Gamma Rays from the Galactic Bulge and Large Extra Dimensions

Michel Cassé, Jacques Paul, Gianfranco Bertone, and Günter Sigl
Phys. Rev. Lett. 92, 111102 – Published 19 March 2004

Abstract

An intriguing feature of extra dimensions is the possible production of Kaluza–Klein gravitons by nucleon-nucleon bremsstrahlung, in the course of core collapse of massive stars, with gravitons then being trapped around the newly born neutron stars and decaying into two gamma rays, making neutron stars gamma-ray sources. We strengthen the limits on the radius of compactification of extra dimensions for a small number n of them, or alternatively the fundamental scale of quantum gravity, considering the gamma-ray emission of the whole population of neutron stars sitting in the Galactic bulge, instead of the closest member of this category. For n=1 the constraint on the compactification radius is R<400   μm.

  • Received 15 September 2003

DOI:https://doi.org/10.1103/PhysRevLett.92.111102

©2004 American Physical Society

Authors & Affiliations

Michel Cassé1,2, Jacques Paul1,3,*, Gianfranco Bertone2, and Günter Sigl2,3

  • 1DAPNIA/Service d’Astrophysique, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
  • 2Institut d’Astrophysique de Paris, 98bis, Boulevard Arago, 75014 Paris, France
  • 3Fédération de Recherche Astroparticule et Cosmologie, Université Paris 7, 2 place Jussieu, 75251 Paris Cedex 05, France

  • *Corresponding author. Electronic address: jpaul@cea.fr

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Issue

Vol. 92, Iss. 11 — 19 March 2004

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