On Gravitational Casimir Effect and Stefan-Boltzmann Law at Finite Temperature
Gravitons are described by the propagator in teleparallel gravity in nearly flat space-time. Finite temperature is introduced by using Thermofield Dynamics formalism. The gravitational Casimir effect and Stefan-Boltzmann law are calculated as a function of temperature. Then an equation of state for...
Saved in:
| Main Authors: | , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Wiley
2019-01-01
|
| Series: | Advances in High Energy Physics |
| Online Access: | http://dx.doi.org/10.1155/2019/2031075 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1832549306403389440 |
|---|---|
| author | S. C. Ulhoa A. F. Santos T. F. Furtado F. C. Khanna |
| author_facet | S. C. Ulhoa A. F. Santos T. F. Furtado F. C. Khanna |
| author_sort | S. C. Ulhoa |
| collection | DOAJ |
| description | Gravitons are described by the propagator in teleparallel gravity in nearly flat space-time. Finite temperature is introduced by using Thermofield Dynamics formalism. The gravitational Casimir effect and Stefan-Boltzmann law are calculated as a function of temperature. Then an equation of state for gravitons is determined. |
| format | Article |
| id | doaj-art-6c72b71bb1e8488a9d899b0777ae7075 |
| institution | Kabale University |
| issn | 1687-7357 1687-7365 |
| language | English |
| publishDate | 2019-01-01 |
| publisher | Wiley |
| record_format | Article |
| series | Advances in High Energy Physics |
| spelling | doaj-art-6c72b71bb1e8488a9d899b0777ae70752025-02-03T06:11:38ZengWileyAdvances in High Energy Physics1687-73571687-73652019-01-01201910.1155/2019/20310752031075On Gravitational Casimir Effect and Stefan-Boltzmann Law at Finite TemperatureS. C. Ulhoa0A. F. Santos1T. F. Furtado2F. C. Khanna3International Center of Physics, Instituto de Física, Universidade de Brasília, 70910-900 Brasília, DF, BrazilInstituto de Física, Universidade Federal de Mato Grosso, 78060-900 Cuiabá, Mato Grosso, BrazilInstituto de Física, Universidade de Brasília, 70910-900 Brasília, DF, BrazilDepartment of Physics and Astronomy, University of Victoria, BC V8P 5C2, CanadaGravitons are described by the propagator in teleparallel gravity in nearly flat space-time. Finite temperature is introduced by using Thermofield Dynamics formalism. The gravitational Casimir effect and Stefan-Boltzmann law are calculated as a function of temperature. Then an equation of state for gravitons is determined.http://dx.doi.org/10.1155/2019/2031075 |
| spellingShingle | S. C. Ulhoa A. F. Santos T. F. Furtado F. C. Khanna On Gravitational Casimir Effect and Stefan-Boltzmann Law at Finite Temperature Advances in High Energy Physics |
| title | On Gravitational Casimir Effect and Stefan-Boltzmann Law at Finite Temperature |
| title_full | On Gravitational Casimir Effect and Stefan-Boltzmann Law at Finite Temperature |
| title_fullStr | On Gravitational Casimir Effect and Stefan-Boltzmann Law at Finite Temperature |
| title_full_unstemmed | On Gravitational Casimir Effect and Stefan-Boltzmann Law at Finite Temperature |
| title_short | On Gravitational Casimir Effect and Stefan-Boltzmann Law at Finite Temperature |
| title_sort | on gravitational casimir effect and stefan boltzmann law at finite temperature |
| url | http://dx.doi.org/10.1155/2019/2031075 |
| work_keys_str_mv | AT sculhoa ongravitationalcasimireffectandstefanboltzmannlawatfinitetemperature AT afsantos ongravitationalcasimireffectandstefanboltzmannlawatfinitetemperature AT tffurtado ongravitationalcasimireffectandstefanboltzmannlawatfinitetemperature AT fckhanna ongravitationalcasimireffectandstefanboltzmannlawatfinitetemperature |