6533b835fe1ef96bd129ff80
RESEARCH PRODUCT
Short distances, black holes, and TeV gravity
Iván AgullóGonzalo J. OlmoJose Navarro-salassubject
High Energy Physics - TheoryPhysicsGravity (chemistry)High Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHawkingHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsAstrophysics::High Energy Astrophysical PhenomenaSpectrum (functional analysis)Semiclassical physicsFOS: Physical sciencesdescription
The Hawking effect can be rederived in terms of two-point functions and in such a way that it makes it possible to estimate, within the conventional semiclassical theory, the contribution of ultrashort distances at $I^+$ to the Planckian spectrum. Thermality is preserved for black holes with $��l_P << 1$. However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2007-01-17 |