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
Abstract
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Kyohei Kawaguchi, Koutarou Kyutoku, Hiroyuki Nakano, H. Okawa, Masaru Shibata, Keisuke Taniguchi
Abstract
Open-access reader
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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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