Search results for "Cowling"

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Towards asteroseismology of core-collapse supernovae with gravitational-wave observations – I. Cowling approximation

2017

Gravitational waves from core-collapse supernovae are produced by the excitation of different oscillation modes in the protoneutron star (PNS) and its surroundings, including the shock. In this work we study the relationship between the post-bounce oscillation spectrum of the PNS–shock system and the characteristic frequencies observed in gravitational-wave signals from core-collapse simulations. This is a fundamental first step in order to develop a procedure to infer astrophysical parameters of the PNS formed in core-collapse supernovae. Our method combines information from the oscillation spectrum of the PNS, obtained through linear perturbation analysis in general relativity of a backgr…

Astrophysics::High Energy Astrophysical Phenomenaoscillations [Stars]general [Supernovae]Collapse (topology)FOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesAsteroseismologyGeneral Relativity and Quantum CosmologyGravitational waves0103 physical sciencesCuriemedia_common.cataloged_instanceAstrophysics::Solar and Stellar AstrophysicsEuropean unionCowling010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)media_commonAstronomía y AstrofísicaPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)numerical [Methods]010308 nuclear & particles physicsGravitational waveAsteroseismologyAstronomyAstronomy and Astrophysicsneutron [Stars]SupernovaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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Gravitational Waves from Rotating Proto-Neutron Stars

2004

We study the effects of rotation on the quasi normal modes (QNMs) of a newly born proto neutron star (PNS) at different evolutionary stages, until it becomes a cold neutron star (NS). We use the Cowling approximation, neglecting spacetime perturbations, and consider different models of evolving PNS. The frequencies of the modes of a PNS are considerably lower than those of a cold NS, and are further lowered by rotation; consequently, if QNMs were excited in a sufficiently energetic process, they would radiate waves that could be more easily detectable by resonant-mass and interferometric detectors than those emitted by a cold NS. We find that for high rotation rates, some of the g-modes bec…

PhysicsPhysics and Astronomy (miscellaneous)SpacetimeGravitational waveAstrophysics (astro-ph)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsAstrophysicsRotationInstabilityGeneral Relativity and Quantum CosmologyNeutron starNormal modeExcited stateAstrophysics::Solar and Stellar AstrophysicsCowling
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