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First law of thermodynamics and Friedmann-like equations in braneworld cosmology

Xian-Hui Ge

Published 2007-03-28, updated 2007-05-14Version 3

We derive the Friedmann-like equations in braneworld cosmology by imposing the first law of thermodynamics and Bekenstein's area-entropy formula on the apparent horizon of a Friedmann-Roberston-Walker universe in both Randall-Sundrum II gravity and Dvali-Gabadadze-Porrati gravity models. Israel's boundary condition plays an important role in our calculations in both cases, besides the first law of thermodynamics and Bekenstein's area-entropy formula. The results indicate that thermodynamics on the brane world knows the behaviors of gravity.

Comments: 12 pages, no figures,Version 3; minor improvements
Journal: Phys.Lett.B651:49-53,2007
Categories: hep-th, astro-ph, gr-qc, hep-ph
Subjects: 04.50.+h, 98.80.-k
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