2015Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fieldsOpen access

Black hole-neutron star binary merger: Dependence on black hole spin orientation and equation of state

Kyohei Kawaguchi, Koutarou Kyutoku, Hiroyuki Nakano, H. Okawa, Masaru Shibata, Keisuke Taniguchi

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Abstract

Black hole mergers with neutron stars are promising sources of gravitational-wave signals for the new crop of gravitational wave detectors. The impressive numerical relativity simulations carried out in this paper illustrate what to expect when the orientation of the black hole spin and the equation of state of the neutron star are properly taken into account.

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What this paper is about

Black hole mergers with neutron stars are promising sources of gravitational-wave signals for the new crop of gravitational wave detectors. The impressive numerical relativity simulations carried out in this paper illustrate what to expect when the orientation of the black hole spin and the equation of state of the neutron star are properly taken into account.

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Available abstract

Black hole mergers with neutron stars are promising sources of gravitational-wave signals for the new crop of gravitational wave detectors. The impressive numerical relativity simulations carried out in this paper illustrate what to expect when the orientation of the black hole spin and the equation of state of the neutron star are properly taken into account.

Key concepts: Physics, Dimensionless quantity, RADIUS, Neutron star, Black hole (networking), Tilt (camera), Spin (aerodynamics), Equation of state

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