Semiclassical analysis of the scalar geodesic synchrotron radiation in Kerr spacetime

Caio F. B. Macedo, Luís C. B. Crispino, and Vitor Cardoso
Phys. Rev. D 86, 024002 – Published 3 July 2012

Abstract

We analyze the scalar synchrotron radiation emitted by a source in circular orbits, stable and unstable, direct and retrograde, around a rotating black hole within the framework of quantum field theory in curved spacetimes at tree level. We also analyze the radiation which escapes to infinity, showing that, in accordance with superradiance, it can be amplified for the case of direct orbits.

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  • Received 13 April 2012

DOI:https://doi.org/10.1103/PhysRevD.86.024002

© 2012 American Physical Society

Authors & Affiliations

Caio F. B. Macedo* and Luís C. B. Crispino

  • Faculdade de Física, Universidade Federal do Pará, 66075-110, Belém, PA, Brazil

Vitor Cardoso

  • CENTRA, Departamento de Física, Instituto Superior Técnico, Universidade Técnica de Lisboa—UTL, Av. Rovisco Pais 1, 1049 Lisboa, Portugal
  • Department of Physics and Astronomy, The University of Mississippi, University, Mississippi 38677, USA

  • *caiomacedo@ufpa.br
  • crispino@ufpa.br
  • vitor.cardoso@ist.utl.pt

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Issue

Vol. 86, Iss. 2 — 15 July 2012

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