Stars disformally coupled to a shift-symmetric scalar field
Tact Ikeda, Aya Iyonaga, Tsutomu Kobayashi

TL;DR
This paper studies how stars behave when coupled to a shift-symmetric scalar field through disformal transformations, revealing invariance properties and solution branches in the scalar-tensor theory.
Contribution
It demonstrates the disformal invariance of stellar surfaces and analyzes interior and exterior solutions in shift-symmetric disformal scalar-tensor theories.
Findings
Energy density and tangential pressure vanish at star surfaces.
Disformal invariance of stellar surfaces is established.
Two solution branches depend on scalar field velocity.
Abstract
We investigate static and spherically symmetric stars disformally coupled to a scalar field. The scalar field is assumed to be shift symmetric, and hence the conformal and disformal factors of the metric coupled to matter are dependent only on the kinetic term of the scalar field. Assuming that the scalar field is linearly dependent on time, we consider a general shift-symmetric scalar-tensor theory and a general form of the matter energy-momentum tensor that allows for the anisotropic pressure and the heat flux in the radial direction. This is a natural starting point in light of how the gravitational field equations and the energy-momentum tensor transform under a disformal transformation. By inspecting the structure of the hydrostatic equilibrium equation in the presence of the derivative-dependent conformal and disformal factors, we show that the energy density and tangential…
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