Search results for "General Relativity"

showing 10 items of 1057 documents

GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

2018

The LIGO Scientific and Virgo Collaborations have announced the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutron stars estimated from this event suggests that distant, unresolvable binary neutron stars create a significant astrophysical stochastic gravitational-wave background. The binary neutron star background will add to the background from binary black holes, increasing the amplitude of the total astrophysical background relative to previous expectations. In the Advanced LIGO-Virgo frequency band most sensitive to stochastic backgrounds (near 25 Hz), we predict a total astrophysical background with amplitude $\Omega_{\rm…

Design sensitivityneutron star: binarygravitational radiation: stochasticAstronomyX-ray binaryGeneral Physics and AstronomyAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationGravitational wave backgroundGravitational Waves Neutron Stars Stochastic Background Virgo LIGOblack holeLIGOstochastic modelQCQBPhysicsGAMMA-RAY BURSTSSignal to noise ratioStochastic systemsBlack holesGravitational effectsarticleAstrophysics::Instrumentation and Methods for AstrophysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSING[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sources Experimental studies of gravity Gravitational WavesGravitationBinary neutron starsX-ray bursterBinsAstrophysics::High Energy Astrophysical PhenomenaMERGERSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionBinary pulsarNeutron starsSTAR-FORMATIONPhysics and Astronomy (all)General Relativity and Quantum CosmologyBinary black holebinary: coalescence0103 physical sciencesFrequency bandsddc:530RATESINTERFEROMETERS010306 general physicsAstrophysics::Galaxy AstrophysicsNeutronsGravitational Waves010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundgravitational radiationAstronomyNeutron Stars530 Physikbinary: compactsensitivityStarsLIGObackground: stochasticEVOLUTIONsignal noise ratioVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionStellar black holeStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHIGH-REDSHIFTneutron star: coalescencePhysical Review Letters
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Gravitino dark matter with neutralino NLSP in the constrained NMSSM

2010

The gravitino dark matter with neutralino NLSP hypothesis is investigated in the framework of NMSSM. We have considered both the thermal and non-thermal gravitino production mechanisms, and we have taken into account all the collider and cosmological constraints. The maximum allowed reheating temperature after inflation, as well as the maximum allowed gravitino mass are determined.

Inflation (cosmology)PhysicsHistoryParticle physicsDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science ApplicationsEducationlaw.inventionHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)lawNeutralinoGravitinoHigh Energy Physics::ExperimentCollider
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Geometric inequivalence of metric and Palatini formulations of General Relativity

2020

Projective invariance is a symmetry of the Palatini version of General Relativity which is not present in the metric formulation. The fact that the Riemann tensor changes nontrivially under projective transformations implies that, unlike in the usual metric approach, in the Palatini formulation this tensor is subject to a gauge freedom, which allows some ambiguities even in its scalar contractions. In this sense, we show that for the Schwarzschild solution there exists a projective gauge in which the (affine) Kretschmann scalar, K≡R R , can be set to vanish everywhere. This puts forward that the divergence of curvature scalars may, in some cases, be avoided by a gauge transformation of the …

General RelativityNuclear and High Energy PhysicsRiemann curvature tensorFísica-Modelos matemáticosGeneral relativityScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmology//purl.org/becyt/ford/1 [https]symbols.namesakeGeneral Relativity and Quantum Cosmology0103 physical sciencesSchwarzschild metricFísica matemáticaGauge theoryTensorGeometric inequivalence010306 general physicsMathematical PhysicsMathematical physicsPhysics010308 nuclear & particles physicsKretschmann scalar//purl.org/becyt/ford/1.3 [https]Mathematical Physics (math-ph)lcsh:QC1-999Symmetry (physics)symbolslcsh:PhysicsPhysics Letters
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SNe observations in a meatball universe with a local void

2009

We study the impact of cosmic inhomogeneities on the interpretation of observations. We build an inhomogeneous universe model without dark energy that can confront supernova data and yet is reasonably well compatible with the Copernican Principle. Our model combines a relatively small local void, that gives apparent acceleration at low redshifts, with a meatball model that gives sizeable lensing (dimming) at high redshifts. Together these two elements, which focus on different effects of voids on the data, allow the model to mimic the concordance model.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Modular fluxes, elliptic genera, and weak gravity conjectures in four dimensions

2019

We analyse the Weak Gravity Conjecture for chiral four-dimensional F-theory compactifications with N=1 supersymmetry. Extending our previous work on nearly tensionless heterotic strings in six dimensions, we show that under certain assumptions a tower of asymptotically massless states arises in the limit of vanishing coupling of a U(1) gauge symmetry coupled to gravity. This tower contains super-extremal states whose charge-to-mass ratios are larger than those of certain extremal dilatonic Reissner-Nordstrom black holes, precisely as required by the Weak Gravity Conjecture. Unlike in six dimensions, the tower of super-extremal states does not always populate a charge sub-lattice. The main t…

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)FOS: Physical sciencesF-TheoryTopological Strings01 natural sciencesTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheorySuperstrings and Heterotic Strings0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsGauge symmetryPhysicsHeterotic string theory010308 nuclear & particles physicshep-thCharge (physics)SupersymmetryF-theoryHigh Energy Physics - Theory (hep-th)lcsh:QC770-798String DualityMirror symmetryParticle Physics - TheoryString dualityJournal of High Energy Physics
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Are pulsars born with a hidden magnetic field?

2015

The observation of several neutron stars in the center of supernova remnants and with significantly lower values of the dipolar magnetic field than the average radio-pulsar population has motivated a lively debate about their formation and origin, with controversial interpretations. A possible explanation requires the slow rotation of the proto-neutron star at birth, which is unable to amplify its magnetic field to typical pulsar levels. An alternative possibility, the hidden magnetic field scenario, considers the accretion of the fallback of the supernova debris onto the neutron star as responsible for the submergence (or screening) of the field and its apparently low value. In this paper …

Astrophysics::High Energy Astrophysical Phenomenageneral [Pulsars]FOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyPulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstronomía y AstrofísicaPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AstronomyAstronomy and Astrophysicsneutron [Stars]Magnetic fieldmagnetic field [Stars]Work (electrical)Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Horizons in a binary black hole merger II: Fluxes, multipole moments and stability

2020

We study in detail the dynamics and stability of marginally trapped surfaces during a binary black hole merger. This is the second in a two-part study. The first part studied the basic geometric aspects of the world tubes traced out by the marginal surfaces and the status of the area increase law. Here we continue and study the dynamics of the horizons during the merger, again for the head-on collision of two non-spinning black holes. In particular we follow the spectrum of the stability operator during the course of the merger for all the horizons present in the problem and implement systematic spectrum statistics for its analysis. We also study more physical aspects of the merger, namely …

General Relativity and Quantum Cosmology[PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmology
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Quantum gravitational decoherence from fluctuating minimal length and deformation parameter at the Planck scale

2020

Schemes of gravitationally induced decoherence are being actively investigated as possible mechanisms for the quantum-to-classical transition. Here, we introduce a decoherence process due to quantum gravity effects. We assume a foamy quantum spacetime with a fluctuating minimal length coinciding on average with the Planck scale. Considering deformed canonical commutation relations with a fluctuating deformation parameter, we derive a Lindblad master equation that yields localization in energy space and decoherence times consistent with the currently available observational evidence. Compared to other schemes of gravitational decoherence, we find that the decoherence rate predicted by our mo…

High Energy Physics - TheoryLength scaleQuantum decoherenceScienceQuantum physicsGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Quantum spacetime01 natural sciencesGeneral Relativity and Quantum CosmologyArticleGeneral Biochemistry Genetics and Molecular BiologyGravitation0103 physical sciencesMaster equation010306 general physicsQuantumCondensed Matter - Statistical MechanicsPhysicsMesoscopic physicsMultidisciplinaryStatistical Mechanics (cond-mat.stat-mech)010308 nuclear & particles physicsQGeneral ChemistryClassical mechanicsHigh Energy Physics - Theory (hep-th)Quantum gravityQuantum Physics (quant-ph)Theoretical physics
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Particles and energy fluxes from a CFT perspective

2004

We analyze the creation of particles in two dimensions under the action of conformal transformations. We focus our attention on Mobius transformations and compare the usual approach, based on the Bogolubov coefficients, with an alternative but equivalent viewpoint based on correlation functions. In the latter approach the absence of particle production under full Mobius transformations is manifest. Moreover, we give examples, using the moving-mirror analogy, to illustrate the close relation between the production of quanta and energy.

High Energy Physics - TheoryHigh Energy Physics - Theory (hep-th)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyPartícules (Física nuclear)
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Born-Infeld gravity and its functional extensions

2014

We investigate the dynamics of a family of functional extensions of the (Eddington-inspired) Born-Infeld gravity theory, constructed with the inverse of the metric and the Ricci tensor. We provide a generic formal solution for the connection and an Einstein-like representation for the metric field equations of this family of theories. For particular cases we consider applications to the early-time cosmology and find that non-singular universes with a cosmic bounce are very generic and robust solutions.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesClassical field theoryRicci flowGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyClassical unified field theoriesTheoretical physicsEinstein tensorsymbols.namesakeHigh Energy Physics - Theory (hep-th)Born–Infeld modelsymbolsRicci decompositionf(R) gravityRicci curvaturePhysical Review D
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