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2010

On the falloff of radiated energy in black hole spacetimes

Burko, Lior M., Hughes, Scott A.

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Understand

The goal of much research in relativity is to understand gravitational waves generated by a strong-field dynamical spacetime.

Quantities of particular interest for many calculations are the Weyl scalar $\psi_4$, which is simply related to the flux of gravitational waves far from the source, and the flux of energy carried to distant observers, $\dot E$.
Conservation laws guarantee that, in asympotically flat spacetimes, $\psi_4 \propto 1/r$ and $\dot E \propto 1/r^2$ as $r \to \infty$.
Most calculations extract these quantities at some finite extraction radius.

On the falloff of radiated energy in black hole spacetimes · Around

Built on

E. T. Newman and T. W. J. Unti, J. Math. Phys. 3
1962
Earlier work this paper cites.
E. Newman and R. Penrose, J. Math. Phys. 3
1962
Earlier work this paper cites.
W. Kinnersley, J. Math. Phys. 6
1969
Earlier work this paper cites.
S. A. Teukolsky, Astrophys. J. 185
1973
Earlier work this paper cites.

Similar

M. Sasaki and T. Nakamura, Prog. Theor. Phys. 67
1973
Cited alongside, same era.
S. A. Hughes, Phys. Rev. D 61
2000
Cited alongside, same era.
C. Beetle and L. M. Burko, Phys. Rev. Lett. 89
2003
Cited alongside, same era.
A. Nerozzi, C. Beetle, M. Bruni, L. M. Burko, and D. Pollney, Phys. Rev. D 72
Original
2005
Cited alongside, same era.

Then

P. A. Sundararajan, G. Khanna, and S. A. Hughes, Phys. Rev. D 76
2007
Later among the works it cites.
J. L. Barton, D. J. Lazar, D. J. Kennefick, G. Khanna, and L. M. Burko, Phys. Rev. D 78
2008
Later among the works it cites.
J. Winicour, Living Rev. Relativity 12
2009
Later among the works it cites.

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