PreprintCC BY 4.0arXiv
Gravitational entropy in Petrov Type I spacetimes
Abstract
The gravitational entropy proposal of Clifton, Ellis and Tavakol (CET) is based on an effective energy momentum tensor formed by the algebraic decomposition of the 4th order Bel-Robinson tensor. So far the application of the CET proposal has been limited to spacetimes of Petrov types D and N for which this algebraic decomposition is unique. To address this limitation we examine in detail the effective energy momentum tensors that result from the algebraic decomposition of the Bel-Robinson tensor in Petrov type I spacetimes. As a test case we apply these results to the Szekeres models of class II, a Petrov type I analytic solution.
Versions
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BibTeX
@misc{sarma2026gravitational,
title = {{Gravitational entropy in Petrov Type I spacetimes}},
author = {Maharshi Sarma and Sebastián Nájera and Roberto A. Sussman},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2605.20611},
eprint = {2605.20611},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2605.20611},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Gravitational entropy in Petrov Type I spacetimes
AU - Maharshi Sarma
AU - Sebastián Nájera
AU - Roberto A. Sussman
PY - 2026
DA - 2026/10/04
PB - arXiv
DO - 10.48550/arxiv.2605.20611
UR - https://arxiv.org/abs/2605.20611
AB - The gravitational entropy proposal of Clifton, Ellis and Tavakol (CET) is based on an effective energy momentum tensor formed by the algebraic decomposition of the 4th order Bel-Robinson tensor. So far the application of the CET proposal has been limited to spacetimes of Petrov types D and N for which this algebraic decomposition is unique. To address this limitation we examine in detail the effective energy momentum tensors that result from the algebraic decomposition of the Bel-Robinson tensor in Petrov type I spacetimes. As a test case we apply these results to the Szekeres models of class II, a Petrov type I analytic solution.
ER -