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- W4310496978 abstract "In the present paper we derive strong constrains on scalarization in scalar-Gauss-Bonnet (SGB) gravity using observations of pulsars in close binary systems. Since scalarized neutron stars carry a nonzero scalar change, they emit scalar dipole radiation while inspiraling which speeds up the orbital decay. The observations support the conjecture that such radiation is either absent or very small for the observed binary pulsars. Using this, we determine the allowed range of parameters for SGB gravity. We also transfer the derived constraints to black holes in SGB gravity. It turns out that the maximum mass of a scalarized black hole cannot exceed roughly 10 to 20 solar masses, depending on the initial assumptions we make for the nuclear matter equations of state. The black hole scalar charge on the other hand can reach relatively large values that are potentially observable." @default.
- W4310496978 created "2022-12-11" @default.
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- W4310496978 date "2022-12-01" @default.
- W4310496978 modified "2023-10-10" @default.
- W4310496978 title "Constraining scalarization in scalar-Gauss-Bonnet gravity through binary pulsars" @default.
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- W4310496978 doi "https://doi.org/10.1103/physrevd.106.124001" @default.
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