Gravitational radiation from realistic relativistic stars: Odd-parity fluid perturbations

Edward Seidel, Thomas Moore

Research output: Contribution to journalArticlepeer-review

Abstract

Odd-parity gravitational perturbations of a spherically symmetric background are studied in the linearized Einstein theory. A variety of collapse models, based on a May-White hydrodynamic code, are investigated, simulating dust collapse and stellar core collapse typical of type-II supernova models. Numerical results are presented, showing that in this linearized problem a typical core collapse may radiate up to 10-7 Mc2 in gravitational-wave energy.

Original languageEnglish (US)
Pages (from-to)2287-2296
Number of pages10
JournalPhysical Review D
Volume35
Issue number8
DOIs
StatePublished - 1987
Externally publishedYes

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

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