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

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

2001-04-24

arxiv.org/abs/gr-qc/0104074v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Revtex, 4 pages, no figure, submitted to Phys. Rev. Lett

Scientific paper

Source-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.

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