The final fate of binary neutron stars: What happens after the merger?

Matthew D. Duez, Yuk Tung Liu, Stuart L. Shapiro, Branson C. Stephens, Masaru Shibata

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The merger of two neutron stars usually produces a remnant with a mass significantly above the single (nonrotating) neutron star maximum mass. In some cases, the remnant will be stabilized against collapse by rapid, differential rotation. MHD-driven angular momentum transport eventually leads to the collapse of the remnant's core, resulting in a black hole surrounded by a massive accretion torus. Here we present simulations of this process. The plausibility of generating short duration gamma ray bursts through this scenario is discussed.

Original languageEnglish (US)
Title of host publication11th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories - Proc. of the MG11 Meeting on General Relativity
PublisherWorld Scientific Publishing Co. Pte Ltd
Pages1609-1611
Number of pages3
ISBN (Print)9812834265, 9789812834263
DOIs
StatePublished - 2008
Event11th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories, MG 2006 - Berlin, Germany
Duration: Jul 23 2006Jul 29 2006

Publication series

Name11th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories - Proc. of the MG11 Meeting on General Relativity

Other

Other11th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories, MG 2006
Country/TerritoryGermany
CityBerlin
Period7/23/067/29/06

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

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