On the conversion of neutron stars into quark stars
EPJ Web of Conferences, 2014 The possible existence of two families of compact stars, neutron stars and quark stars, naturally leads to a scenario in which a conversion process between the two stellar objects occurs with a consequent release of energy of the order of $10^{53}$ erg.
openaire +3 more sources
Strongly interacting quark matter in massive quark stars
Classical and Quantum GravityAbstract This paper investigates the properties of strongly coupled matter at high baryon densities (ρ B) in quark stars (QSs). The QS model is based on the density-dependent quark mass (DDQM) framework, modified DDQM (MDDQM) by enhancing the single-gluon interaction to generate higher repulsive pressure.
Adamu Issifu +4 more
openaire +2 more sources
The quark strange star in the enlarged Nambu-Jona-Lasinio model [PDF]
, 2002 The strange quark star is investigated within the enlarged SU(3) Nambu-Jona-Lasinio model. The stable quark star can exist until a maximal configuration with ρm = 3.1 × 1015 g cm -3 with Mm = 1.61 M⊙ and Rm = 8.74 km is reached. Strange quarks appear for
Mańka, Ryszard +2 more
core
The Astrophysical Journal LettersWe investigate binary neutron star (BNS) mergers using general-relativistic numerical simulations with hadronic and hybrid equations of state (EOSs), incorporating the latest observations and theoretical constraints.
Sudipta Hensh +6 more
doaj +1 more source
Calculation of the thermodynamic properties of the spin polarized strange quark star in the presence of strong magnetic field [PDF]
, 2012 Documentos apresentados no âmbito do reconhecimento de graus e diplomas estrangeirosIn this thesis, we investigated the strange quark matter (SQM) composed of the spin-up and spin-down; up, down and strange quarks at finite temperature in the presence of
Kayanikhoo, Fatemeh
core
Neutron Star masses from the Field Correlator Method Equation of State
EPJ Web of Conferences, 2014 We analyse the hadron-quark phase transition in neutron stars by confronting the hadronic Equation of State (EoS) obtained according to the microscopic Brueckner-Hartree-Fock many body theory, with the quark matter EoS derived within the Field Correlator
Zappalà D. +3 more
doaj +1 more source
The Spectrum of Low-pTJ/ψ in Heavy-Ion Collisions in a Statistical Two-Body Fractal Model. [PDF]
Entropy (Basel), 2023 Ding H +4 more
europepmc +1 more source
Strongly interacting matter exhibits deconfined behavior in massive neutron stars. [PDF]
Nat Commun, 2023 Annala E +6 more
europepmc +1 more source
Prospects for detecting quark star features with IceCube [PDF]
Core-collapse supernovae (CCSNe) provide a unique environment for studying matter under extreme densities and temperatures, where a phase transition from hadronic to deconfined quark matter may occur.
Durán de las Heras, María
core +2 more sources
Machine Learning Approach to Analyze the Heavy Quark Diffusion Coefficient in Relativistic Heavy Ion Collisions. [PDF]
Entropy (Basel), 2023 Guo R, Li Y, Chen B.
europepmc +1 more source