Correlation between the symmetry energy slope and the deconfinement phase transition
arXiv:2311.00125 · doi:10.1103/PhysRevC.109.045801
Abstract
We study how the nuclear symmetry energy slope () can affect the hadron-quark phase transition and neutron star properties. We show that the main physical quantities as the critical chemical potential and pressure are strongly influenced by the symmetry energy slope. In extreme cases, the total amount of deconfined quarks can reach up to 99 of the hybrid star mass.
arXiv commentPublished version
References in corpus (42)
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- Equations of state for supernovae and compact stars
- Neutron Star Structure and the Neutron Radius of 208Pb
- Evidence for quark-matter cores in massive neutron stars
- Implications of PREX-II on the equation of state of neutron-rich matter
- Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
- Constraining the Symmetry Parameters of the Nuclear Interaction
- Relativistic effective interaction for nuclei, giant resonances, and neutron stars
- Asymmetric nuclear matter:the role of the isovector scalar channel
- Constraints on the Symmetry Energy Using the Mass-Radius Relation of Neutron Stars
- First Order Kaon Condensate
- Nuclear Matter in Relativistic Mean Field Theory with Isovector Scalar Meson
- Probing the Symmetry Energy with the Spectral Pion Ratio
- On the appearance of hyperons in neutron stars
- Equation of state for neutron stars in SU(3) flavor symmetry
- Neutron star properties and the symmetry energy
- The Equation of State for the Nucleonic and Hyperonic Core of Neutron Stars
- Phase transitions in dense matter and the maximum mass of neutron stars
- Phase Transitions and the Mass-Radius Curves of Relativistic Stars
- What do we learn about vector interactions from GW170817?
- Interplay between Particles and Hyperons in Neutron Stars
- Constraints on the Symmetry Energy from PREX-II in the Multimessenger Era
- Modified MIT bag Models -- part I: Thermodynamic consistency, stability windows and symmetry group
- Two-solar-mass hybrid stars: a two model description with the Nambu-Jona-Lasinio quark model
- Modified MIT Bag Models -- part II: QCD phase diagram and hot quark stars
- On the nature of the mass-gap object in the GW190814 event
- Nucleonic metamodelling in light of multimessenger, PREX-II and CREX data
- Broken SU(6) symmetry and massive hybrid stars
- Neutron star structure and collective excitations of finite nuclei
- Studies of the structure of massive hybrid stars within a modified NJL model
- The baryon coupling scheme in an unified SU(3) and SU(6) symmetry formalism
- Do Delta Baryons Play a Role in Neutron Stars?
- A Bayesian analysis of the properties of hybrid stars with the NJL model
- Effects of the Symmetry Energy and its Slope on Neutron Star Properties
- Maximum latent heat of neutron star matter independently of General Relativity
- Implications of supermassive neutron stars for the form of the equation of state of hybrid stars
- Latent heat of nuclear matter
- Imprints of the nuclear symmetry energy slope in gravitational wave signals emanating from neutron stars
- A closer look at the Yukawa's interaction from a symmetry group perspective
- Phase transitions and latent heat in magnetized matter