Abstract
We discuss whether an appropriately defined dimensionless scalar function might be an acceptable candidate for the gravitational entropy, by explicitly considering Szekeres and Bianchi type VI h models that admit an isotropic singularity. We also briefly discuss other possible gravitational entropy functions, including an appropriate measure of the velocity dependent Bel-Robinson tensor.
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PACS: 04.20.-q 95.30.Sf 98.80.Jk
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Pelavas, N., Coley, A. Gravitational Entropy in Cosmological Models. Int J Theor Phys 45, 1258–1266 (2006). https://doi.org/10.1007/s10773-006-9124-1
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DOI: https://doi.org/10.1007/s10773-006-9124-1