Zobrazeno 1 - 10
of 449
pro vyhledávání: '"Margueron J."'
The meaningful correlations between the zero-sound modes and the stiffness of the nuclear equation of state (EOS) are uncovered in nuclear matter with the relativistic mean-field theory. It is demonstrated that the high-density zero-sound modes merel
Externí odkaz:
http://arxiv.org/abs/2310.16759
A relativistic Hartree-Fock Lagrangian including a chiral potential and nucleon polarisation is investigated in hopes of providing a better description of dense nuclear matter. We fully consider the contribution of the exchange Fock term to the energ
Externí odkaz:
http://arxiv.org/abs/2304.01817
In this paper we discuss the combined effects on nuclear matter properties of the quark confinement mechanism in nucleon and of the chiral effective potential resulting from the spontaneous breaking of the chiral symmetry in nuclear matter. Based on
Externí odkaz:
http://arxiv.org/abs/2304.01036
Publikováno v:
Phys. Rev. C 108, 035810 (2023)
We investigate the question of the nature of compact stars, considering they may be neutron stars or hybrid stars containing a quark core, within the present constraints given by gravitational waves, radio-astronomy, X-ray emissions from millisecond
Externí odkaz:
http://arxiv.org/abs/2303.18133
In view of the next LIGO-Virgo-KAGRA Observing period O4 (to start in Spring 2023), we address the question of the ability of the interferometers network to discriminate among different neutron stars equation of states better than what was possible w
Externí odkaz:
http://arxiv.org/abs/2302.04147
A compressible liquid-drop model (CLDM) is used to correlate uncertainties associated with the properties of the neutron star (NS) crust with theoretical estimates of the uncertainties associated with the equation of state (EOS) of homogeneous neutro
Externí odkaz:
http://arxiv.org/abs/2110.00441
Publikováno v:
Eur.Phys.J.A 58 (2022) 5, 84
We explore three different classes of relativistic approaches applied to the description of dense nuclear matter: a Walecka-type relativistic mean field model (RMF), an extension including an effective chiral potential (RMF-C) and a further extension
Externí odkaz:
http://arxiv.org/abs/2109.05374
Gravitational wave-forms from coalescences of binary black hole systems and binary neutron star systems with low tidal effects can hardly be distinguished if the two systems have similar masses. In the absence of discriminating power based on the gra
Externí odkaz:
http://arxiv.org/abs/2106.05805
Closed shell charmed hypernuclei $^5_{\Lambda_c}$Li, $^{17}_{\Lambda_c}$F, $^{41}_{\Lambda_c}$Sc, $^{57}_{\Lambda_c}$Cu, $^{133}_{\Lambda_c}$Sb and $^{209}_{\Lambda_c}$Bi are calculated within Hartree-Fock approach by using three different force sets
Externí odkaz:
http://arxiv.org/abs/2106.04491
We suggest an extension to isospin asymmetric matter of the quarkyonic model from McLerran and Reddy. This extension allows us to construct the $\beta$-equilibrium between quarks, nucleons and leptons. The concept of the quarkyonic matter originates
Externí odkaz:
http://arxiv.org/abs/2103.10209