Landau coefficients for scalarization phase transitions are calculated from first principles via reduction of the theory's energy functional to an effective energy function.
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Linear coupling and rotation in scalar-tensor theories produce a complex phase transition landscape for scalarized neutron stars, with rotation increasing critical masses and Landau theory revealing overlooked solution branches.
Scalarized boson stars support qualitatively different Polish Doughnut disks than GR counterparts, including possible two-centered configurations and stable orbits to the center.
citing papers explorer
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Underlying mechanisms of phase transitions in scalar-tensor theories
Landau coefficients for scalarization phase transitions are calculated from first principles via reduction of the theory's energy functional to an effective energy function.
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Phase transition structure of scalarized neutron stars: the effect of rotation and linear coupling
Linear coupling and rotation in scalar-tensor theories produce a complex phase transition landscape for scalarized neutron stars, with rotation increasing critical masses and Landau theory revealing overlooked solution branches.
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Boson Stars surrounded by Polish Doughnuts in Scalar-Tensor Theory
Scalarized boson stars support qualitatively different Polish Doughnut disks than GR counterparts, including possible two-centered configurations and stable orbits to the center.