Sources of Gravitational Radiation

Presentations

• How big a bump can you make on a neutron star?

  ORAL

  April 17, 2005, 8:30 AM – April 17, 2005, 8:42 AM

  Authors

  • Benjamin J. Owen

    • Pennsylvania State University
    • Penn State

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• Gravitomagnetic Love numbers and neutron star stability

  ORAL

  April 17, 2005, 8:42 AM – April 17, 2005, 8:54 AM

  Authors

  • Marc Favata

    • Cornell University

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• Diagnosing low $T/W$ dynamical instabilities in differentially rotating stars

  ORAL

  April 17, 2005, 8:54 AM – April 17, 2005, 9:06 AM

  Authors

  • Shin Yoshida

    • Department of Physics, University of Wisconsin-Milwaukee

  • Motoyuki Saijo

    • Kyoto University, Japan

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• Astrophysical constraints on EMRIs

  ORAL

  April 17, 2005, 9:06 AM – April 17, 2005, 9:18 AM

  Authors

  • Shane L. Larson

    • CGWP, Penn State

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• Self force on a static scalar charge in Schwarzschild spacetime

  ORAL

  April 17, 2005, 9:18 AM – April 17, 2005, 9:30 AM

  Authors

  • Swapnil Tripathi

    • University of Wisconsin -- Milwaukee

  • Alan Wiseman

  • Tobias Keidl

  • John Friedman

    • University of Wisconsin-Milwaukee
    • University of Wisconsin - Milwaukee

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• Post-Minkowski action for point-particles and a helically symmetric binary solution

  ORAL

  April 17, 2005, 9:30 AM – April 17, 2005, 9:42 AM

  Authors

  • John Friedman

    • University of Wisconsin-Milwaukee
    • University of Wisconsin - Milwaukee

  • Koji Uryu

    • SISSA, Trieste, Italy
    • SISSA

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• Computing self-forces with the Quinn-Wald axioms

  ORAL

  April 17, 2005, 9:42 AM – April 17, 2005, 9:54 AM

  Authors

  • Alan Wiseman

  • John L. Friedman

  • Tobias Keidl

  • Swapnil Tripathi

    • University of Wisconsin -- Milwaukee

  • Samuel Gralla

    • Yale University

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