Model for the completeness of quasinormal modes of relativistic stellar oscillations

Details Model for the completeness of quasinormal modes of relativistic stellar oscillations Model for the completeness of quasinormal modes of relativistic stellar oscillations

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvl..68.1973p&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 68, March 30, 1992, p. 1973-1976.

Astronomy and Astrophysics

Astronomy

17

Astronomical Models, Relativistic Effects, Stellar Oscillations, Stellar Radiation, Cauchy Problem, Space-Time Functions, Stellar Interiors

Scientific paper

This paper presents a model which clarifies the extent to which quasi-normal modes can be complete, in the sense of normal modes. It is found that for a specific class of Cauchy data (that describing purely outgoing radiation) an expansion of the dynamics in terms of quasi-normal modes can be constructed. For more general Cauchy data, it is shown that no useful distinction is possible between data that do and do not stimulate quasi-normal oscillations.

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