Search results for "gravitation: collapse"

showing 2 items of 2 documents

Method to compute the stress-energy tensor for a quantized scalar field when a black hole forms from the collapse of a null shell

2020

A method is given to compute the stress-energy tensor for a massless minimally coupled scalar field in a spacetime where a black hole forms from the collapse of a spherically symmetric null shell in four dimensions. Part of the method involves matching the modes for the in vacuum state to a complete set of modes in Schwarzschild spacetime. The other part involves subtracting from the unrenormalized expression for the stress-energy tensor when the field is in the in vacuum state, the corresponding expression when the field is in the Unruh state and adding to this the renormalized stress-energy tensor for the field in the Unruh state. The method is shown to work in the two-dimensional case wh…

High Energy Physics - Theorydimension: 4space-time: SchwarzschildField (physics)Vacuum stateFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)coupling: scalarcoupling: minimal01 natural sciencesGeneral Relativity and Quantum Cosmologyrenormalizationvacuum stateGeneral Relativity and Quantum Cosmologyblack hole: formation0103 physical sciencesStress–energy tensorsymmetry: rotationTensordimension: 2010306 general physicsMathematical physicsPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsshell modelfield theory: scalarfield theory in curved spacegravitation: collapseBlack holeFormal aspects of field theoryUnruh effectHigh Energy Physics - Theory (hep-th)tensor: energy-momentum[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]quantizationSchwarzschild radiusScalar fieldPhysical Review D
researchProduct

Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae

2021

The eventual detection of gravitational waves from core-collapse supernovae (CCSN) will help improve our current understanding of the explosion mechanism of massive stars. The stochastic nature of the late post-bounce gravitational wave signal due to the non-linear dynamics of the matter involved and the large number of degrees of freedom of the phenomenon make the source parameter inference problem very challenging. In this paper we take a step towards that goal and present a parameter estimation approach which is based on the gravitational waves associated with oscillations of proto-neutron stars (PNS). Numerical simulations of CCSN have shown that buoyancy-driven g-modes are responsible …

noiseGravitational-wave observatorygravitational radiation: stochasticAstrophysics::High Energy Astrophysical Phenomenaprotoneutron starDegrees of freedom (physics and chemistry)FOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciences7. Clean energyGeneral Relativity and Quantum CosmologyEinstein Telescopeeffect: nonlinearsupernova0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]LIGOnumerical calculations010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)equation of statePhysicsSolar massmass: solarEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationoscillationgravitational radiation detectorLIGOgravitation: collapsedetector: sensitivitystar: massiveSupernovaStarswave: modelVIRGO13. Climate actiongravitational radiation: emission[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]galaxyAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics and astroparticle physics
researchProduct