A practical formula for the radiated angular momentum

dc.creatorLousto, Carlos O.
dc.creatorZlochower, Yosef
dc.date2007-03-09
dc.date2007-06-10
dc.date.accessioned2026-07-07T11:21:52Z
dc.date.available2026-07-07T11:21:52Z
dc.descriptionWe present a simple formula for the radiated angular momentum based on a spin-weighted spherical harmonic decomposition of the Weyl scalar psi_4 representing outgoing radiation in the Kinnersley tetrad. We test our formula by measuring the radiated angular momentum from three simulations of non-spinning equal-mass black-hole binary with orbital angular momentum aligned along the x, y, and z axes respectively. We find that the radiated angular momentum agrees with the differences in the remnant horizon spins and the initial angular momentum for each system.
dc.description4 pages, revtex4, Accepted to PRD
dc.identifierhttps://arxiv.org/abs/gr-qc/0703061
dc.identifierhttp://arxiv.org/abs/gr-qc/0703061
dc.identifierPhys.Rev.D76:041502,2007
dc.identifierdoi:10.1103/PhysRevD.76.041502
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194390
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleA practical formula for the radiated angular momentum
dc.typetext

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