Extra Spin-Rotation Coupling Effect in a Radiating Kerr Space-time

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dc.creatorWu, S. Q.
dc.creatorCai, X.
dc.date2001-04-24
dc.date.accessioned2026-07-07T03:25:51Z
dc.date.available2026-07-07T03:25:51Z
dc.descriptionSource-less wave equations are derived for massless scalar, neutrino and electromagnetic perturbations of a radiating Kerr space-time, and the Hawking radiation of massless particles with spin $s =0, 1/2$ and 1 in this geometry is investigated by using a method of the generalized tortoise coordinate transformation. An extra interaction between the spin of particles and the rotation of the hole displays in the thermal spectra of Hawking radiation of massless particles with spin $s = 1/2, 1$ in the evaporating Kerr space-time. The character of such effect is its obvious dependence on different helicity states of particles with higher spin.
dc.descriptionRevtex, 4 pages, no figure, submitted to Phys. Rev. Lett
dc.identifierhttps://arxiv.org/abs/gr-qc/0104074
dc.identifierhttp://arxiv.org/abs/gr-qc/0104074
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33871
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleExtra Spin-Rotation Coupling Effect in a Radiating Kerr Space-time
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