Search results for "Polytrope"

showing 2 items of 2 documents

Relativistic simulations of black hole-neutron star coalescence: the jet emerges

2014

We perform magnetohydrodynamic simulations in full general relativity (GRMHD) of a binary black hole-neutron star on a quasicircular orbit that undergoes merger. The binary mass ratio is 3:1, the black hole initial spin parameter $a/m=0.75$ ($m$ is the black hole Christodoulou mass) aligned with the orbital angular momentum, and the neutron star is an irrotational $\Gamma=2$ polytrope. About two orbits prior to merger (at time $t=t_B$), we seed the neutron star with a dynamically weak interior dipole magnetic field that extends into the stellar exterior. At $t=t_B$ the exterior has a low-density atmosphere with constant plasma parameter $\beta\equiv P_{\rm gas}/P_{\rm mag}$. Varying $\beta$…

AstrofísicaAngular momentumGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsMass ratioPolytropeBlack holeNeutron starSpace and Planetary ScienceAstronomiaAstrophysics::Earth and Planetary AstrophysicsGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena
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Pulsar spin-down luminosity: Simulations in general relativity

2014

Adopting our new method for matching general relativistic, ideal magnetohydrodynamics to its force-free limit, we perform the first systematic simulations of force-free pulsar magnetospheres in general relativity. We endow the neutron star with a general relativistic dipole magnetic field, model the interior with ideal magnetohydrodynamics, and adopt force-free electrodynamics in the exterior. Comparing the spin-down luminosity to its corresponding Minkowski value, we find that general relativistic effects give rise to a modest enhancement: the maximum enhancement for $n=1$ polytropes is $\sim 23\%$. Evolving a rapidly rotating $n=0.5$ polytrope we find an even greater enhancement of $\sim …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrofísicaNuclear and High Energy Physics010308 nuclear & particles physicsGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology3. Good healthLuminosityPolytropeNeutron starNumerical relativityDipolePulsar0103 physical sciencesAstronomiaRelativistic quantum chemistryAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysics
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