Gravitational Waveforms from Inspiralling Binaries
ORAL · M12
Presentations
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Evolution of the Carter constant for inspirals into a black hole: effects of the quadrupole and quadratic in spin
ORAL
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Authors
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Tanja Hinderer
Cornell University
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Eanna Flanagan
Cornell University
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Gravitational radiation reaction for inspiralling binaries - spin-spin effects to 3.5 post-Newtonian order
ORAL
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Authors
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Han Wang
Washington University in St.Louis
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Clifford Will
Washington University in St. Louis, Washington University in St.Louis, Washington University at St. Louis
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Spin-orbit Gravitational Radiation Reaction for Two-body Systems
ORAL
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Authors
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Jing Zeng
Washington University in St. Louis
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Clifford Will
Washington University in St. Louis, Washington University in St.Louis, Washington University at St. Louis
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Mapping spacetime geometry with gravitational wave observatories
ORAL
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Authors
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Chao Li
Caltech
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Geoffrey Lovelace
Caltech, California Institute of Technology
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Approximate methods for building extreme mass ratio inspiral waveforms
ORAL
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Authors
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Scott Hughes
Massachusetts Institute of Technology
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Accurate time--domain gravitational waveforms for extreme-mass-ratio binaries
ORAL
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Authors
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Gaurav Khanna
University of Massachusetts at Dartmouth
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Lior M. Burko
University of Alabama in Huntsville
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Gravitational waves from extreme mass ratio inspirals: A numerical model for the singular source term in the time domain
ORAL
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Authors
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Pranesh Adhyam Sundararajan
MIT
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Gaurav Khanna
University of Massachusetts, Dartmouth
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