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 language | English (US) |
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Pages (from-to) | 2287-2296 |
Number of pages | 10 |
Journal | Physical Review D |
Volume | 35 |
Issue number | 8 |
DOIs | |
State | Published - 1987 |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)