On the structure of gravitational wave bursts: Implosion with finite kinetic energy

Details On the structure of gravitational wave bursts: Implosion with finite kinetic energy On the structure of gravitational wave bursts: Implosion with finite kinetic energy

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phlb...98..381f&link_type=abstract

Physics Letters B, Volume 98, Issue 5, p. 381-384.

Physics

14

Scientific paper

The structure of a gravitational wave burst emitted by a particle radially imploding into a Schwarzschild black hole with a finite kinetic energy at infinity is analyzed in the framework of the Zerilli-Regge-Wheeler formalism. The three components of the burst, (a) precursor, (b) main burst, (c) ringing tail, are analyzed and the results compared and contrasted with those obtained for a particle initially at rest at infinity. The ringing tail of the burst is studied in terms of the normal modes of a black hole.

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