ar X iv : 0 70 8 . 42 02 v 2 [ as tr o - ph ] 2 7 Se p 20 07 Gravitational waves from black - hole mergers
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چکیده
By JOHN G. BAKER , WILL IAM D. BOGGS , JOAN M. CENTRELLA , BERNARD J. KELLY , SEAN T. McWILLIAMS , AND JAMES R. v an METER Gravitational Astrophysics Laboratory, NASA Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, USA University of Maryland, Department of Physics, College Park, MD 20742, USA Center for Space Science & Technology, University of Maryland Baltimore County, Physics Department, 1000 Hilltop Circle, Baltimore, MD 21250, USA
منابع مشابه
ar X iv : 0 70 8 . 42 02 v 1 [ as tr o - ph ] 3 0 A ug 2 00 7 Gravitational waves from black -
By JOHN G. BAKER , WILL IAM D. BOGGS , JOAN M. CENTRELLA , BERNARD J. KELLY , SEAN T. McWILLIAMS , AND JAMES R. v an METER Gravitational Astrophysics Laboratory, NASA Goddard Space Flight Center, 8800 Greenbelt Rd., Greenbelt, MD 20771, USA University of Maryland, Department of Physics, College Park, MD 20742, USA Center for Space Science & Technology, University of Maryland Baltimore County, P...
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The dynamics of galactic nuclei reflects the presence of supermassive black holes (SBHs) in many ways. Single SBHs act as sinks, destroying a mass in stars equal to their own mass in roughly one relaxation time and forcing nuclei to expand. Formation of binary SBHs displaces a mass in stars roughly equal to the binary mass, creating low-density cores and ejecting hyper-velocity stars. Gravitati...
متن کاملA “nu” look at gravitational waves: The black hole birth rate from neutrinos combined with the merger rate from LIGO
Wemake projections for measuring the black hole birth rate from the diffuse supernova neutrino background (DSNB) by future neutrino experiments, and constrain the black hole merger fraction , when combined with information on the black hole merger rate from gravitational wave experiments such as LIGO. The DSNB originates from neutrinos emitted by all the supernovae in the Universe, and is expec...
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تاریخ انتشار 2008