Quasilocal Energy of FRW Universe

Details Quasilocal Energy of FRW Universe Quasilocal Energy of FRW Universe

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aps..aprg11006a&link_type=abstract

American Physical Society, 2009 APS April Meeting, May 2-5, 2009, abstract #G11.006

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Scientific paper

The quasilocal energy of an arbitrary FRW model of the universe is calculated. The results have the correct behavior in the small-sphere limit. Higher order corrections are found when comparing these results to classical calculations of cosmological energy. This example is unique in that it involves a non-stationary spacetime. As previous definitions are inadequate, a more precise definition of quasilocal energy is provided to accommodate non-stationary spacetimes.

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