Zobrazeno 1 - 10
of 1 855
pro vyhledávání: '"Burgio , G."'
We investigate nonradial $f$-mode oscillations of hybrid neutron stars in full general relativity, employing hybrid equations of state describing a nuclear outer core and a pasta-phase transition to a quark-matter core. The validity of various univer
Externí odkaz:
http://arxiv.org/abs/2411.15697
We investigate possible correlations between the stiffness of the symmetry energy at saturation density, the so-called $L$ parameter, and the neutron skin thickness of ${^{48}}$Ca and ${^{208}}$Pb, for which the recent measurements from the CREX and
Externí odkaz:
http://arxiv.org/abs/2410.15856
We investigate radial oscillations of proto-neutron stars, employing equations of state described by the Brueckner-Hartree-Fock theory or the relativistic mean field model, and assuming isentropy and fixed lepton fractions for the internal structure.
Externí odkaz:
http://arxiv.org/abs/2408.06599
We systematically study the observable properties of dark-matter admixed neutron stars, employing a realistic nuclear EOS in combination with self-interacting fermionic dark matter respecting constraints on the self-interaction cross section. Deviati
Externí odkaz:
http://arxiv.org/abs/2403.17024
Publikováno v:
Phys. Rev. D 109, 123018 (2024)
We study the cooling of isolated neutron stars, employing different nuclear equations of state with or without active direct Urca process, and investigate the interplay with the nuclear pairing gaps. We find that a consistent description of all curre
Externí odkaz:
http://arxiv.org/abs/2403.02222
We study the effects of dark matter on the properties of neutron stars by employing a DM-admixed model. The Brueckner-Hartree-Fock theory with realistic three-body forces and a generic bosonic self-interacting dark matter model describe the equations
Externí odkaz:
http://arxiv.org/abs/2307.11313
We investigate non-radial oscillations of pure and hybrid neutron stars, employing equations of state of nuclear matter from Brueckner-Hartree-Fock theory, and of quark matter from the Dyson-Schwinger quark model, performing a Gibbs construction for
Externí odkaz:
http://arxiv.org/abs/2303.07086
A microscopic nuclear equation of state compatible with all current astrophysical constraints constructed within the Brueckner-Hartree-Fock formalism is presented and extended in a consistent way to finite temperature. The effects of finite temperatu
Externí odkaz:
http://arxiv.org/abs/2207.12146
A set of microscopic, covariant density-functional, and non-relativistic Skyrme-type equations of state is employed to study the structure of purely nucleonic neutron stars at finite temperature. After examining the agreement with presently available
Externí odkaz:
http://arxiv.org/abs/2112.05323