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Updated: Jun 12, 2026

Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Exploring binary-neutron-star-merger scenario of short-gamma-ray bursts by gravitational-wave observation
Kenta Kiuchi1, Yuichiro Sekiguchi, Masaru Shibata
1Department of Physics, Waseda University, 3-4-1 Okubo, Shinjuku-ku, Tokyo 169-8555, Japan.
Abstract:
We elucidate the feature of gravitational waves (GWs) from a binary-neutron-star merger collapsing to a black hole by general relativistic simulation. We show that GW spectrum imprints the coalescence dynamics, formation process of disk, equation of state for neutron stars, total masses, and mass ratio. A formation mechanism of the central engine of short-gamma-ray bursts, which are likely to be composed of a black hole and surrounding disk, therefore could be constrained by GW observation.
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