|
Author |
Title ![sorted by Title field, descending order (down)](img/sort_desc.gif) |
Year |
Publication |
Volume |
Pages |
Links |
|
Anderson, P.R.; Siahmazgi, S.G.; Clark, R.D.; Fabbri, A. |
Method to compute the stress-energy tensor for a quantized scalar field when a black hole forms from the collapse of a null shell |
2020 |
Physical Review D |
102 |
125035 - 26pp |
|
|
Anderson, P.R.; Fabbri, A.; Balbinot, R. |
Low frequency gray-body factors and infrared divergences: Rigorous results |
2015 |
Physical Review D |
91 |
064061 - 18pp |
|
|
Anderson, P.R.; Clark, R.D.; Fabbri, A.; Good, M.R.R. |
Late time approach to Hawking radiation: Terms beyond leading order |
2019 |
Physical Review D |
100 |
061703 - 5pp |
|
|
Babichev, E.; Fabbri, A. |
Instability of black holes in massive gravity |
2013 |
Classical and Quantum Gravity |
30 |
152001 - 7pp |
|
|
Coutant, A.; Fabbri, A.; Parentani, R.; Balbinot, R.; Anderson, P.R. |
Hawking radiation of massive modes and undulations |
2012 |
Physical Review D |
86 |
064022 - 17pp |
|
|
Anderson, P.R.; Balbinot, R.; Fabbri, A.; Parentani, R. |
Hawking radiation correlations in Bose-Einstein condensates using quantum field theory in curved space |
2013 |
Physical Review D |
87 |
124018 - 18pp |
|
|
Balbinot, R.; Fabbri, A.; Mayoral, C. |
Hawking effect in BECs acoustic white holes |
2013 |
European Physical Journal Plus |
128 |
16 - 21pp |
|
|
Anderson, P.R.; Balbinot, R.; Fabbri, A.; Parentani, R. |
Gray-body factor and infrared divergences in 1D BEC acoustic black holes |
2014 |
Physical Review D |
90 |
104044 - 6pp |
|
|
Mauro, S.; Balbinot, R.; Fabbri, A.; Shapiro, I.L. |
Fourth derivative gravity in the auxiliary fields representation and application to the black-hole stability |
2015 |
European Physical Journal Plus |
130 |
135 - 8pp |
|
|
Carusotto, I.; Balbinot, R.; Fabbri, A.; Recati, A. |
Density correlations and analog dynamical Casimir emission of Bogoliubov phonons in modulated atomic Bose-Einstein condensates |
2010 |
European Physical Journal D |
56 |
391-404 |
|