TY - JOUR
T1 - Gravitational radiation from realistic relativistic stars
T2 - Odd-parity fluid perturbations
AU - Seidel, Edward
AU - Moore, Thomas
PY - 1987
Y1 - 1987
N2 - 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.
AB - 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.
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U2 - 10.1103/PhysRevD.35.2287
DO - 10.1103/PhysRevD.35.2287
M3 - Article
AN - SCOPUS:0001152753
VL - 35
SP - 2287
EP - 2296
JO - Physical review D: Particles and fields
JF - Physical review D: Particles and fields
SN - 1550-7998
IS - 8
ER -