Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientist
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
Scientist
Cornell University
Cornell University, Ithaca, NY
Center for Radiophysics and Space Research and Departments of Astronomy and Physics, Cornell University, Ithaca, New York 14853, USA
Physics Department, Cornell University, Ithaca, New York 14853 and Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138
Cornell Univ., Ithaca, NY, US
Center for Radiophysics and Space Research and Departments of Astronomy Physics, Cornell University, Ithaca, New York 14853
Center for Radiophysics and Space Research, Cornell University, Ithaca, New York 14853
Center for Radiophysics and Space Research and Department of Astronomy and Department of Physics, Cornell University, Ithaca, New York 14853
Saul A. Teukolsky and Ira Wasserman are in the Departments of Physics and Astronomy, Space Sciences Building, Cornell University, Ithaca, New York 14853, USA Univ., USA
Cornell University, Ithaca, NY, US
Center for Radiophysics and Space Research
Center for Radiophysics and Space Research, and Departments of Astronomy and Physics, Cornell University, Ithaca, New York 14853, USA
Center for Radiophysics and Space Research, and Departments of Astronomy and Physics, Cornell University, Ithaca, New York 14853
Cornell Univ., Ithaca, NY
California Institute of Technology
Cornell Univ., Ithaca, NY.
Center for Radiophysics and Space Research, Department of Astronomy, and Department of Physics, Cornell University, Ithaca, New York 14853
California Institute of Technology, Pasadena, California 91109
California Institute of Technology, Pasadena, Calif.
Department of Physics, Center for Radiophysics and Space Research
Cornell University, Ithaca, NY; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Cornell University, Ithaca, N.Y.
Cornell
3D simulations of linearized scalar fields in Kerr spacetime
A hydrodynamical model for the explosion of a neutron star just below the minimum mass
A multidomain spectral method for solving elliptic equations
A Nonlinear Coupling Network to Simulate the Development of the r-mode Instablility in Neutron Stars I. Construction
A Nonlinear Coupling Network to Simulate the Development of the r-mode Instablility in Neutron Stars II. Dynamics
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