… equation of state, we obtain a less massive Bose-Einstein condensate star compared to …
boson star is insensitive to the change of matter temperature. However, the mass of a boson star …

… In Newtonian approximation we also consider stars at finite temperature, in which case the
bosons are no longer fully condensed. Section 3 discusses several models for boson stars in …

… stars due to the formation of Cooper pairs among the superfluid neutrons. To this end we
study the condensation of bosonic … We consider a finite-temperature scenario, generalizing …

… model at zero temperature and magnetic field gives stars with maximum masses … finite
temperature on BECS models. We will consider a naked star fully composed of interacting bosons. …

… EOS parameters—boson mass and strength … star at finite temperature considered in Ref.
[48] suggests that the maximum mass of the star remains unaffected by changes in temperature …

… Boson stars are gravitationally … stability criteria for fluid stars. With this in mind, I investigate
the dynamical instability of boson stars against chargeconserving, small radial perturbations. …

… Instead, if constructed larger than a galaxy, could a boson star serve as the dark matter halo
… to charged boson stars and fermion-boson stars. Rotating boson stars are found to have an …

… Our key simplification is to include only boson emission or absorption (… of temperature
and FIB absorption rate in a star, we derive explicit volume-integral expressions for the boson …

… In this paper we study boson stars made up of real scalar \(j>4 self-interacting fields at
finite temperature. For the reason of their equation of state, we call these configurations "…

… boson stars account for this non-baryonic part of dark matter [17], [18], [19]. Boson stars are
… –0) instead of electromagnetic fields, ie spin–1 bosons. If scalar fields exist in nature, such …