dc.contributor.author |
Siahaan, Haryanto Mangaratua |
|
dc.date.accessioned |
2017-03-21T02:54:39Z |
|
dc.date.available |
2017-03-21T02:54:39Z |
|
dc.date.issued |
2016 |
|
dc.identifier |
DOI 10.1140/epjc/s10052-016-3986-z |
|
dc.identifier.uri |
http://hdl.handle.net/123456789/1054 |
|
dc.description |
EUROPEAN PHYSICAL JOURNAL C; (2016) 76 |
|
dc.description.abstract |
The discussions of Hawking radiation via tunneling
method have been performed extensively in the case
of scalar particles. Moreover, there are also several works
in discussing the tunneling method for Hawking radiation
by using higher spins, e.g. neutrino, photon, and gravitino,
in the background of static black holes. Interestingly, it is
found that the Hawking temperature for static black holes
using the higher spins particles has no difference compared
to the one computed using scalars. In this paper, we study
the Hawking radiation for a spherically symmetric and time
dependent black holes using the tunneling of Dirac particles,
photon, and gravitino. We find that the obtained Hawking
temperature is similar to the one derived in the tunneling
method by using scalars. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Springer Berlin Heidelberg |
en_US |
dc.relation.ispartofseries |
EUROPEAN PHYSICAL JOURNAL C; (2016) 76 |
|
dc.title |
Higher Spins Tunneling from a Time Dependent and Spherically Symmetric Black Hole |
en_US |
dc.type |
Journal Articles |
en_US |