Equation of state of strongly magnetized matter with hyperons and -resonances
arXiv:2010.00981 · doi:10.3390/particles3040043
Abstract
We construct a new equation of state for the baryonic matter under an intense magnetic field within the framework of covariant density functional theory. The composition of matter includes hyperons as well as -resonances. The extension of the nucleonic functional to the hypernuclear sector is constrained by the experimental data on and -hypernuclei. We find that the equation of state stiffens with the inclusion of the magnetic field, which increases the maximum mass of neutron star compared to the non-magnetic case. In addition, the strangeness fraction in the matter is enhanced. Several observables, like the Dirac effective mass, particle abundances, etc show typical oscillatory behavior as a function of the magnetic field and/or density which is traced back to the occupation pattern of Landau levels.
arXiv comment16 pages, 8 figures, Accepted in journal "Particles", Corrected some typos. Matches with published version
References in corpus (44)
- A Massive Pulsar in a Compact Relativistic Binary
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- 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
- Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Physics of Strongly Magnetized Neutron Stars
- Magnetars: the physics behind observations
- The Equation of State of Neutron-Star Matter in Strong Magnetic Fields
- Effects of Strong Magnetic Fields on Neutron Star Structure
- Density Dependent Hadron Field Theory
- Magneto--thermal evolution of neutron stars
- Blast Waves from Magnetar Flares and Fast Radio Bursts
- Quantizing magnetic field and quark-hadron phase transition in a neutron star
- Dense nuclear matter in a strong magnetic field
- Can very compact and very massive neutron stars both exist?
- The Massive Pulsar PSR J1614-2230: Linking Quantum Chromodynamics, Gamma-ray Bursts, and Gravitational Wave Astronomy
- Twisted-torus configurations with large toroidal magnetic fields in relativistic stars
- Implications of a "Fast Radio Burst" from a Galactic Magnetar
- Structure and deformations of strongly magnetized neutron stars with twisted torus configurations
- Relativistic models of magnetars: the twisted-torus magnetic field configuration
- Periodicity in recurrent fast radio bursts and the origin of ultra long period magnetars
- Competition between delta isobars and hyperons and properties of compact stars
- Application of the density dependent hadron field theory to neutron star matter
- Precessing flaring magnetar as a source of repeating FRB 180916.J0158+65
- Magnetic, thermal and rotational evolution of isolated neutron stars
- The Equation of State for the Nucleonic and Hyperonic Core of Neutron Stars
- Critical Density and Impact of Resonance Formation in Neutron Stars
- Periodic Fast Radio Bursts with Neutron Star Free/Radiative Precession
- A third family of super dense stars in the presence of antikaon condensates
- Confronting GW190814 with hyperonization in dense matter and hypernuclear compact stars
- Implications from GW170817 for -isobar admixed hypernuclear compact stars
- Hypernuclear matter in strong magnetic field
- Stellar matter with a strong magnetic field within density-dependent relativistic models
- Magnetar superconductivity versus magnetism: neutrino cooling processes
- Hypernuclear stars from relativistic Hartree-Fock density functional theory
- Constraining compact star properties with nuclear saturation parameters
- Magnetic field distribution in magnetars
- Deformation of a magnetized neutron star
- Spin-polarized neutron matter: Critical unpairing and BCS-BEC precursor
- The Influence of the Magnetic Field on the Properties of Neutron Star Matter
- The Rarita-Schwinger Particles Under de Influence of Strong Magnetic Fields
- From microphysics to dynamics of magnetars
- Rapid rotational crust-core relaxation in magnetars
Cited by in corpus (23)
- Heavy Baryons in Compact Stars
- Dense matter equation of state of a massive neutron star with anti-kaon condensation
- Massive -resonance admixed hypernuclear stars with anti-kaon condensations
- Delta Baryons in Neutron-Star Matter under Strong Magnetic Fields
- Heavy Magnetic Neutron Stars
- Hybrid stars are compatible with recent astrophysical observations
- Equation of state and composition of proto-neutron stars and merger remnants with hyperons
- Delta baryons in neutron stars
- Oscillating magnetised hybrid stars under the magnifying glass of multi-messenger observations
- Exploring the effects of Delta Baryons in magnetars
- Universal relations for compact stars with exotic degrees of freedom
- Baryonic dense matter in view of gravitational-wave observations
- Influence of the nuclear symmetry energy slope on observables of compact stars with -admixed hypernuclear matter
- (Anti)kaon condensation in strongly magnetized dense matter
- Neutron star structure with a new force between quarks
- Probing the impact of Delta-Baryons on Nuclear Matter and Non-Radial Oscillations in Neutron Stars
- Massive neutron stars as mass gap candidates: Exploring equation of state and magnetic field
- Oscillating Magnetized Color Superconducting Quark Stars
- Strongly interacting matter in extreme magnetic fields
- Effects of Phi and -meson on properties of hyperon stars including resonance
- Tension between implications from PREX-2 data and gravitational tidal response on dense matter equation of state
- Kaon-meson coupling from SU(3) flavour symmetry and application to antikaon condensed dense matter in neutron star
- Effects of anisotropy on strongly magnetized neutron and strange quark stars in general relativity