On gravitational Casimir effect and Stefan-Boltzmann law at finite temperature (Q2318428)
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| Language | Label | Description | Also known as |
|---|---|---|---|
| English | On gravitational Casimir effect and Stefan-Boltzmann law at finite temperature |
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On gravitational Casimir effect and Stefan-Boltzmann law at finite temperature (English)
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15 August 2019
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Summary: 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.
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