Gravitational waves and the formation of accretion disks in the merger of black hole-neutron star binaries

Details Gravitational waves and the formation of accretion disks in the merger of black hole-neutron star binaries Gravitational waves and the formation of accretion disks in the merger of black hole-neutron star binaries

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aps..4cf.h5002b&link_type=abstract

American Physical Society, Fall 2009 Meeting of the Four Corners Section of the APS, October 23-24, 2009, abstract #H5.002

Physics

Scientific paper

We describe our work on the evolution of binary systems that consist of a neutron star and a black hole. With a detailed study of the evolution of such systems we are able to compute gravitational wave signatures for the late in spiral and merger phases for these binaries. In addition we explore some of the conditions required to create an accretion disk from such systems. We will present results for these gravitational wave signatures and accretion disks for neutron stars that are both magnetized and unmagnetized.

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