Greybody Factors for Black Holes in Four Dimensions: Particles with Spin

Details Greybody Factors for Black Holes in Four Dimensions: Particles with Spin Greybody Factors for Black Holes in Four Dimensions: Particles with Spin

1997-12-11

arxiv.org/abs/hep-th/9712118v1

Phys.Rev.D57:6297-6310,1998

Physics

High Energy Physics

High Energy Physics - Theory

25 pages, Latex

Scientific paper

10.1103/PhysRevD.57.6297

We compute the emission spectrum of minimally coupled particles with spin that are Hawking radiated from four dimensional black holes in string theory. For a range of the black hole parameters the result has a product structure that may be interpreted in terms of the respective right- and left-moving thermal correlation functions of an effective string model. For spin-one and spin-two particles a novel cancellation between contributions to the wave function is needed to ensure this outcome. The form of the spectra suggests that the four-dimensional effective string description is ``heterotic'': particles with spin are emitted from the right-moving sector, only.

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