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- W4364377973 abstract "Abstract Proto-neutron stars are born when a highly evolved and massive star collapses under gravity. In this paper, we investigate the spontaneous scalarization in proto-neutron stars. Based on the scalar tensor theory of gravity as well as the physical conditions in proto-neutron star, we examine the structure of proto-neutron star. To describe the fluid in proto-neutron star, we utilize SU (2) chiral sigma model and the finite temperature extension of the Brueckner–Bethe–Goldstone quantum many-body theory in the Brueckner–Hartree–Fock approximation. Here, we apply the equation of state of proto-neutron stars considering different cases i.e. hot pure neutron matter and hot $$beta $$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mi>β</mml:mi> </mml:math> -stable neutron star matter without neutrino trapping as well as with neutrino trapping. The effects of temperature and entropy of proto-neutron stars on the star structure are also studied. Our results confirm that the spontaneous scalarization is affected by different physical conditions in proto-neutron stars." @default.
- W4364377973 created "2023-04-12" @default.
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- W4364377973 creator A5081472984 @default.
- W4364377973 date "2023-04-11" @default.
- W4364377973 modified "2023-10-01" @default.
- W4364377973 title "Spontaneous scalarization in proto-neutron stars" @default.
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- W4364377973 doi "https://doi.org/10.1140/epjc/s10052-023-11443-9" @default.
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