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http://hdl.handle.net/2248/2264
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DC Field | Value | Language |
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dc.contributor.author | Rothman, Tony | - |
dc.contributor.author | Anninos, Peter | - |
dc.date.accessioned | 2008-05-05T12:08:52Z | - |
dc.date.available | 2008-05-05T12:08:52Z | - |
dc.date.issued | 1997 | - |
dc.identifier.citation | BASI, Vol. 25, No. 3, pp. 395 - 399 | en |
dc.identifier.uri | http://hdl.handle.net/2248/2264 | - |
dc.description.abstract | We develop a formulation of the entropy of the gravitational field by adopting the statistical mechanics expression for entropy S = lnΩ, where Ω is the phase space of the field bounded by a Hamiltonian. Phase space is calculated for gravitational waves and radiation and density perturbations in expanding FLRW spacetimes, attributing entropy to a lack of knowledge in the exact field configuration. In all cases, S behaves monotonically as required for a definition of gravitational entropy and is a good measure of inhomogeneity. It also reduces to black-hole entropy under appropriate circumstances. | en |
dc.format.extent | 388428 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of India | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1997BASI...25..395R | en |
dc.subject | Black-Hole entropy | en |
dc.subject | Spacetimes | en |
dc.subject | Measure of Inhomogeneity | en |
dc.title | Entropy of the gravitational field | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
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Rothman.pdf | 379.32 kB | Adobe PDF | View/Open |
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