Do collapsed boson stars result in new types of black holes? I Peña, D Sudarsky Classical and Quantum Gravity 14 (11), 3131, 1997 | 94 | 1997 |
Nonparadoxical loss of information in black hole evaporation in a quantum collapse model SK Modak, L Ortíz, I Pena, D Sudarsky Physical Review D 91 (12), 124009, 2015 | 47 | 2015 |
Black hole evaporation: information loss but no paradox SK Modak, L Ortíz, I Pena, D Sudarsky General Relativity and Gravitation 47, 1-55, 2015 | 34 | 2015 |
Black hole evaporation: information loss but no paradox SK Modak, L Ortíz, I Pena, D Sudarsky General Relativity and Gravitation 47, 1-55, 2015 | 34 | 2015 |
On the possibility of measuring the Unruh effect I Peña, D Sudarsky Foundations of Physics 44, 689-708, 2014 | 20 | 2014 |
Numerical evidence against black holes with non-minimally coupled scalar hair I Peña, D Sudarsky Classical and Quantum Gravity 18 (8), 1461, 2001 | 11 | 2001 |
On a puzzle about bremsstrahlung as described by coaccelerated observers I Pena, C Chryssomalakos, A Corichi, D Sudarsky Physical Review D 72 (8), 084018, 2005 | 5 | 2005 |
Non-paradoxical loss of information in black hole evaporation SK Modak, L Ortíz, I Pena, D Sudarsky arXiv preprint arXiv:1408.3062, 2014 | 2 | 2014 |