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astro-phDec 9, 2008
8
citations (OpenAlex)
authors
  • J. Barbieri
  • G. Chapline
institutions
  • Lawrence Livermore National Laboratory
  • Naval Air Warfare Center Weapons Division
arXiv abstractPDF
paper

A signature for the absence of event horizons

arXiv:0812.0833 · doi:10.1016/j.physletb.2012.02.003

Abstract

A sharp dip in the spectrum of gamma rays coming from compact objects below 70 MeV would be an unambiguous signal that compact astrophysical objects have a physical surface, and there is no event horizon. Observation of this effect would open a window for the empirical study of Planck scale physics

arXiv comment6 pages, 2 figures

References in corpus (7)

  • Advection-Dominated Accretion and the Black Hole Event Horizon
  • Early SPI/INTEGRAL measurements of galactic 511 keV line emission from positron annihilation
  • Stringent Constraint on Galactic Positron Production
  • Early SPI/INTEGRAL contraints on the morphology of the 511 keV line emission in the 4th galactic quadrant
  • Quantum Phase Transitions and the Breakdown of Classical General Relativity
  • Gamma-ray continuum emission from the inner Galactic region as observed with INTEGRAL/SPI
  • Stochastic Acceleration in the Galactic Center HESS Source

Cited by in corpus (3)

  • Effect of massive graviton on dark energy star structure
  • Model-independent constraints on r^-3 extra-interactions from orbital motions
  • Spherically symmetric vacuum solutions arising from trace dynamics modifications to gravitation
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