E-prints of Interest: 2010

General Relativity and Quantum Cosmology (gr-qc)

• Evolutions of Magnetized and Rotating Neutron Stars(arXiv:1001.0575)
• Relativistic Bose-Einstein Condensates: a new system for analogue models of gravity (arXiv:1001.1044)
• Killing Tensors and Symmetries(arXiv:1003.0019)
• Binary spinning black hole Hamiltonian in canonical center-of-mass and rest-frame coordinates through higher post-Newtonian order(arXiv:1003.0390)
• Binary black hole merger gravitational waves and recoil in the large mass ratio limit(arXiv:1003.0485)
• Post-Minkowskian closed-form Hamiltonian for gravitating N-body systems(arXiv:1003.0561)
• Binary black hole merger in the extreme-mass-ratio limit: a multipolar analysis(arXiv:1003.0597)
• Semianalytical estimates of scattering thresholds and gravitational radiation in ultrarelativistic black hole encounters(arXiv:1003.0812)
• Time Step Size Limitation Introduced by the BSSN Gamma Driver(arXiv:1003.0859)
• Dynamical spacetimes and gravitational radiation in a Fully Constrained Formulation(arXiv:1003.0868)
• Understanding the "anti-kick" in the merger of binary black holes(arXiv:1003.0873)
• Ultra-relativistic grazing collisions of black holes(arXiv:1003.0882)
• On the local existence of maximal slicings in spherically symmetric spacetimes(arXiv:1003.1014)
• Compact binary coalescence and the science case for Einstein Telescope(arXiv:1003.1386)
• Averaging geometrical objects on a differentiable manifold(arXiv:1003.2014)
• Motion and gravitational wave forms of eccentric compact binaries with orbital-angular-momentum-aligned spins under next-to-leading order in spin-orbit and leading order in spin(1)-spin(2) and spin-squared couplings(arXiv:1003.2735)
• Remark on non-existence of self-similar solutions in 4+1 vacuum gravitational collapse(arXiv:1003.3306)
• Constraint-preserving boundary conditions in the 3+1 first-order approach(arXiv:1003.3328)
• Gravity-induced vacuum dominance(arXiv:1003.3421)
• The gravitational-wave memory effect(arXiv:1003.3486)
• Singular perturbation techniques in the gravitational self-force problem(arXiv:1003.3954)
• The Cauchy problem for metric-affine f(R)-gravity in presence of a Klein-Gordon scalar field(arXiv:1003.4280)
• Nonminimal coupling for the gravitational and electromagnetic fields: Traversable electric wormholes(arXiv:1003.4584)
• Dynamical shift condition for unequal mass black hole binaries(arXiv:1003.4681)
• Dynamic transition to spontaneous scalarization in boson stars(arXiv:1003.4767)
• Outflows from accreting super-spinars(arXiv:1003.4821)
• Advancing Tests of Relativistic Gravity via Laser Ranging to Phobos(arXiv:1003.4961)
• An introduction to the theory of rotating relativistic stars(arXiv:1003.5015)
• Symplectic Integration of Post-Newtonian Equations of Motion with Spin(arXiv:1003.5122)
• Method of Matched Expansions & the Singularity Structure of the Green Function(arXiv:1003.5790)

• Lensing By Sgr A* as a Probe of Modified Gravity(arXiv:1004.0379)
• Bobbing and Kicks in Electromagnetism and Gravity(arXiv:1004.0679)
• Hyperboloidal evolution of test fields in three spatial dimensions(arXiv:1004.0760)
• Observing mergers of non-spinning black-hole binaries(arXiv:1004.0961)
• Mathematical general relativity: a sampler(arXiv:1004.1016)
• Gravitational waves astronomy: the ultimate test for Einstein's General Relativity(arXiv:1004.1293)
• Numerical evolution of multiple black holes with accurate initial data(arXiv:1004.1353)
• Construction of N-body initial data sets in general relativity(arXiv:1004.1355)
• A new look at loop quantum gravity(arXiv:1004.1780)
• Emergent Horizons in the Laboratory(arXiv:1004.2586)
• Influence of self-gravity on the runaway instability of black hole-torus systems(arXiv:1004.3102)
• A new three-dimensional general-relativistic hydrodynamics code(arXiv:1004.3849)
• Gravitational memory in binary black hole mergers(arXiv:1004.4209)
• Measuring orbital eccentricity and periastron advance in quasi-circular black hole simulations(arXiv:1004.4697)

• Maximum black-hole spin from quasi-circular binary mergers(arXiv:1005.0627)
• Gravitational Waves from Core Collapse Supernovae(arXiv:1005.0779)
• Spectral methods for the wave equation in second-order form(arXiv:1005.2922)
• Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries(arXiv:1005.3306)
• Testing gravitational parity violation with coincident gravitational waves and short gamma-ray bursts(arXiv:1005.3310)
• Gravitational Waves, Sources, and Detectors(arXiv:1005.4735)
• Statistical constraints on binary black hole inspiral dynamics(arXiv:1005.5560)
• Next to leading order spin-orbit effects in the motion of inspiralling compact binaries(arXiv:1005.5730)

• Notes on the integration of numerical relativity waveforms(arXiv:1006.1632)
• Mergers of Magnetized Neutron Stars with Spinning Black Holes: Disruption, Accretion and Fallback(arXiv:1006.2839)
• Numerical relativity for D dimensional space-times: head-on collisions of black holes and gravitational wave extraction(arXiv:1006.3081)
• Highly accurate and efficient self-force computations using time-domain methods: Error estimates, validation, and optimization(arXiv:1006.3788)
• Semi-Analytic Stellar Structure in Scalar-Tensor Gravity(arXiv:1006.4411)
• Jang's equation and its applications to marginally trapped surfaces(arXiv:1006.4601)

• On the initial-value problem of the Maxwell-Lorentz equations(arXiv:1007.0953)
• Evolution of a mass-less test scalar field on Boson Stars space-times(arXiv:1007.1162)
• Magnetospheres of Black Hole Systems in Force-Free Plasma(arXiv:1007.1198)
• Gravitational Waves from Coalescing Binary Sources(arXiv:1007.1358)
• On the proximity of black hole horizons: lessons from Vaidya(arXiv:1007.1642)
• Binary neutron-star mergers with Whisky and SACRA: First quantitative comparison of results from independent general-relativistic hydrodynamics codes(arXiv:1007.1754)
• Binary Pulsar Constraints on the Parameterized post-Einsteinian Framework(arXiv:1007.1995)
• Dynamical evolution of a scalar field coupling to Einstein's tensor in the Reissner-Nordström black hole spacetime(arXiv:1007.2019)
• A hybrid method for understanding black-hole mergers: head-on case(arXiv:1007.2024)
• Linear Stability Analysis and the Speed of Gravitational Waves in Dynamical Chern-Simons Modified Gravity(arXiv:1007.2429)
• High-Accuracy Comparison between the Post-Newtonian and Self-Force Dynamics of Black-Hole Binaries(arXiv:1007.2614)
• Critical Phenomena in Neutron Stars II: Head-on Collisions(arXiv:1007.2797)
• Critical Phenomena in Neutron Stars I: Linearly Unstable Nonrotating Models(arXiv:1007.2809)
• Simulations of black-hole binaries with unequal masses or non-precessing spins: accuracy, physical properties, and comparison with post-Newtonian results(arXiv:1007.4789)

• Action principle for Numerical Relativity evolution systems(arXiv:1008.0747)
• Dynamical damping terms for symmetry-seeking shift conditions(arXiv:1008.2212)
• On critical collapse of gravitational waves(arXiv:1008.3319)
• Conservative self-force correction to the innermost stable circular orbit: comparison with multiple post-Newtonian-based methods(arXiv:1008.4622)
• Test bodies and naked singularities: is the self-force the cosmic censor?(arXiv:1008.5159)

• Extreme-Mass-Ratio-Black-Hole-Binary Evolutions with Numerical Relativity(arXiv:1009.0292)
• Analytic modelling of tidal effects in the relativistic inspiral of binary neutron stars(arXiv:1009.0521)
• Uniqueness of Flat Spherically Symmetric Spacelike Hypersurfaces Admitted by Spherically Symmetric Static Spactimes(arXiv:1009.0586)
• The Initial-Boundary Value Problem in General Relativity(arXiv:1009.0589)
• Probing the small distance structure of canonical quantum gravity using the conformal group(arXiv:1009.0669)
• Two-dimensional quantum black holes: Numerical methods(arXiv:1009.1440)
• Multipole moments for black objects in five dimensions(arXiv:1009.1486)
• Causal Set Phenomenology(arXiv:1009.1593)
• Awaking the vacuum in relativistic stars(arXiv:1009.1771)
• Intermediate-mass-ratio-inspirals in the Einstein Telescope: I. Signal-to-noise ratio calculations(arXiv:1009.1985)
• The Problem of Time in Quantum Gravity(arXiv:1009.2157)
• Shape Quantities for Relational Quadrilateralland(arXiv:1009.2161)
• Gravitational collapse with non-vanishing tangential pressure(arXiv:1009.2169)
• Carter-like constants of motion in the Newtonian and relativistic two-center problems(arXiv:1009.2839)
• Remarks on the Myers-Perry and Einstein Gauss-Bonnet Rotating Solutions(arXiv:1009.3030)
• Phenomenology of the Lense-Thirring effect in the Solar System(arXiv:1009.3225)
• Conformal Superspace: the configuration space of general relativity(arXiv:1009.3559)
• Perfect Fluid Dark Matter(arXiv:1009.3572)
• Supersymmetric classical cosmology(arXiv:1009.4233)
• Hawking radiation from ultrashort laser pulse filaments(arXiv:1009.4634)
• Mode coupling of Schwarzschild perturbations: Ringdown frequencies(arXiv:1009.4665)
• Conservative, gravitational self-force for a particle in circular orbit around a Schwarzschild black hole in a Radiation Gauge(arXiv:1009.4876)
• Post-1-Newtonian quadrupole tidal interactions in binary systems(arXiv:1009.4919)
• Transient resonances in the inspirals of point particles into black holes(arXiv:1009.4923)
• Gravitational waves from binaries on unbound orbits(arXiv:1009.5042)
• Thick disk accretion in Kerr space-time with arbitrary spin parameters(arXiv:1009.5080)
• High-order perturbations of a spherical collapsing star(arXiv:1009.5605)
• Accuracy and effectualness of closed-form, frequency-domain waveforms for non-spinning black hole binaries(arXiv:1009.5998)
• Extreme Mass-Ratio Inspirals in the Effective-One-Body Approach: Quasi-Circular, Equatorial Orbits around a Spinning Black Hole(arXiv:1009.6013)
• An Efficient Time-Domain Method to Model Extreme-Mass-Ratio Inspirals(arXiv:1009.6073)
• Analytical solution of the geodesic equation in Kerr-(anti) de Sitter space-times(arXiv:1009.6117)
• Constraining properties of the black hole population using LISA(arXiv:1009.6172)
• Heat conduction in relativistic neutral gases revisited(arXiv:1009.6220)

• Testing Modified Gravity with Gravitational Wave Astronomy(arXiv:1010.0062)
• Weak Field Approach in f(R)-Gravity(arXiv:1010.0099)
• Constraint preserving boundary conditions for the Z4c formulation of general relativity(arXiv:1010.0523)
• Collision of an innermost stable circular orbit particle around a Kerr black hole(arXiv:1010.0962)
• f(T) gravity and local Lorentz invariance(arXiv:1010.1041)
• The Well-posedness of the Null-Timelike Boundary Problem for Quasilinear Waves(arXiv:1010.1201)
• The interior structure of astronomically realistic rotating black holes 1. Motivation and summary(arXiv:1010.1269)
• The interior structure of astronomically realistic rotating black holes 2. Uncharged black holes(arXiv:1010.1271)
• The interior structure of astronomically realistic rotating black holes 3. Charged black holes(arXiv:1010.1272)
• Relativistic heat conduction: the kinetic theory approach and comparison with Marle's model(arXiv:1010.1477)
• Time evolution of a non-singular primordial black hole(arXiv:1010.1578)
• Collapse and dispersal in massless scalar field models(arXiv:1010.1757)
• Applications of hidden symmetries to black hole physics(arXiv:1010.1792)
• Gravitational wave astronomy: the definitive test for the "Einstein frame versus Jordan frame" controversy(arXiv:1010.2086)
• The Final Merger of Black-Hole Binaries(arXiv:1010.2165)
• Collinear solution to the general relativistic three-body problem(arXiv:1010.2284)
• The "non-Kerrness" of domains of outer communication of black holes and exteriors of stars(arXiv:1010.2421)
• Can Hamiltonians be boundary observables in Parametrized Field Theories?(arXiv:1010.2535)
• Conservative corrections to the innermost stable circular orbit (ISCO) of a Kerr black hole: a new gauge-invariant post-Newtonian ISCO condition, and the ISCO shift due to test-particle spin and the gravitational self-force(arXiv:1010.2553)
• Teleparallel equivalent of general relativity: a critical review(arXiv:1010.2654)
• Reheating via a generalized non-minimal coupling of curvature to matter(arXiv:1010.2698)
• Simulating merging binary black holes with nearly extremal spins(arXiv:1010.2777)
• Surprising Connections Between General Relativity and Condensed Matter(arXiv:1010.2784)
• Banks of templates for directed searches of gravitational waves from spinning neutron stars(arXiv:1010.2879)
• A Simple method to set up low eccentricity initial data for moving puncture simulations(arXiv:1010.2936)
• Gravitational Lensing from a Spacetime Perspective(arXiv:1010.3416)
• An Exploration of OpenCL for a Numerical Relativity Application(arXiv:1010.3816)
• Gravitational wave energy spectrum of a parabolic encounter(arXiv:1010.3865)
• Up to eleven: radiation from particles with arbitrary energy falling into higher-dimensional black holes(arXiv:1010.3874)
• Formulations of the 3+1 evolution equations in curvilinear coordinates(arXiv:1010.4013)
• Perturbative Analysis of a Stationary Magnetosphere in an Extreme Black Hole Spacetime : On the Meissner-like Effect of an Extreme Black Hole(arXiv:1010.4104)
• Thermodynamics of magnetized binary compact objects(arXiv:1010.4409)
• Exploring the Use of Numerical Relativity Waveforms in Burst Analysis of Precessing Black Hole Mergers(arXiv:1010.5200)
• Self force via m-mode regularization and 2+1D evolution: Foundations and a scalar-field implementation on Schwarzschild(arXiv:1010.5255)
• Black-hole binaries, gravitational waves, and numerical relativity(arXiv:1010.5260)
• Screening of cosmological constant in non-local gravity(arXiv:1010.5375)
• Acceleration of colliding shells around a black hole -- Validity of test particle approximation in BSW process(arXiv:1010.5438)
• Trumpet slices of the Schwarzschild-Tangherlini spacetime(arXiv:1010.5723)
• Gauge Gravity: a forward-looking introduction(arXiv:1010.5822)

• The Conformal Constraint in Canonical Quantum Gravity(arXiv:1011.0061)
• Second-order hyperbolic Fuchsian systems and applications(arXiv:1011.0270)
• Intermediate-mass-ratio-inspirals in the Einstein Telescope. II. Parameter estimation errors(arXiv:1011.0421)
• Modeling maximum astrophysical gravitational recoil velocities(arXiv:1011.0593)
• Head-on collisions of unequal mass black holes in D=5 dimensions(arXiv:1011.0742)
• Stability and Quasinormal Modes of Black holes in Tensor-Vector-Scalar theory: Scalar Field Perturbations(arXiv:1011.0747)
• Path Integrals and the WKB approximation in Loop Quantum Cosmology(arXiv:1011.1024)
• Next-to-leading order spin-orbit and spin(a)-spin(b) Hamiltonians for n gravitating spinning compact objects(arXiv:1011.1179)
• Quasinormal modes, scattering and Hawking radiation of Kerr-Newman black holes in a magnetic field(arXiv:1011.1843)
• Modeling Gravitational Recoil Using Numerical Relativity(arXiv:1011.2210)
• Gravitational lensing by a regular black hole(arXiv:1011.2455)
• On the hyperbolicity of Maxwell's equations with a local constitutive law(arXiv:1011.2536)
• Horizon dynamics in perturbed Kerr spacetimes(arXiv:1011.2601)
• Perturbative effects of spinning black holes with applications to recoil velocities(arXiv:1011.2767)
• Superkicks in ultrarelativistic encounters of spinning black holes(arXiv:1011.3281)
• A Unified Theory of Non-Linear Electrodynamics and Gravity(arXiv:1011.3641)
• Gravitational Waves from the $r$-mode instability of neutron stars: effect of magnetic field(arXiv:1011.3738)
• Thirty years of studies of integrable reductions of Einstein's field equations(arXiv:1011.3846)
• Post-Newtonian effects on Lagrange's equilateral triangular solution for the three-body problem(arXiv:1011.3886)
• A Characteristic Extraction Tool for Gravitational Waveforms(arXiv:1011.4223)
• Stability of the puncture method with a generalized BSSN formulation(arXiv:1011.4407)
• Junction conditions at spacetime singularities(arXiv:1011.4702)
• A new framework for analyzing the effects of small scale inhomogeneities in cosmology(arXiv:1011.4920)
• Resonant recoil in extreme mass ratio binary black hole mergers(arXiv:1011.4987)
• General formulation of general-relativistic higher-order gauge-invariant perturbation theory(arXiv:1011.5272)
• Stationary, Axisymmetric Neutron Stars with Meridional Circulation in General Relativity(arXiv:1011.5475)
• Statistical Properties of Cosmological Billiards(arXiv:1011.5797)
• Strong Gravitational Lensing by Sgr A*(arXiv:1011.5848)
• Comparing space+time decompositions in the post-Newtonian limit(arXiv:1011.6024)
• Surprises in the Evaporation of 2-Dimensional Black Holes(arXiv:1011.6442)
• Heat conduction in relativistic systems: alternatives and perspectives(arXiv:1011.6628)

• Evaporation of 2-Dimensional Black Holes(arXiv:1012.0077)
• Gravitational Wave Extraction in Simulations of Rotating Stellar Core Collapse(arXiv:1012.0595)
• Hybrid black-hole binary initial data(arXiv:1012.0886)
• Sensitivity Studies for Third-Generation Gravitational Wave Observatories(arXiv:1012.0908)
• Does an atom interferometer test the gravitational redshift at the Compton frequency?(arXiv:1012.1194)
• Reducing orbital eccentricity of precessing black-hole binaries(arXiv:1012.1549)
• Binary black hole coalescence in the extreme-mass-ratio limit: testing and improving the effective-one-body multipolar waveform(arXiv:1012.2456)
• The Status of Black-Hole Binary Merger Simulations with Numerical Relativity(arXiv:1012.2872)
• Tracking the precession of compact binaries from their gravitational-wave signal(arXiv:1012.2879)
• Magnetars oscillations in the presence of a crust(arXiv:1012.3103)
• Effective Gravitational Wave Stress-energy Tensor in Alternative Theories of Gravity(arXiv:1012.3144)
• Black-hole binaries go to eleven orbits(arXiv:1012.3173)
• The trumpet solution from spherical gravitational collapse with puncture gauges(arXiv:1012.3703)
• Full-analytic frequency-domain gravitational wave forms from eccentric compact binaries to 2PN accuracy(arXiv:1012.3894)
• Generalizations of teleparallel gravity and local Lorentz symmetry(arXiv:1012.4039)
• Stereoscopic visualization in curved spacetime: seeing deep inside a black hole(arXiv:1012.4043)
• Characterization of the gravitational wave emission of three black holes(arXiv:1012.4423)
• The causal structure of spacetime is a parameterized Randers geometry(arXiv:1012.4467)
• Loop quantum gravity: the first twenty five years(arXiv:1012.4707)
• Some generalizations of the Raychaudhuri equation(arXiv:1012.4806)
• Frame-Dragging Vortexes and Tidal Tendexes Attached to Colliding Black Holes: Visualizing the Curvature of Spacetime(arXiv:1012.4869)
• Quasinormal modes for the charged Vaidya metric(arXiv:1012.5110)
• Forced motion near black holes(arXiv:1012.5111)
• Conformal transformations and Nordström's scalar theory of gravity(arXiv:1012.5386)
• Ideal Gas in a strong Gravitational field: Area dependence of Entropy(arXiv:1012.5421)
• A Fast Frequency-Domain Algorithm for Gravitational Self-Force: I, Circular Orbits in Schwarzschild Spacetime(arXiv:1012.5860)
• From laboratory experiments to LISA Pathfinder: achieving LISA geodesic motion(arXiv:1012.5968)