Quasilocal Energy in FRW Cosmology

Details Quasilocal Energy in FRW Cosmology Quasilocal Energy in FRW Cosmology

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..aprx14003a&link_type=abstract

American Physical Society, APS April Meeting 2010, February 13-16, 2010, abstract #X14.003

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The quasilocal energy (QLE) of a generic FRW model of the universe is calculated. The calculation is performed using several different formulations of QLE and the results are compared. The non-stationary nature of this example serves to differentiate competing formulations of QLE. Certain formulations are shown to have incorrect classical limits. Also, the QLE is used to calculate the entropy of several specific FRW models, providing a check on other methods of entropy calculation. )

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