Published February 18, 2002 | Version v1
Journal article

Stringent neutron-star limits on large extra dimensions

  • 1. Max-Planck-Institut fuer Physik (Werner-Heisenberg-Institut), Foehringer Ring 6, 80805 Munich (Germany)
  • 2. NORDITA, Blegdamsvej 17, 2100 Copenhagen (Denmark)

Description

Supernovae (SNe) are copious sources for Kaluza-Klein (KK) gravitons which are generic for theories with large extra dimensions. These massive particles are produced with average velocities ≅0.5c so that many of them are gravitationally retained by the SN core. Every neutron star thus has a halo of KK gravitons which decay into νν-bar, e+e- , and γγ on time scales ≅109 years. The EGRET γ -flux limits (Eγ≅100 MeV ) for nearby neutron stars constrain the compactification scale for n=2 extra dimensions to M > or approx. 500 TeV , and M > or approx. 30 TeV for n=3 . The requirement that neutron stars are not excessively heated by KK decays implies M > or approx. 1700 TeV for n=2 , and M > or approx. 60 TeV for n=3

Additional details

Publishing Information

Journal Title
Physical Review Letters
Journal Volume
88
Journal Issue
7
Journal Page Range
p. 071301-071301.4
ISSN
0031-9007
CODEN
PRLTAO

Optional Information

Notes
(c) 2002 The American Physical Society