Mostra el registre complet de l'element
Fabbri, Alessandro; Navarro Salas, José | |||
Aquest document és un/a article, creat/da en: 2005 | |||
Este documento está disponible también en : 10.1142/S0218271805007966 |
|||
|
|||
The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope that the divergent blueshift in frequency, associated to the presence of a black hole horizon, could be smoothed out for the energy. Using simple arguments based on Einstein's equivalence principle, we show that this is only possible if a black hole emits, in a first approximation, not just a single particle, but thermal radiation. | |||
Veure al catàleg Trobes | |||