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.
Volume 294 -
The 3rd International Symposium on “Quest for the Origin of Particles and the Universe" (KMI2017) -
Poster Presentations
Relativistic Stars in Massive Gravity
Full text:
pdf
Pre-published on:
November 22, 2017
Published on:
November 24, 2017
Abstract
DOI: https://doi.org/10.22323/1.294.0041
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.
Open Access
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.