104029</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103518">
    <title>Cosmology with unparticles</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103518</link>
    <description>Author(s): Bohdan Grzadkowski and Jos&#233; Wudka&lt;br/&gt;We discuss cosmological consequences of the existence of physics beyond the standard model that exhibits Banks-Zaks and unparticle behavior in the UV and IR, respectively. We first derive the equation of state for unparticles and use it to obtain the temperature dependence of the corresponding energ...&lt;br/&gt;[Phys. Rev. D 80, 103518] Published Fri Nov 20, 2009</description>
    <dc:creator>Bohdan Grzadkowski and Jos&#233; Wudka</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/PhysRevD.80.103518</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103518</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.096006">
    <title>On a CP anisotropy measurement in the Dalitz plot</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.096006</link>
    <description>Author(s): I. Bediaga, I. I. Bigi, A. Gomes, G. Guerrer, J. Miranda, and A. C. dos Reis&lt;br/&gt;We describe a novel use of the Dalitz plot to probe CP symmetry in three-body modes of B and D mesons. It is based on an observable inspired by astronomers&#8217; practice, namely the significance in the difference between corresponding Dalitz plot bins. It provides a model-independent mapping of local ...&lt;br/&gt;[Phys. Rev. D 80, 096006] Published Fri Nov 20, 2009</description>
    <dc:creator>I. Bediaga, I. I. Bigi, A. Gomes, G. Guerrer, J. Miranda, and A. C. dos Reis</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/PhysRevD.80.096006</dc:identifier>
    <dc:source>Phys. Rev. D 80, 096006</dc:source>
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    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.094015">
    <title>CP violation in B_{q}  decays and final state strong phases</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.094015</link>
    <description>Author(s): Fayyazuddin&lt;br/&gt;Using the unitarity, SU(2) and C invariance of hadronic interactions, the bounds on final state phases are derived. It is shown that values obtained for the final state phases relevant for the direct CP asymmetries A_{CP} (B^{0} &#8594;K^{+} &#960;^{-} ,K^{0} &#960;^{0} ) are compatible with experimental values...&lt;br/&gt;[Phys. Rev. D 80, 094015] Published Fri Nov 20, 2009</description>
    <dc:creator>Fayyazuddin</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/PhysRevD.80.094015</dc:identifier>
    <dc:source>Phys. Rev. D 80, 094015</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
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    <prism:issueIdentifier>9</prism:issueIdentifier>
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    <prism:startingPage>094015</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.094014">
    <title>Baryon magnetic moments in large-N_{c}  chiral perturbation theory</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.094014</link>
    <description>Author(s): Rub&#233;n Flores-Mendieta&lt;br/&gt;The baryon magnetic and transition magnetic moments are computed in heavy baryon chiral perturbation theory in the large-N_{c} limit, where N_{c} is the number of colors. One-loop nonanalytic corrections of orders m_{q}^{1/2} and m_{q} ln&#8289;m_{q} are incorporated into the analysis, where contributio...&lt;br/&gt;[Phys. Rev. D 80, 094014] Published Fri Nov 20, 2009</description>
    <dc:creator>Rub&#233;n Flores-Mendieta</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/PhysRevD.80.094014</dc:identifier>
    <dc:source>Phys. Rev. D 80, 094014</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>094014</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.093004">
    <title>One vanishing minor in the neutrino mass matrix</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.093004</link>
    <description>Author(s): E. I. Lashin and N. Chamoun&lt;br/&gt;We study a specific texture of the neutrino mass matrix, namely the models with one 2&#215;2 subdeterminant equal to zero. We carry out a complete phenomenological analysis with all possible relevant correlations. Every pattern of the six possible ones is found able to accommodate the experimental data,...&lt;br/&gt;[Phys. Rev. D 80, 093004] Published Fri Nov 20, 2009</description>
    <dc:creator>E. I. Lashin and N. Chamoun</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/PhysRevD.80.093004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 093004</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>093004</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.092007">
    <title>Observation and polarization measurement of B^{0} &#8594;a_{1} (1260)^{+} a_{1} (1260)^{-}  decay</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.092007</link>
    <description>Author(s): B. Aubert et al.&lt;br/&gt;We present measurements of the branching fraction B and longitudinal polarization fraction f_{L} for B^{0} &#8594;a_{1} (1260)^{+} a_{1} (1260)^{-} decays, with a_{1} (1260)^{&#177;} &#8594;&#960;^{-} &#960;^{+} &#960;^{&#177;} . The data sample, collected with the BABAR detector at the SLAC National Accelerator Laboratory, re...&lt;br/&gt;[Phys. Rev. D 80, 092007] Published Fri Nov 20, 2009</description>
    <dc:creator>B. Aubert et al.</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/PhysRevD.80.092007</dc:identifier>
    <dc:source>Phys. Rev. D 80, 092007</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
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    <dc:subject>D1</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.092006">
    <title>Measurement of the top quark mass in final states with two leptons</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.092006</link>
    <description>Author(s): V. M. Abazov et al.&lt;br/&gt;We present measurements of the top quark mass (m_{t} ) in tt [over &#175;] candidate events with two final state leptons using 1&#8201;&#8201;fb^{-1} of data collected by the D0 experiment. Our data sample is selected by requiring two fully identified leptons or by relaxing one lepton requirement to an isolated...&lt;br/&gt;[Phys. Rev. D 80, 092006] Published Fri Nov 20, 2009</description>
    <dc:creator>V. M. Abazov et al.</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/PhysRevD.80.092006</dc:identifier>
    <dc:source>Phys. Rev. D 80, 092006</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>092006</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.092005">
    <title>Measurements of the &#964; mass and the mass difference of the &#964;^{+}  and &#964;^{-}  at BABAR</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.092005</link>
    <description>Author(s): B. Aubert et al.&lt;br/&gt;We present the result from a precision measurement of the mass of the &#964; lepton, M_{&#964;} , based on 423&#8201;&#8201;fb^{-1} of data recorded at the &#933;(4S) resonance with the BABAR detector. Using a pseudomass endpoint method, we determine the mass to be 1776.68&#177;0.12(stat)&#177;0.41(syst)&#8201;&#8201;MeV. We also meas...&lt;br/&gt;[Phys. Rev. D 80, 092005] Published Fri Nov 20, 2009</description>
    <dc:creator>B. Aubert et al.</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/PhysRevD.80.092005</dc:identifier>
    <dc:source>Phys. Rev. D 80, 092005</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>092005</prism:startingPage>
    <dc:subject>D1</dc:subject>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104028">
    <title>Spin-spin interaction in the spin-precession equations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104028</link>
    <description>Author(s): J&#225;nos Maj&#225;r&lt;br/&gt;One of the most active field of research in general relativity is the description of the spin properties of astrophysical objects. The main tool in the description of the gravitational waves emitted by compact binary systems in the inspiral era is the post-Newtonian (PN) approximation, where spin ef...&lt;br/&gt;[Phys. Rev. D 80, 104028] Published Thu Nov 19, 2009</description>
    <dc:creator>J&#225;nos Maj&#225;r</dc:creator>
    <dc:date>2009-11-19T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104028</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104028</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>2009-11-19T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104028</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103517">
    <title>Impact of a strongly first-order phase transition on the abundance of thermal relics</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103517</link>
    <description>Author(s): Carroll Wainwright and Stefano Profumo&lt;br/&gt;We study the impact of a strongly first-order electroweak phase transition on the thermal relic abundance of particle species that could constitute the dark matter and that decoupled before the phase transition occurred. We define a dilution factor induced by generic first-order phase transitions, a...&lt;br/&gt;[Phys. Rev. D 80, 103517] Published Thu Nov 19, 2009</description>
    <dc:creator>Carroll Wainwright and Stefano Profumo</dc:creator>
    <dc:date>2009-11-19T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103517</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103517</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>2009-11-19T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103517</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103516">
    <title>CMB lensing constraints on dark energy and modified gravity scenarios</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103516</link>
    <description>Author(s): Erminia Calabrese, Asantha Cooray, Matteo Martinelli, Alessandro Melchiorri, Luca Pagano, An&#382;e Slosar, and George F. Smoot&lt;br/&gt;Weak gravitational lensing leaves a characteristic imprint on the cosmic microwave background temperature and polarization angular power spectra. Here, we investigate the possible constraints on the integrated lensing potential from future cosmic microwave background angular spectra measurements exp...&lt;br/&gt;[Phys. Rev. D 80, 103516] Published Thu Nov 19, 2009</description>
    <dc:creator>Erminia Calabrese, Asantha Cooray, Matteo Martinelli, Alessandro Melchiorri, Luca Pagano, An&#382;e Slosar, and George F. Smoot</dc:creator>
    <dc:date>2009-11-19T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103516</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103516</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>2009-11-19T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103516</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.096005">
    <title>S_{4}  as a natural flavor symmetry for lepton mixing</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.096005</link>
    <description>Author(s): Federica Bazzocchi and Stefano Morisi&lt;br/&gt;Group theoretical arguments seem to indicate the discrete symmetry S_{4} as the minimal flavor symmetry compatible with tribimaximal neutrino mixing. We prove in a model-independent way that indeed S_{4} can realize exact tribimaximal mixing through different symmetry breaking patterns. We present t...&lt;br/&gt;[Phys. Rev. D 80, 096005] Published Thu Nov 19, 2009</description>
    <dc:creator>Federica Bazzocchi and Stefano Morisi</dc:creator>
    <dc:date>2009-11-19T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.096005</dc:identifier>
    <dc:source>Phys. Rev. D 80, 096005</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>2009-11-19T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>096005</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.094013">
    <title>Factorization structure of gauge theory amplitudes and application to hard scattering processes at the LHC</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.094013</link>
    <description>Author(s): Jui-yu Chiu, Andreas Fuhrer, Randall Kelley, and Aneesh V. Manohar&lt;br/&gt;Previous work on electroweak radiative corrections to high-energy scattering using soft-collinear effective theory (SCET) has been extended to include external transverse and longitudinal gauge bosons and Higgs bosons. This allows one to compute radiative corrections to all parton-level hard scatter...&lt;br/&gt;[Phys. Rev. D 80, 094013] Published Thu Nov 19, 2009</description>
    <dc:creator>Jui-yu Chiu, Andreas Fuhrer, Randall Kelley, and Aneesh V. Manohar</dc:creator>
    <dc:date>2009-11-19T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.094013</dc:identifier>
    <dc:source>Phys. Rev. D 80, 094013</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>2009-11-19T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>094013</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.091702">
    <title>Yukawa alignment in the two-Higgs-doublet model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.091702</link>
    <description>Author(s): Antonio Pich and Paula Tuz&#243;n&lt;br/&gt;In multi-Higgs-doublet models the alignment in flavor space of the relevant Yukawa matrices guarantees the absence of tree-level flavor-changing couplings of the neutral scalar fields. We analyze the consequences of this condition within the two-Higgs-doublet model and show that it leads to a generi...&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. D 80, 091702] Published Thu Nov 19, 2009</description>
    <dc:creator>Antonio Pich and Paula Tuz&#243;n</dc:creator>
    <dc:date>2009-11-19T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.091702</dc:identifier>
    <dc:source>Phys. Rev. D 80, 091702</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>2009-11-19T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>091702</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104027">
    <title>Quantization of higher spin fields</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104027</link>
    <description>Author(s): J. W. Wagenaar and T. A. Rijken&lt;br/&gt;In this article we quantize (massive) higher spin (1&#8804;j&#8804;2) fields by means of Dirac&#8217;s constrained Hamilton procedure both in the situation were they are totally free and were they are coupled to (an) auxiliary field(s). A full constraint analysis and quantization is presented by determining and...&lt;br/&gt;[Phys. Rev. D 80, 104027] Published Wed Nov 18, 2009</description>
    <dc:creator>J. W. Wagenaar and T. A. Rijken</dc:creator>
    <dc:date>2009-11-18T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104027</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104027</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>2009-11-18T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104027</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.105019">
    <title>Quantum corrections to the Larmor radiation formula in scalar electrodynamics</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.105019</link>
    <description>Author(s): A. Higuchi and P. J. Walker&lt;br/&gt;We use the semiclassical approximation in perturbative scalar quantum electrodynamics to calculate the quantum correction to the Larmor radiation formula to first order in Planck&#8217;s constant in the nonrelativistic approximation, choosing the initial state of the charged particle to be a momentum ei...&lt;br/&gt;[Phys. Rev. D 80, 105019] Published Tue Nov 17, 2009</description>
    <dc:creator>A. Higuchi and P. J. Walker</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.105019</dc:identifier>
    <dc:source>Phys. Rev. D 80, 105019</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>105019</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.105018">
    <title>Asymptotically free four-Fermi theory in 4 dimensions at the z=3 Lifshitz-like fixed point</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.105018</link>
    <description>Author(s): Avinash Dhar, Gautam Mandal, and Spenta R. Wadia&lt;br/&gt;We show that a Nambu-Jona-Lasinio type four-fermion coupling at the z=3 Lifshitz-like fixed point in 3+1 dimensions is asymptotically free and generates a mass scale dynamically. This result is nonperturbative in the limit of a large number of fermion species. The theory is ultraviolet complete and ...&lt;br/&gt;[Phys. Rev. D 80, 105018] Published Tue Nov 17, 2009</description>
    <dc:creator>Avinash Dhar, Gautam Mandal, and Spenta R. Wadia</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.105018</dc:identifier>
    <dc:source>Phys. Rev. D 80, 105018</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>105018</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104026">
    <title>Electromagnetic absorption cross section of Reissner-Nordstr&#246;m black holes revisited</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104026</link>
    <description>Author(s): Lu&#237;s C. B. Crispino, Atsushi Higuchi, and Ednilton S. Oliveira&lt;br/&gt;The absorption cross section of Reissner-Nordstr&#246;m black holes for the electromagnetic field is computed numerically for arbitrary frequencies, taking into account the coupling of the electromagnetic and gravitational perturbations. We also compute the conversion coefficients of electromagnetic to ...&lt;br/&gt;[Phys. Rev. D 80, 104026] Published Tue Nov 17, 2009</description>
    <dc:creator>Lu&#237;s C. B. Crispino, Atsushi Higuchi, and Ednilton S. Oliveira</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104026</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104026</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104026</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104025">
    <title>Hamiltonian of a spinning test particle in curved spacetime</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104025</link>
    <description>Author(s): Enrico Barausse, Etienne Racine, and Alessandra Buonanno&lt;br/&gt;Using a Legendre transformation, we compute the unconstrained Hamiltonian of a spinning test particle in a curved spacetime at linear order in the particle spin. The equations of motion of this unconstrained Hamiltonian coincide with the Mathisson-Papapetrou-Pirani equations. We then use the formali...&lt;br/&gt;[Phys. Rev. D 80, 104025] Published Tue Nov 17, 2009</description>
    <dc:creator>Enrico Barausse, Etienne Racine, and Alessandra Buonanno</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104025</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104025</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104025</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104024">
    <title>Emergence of scalar matter from spin foam model</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104024</link>
    <description>Author(s): Peng Xu and Yongge Ma&lt;br/&gt;A spin foam model of three dimensional gravity nonminimally coupled with a scalar field is studied. By discretization of the scalar field, the model is worked out precisely in a purely combinational way. It is shown that the quantum physics of the scalar matter is totally encoded into the modified d...&lt;br/&gt;[Phys. Rev. D 80, 104024] Published Tue Nov 17, 2009</description>
    <dc:creator>Peng Xu and Yongge Ma</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104024</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104024</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104024</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.104023">
    <title>Accretion process onto super-spinning objects</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.104023</link>
    <description>Author(s): Cosimo Bambi, Katherine Freese, Tomohiro Harada, Rohta Takahashi, and Naoki Yoshida&lt;br/&gt;The accretion process onto spinning objects in Kerr spacetimes is studied with numerical simulations. Our results show that accretion onto compact objects with Kerr parameter (characterizing the spin) |a|&lt;M and |a|&gt;M is very different. In the superspinning case, for |a| moderately larger than M, the accretion ...&lt;br/&gt;[Phys. Rev. D 80, 104023] Published Tue Nov 17, 2009</description>
    <dc:creator>Cosimo Bambi, Katherine Freese, Tomohiro Harada, Rohta Takahashi, and Naoki Yoshida</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.104023</dc:identifier>
    <dc:source>Phys. Rev. D 80, 104023</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>104023</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.103515">
    <title>Holes in the static Einstein universe and a model of the cosmological voids</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.103515</link>
    <description>Author(s): Andrzej Odrzywo&#322;ek&lt;br/&gt;A spherically symmetric, static model of the cosmological voids is constructed in the framework of the Tolman-Oppenheimer-Volkov equation with the cosmological constant. Extension of the Tooper result (dimensionless form of the TOV equation) is provided for nonzero &#923;. Then, the equation is simplifi...&lt;br/&gt;[Phys. Rev. D 80, 103515] Published Tue Nov 17, 2009</description>
    <dc:creator>Andrzej Odrzywo&#322;ek</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.103515</dc:identifier>
    <dc:source>Phys. Rev. D 80, 103515</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>103515</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.102004">
    <title>Bayesian reconstruction of gravitational wave burst signals from simulations of rotating stellar core collapse and bounce</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.102004</link>
    <description>Author(s): Christian R&#246;ver, Marie-Anne Bizouard, Nelson Christensen, Harald Dimmelmeier, Ik Siong Heng, and Renate Meyer&lt;br/&gt;Presented in this paper is a technique that we propose for extracting the physical parameters of a rotating stellar core collapse from the observation of the associated gravitational wave signal from the collapse and core bounce. Data from interferometric gravitational wave detectors can be used to ...&lt;br/&gt;[Phys. Rev. D 80, 102004] Published Tue Nov 17, 2009</description>
    <dc:creator>Christian R&#246;ver, Marie-Anne Bizouard, Nelson Christensen, Harald Dimmelmeier, Ik Siong Heng, and Renate Meyer</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.102004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 102004</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>102004</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.101302">
    <title>Cosmic steps in modeling dark energy</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.101302</link>
    <description>Author(s): Tower Wang&lt;br/&gt;Past and recent data analyses gave some hints of steps in dark energy. Considering dark energy as a dynamical scalar field, we investigate several models with various steps: a step in the scalar potential, a step in the kinetic term, a step in the energy density, and a step in the equation-of-state ...&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. D 80, 101302] Published Tue Nov 17, 2009</description>
    <dc:creator>Tower Wang</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.101302</dc:identifier>
    <dc:source>Phys. Rev. D 80, 101302</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>101302</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.096004">
    <title>Violation of CP and T in semileptonic decays due to scalar interactions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.096004</link>
    <description>Author(s): G. L&#243;pez Castro, L. L&#243;pez-Lozano, and A. Rosado&lt;br/&gt;Observing charge-parity (CP) or time-reversal (T) violations in the leptonic sector will give useful information to elucidate the nature of neutrinos. CP-violating couplings in charged leptonic currents carry out the weak phases necessary to break these symmetries. Here we study the interference of ...&lt;br/&gt;[Phys. Rev. D 80, 096004] Published Tue Nov 17, 2009</description>
    <dc:creator>G. L&#243;pez Castro, L. L&#243;pez-Lozano, and A. Rosado</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.096004</dc:identifier>
    <dc:source>Phys. Rev. D 80, 096004</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>096004</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.80.094012">
    <title>Y(4260) as a J/&#968;KK [over &#175;]  system</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.80.094012</link>
    <description>Author(s): A. Mart&#237;nez Torres, K. P. Khemchandani, D. Gamermann, and E. Oset&lt;br/&gt;A study of the J/&#968;&#960;&#960; and J/&#968;KK [over &#175;] systems, treating them as coupled channels, has been made by solving the Faddeev equations, with the purpose of investigating the possibility of generation of the J^{PC} =1^{--} , Y(4260) resonance due to the interaction between these three mesons. In ord...&lt;br/&gt;[Phys. Rev. D 80, 094012] Published Tue Nov 17, 2009</description>
    <dc:creator>A. Mart&#237;nez Torres, K. P. Khemchandani, D. Gamermann, and E. Oset</dc:creator>
    <dc:date>2009-11-17T00:00:00-05:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.80.094012</dc:identifier>
    <dc:source>Phys. Rev. D 80, 094012</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>2009-11-17T00:00:00-05:00</prism:publicationDate>
    <prism:startingPage>094012</prism:startingPage>
    <dc:subject>D1</dc:subject>
    <prism:section>D1</prism:section>
  </item>
</rdf:RDF>
