Main Image
Volume 294 - The 3rd International Symposium on “Quest for the Origin of Particles and the Universe" (KMI2017) - Poster Presentations
Relativistic Stars in Massive Gravity
M. Yamazaki,* T. Katsuragawa, S.i. Nojiri, S.D. Odintsov
*corresponding author
Full text: pdf
Pre-published on: 2017 November 22
Published on: 2017 November 24
Abstract
Maximal mass of relativistic star is one of the quantities
which may distinguish modified gravity theories
because it is strongly influenced by the short-range behavior of gravitation.
We derive modified Tolman-Oppenheimer-Volkoff equations for the de Rham-Gabadadze-Tolley (dRGT) massive gravity with the flat reference metric. We find that new constraint equations appear and that the maximum masses in the minimal model of dRGT massive gravity become smaller than those in the general relativity.
DOI: https://doi.org/10.22323/1.294.0041
Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.