Feasibility of dark matter admixed neutron star based on recent observational constraints
arXiv:2408.03780 · doi:10.1051/0004-6361/202451879
Abstract
The equation of state (EOS) for neutron stars is modeled using the Relativistic Mean Field (RMF) approach with a mesonic nonlinear (NL) interaction, a modified sigma cut potential (NL- cut), and the influences of dark matter in the NL (NL DM). Using a Bayesian analysis framework, we evaluate the plausibility and impact of each scenario. Experimental constraints on the general properties of finite nuclei and heavy ion collisions, along with astrophysical observational data on neutron star radii and tidal deformation, have been taken into account. It was shown that all models, including the PREX-II data, were less favored, indicating that this experimental data seemed to be in tension with the other constraints included in the inference procedure, and were incompatible with chiral effective field theoretical calculations of pure neutron matter. Considering the models with no PREX-II constraints, we find the model NL- cut with the largest Bayes evidence, indicating that the constraints considered favor the stiffening of the EOS at large densities. Conversely, the neutron star with a dark matter component is the least favorable case in light of recent observational constraints, among different scenarios considered here. The and modes were calculated within the Cowling approximation, and it can be seen that modes are sensitive to the EOS. An analysis of the slopes of the mass-radius curves and -mode mass curves has indicated that these quantities may help distinguish the different scenarios.We also analyzed the impact of new PSR J0437-4715 measurements on neutron star mass-radius estimates, noting a 0.2 km reduction in the 90\% CI upper boundary across all models and a significant Bayes evidence decrease, indicating potential conflicts with previous data or the necessity for more adaptable models.
arXiv comment18 pages, 10 figures and 6 tables
References in corpus (119)
- GW170817: Measurements of Neutron Star Radii and Equation of State
- 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
- X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue
- A New Parameterization for the Lagrangian Density of Relativistic Mean Field Theory
- Determination of the Equation of State of Dense Matter
- 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
- Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620
- Isospin Asymmetry in Nuclei and Neutron Stars
- Composition and thermodynamics of nuclear matter with light clusters
- Neutron Star Structure and the Neutron Radius of 208Pb
- Equation of state and neutron star properties constrained by nuclear physics and observation
- Neutron-Rich Nuclei in Heaven and Earth
- New constraints on radii and tidal deformabilities of neutron stars from GW170817
- Evidence for quark-matter cores in massive neutron stars
- Constraints on the density dependence of the symmetry energy
- Accurate Determination of the Neutron Skin Thickness of Pb through Parity-Violation in Electron Scattering
- Implications of PREX-II on the equation of state of neutron-rich matter
- The non-gravitational interactions of dark matter in colliding galaxy clusters
- Cold Quark Matter
- Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
- Relativistic Mean-Field Theory and the High-Density Nuclear Equation of State
- Strangeness in nuclear physics
- Nuclear energy density optimization: Large deformations
- WIMP Annihilation and Cooling of Neutron Stars
- Relativistic effective interaction for nuclei, giant resonances, and neutron stars
- Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
- Quarkyonic Matter and Neutron Stars
- Constraining the Equation of State of Neutron Stars from Binary Mergers
- Measurement of the neutron lifetime using a gravitational trap and a low-temperature Fomblin coating
- A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715
- Improved Determination of the Neutron Lifetime
- Neutron Stars and the Nuclear Equation of State
- Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
- Constraining neutron star matter with QCD
- Symmetry energy from elliptic flow in 197Au + 197Au
- Dark Matter Interpretation of the Neutron Decay Anomaly
- Constraining the neutron star equation of state with gravitational wave signals from coalescing binary neutron stars
- Lorentz Invariance in Chiral Kinetic Theory
- Strangeness in Nuclei and Neutron Stars
- Nonparametric Inference of Neutron Star Composition, Equation of State, and Maximum Mass with GW170817
- Neutron Stars in f(R) Gravity with Perturbative Constraints
- Postmerger Gravitational-Wave Signatures of Phase Transitions in Binary Mergers
- Dark Matter Effects On Neutron Star Properties
- Compact stars made of fermionic dark matter
- Asymmetric nuclear matter based on chiral two- and three-nucleon interactions
- Measurement of the neutron lifetime using an asymmetric magneto- gravitational trap and in situ detection
- Constraining the nuclear matter equation of state around twice saturation density
- Bosonic Dark Matter in Neutron Stars and its Effect on Gravitational Wave Signal
- Probing the Symmetry Energy with the Spectral Pion Ratio
- Neutron Lifetime and Axial Coupling Connection
- Multimessenger constraints for ultra-dense matter
- Dark halos around neutron stars and gravitational waves
- Strongly interacting matter exhibits deconfined behavior in massive neutron stars
- Trace anomaly as signature of conformality in neutron stars
- The dark matter effect on realistic equation of state in neutron stars
- Effects of dark matter on the nuclear and neutron star matter
- Neutron stars: new constraints on asymmetric dark matter
- The Equation of State for the Nucleonic and Hyperonic Core of Neutron Stars
- Testing dark decays of baryons in neutron stars
- The Vlasov formalism for extended relativistic mean field models: the crust-core transition and the stellar matter equation of state
- Electric Dipole Polarizability in Pb as a Probe of the Symmetry Energy and Neutron Matter around
- Dark matter admixed neutron star as a possible compact component in the GW190814 merger event
- Confronting nuclear equation of state in the presence of dark matter using GW170817 observation in relativistic mean field theory approach
- Stellar properties and nuclear matter constraints
- Determination of the Equation of State from Nuclear Experiments and Neutron Star Observations
- What is the nature of the HESS J1731-347 compact object?
- Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter
- Constraining the symmetry energy with heavy-ion collisions and Bayesian analyses
- A Spectral Approach to the Relativistic Inverse Stellar Structure Problem
- Symmetry Energy III: Isovector Skins
- Constraining bosonic asymmetric dark matter with neutron star mass-radius measurements
- Search for the Neutron Decay n X+ where X is a dark matter particle
- Decoding the Density Dependence of the Nuclear Symmetry Energy
- Dark matter admixed neutron star properties in the light of X-ray pulse profile observations
- Tidal Deformability of Dark Matter Admixed Neutron Stars
- Bosonic Dark Matter in Light of the NICER Precise Mass-Radius Measurements
- Tidal Love numbers of neutron stars in gravity
- Constraints on dark matter self-interaction from the internal density profiles of X-COP galaxy clusters
- Feasability of constraining the curvature parameter of the symmetry energy using elliptic flow data
- The effects of self-interacting bosonic dark matter on neutron star properties
- Spanning the full range of neutron star properties within a microscopic description
- Impacts of dark matter on the -mode oscillation of hyperon star
- Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars
- Tidal Deformability of Fermion-Boson Stars: Neutron Stars Admixed with Ultra-Light Dark Matter
- Constraints on Skyrme Equations of State from Properties of Doubly Magic Nuclei and Ab-Initio Calculations of Low-Density Neutron Matter
- Tidal Love Numbers of Novel and Admixed Celestial Objects
- Study of Dark-Matter Admixed Neutron Stars using the Equation of State from the Rotational Curves of Galaxies
- Radial Oscillations of Dark Matter admixed Neutron Stars
- Dark matter effects on tidal deformabilities and moment of inertia in a hadronic model with short-range correlations
- Comprehensive study of compact stars with dark matter
- Implications of Feebly Interacting Dark Sector on Neutron Star Properties and Constraints from GW170817
- Making a soft relativistic mean-field equation of state stiffer at high density
- Dark matter effects on hybrid star properties
- Bayesian inference of signatures of hyperons inside neutron stars
- R-modes as a New Probe of Dark Matter in Neutron Stars
- Neutron's Dark Secret
- Constraining properties of asymmetric dark matter candidates from gravitational-wave observations
- Effects of Dark Matter on -mode oscillations of Neutron Stars
- Kaon meson condensate in neutron star matter including hyperons
- Feeble DM-SM Interaction via New Scalar and Vector Mediators in Rotating Neutron Stars
- Dark particle mass effects on neutron star properties from a short-range correlated hadronic model
- nEoS: Neutron Star Equation of State from hadron physics alone
- Neutron to Dark Matter Decay in Neutron Stars
- Dark matter effects on the properties of neutron stars: optical radii
- Quasi-equilibrium configurations of binary systems of dark matter admixed neutron stars
- Rotating dark matter admixed neutron stars
- Vector dark boson mediated feeble interaction between fermionic dark matter and strange quark matter in quark stars
- Implications of comprehensive nuclear and astrophysics data on the equations of state of neutron star matter
- Bosonic dark matter dynamics in hybrid neutron stars
- Astrophysics and Nuclear Physics Informed Interactions in Dense Matter: Inclusion of PSR J0437-4715
- Massive neutron star with strangeness in a relativistic mean-field model with a high-density cut-off
- The impact of asymmetric dark matter on the thermal evolution of nucleonic and hyperonic compact stars
- Theoretical bounds on dark matter masses
- Effect of the -cut potential on the properties of neutron stars with or without a hyperonic core
- Nambu-Jona-Lasinio description of hadronic matter from a Bayesian approach
- Effects of Onset of Phase Transition on Binary Neutron Star Mergers
- Unveiling a universal relationship between the f(R) parameter and neutron star properties
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- Thermodynamic Consistent Description of Compact Stars of Two Interacting Fluids: The Case of Neutron Stars with Higgs Portal Dark Matter
- Exploring -resonance in neutron stars: implications from astrophysical and nuclear observations
- Observational Probes of the Neutron Star Equation of State with Hyperons, Bosonic Dark Matter, and Quark Matter
- Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons
- Effect of Dark matter and -cut potential on radial and non-radial oscillation modes in neutron stars
- Probing Strange Dark Matter through -mode Oscillations of Neutron Stars with Hyperons and Quark Matter
- Effects of light-mass fermionic dark matter on the equilibrium and stability of white dwarfs