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Static, spherically symmetric objects in Type-II minimally modified gravity

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arxiv 2110.14496 v1 pith:NMC34QXT submitted 2021-10-27 gr-qc hep-th

Antonio De Felice , Shinji Mukohyama , Masroor C. Pookkillath This is my paper
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Static, spherically symmetric solutions representing stars made of barotropic perfect fluid are studied in the context of two theories of type-II minimally modified gravity, VCDM and VCCDM. Both of these theories share the property that no additional degree of freedom is introduced in the gravity sector, and propagate only two gravitational waves besides matter fields, as in General Relativity (GR). We find that, on imposing physical boundary conditions on the Misner-Sharp mass of the system, the solutions in V(C)CDM exactly coincide with the ones in GR, namely they also satisfy the Tolman-Oppenheimer-Volkoff equation.

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