Anisotropic Strange Stars in the Spotlight: Unveiling Constraints through Observational Data
arXiv:2306.00326 · doi:10.1093/mnras/stad2554
Abstract
Motivated by the recent suggestions that very massive pulsar (PSR J0952-0607) and very light compact object (HESS J1731-347) exist, in this article, we revisit the possibility of such objects being strange stars instead of the standard hadronic neutron stars. We study the possible presence of local anisotropy and how it affects the macroscopic properties of strange stars and compare our results with the recent constraints presented in the literature. We found that the presence of anisotropy increases the maximum mass, the radius of the canonical star, and its tidal deformability for positive values of and the opposite for negative values. We also show that although we cannot rule out the possibility of very compact objects being standard hadronic neutron stars, strange stars easily fulfill most of the observational constraints.
arXiv comment5 pages, 2 figures, 1 table, Published in MNRAS
References in corpus (32)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- A Massive Pulsar in a Compact Relativistic Binary
- GW170817: Measurements of Neutron Star Radii and Equation of State
- 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
- Tidal Love numbers of neutron stars
- PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star
- Stringent constraints on neutron-star radii from multimessenger observations and nuclear theory
- Phases of dense matter in neutron stars
- Effects of Strong Magnetic Fields on Neutron Star Structure
- Neutron star tidal deformability and equation of state constraints
- Non-radial oscillations of anisotropic neutron stars in the Cowling approximation
- Equilibrium models of relativistic stars with a toroidal magnetic field
- Radial pulsations and stability of anisotropic stars with quasi-local equation of state
- Twisted-torus configurations with large toroidal magnetic fields in relativistic stars
- Structure and deformations of strongly magnetized neutron stars with twisted torus configurations
- Relativistic stars with poloidal and toroidal magnetic fields and meridional flow
- Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition
- Vector interaction enhanced bag model for astrophysical applications
- Relativistic models for Superconducting-Superfluid Mixtures
- Radial stability of anisotropic strange quark stars
- Relativistic models of magnetars: Nonperturbative analytical approach
- The tidal deformability of an anisotropic compact star: Implications of GW170817
- Modified MIT bag Models -- part I: Thermodynamic consistency, stability windows and symmetry group
- The role of currents distribution in general relativistic equilibria of magnetized neutron stars
- 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
- Love relation for an anisotropic neutron star
- Gravitational Wave Signatures of Highly Magnetized Neutron Stars
- The hadronic equation of state of HESS J1731-347 from the relativistic mean-field model with tensor coupling
Cited by in corpus (18)
- What is the nature of the HESS J1731-347 compact object?
- Quark Models and Radial Oscillations: Decoding the HESS J1731-347 Compact Object's Equation of State
- Relativistic mean field model for ultra-compact low mass neutron star of HESS J1731-347
- Hybrid stars in light of the HESS J1731-347 remnant and the PREX-II experiment
- Could a slow stable hybrid star explain the central compact object in HESS~J1731-347?
- Probing the Impact of WIMP Dark Matter on Universal Relations, GW170817 Posterior and Radial Oscillations
- Moment of inertia and compactness of quark stars within the context of gravity
- A Bayesian study of quark models in view of recent astrophysical constraints
- Speed of sound bounds and first-order phase transitions in compact stars
- Universal relations for anisotropic interacting quark stars
- Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars
- Spherically symmetric anisotropic strange stars
- Role of local anisotropy in hybrid stars
- Strange stars admixed with dark matter: equiparticle model in a two fluid approach
- Confronting recent light compact star observations with color-flavor locked quark matter
- Anisotropic pressure effect on central EOS of PSR J0740+6620 in the light of dimensionless TOV equation
- Gravitational-Wave Constraints on Neutron-Star Pressure Anisotropy via Universal Relations
- On the Cooling of Compact Stars in Light of the HESS J1731-347 Remnant