Higher Spins Tunneling from a Time Dependent and Spherically Symmetric Black Hole

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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


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