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    <description>Recently published articles in Phys. Rev. D in the Table of Content section "General relativity, gravitation"</description>
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    <title>Classical thermodynamics of gravitational collapse</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.104003</link>
    <description>Author(s): Z. Gecse and S. Khlebnikov&lt;br/&gt;We study numerically gravitational collapse of a spherically symmetric instanton particle in five dimensions. We show that the late stages of the process are characterized by a nearly constant &#8220;free energy,&#8221; the value of which matches (within numerical uncertainties) the value obtained from stan...&lt;br/&gt;[Phys. Rev. D 77, 104003] Published Mon May 05, 2008</description>
    <dc:creator>Z. Gecse and S. Khlebnikov</dc:creator>
    <dc:date>2008-05-05T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.104003</dc:identifier>
    <dc:source>Phys. Rev. D 77, 104003</dc:source>
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    <title>Quasilocal contribution to the scalar self-force: Geodesic motion</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.104002</link>
    <description>Author(s): Adrian C. Ottewill and Barry Wardell&lt;br/&gt;We consider a scalar charge travelling in a curved background space-time. We calculate the quasilocal contribution to the scalar self-force experienced by such a particle following a geodesic in a general space-time. We also show that if we assume a massless field and a vacuum background space-time,...&lt;br/&gt;[Phys. Rev. D 77, 104002] Published Mon May 05, 2008</description>
    <dc:creator>Adrian C. Ottewill and Barry Wardell</dc:creator>
    <dc:date>2008-05-05T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.104002</dc:identifier>
    <dc:source>Phys. Rev. D 77, 104002</dc:source>
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    <title>Higher-order-in-spin interaction Hamiltonians for binary black holes from source terms of Kerr geometry in approximate ADM coordinates</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.104001</link>
    <description>Author(s): Steven Hergt and Gerhard Sch&#228;fer&lt;br/&gt;The Kerr metric outside the ergosphere is transformed into Arnowitt-Deser-Misner coordinates up to the orders 1/r^{4} and a^{2} , respectively, in radial coordinate r and reduced angular momentum variable a, starting from the Kerr solution in quasi-isotropic as well as harmonic coordinates. The dist...&lt;br/&gt;[Phys. Rev. D 77, 104001] Published Mon May 05, 2008</description>
    <dc:creator>Steven Hergt and Gerhard Sch&#228;fer</dc:creator>
    <dc:date>2008-05-05T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.104001</dc:identifier>
    <dc:source>Phys. Rev. D 77, 104001</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.101501">
    <title>Close encounters of three black holes</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.101501</link>
    <description>Author(s): Manuela Campanelli, Carlos O. Lousto, and Yosef Zlochower&lt;br/&gt;We present the first fully relativistic long-term numerical evolutions of three equal-mass black holes in a system consisting of a third black hole in a close orbit about a black-hole binary. These close-three-black-hole systems have very different merger dynamics from black-hole binaries; displayin...&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 77, 101501] Published Mon May 05, 2008</description>
    <dc:creator>Manuela Campanelli, Carlos O. Lousto, and Yosef Zlochower</dc:creator>
    <dc:date>2008-05-05T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.101501</dc:identifier>
    <dc:source>Phys. Rev. D 77, 101501</dc:source>
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    <title>Hydrogen atom in Palatini theories of gravity</title>
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    <description>Author(s): Gonzalo J. Olmo&lt;br/&gt;We study the effects that the gravitational interaction of f(R) theories of gravity in Palatini formalism has on the stationary states of the hydrogen atom. We show that the role of gravity in this system is very important for Lagrangians f(R) with terms that grow at low curvatures, which have been ...&lt;br/&gt;[Phys. Rev. D 77, 084021] Published Wed Apr 30, 2008</description>
    <dc:creator>Gonzalo J. Olmo</dc:creator>
    <dc:date>2008-04-30T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084021</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084021</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084020">
    <title>Einsteinian gravity from BRST quantization of a topological action</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084020</link>
    <description>Author(s): Eckehard W. Mielke&lt;br/&gt;In order to deduce Einsteinian gravity from a topological action, we start from the metric-free Pontrjagin invariant in four dimensions. Using the Becchi-Rouet-Stora-Tyutin antifield formalism with a double duality gauge fixing, we obtain a consistent quantization in spaces of double dual curvature....&lt;br/&gt;[Phys. Rev. D 77, 084020] Published Mon Apr 28, 2008</description>
    <dc:creator>Eckehard W. Mielke</dc:creator>
    <dc:date>2008-04-28T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084020</dc:identifier>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084019">
    <title>Evolution of perturbations of squashed Kaluza-Klein black holes: Escape from instability</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084019</link>
    <description>Author(s): Hideki Ishihara, Masashi Kimura, Roman A. Konoplya, Keiju Murata, Jiro Soda, and Alexander Zhidenko&lt;br/&gt;The squashed Kaluza-Klien (KK) black holes differ from the Schwarzschild black holes with asymptotic flatness or the black strings even at energies for which the KK modes are not excited yet, so that squashed KK black holes open a window in higher dimensions. Another important feature is that the sq...&lt;br/&gt;[Phys. Rev. D 77, 084019] Published Mon Apr 28, 2008</description>
    <dc:creator>Hideki Ishihara, Masashi Kimura, Roman A. Konoplya, Keiju Murata, Jiro Soda, and Alexander Zhidenko</dc:creator>
    <dc:date>2008-04-28T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084019</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084019</dc:source>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084018">
    <title>Do f(R) theories matter?</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084018</link>
    <description>Author(s): O. Bertolami and J. P&#225;ramos&lt;br/&gt;We consider a modified action functional with a nonminimum coupling between the scalar curvature and the matter Lagrangian, and study its consequences on stellar equilibrium. Particular attention is paid to the validity of the Newtonian regime, and on the boundary and exterior matching conditions, a...&lt;br/&gt;[Phys. Rev. D 77, 084018] Published Fri Apr 25, 2008</description>
    <dc:creator>O. Bertolami and J. P&#225;ramos</dc:creator>
    <dc:date>2008-04-25T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084018</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084018</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>2008-04-25T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084018</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.77.084017">
    <title>Faithful effective-one-body waveforms of equal-mass coalescing black-hole binaries</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084017</link>
    <description>Author(s): Thibault Damour, Alessandro Nagar, Ernst Nils Dorband, Denis Pollney, and Luciano Rezzolla&lt;br/&gt;We compare a recently derived, resummed high post-Newtonian accuracy effective-one-body (EOB) quadrupolar waveform to the results of a numerical simulation of the inspiral and merger of an equal-mass black-hole binary. We find a remarkable agreement, both in phase and in amplitude, with a maximal de...&lt;br/&gt;[Phys. Rev. D 77, 084017] Published Tue Apr 22, 2008</description>
    <dc:creator>Thibault Damour, Alessandro Nagar, Ernst Nils Dorband, Denis Pollney, and Luciano Rezzolla</dc:creator>
    <dc:date>2008-04-22T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084017</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084017</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:startingPage>084017</prism:startingPage>
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  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084016">
    <title>Microcausality in curved space-time</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084016</link>
    <description>Author(s): Sergei Dubovsky, Alberto Nicolis, Enrico Trincherini, and Giovanni Villadoro&lt;br/&gt;It is well known that in Lorentz-invariant quantum field theories in flat space the commutator of spacelike separated local operators vanishes (microcausality). We provide two different arguments showing that this is a consequence of the causal structure of the classical theory, rather than of Loren...&lt;br/&gt;[Phys. Rev. D 77, 084016] Published Thu Apr 17, 2008</description>
    <dc:creator>Sergei Dubovsky, Alberto Nicolis, Enrico Trincherini, and Giovanni Villadoro</dc:creator>
    <dc:date>2008-04-17T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084016</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084016</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:publicationDate>2008-04-17T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084016</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.77.084015">
    <title>Merger of black hole and neutron star in general relativity: Tidal disruption, torus mass, and gravitational waves</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084015</link>
    <description>Author(s): Masaru Shibata and Keisuke Taniguchi&lt;br/&gt;We study the properties of the merger of black hole&#8211;neutron star (BH-NS) binaries in fully general relativistic simulation, focusing on the case that the NS is tidally disrupted. We prepare BH-NS binaries in a quasicircular orbit as the initial condition in which the BH is modeled by a nonspinning...&lt;br/&gt;[Phys. Rev. D 77, 084015] Published Thu Apr 17, 2008</description>
    <dc:creator>Masaru Shibata and Keisuke Taniguchi</dc:creator>
    <dc:date>2008-04-17T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084015</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084015</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>084015</prism:startingPage>
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    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.081502">
    <title>Circularization and final spin in eccentric binary-black-hole inspirals</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.081502</link>
    <description>Author(s): Ian Hinder, Birjoo Vaishnav, Frank Herrmann, Deirdre M. Shoemaker, and Pablo Laguna&lt;br/&gt;We present results from numerical relativity simulations of equal-mass, nonspinning binary-black-hole inspirals and mergers with initial eccentricities e&#8804;0.8 and coordinate separations D&#8805;12M of up to 9 orbits (18 gravitational wave cycles). We extract the mass M_{f} and spin a_{f} of the final b...&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 77, 081502] Published Thu Apr 17, 2008</description>
    <dc:creator>Ian Hinder, Birjoo Vaishnav, Frank Herrmann, Deirdre M. Shoemaker, and Pablo Laguna</dc:creator>
    <dc:date>2008-04-17T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.081502</dc:identifier>
    <dc:source>Phys. Rev. D 77, 081502</dc:source>
    <dc:format>text/html</dc:format>
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    <prism:publicationName>Physical Review D</prism:publicationName>
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    <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.77.084014">
    <title>Solar system tests of scalar field models with an exponential potential</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084014</link>
    <description>Author(s): J. P&#225;ramos and O. Bertolami&lt;br/&gt;We consider a scenario where the dynamics of a scalar field is ruled by an exponential potential, such as those arising from some quintessence-type models, and aim at obtaining phenomenological manifestations of this entity within our Solar System. To do so, we assume a perturbative regime, derive t...&lt;br/&gt;[Phys. Rev. D 77, 084014] Published Wed Apr 16, 2008</description>
    <dc:creator>J. P&#225;ramos and O. Bertolami</dc:creator>
    <dc:date>2008-04-16T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084014</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084014</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-16T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084014</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084013">
    <title>Nonminimal coupling for the gravitational and electromagnetic fields: Black hole solutions and solitons</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084013</link>
    <description>Author(s): Alexander B. Balakin, Vladimir V. Bochkarev, and Jos&#233; P. Lemos&lt;br/&gt;Using a Lagrangian formalism, a three-parameter nonminimal Einstein-Maxwell theory is established. The three parameters q_{1} , q_{2} , and q_{3} characterize the cross-terms in the Lagrangian, between the Maxwell field and terms linear in the Ricci scalar, Ricci tensor, and Riemann tensor, respecti...&lt;br/&gt;[Phys. Rev. D 77, 084013] Published Tue Apr 15, 2008</description>
    <dc:creator>Alexander B. Balakin, Vladimir V. Bochkarev, and Jos&#233; P. Lemos</dc:creator>
    <dc:date>2008-04-15T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084013</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084013</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-15T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084013</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084012">
    <title>Scalar field equations from quantum gravity during inflation</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084012</link>
    <description>Author(s): E. O. Kahya and R. P. Woodard&lt;br/&gt;We exploit a previous computation of the self-mass-squared from quantum gravity to include quantum corrections to the scalar evolution equation. The plane wave mode functions are shown to receive no significant one loop corrections at late times. This result probably applies as well to the inflaton ...&lt;br/&gt;[Phys. Rev. D 77, 084012] Published Tue Apr 15, 2008</description>
    <dc:creator>E. O. Kahya and R. P. Woodard</dc:creator>
    <dc:date>2008-04-15T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084012</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084012</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-15T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084012</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084011">
    <title>Euclidean analysis of the entropy functional formalism</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084011</link>
    <description>Author(s): &#211;scar J. Dias and Pedro J. Silva&lt;br/&gt;The attractor mechanism implies that the supersymmetric black hole near-horizon solution is defined only in terms of the conserved charges and is therefore independent of asymptotic moduli. Starting only with the near-horizon geometry, Sen&#8217;s entropy functional formalism computes the entropy of an ...&lt;br/&gt;[Phys. Rev. D 77, 084011] Published Mon Apr 14, 2008</description>
    <dc:creator>&#211;scar J. Dias and Pedro J. Silva</dc:creator>
    <dc:date>2008-04-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084011</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084011</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084011</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084010">
    <title>Growth of structure in theories with a dynamical preferred frame</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084010</link>
    <description>Author(s): T. G Zlosnik, P. G. Ferreira, and G. D. Starkman&lt;br/&gt;We study the cosmological stability of a class of theories with a dynamical preferred frame. For a range of actions, we find cosmological solutions which are compatible with observations of the recent history of the Universe: a matter-dominated era followed by accelerated expansion. We then study th...&lt;br/&gt;[Phys. Rev. D 77, 084010] Published Mon Apr 14, 2008</description>
    <dc:creator>T. G Zlosnik, P. G. Ferreira, and G. D. Starkman</dc:creator>
    <dc:date>2008-04-14T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084010</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084010</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-14T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084010</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.087501">
    <title>Quasinormal modes and thermodynamic phase transitions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.087501</link>
    <description>Author(s): Emanuele Berti and Vitor Cardoso&lt;br/&gt;It has recently been suggested that scalar, Dirac, and Rarita-Schwinger perturbations are related to thermodynamic phase transitions of charged (Reissner-Nordstr&#246;m) black holes. In this Brief Report we show that this result is probably a numerical coincidence, and that the conjectured correspondenc...&lt;br/&gt;[Phys. Rev. D 77, 087501] Published Fri Apr 11, 2008</description>
    <dc:creator>Emanuele Berti and Vitor Cardoso</dc:creator>
    <dc:date>2008-04-11T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.087501</dc:identifier>
    <dc:source>Phys. Rev. D 77, 087501</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-11T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>087501</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084009">
    <title>Learning about compact binary merger: The interplay between numerical relativity and gravitational-wave astronomy</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084009</link>
    <description>Author(s): Thomas Baumgarte, Patrick R. Brady, Jolien D Creighton, Luis Lehner, Frans Pretorius, and Ricky DeVoe&lt;br/&gt;Activities in data analysis and numerical simulation of gravitational waves have to date largely proceeded independently. In this work we study how waveforms obtained from numerical simulations could be effectively used within the data analysis effort to search for gravitational waves from black hol...&lt;br/&gt;[Phys. Rev. D 77, 084009] Published Fri Apr 11, 2008</description>
    <dc:creator>Thomas Baumgarte, Patrick R. Brady, Jolien D Creighton, Luis Lehner, Frans Pretorius, and Ricky DeVoe</dc:creator>
    <dc:date>2008-04-11T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084009</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084009</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-11T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084009</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084008">
    <title>Regularization of fields for self-force problems in curved spacetime: Foundations and a time-domain application</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084008</link>
    <description>Author(s): Ian Vega and Steven Detweiler&lt;br/&gt;We propose an approach for the calculation of self-forces, energy fluxes and waveforms arising from moving point charges in curved spacetimes. As opposed to mode-sum schemes that regularize the self-force derived from the singular retarded field, this approach regularizes the retarded field itself. ...&lt;br/&gt;[Phys. Rev. D 77, 084008] Published Tue Apr 08, 2008</description>
    <dc:creator>Ian Vega and Steven Detweiler</dc:creator>
    <dc:date>2008-04-08T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084008</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084008</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-08T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084008</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084007">
    <title>Mathematical issues in a fully constrained formulation of the Einstein equations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084007</link>
    <description>Author(s): Isabel Cordero-Carri&#243;n, Jos&#233; Mar&#237;a Ib&#225;&#241;ez, Eric Gourgoulhon, Jos&#233; Luis Jaramillo, and J&#233;r&#244;me Novak&lt;br/&gt;Bonazzola, Gourgoulhon, Grandcl&#233;ment, and Novak [Phys. Rev. D 70, 104007 (2004)] proposed a new formulation for 3+1 numerical relativity. Einstein equations result, according to that formalism, in a coupled elliptic-hyperbolic system. We have carried out a preliminary analysis of the mathematical s...&lt;br/&gt;[Phys. Rev. D 77, 084007] Published Mon Apr 07, 2008</description>
    <dc:creator>Isabel Cordero-Carri&#243;n, Jos&#233; Mar&#237;a Ib&#225;&#241;ez, Eric Gourgoulhon, Jos&#233; Luis Jaramillo, and J&#233;r&#244;me Novak</dc:creator>
    <dc:date>2008-04-07T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084007</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084007</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-07T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084007</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084006">
    <title>Induced gravity on intersecting brane worlds: Maximally symmetric solutions</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084006</link>
    <description>Author(s): Olindo Corradini, Kazuya Koyama, and Gianmassimo Tasinato&lt;br/&gt;We explore models of intersecting brane worlds with induced gravity terms on codimension-one branes and on their intersection. Maximally symmetric solutions for the branes and the intersection are found. We find new self-accelerating solutions. In a 6D spacetime, the solutions realize the seesaw mod...&lt;br/&gt;[Phys. Rev. D 77, 084006] Published Mon Apr 07, 2008</description>
    <dc:creator>Olindo Corradini, Kazuya Koyama, and Gianmassimo Tasinato</dc:creator>
    <dc:date>2008-04-07T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084006</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084006</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-07T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084006</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084005">
    <title>Extremality conditions for isolated and dynamical horizons</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084005</link>
    <description>Author(s): Ivan Booth and Stephen Fairhurst&lt;br/&gt;A maximally rotating Kerr black hole is said to be extremal. In this paper we introduce the corresponding restrictions for isolated and dynamical horizons. These reduce to the standard notions for Kerr but in general do not require the horizon to be either stationary or rotationally symmetric. We co...&lt;br/&gt;[Phys. Rev. D 77, 084005] Published Mon Apr 07, 2008</description>
    <dc:creator>Ivan Booth and Stephen Fairhurst</dc:creator>
    <dc:date>2008-04-07T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084005</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084005</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-07T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084005</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084004">
    <title>Unified geometric description of black hole thermodynamics</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084004</link>
    <description>Author(s): Jos&#233; L. &#193;lvarez, Hernando Quevedo, and Alberto S&#225;nchez&lt;br/&gt;In the space of thermodynamic equilibrium states we introduce a Legendre invariant metric which contains all the information about the thermodynamics of black holes. The curvature of this thermodynamic metric becomes singular at those points where, according to the analysis of the heat capacities, p...&lt;br/&gt;[Phys. Rev. D 77, 084004] Published Mon Apr 07, 2008</description>
    <dc:creator>Jos&#233; L. &#193;lvarez, Hernando Quevedo, and Alberto S&#225;nchez</dc:creator>
    <dc:date>2008-04-07T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084004</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084004</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-07T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084004</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084003">
    <title>Dirac fields in loop quantum gravity and big bang nucleosynthesis</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084003</link>
    <description>Author(s): Martin Bojowald, Rupam Das, and Robert J. Scherrer&lt;br/&gt;Big bang nucleosynthesis requires a fine balance between equations of state for photons and relativistic fermions. Several corrections to equation of state parameters arise from classical and quantum physics, which are derived here from a canonical perspective. In particular, loop quantum gravity al...&lt;br/&gt;[Phys. Rev. D 77, 084003] Published Mon Apr 07, 2008</description>
    <dc:creator>Martin Bojowald, Rupam Das, and Robert J. Scherrer</dc:creator>
    <dc:date>2008-04-07T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084003</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084003</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-07T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084003</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.081501">
    <title>Next-to-leading order gravitational spin(1)-spin(2) dynamics in Hamiltonian form</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.081501</link>
    <description>Author(s): Jan Steinhoff, Steven Hergt, and Gerhard Sch&#228;fer&lt;br/&gt;Based on recent developments by the authors a next-to-leading order spin(1)-spin(2) Hamiltonian is derived for the first time. The result is obtained within the canonical formalism of Arnowitt, Deser, and Misner (ADM) utilizing their generalized isotropic coordinates. A comparison with other methods...&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 77, 081501] Published Fri Apr 04, 2008</description>
    <dc:creator>Jan Steinhoff, Steven Hergt, and Gerhard Sch&#228;fer</dc:creator>
    <dc:date>2008-04-04T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.081501</dc:identifier>
    <dc:source>Phys. Rev. D 77, 081501</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-04T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>081501</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084002">
    <title>Fully general relativistic simulations of black hole-neutron star mergers</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084002</link>
    <description>Author(s): Zachariah B. Etienne, Joshua A. Faber, Yuk Tung Liu, Stuart L. Shapiro, Keisuke Taniguchi, and Thomas W. Baumgarte&lt;br/&gt;Black hole-neutron star (BHNS) binaries are expected to be among the leading sources of gravitational waves observable by ground-based detectors, and may be the progenitors of short-hard gamma-ray bursts (SGRBs) as well. We discuss our new fully general relativistic calculations of merging BHNS bina...&lt;br/&gt;[Phys. Rev. D 77, 084002] Published Wed Apr 02, 2008</description>
    <dc:creator>Zachariah B. Etienne, Joshua A. Faber, Yuk Tung Liu, Stuart L. Shapiro, Keisuke Taniguchi, and Thomas W. Baumgarte</dc:creator>
    <dc:date>2008-04-02T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084002</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084002</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-02T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084002</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.084001">
    <title>Gauge drivers for the generalized harmonic Einstein equations</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.084001</link>
    <description>Author(s): Lee Lindblom, Keith D. Matthews, Oliver Rinne, and Mark A. Scheel&lt;br/&gt;The generalized harmonic representation of Einstein&#8217;s equations is manifestly hyperbolic for a large class of gauge conditions. Unfortunately most of the useful gauges developed over the past several decades by the numerical relativity community are incompatible with the hyperbolicity of the equat...&lt;br/&gt;[Phys. Rev. D 77, 084001] Published Tue Apr 01, 2008</description>
    <dc:creator>Lee Lindblom, Keith D. Matthews, Oliver Rinne, and Mark A. Scheel</dc:creator>
    <dc:date>2008-04-01T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.084001</dc:identifier>
    <dc:source>Phys. Rev. D 77, 084001</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>8</prism:issueIdentifier>
    <prism:publicationDate>2008-04-01T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>084001</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.064035">
    <title>Inspiralling compact binaries in quasi-elliptical orbits: The complete third post-Newtonian energy flux</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.064035</link>
    <description>Author(s): K. G. Arun, Luc Blanchet, Bala R. Iyer, and Moh&#8217;d S. Qusailah&lt;br/&gt;The instantaneous contributions to the third post-Newtonian (3PN) gravitational wave luminosity from the inspiral phase of a binary system of compact objects moving in a quasi-elliptical orbit is computed using the multipolar post-Minkowskian wave generation formalism. The necessary inputs for this ...&lt;br/&gt;[Phys. Rev. D 77, 064035] Published Mon Mar 31, 2008</description>
    <dc:creator>K. G. Arun, Luc Blanchet, Bala R. Iyer, and Moh&#8217;d S. Qusailah</dc:creator>
    <dc:date>2008-03-31T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.064035</dc:identifier>
    <dc:source>Phys. Rev. D 77, 064035</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>6</prism:issueIdentifier>
    <prism:publicationDate>2008-03-31T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>064035</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
  <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevD.77.064034">
    <title>Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbits</title>
    <link>http://link.aps.org/doi/10.1103/PhysRevD.77.064034</link>
    <description>Author(s): K. G. Arun, Luc Blanchet, Bala R. Iyer, and Moh&#8217;d S. Qusailah&lt;br/&gt;The far-zone flux of energy contains hereditary (tail) contributions that depend on the entire past history of the source. Using the multipolar post-Minkowskian wave generation formalism, we propose and implement a semianalytical method in the frequency domain to compute these contributions from the...&lt;br/&gt;[Phys. Rev. D 77, 064034] Published Mon Mar 31, 2008</description>
    <dc:creator>K. G. Arun, Luc Blanchet, Bala R. Iyer, and Moh&#8217;d S. Qusailah</dc:creator>
    <dc:date>2008-03-31T00:00:00-04:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:identifier>10.1103/PhysRevD.77.064034</dc:identifier>
    <dc:source>Phys. Rev. D 77, 064034</dc:source>
    <dc:format>text/html</dc:format>
    <dc:type>article</dc:type>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>77</prism:volume>
    <prism:issueIdentifier>6</prism:issueIdentifier>
    <prism:publicationDate>2008-03-31T00:00:00-04:00</prism:publicationDate>
    <prism:startingPage>064034</prism:startingPage>
    <dc:subject>D15</dc:subject>
    <prism:section>D15</prism:section>
  </item>
</rdf:RDF>
