Search results for "General Relativity and Cosmology"

showing 8 items of 8 documents

New horizons for fundamental physics with LISA

2022

K. G. Arun et al.

AstrofísicaPROTOPLANET MIGRATIONFísica-Modelos matemáticosPhysics and Astronomy (miscellaneous)gr-qcFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)GRAVITATIONAL-WAVEShorizonFundamental physicGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGravitational wavesLIGO (Observatory)Tests of general relativitySettore FIS/05 - Astronomia e AstrofisicaDARK-MATTERFísica matemáticaKOZAI MECHANISMHigh Energy PhysicsGENERAL-RELATIVITYFundamental physics; Gravitational waves; LISA; Tests of general relativityFundamental physicsPRIMORDIAL BLACK-HOLESLISAScience & TechnologyGeneral Relativity and Cosmology83CXXPhysicsgravitation: interactiongravitational radiationFísicaCompactQUANTUM-GRAVITYPhysical SciencesAstronomia[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]fundamental physics; gravitational waves; LISA; test of general relativityMODIFIED GRAVITYtest of general relativityGravitational waveMULTIPOLE MOMENTSHUBBLE CONSTANT
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Ricci Reheating

2019

We present a model for viable gravitational reheating involving a scalar field directly coupled to the Ricci curvature scalar. Crucial to the model is a period of kination after inflation, which causes the Ricci scalar to change sign thus inducing a tachyonic effective mass $m^{2} \propto -H^2$ for the scalar field. The resulting tachyonic growth of the scalar field provides the energy for reheating, allowing for temperatures high enough for thermal leptogenesis. Additionally, the required period of kination necessarily leads to a blue-tilted primordial gravitational wave spectrum with the potential to be detected by future experiments. We find that for reheating temperatures $T_{\rm RH} \l…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsGeneral Relativity and Cosmologygr-qcFOS: Physical sciencesAstronomy and Astrophysicshep-phAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)7. Clean energy01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesastro-ph.CO010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsParticle Physics - Phenomenology
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Robust constraint on Lorentz violation using Fermi-LAT gamma-ray burst data

2018

Models of quantum gravity suggest that the vacuum should be regarded as a medium with quantum structure that may have non-trivial effects on photon propagation, including the violation of Lorentz invariance. Fermi Large Area Telescope (LAT) observations of gamma-ray bursts (GRBs) are sensitive probes of Lorentz invariance, via studies of energy-dependent timing shifts in their rapidly-varying photon emissions. In this paper we analyze the Fermi-LAT measurements of high-energy gamma rays from GRBs with known redshifts, allowing for the possibility of energy-dependent variations in emission times at the sources as well as a possible non-trivial refractive index in vacuo for photons. We use st…

Astrophysics and AstronomyPhotongr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsLorentz covariance01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesSensitivity (control systems)010306 general physicsParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HE010308 nuclear & particles physicsGeneral Relativity and CosmologyGamma rayhep-phRedshiftHigh Energy Physics - PhenomenologyAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burstEnergy (signal processing)Fermi Gamma-ray Space Telescope
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Quantum transport and the phase space structure of the Wightman functions

2019

We study the phase space structure of exact quantum Wightman functions in spatially homogeneous, temporally varying systems. In addition to the usual mass shells, the Wightman functions display additional coherence shells around zero frequency $k_0=0$, which carry the information of the local quantum coherence of particle-antiparticle pairs. We find also other structures, which encode non-local correlations in time, and discuss their role and decoherence. We give a simple derivation of the cQPA formalism, a set of quantum transport equations, that can be used to study interacting systems including the local quantum coherence. We compute quantum currents created by a temporal change in a par…

High Energy Physics - TheoryNuclear and High Energy PhysicsAstrophysics and AstronomyLEPTOGENESISCosmology and Nongalactic Astrophysics (astro-ph.CO)Quantum decoherencegr-qcFOS: Physical sciencesSemiclassical physicsGeneral Relativity and Quantum Cosmology (gr-qc)114 Physical sciences01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityThermal Field Theory010306 general physicsQuantumELECTROWEAK BARYOGENESISParticle Physics - PhenomenologyPhysicsThermal quantum field theory010308 nuclear & particles physicsGeneral Relativity and Cosmologyhep-thhep-phFermionFERMIONSBaryogenesisHigh Energy Physics - PhenomenologyCP violationClassical mechanicsHigh Energy Physics - Theory (hep-th)Phase spaceastro-ph.COlcsh:QC770-798Quantum Dissipative SystemsParticle Physics - TheoryAstrophysics - Cosmology and Nongalactic AstrophysicsCoherence (physics)
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Cosmological Constant and Local Gravity

2010

We discuss the linearization of Einstein equations in the presence of a cosmological constant, by expanding the solution for the metric around a flat Minkowski space-time. We demonstrate that one can find consistent solutions to the linearized set of equations for the metric perturbations, in the Lorentz gauge, which are not spherically symmetric, but they rather exhibit a cylindrical symmetry. We find that the components of the gravitational field satisfying the appropriate Poisson equations have the property of ensuring that a scalar potential can be constructed, in which both contributions, from ordinary matter and Lambda > 0, are attractive. In addition, there is a novel tensor potentia…

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)De Sitter spaceFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyDe Sitter universeLinearized gravity0103 physical sciencesMinkowski spaceSchwarzschild metric010303 astronomy & astrophysicsMathematical physicsPhysicsInhomogeneous cosmology010308 nuclear & particles physicsGeneral Relativity and CosmologyFísicaClassical mechanicsLorenz gauge conditionHigh Energy Physics - Theory (hep-th)Einstein field equationsAstrophysics - Cosmology and Nongalactic Astrophysics
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Limits on neutrino Lorentz violation from multimessenger observations of TXS 0506+056

2019

The observation by the IceCube Collaboration of a high-energy ($E \gtrsim 200$ TeV) neutrino from the direction of the blazar TXS 0506+056 and the coincident observations of enhanced $\gamma$-ray emissions from the same object by MAGIC and other experiments can be used to set stringent constraints on Lorentz violation in the propagation of neutrinos that is linear in the neutrino energy: $\Delta v = - E/M_1$, where $\Delta v$ is the deviation from the velocity of light, and $M_1$ is an unknown high energy scale to be constrained by experiment. Allowing for a difference in neutrino and photon propagation times of $\sim 10$ days, we find that $M_1 \gtrsim 3 \times 10^{16}$ GeV. This improves …

High Energy Physics - TheoryNuclear and High Energy PhysicsHigh energyParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Lorentz transformationgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesComputer Science::Digital LibrariesGeneral Relativity and Quantum CosmologyIceCubesymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Coincident0103 physical sciences010306 general physicsBlazarParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEMultimessenger010308 nuclear & particles physicsGeneral Relativity and Cosmologyhep-thHigh Energy Physics::PhenomenologyLorentz violationGamma rayhep-phlcsh:QC1-999High Energy Physics - PhenomenologyPhoton propagationHigh Energy Physics - Theory (hep-th)Astrophysical neutrinosVelocity of lightsymbolsastro-ph.COHigh Energy Physics::ExperimentNeutrinoTXS 0506+056Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - Theorylcsh:PhysicsBlazarsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters
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Space-Time Foam may Violate the Principle of Equivalence

2003

The interactions of different particle species with the foamy space-time fluctuations expected in quantum gravity theories may not be universal, in which case different types of energetic particles may violate Lorentz invariance by varying amounts, violating the equivalence principle. We illustrate this possibility in two different models of space-time foam based on D-particle fluctuations in either flat Minkowski space or a stack of intersecting D-branes. Both models suggest that Lorentz invariance could be violated for energetic particles that do not carry conserved charges, such as photons, whereas charged particles such electrons would propagate in a Lorentz-inavariant way. The D-brane …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGeneral Relativity and CosmologySpace timeAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsElectronGeneral Relativity and Quantum Cosmology (gr-qc)Lorentz covarianceAstrophysicsGeneral Relativity and Quantum CosmologyAtomic and Molecular Physics and OpticsCharged particleGluonHigh Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Minkowski spaceQuantum gravityPhenomenology (particle physics)
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Cuckoo's Eggs in Neutron Stars: Can LIGO Hear Chirps from the Dark Sector?

2018

We explore in detail the possibility that gravitational wave signals from binary inspirals are affected by a new force that couples only to dark matter particles. We discuss the impact of both the new force acting between the binary partners as well as radiation of the force carrier. We identify numerous constraints on any such scenario, ultimately concluding that observable effects on the dynamics of binary inspirals due to such a force are not possible if the dark matter is accrued during ordinary stellar evolution. Constraints arise from the requirement that the astronomical body be able to collect and bind at small enough radius an adequate number of dark matter particles, from the requ…

Nuclear and High Energy PhysicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativitymedia_common.quotation_subjectgr-qcDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsStellar evolutionmedia_commonParticle Physics - PhenomenologyPhysics010308 nuclear & particles physicsStar formationGravitational wavehep-exGeneral Relativity and CosmologyFifth forcehep-phCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyNeutron starBeyond Standard Modelastro-ph.COlcsh:QC770-798Particle Physics - ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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