The Physics of Neutron Stars

Abstract

Neutron stars are some of the densest manifestations of massive objects in the universe. They are ideal astrophysical laboratories for testing theories of dense matter physics and provide connections among nuclear physics, particle physics and astrophysics. Neutron stars may exhibit conditions and phenomena not observed elsewhere, such as hyperon-dominated matter, deconfined quark matter, superfluidity and superconductivity with critical temperatures near $10^{10}$ kelvin, opaqueness to neutrinos, and magnetic fields in excess of $10^{13}$ Gauss. Here, we describe the formation, structure, internal composition and evolution of neutron stars. Observations that include studies of binary pulsars, thermal emission from isolated neutron stars, glitches from pulsars and quasi-periodic oscillations from accreting neutron stars provide information about neutron star masses, radii, temperatures, ages and internal compositions.

22 pages, 4 figures and 1 table

Cited by in corpus (765)

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• A Radio Pulsar Spinning at 716 Hz
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• The NANOGrav Nine-year Data Set: Mass and Geometric Measurements of Binary Millisecond Pulsars
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• A Radio Pulsar/X-ray Binary Link
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• Signatures of magnetar central engines in short GRB lightcurves
• The Evolution of Compact Binary Star Systems
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• Science with ASKAP - the Australian Square Kilometre Array Pathfinder
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• Swift observations of GRB 070110: an extraordinary X-ray afterglow powered by the central engine
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• Twenty-One Millisecond Pulsars in Terzan 5 Using the Green Bank Telescope
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• The Millisecond Magnetar Central Engine in short GRBs
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• How viscous is a superfluid neutron star core?
• The bottom magnetic field and magnetosphere evolution of neutron star in low mass X-ray binary
• Binary and Millisecond Pulsars
• Constraining the High-Density Behavior of Nuclear Symmetry Energy with the Tidal Polarizability of Neutron Stars
• The Ultimate Energy Density of Observable Cold Matter
• The relativistic pulsar-white dwarf binary PSR J1738+0333 I. Mass determination and evolutionary history
• Taking the Measure of the Universe: Precision Astrometry with SIM PlanetQuest
• Isospin-dependent properties of asymmetric nuclear matter in relativistic mean-field models
• Accelerating incoherent dedispersion
• Recent observation of short range nucleon correlations in nuclei and their implications for the structure of nuclei and neutron stars
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• First observation of an attractive interaction between a proton and a multi-strange baryon
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• Gravitational waves from black hole-neutron star binaries I: Classification of waveforms
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• Near-threshold pion production with radioactive beams at the Rare Isotope Accelerator
• Gravitational waves from nonspinning black hole-neutron star binaries: dependence on equations of state
• Do we understand the incompressibility of neutron-rich matter?
• Black hole-neutron star binary merger: Dependence on black hole spin orientation and equations of state
• Impact of the symmetry energy on the outer crust of non-accreting neutron stars
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• Complexity and neutron stars structure
• Neutron star properties in density-dependent relativistic Hartree-Fock theory
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• Magnetars: super(ficially) hot and super(fluid) cool
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• Accreting Millisecond X-Ray Pulsars
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• Narrowband searches for continuous and long-duration transient gravitational waves from known pulsars in the LIGO-Virgo third observing run
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• Breaking the sound barrier in AdS/CFT
• Nuclear matter symmetry energy and the symmetry energy coefficient in the mass formula
• General relativistic treatment of $f$-mode oscillations of hyperonic stars
• Statistical description of complex nuclear phases in supernovae and proto-neutron stars
• Frequency domain model of $f$-mode dynamic tides in gravitational waveforms from compact binary inspirals
• Hyperon effects in covariant density functional theory with recent astrophysical observations
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• Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO--Virgo data
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• Measurement of hyper triton lifetime in Au + Au collisions at the Relativistic Heavy-Ion Collider
• Symmetry energy of cold nucleonic matter within a relativistic mean field model encapsulating effects of high momentum nucleons induced by short-range correlations
• Preparing the next gravitational million-body simulations: Evolution of single and binary stars in Nbody6++GPU, MOCCA and McLuster
• Single-nucleon potential decomposition of the nuclear symmetry energy
• Why is the nuclear symmetry energy so uncertain at supra-saturation densities?
• In-medium effects for nuclear matter in the Fermi energy domain
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• Neutron stars in $f(\mathcal{R},\mathcal{T})$ gravity using realistic equations of state in the light of massive pulsars and GW170817
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• Perturbative QCD and the Neutron Star Equation of State
• Oscillation modes of hybrid stars within the relativistic Cowling approximation
• Maximum mass of compact stars from gravitational wave events with finite-temperature equations of state
• The Tarantula Massive Binary Monitoring VI: Characterisation of hidden companions in 51 single-lined O-type binaries, a flat mass-ratio distribution, and black-hole binary candidates
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• Investigating Signatures of Phase Transitions in Neutron-Star Cores
• Imprints of the nuclear symmetry energy on the tidal deformability of neutron stars
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• Tracing the evolution of the symmetry energy of hot nuclear fragments from the compound nucleus towards multifragmentation
• Quark magnetar in three-flavor Nambu--Jona-Lasinio model with vector interaction and magnetized gluon potential
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• Electron-muon heat conduction in neutron star cores via the exchange of transverse plasmons
• Constraining the density slope of nuclear symmetry energy at subsaturation densities using electric dipole polarizability in ${}^{208}$Pb
• Density dependence of nuclear symmetry energy constrained by mean-field calculations
• The origin of RXJ1856.5-3754 and RXJ0720.4-3125 -- updated using new parallax measurements
• Tidal Love Numbers of Black Holes and Neutron Stars in the Presence of Higher Dimensions: Implications of GW170817
• What the Timing of Millisecond Pulsars Can Teach us about Their Interior
• Higher-order symmetry energy of nuclear matter and the inner edge of neutron star crusts
• Maximum Baryon Masses for Static Neutron Stars in $f(R)$ Gravity
• The Influence of in-medium NN cross-sections, symmetry potential and impact parameter on the isospin observables
• Equation of state of dense matter in the multimessenger era
• Constraints on the time variation of the gravitational constant using gravitational-wave observations of binary neutron stars
• Effects of the equation of state on the bulk properties of maximally-rotating neutron stars
• Superradiance in rotating stars and pulsar-timing constraints on dark photons
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• New Self-Similar Solutions of Polytropic Gas Dynamics
• Validating relativistic models of nuclear structure against theoretical, experimental, and observational constraints
• Neutrino Emission from Ungapped Quark Matter
• Mass and radius formulas for low-mass neutron stars
• ${}_{\Lambda }^3\mathrm{H}$ and ${}_{\bar{\Lambda }}^3\bar{\mathrm{H}}$ lifetime measurement in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=$ 5.02 TeV via two-body decay
• Magnetar central engine and possible gravitational wave emission of nearby short GRB 160821B
• Relativistic models of the neutron-star matter equation of state
• Status and perspectives of Continuous Gravitational Wave searches
• Stability windows for proto-quark stars
• Compact stars in the braneworld: a new branch of stellar configurations with arbitrarily large mass
• Analytical relations between nuclear symmetry energy and single-nucleon potentials in isospin asymmetric nuclear matter
• The GMRT High Resolution Southern Sky Survey for pulsars and transients -I. Survey description and initial discoveries
• On the mass of the neutron star in V395 Car/2S 0921-630
• Constraining the relativistic mean-field model equations of state with gravitational wave observations
• Imposing multi-physics constraints at different densities on the Neutron Star Equation of State
• Symmetry energy at supra-saturation densities via the Gravitational Waves from GW170817
• Quark-hadron continuity beyond Ginzburg-Landau paradigm
• Equation of State of Dense Matter from a density dependent relativistic mean field model
• Peeling off neutron skins from neutron-rich nuclei: Constraints on the symmetry energy from neutron-removal cross sections
• Continuous-wave gravitational radiation from pulsar glitch recovery
• Gravitational wave background from rotating neutron stars
• Quantum Monte Carlo calculations of symmetric nuclear matter
• Discovery of an Isolated Compact Object at High Galactic Latitude
• The High Time Resolution Universe Survey II: Discovery of 5 Millisecond Pulsars
• The Nuclear Tensor Interaction in Covariant Energy Density Functional
• Multi-physics constraints at different densities to probe nuclear symmetry energy in hyperonic neutron stars
• Hypernuclear stars from relativistic Hartree-Fock density functional theory
• Andreev-Bashkin effect in superfluid cold gases mixture
• Extended Skyrme interactions for nuclear matter, finite nuclei and neutron stars
• Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energy
• Constraining extra-spatial dimensions with observations of GW170817
• Effects of $\omega$ meson self-coupling on the properties of finite nuclei and neutron stars
• Constraints for weakly interacting light bosons from existence of massive neutron stars
• Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter
• Neutron stars in $f(R,L_m,T)$ gravity
• The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture at zero temperature
• Tidal Deformabilities of Neutron Stars in scalar-Gauss-Bonnet Gravity and Their Applications to Multimessenger Tests of Gravity
• The QCD Axion at Finite Density
• Determining the nuclear neutron distribution from Coherent Elastic neutrino-Nucleus Scattering: current results and future prospects
• Low-mass neutron stars: universal relations, the nuclear symmetry energy and gravitational radiation
• Settling accretion onto slowly rotating X-ray pulsars
• Energy dependence of pion in-medium effects on π^-/π^+ ratio in heavy-ion collisions
• Colloquium: Comparison of Astrophysical and Terrestrial Frequency Standards
• Neutron Skin Thickness of 90Zr Determined By Charge Exchange Reactions
• Effects of isospin and momentum dependent interactions on thermal properties of asymmetric nuclear matter
• Geometric inequalities for axially symmetric black holes
• Constraining mean-field models of the nuclear matter equation of state at low densities
• Relativistic Brueckner-Hartree-Fock in nuclear matter without the average momentum approximation
• Large and massive neutron stars: Implications for the sound speed in dense QCD
• Quark stars under strong magnetic fields
• Neutron Stars with Baryon Number Violation, Probing Dark Sectors
• $R^p$ Attractors Static Neutron Star Phenomenology
• Probing the isospin dependence of the in-medium nucleon-nucleon cross sections with radioactive beams
• Pulsar kicks by anisotropic neutrino emission from quark matter in strong magnetic fields
• Measurement of the lifetime and $\Lambda$ separation energy of ${}_{\Lambda }^3\mathrm{H}$
• Non extensive thermodynamics and neutron star properties
• Bayesian parameter constraints for neutron star masses and radii using X-ray timing observations of accretion-powered millisecond pulsars
• Universal Inflationary Attractors Implications on Static Neutron Stars
• Predicting the moment of inertia of pulsar J0737-3039A from Bayesian modeling of the nuclear equation of state
• $I-$Love$-C$ relation for an anisotropic neutron star
• Neutron stars with isovector scalar correlations
• Triton-${}^3$He relative and differential flows as probes of the nuclear symmetry energy at supra-saturation densities
• Halo phenomenon in finite many-fermion systems. Atom-positron complexes and large-scale study of atomic nuclei
• Mechanical Properties of non-accreting Neutron Star Crusts
• Inflationary Attractors Predictions for Static Neutron Stars in the Mass-Gap Region
• Broadband modelling of short gamma-ray bursts with energy injection from magnetar spin-down and its implications for radio detectability
• Detection and timing of gamma-ray pulsations from the $707$ Hz pulsar J0952$-$0607
• Spin Period Evolution of Recycled Pulsar in Accreting Binary
• What can we learn from "internal plateaus"? The peculiar afterglow of GRB 070110
• A systematic study of the ${\pi }^{-}/{\pi }^{+}$ ratio in heavy-ion collisions with the same neutron/proton ratio but different masses
• New insights into nuclear physics and weak mixing angle using electroweak probes
• Post-Tolman-Oppenheimer-Volkoff formalism for relativistic stars
• Gauss-Bonnet boson stars
• Neutron Stars in Scalar-tensor Gravity with Quartic Order Scalar Potential
• Evolution of the symmetry energy of hot neutron-rich matter formed in heavy-ion reactions
• Asymmetric nuclear matter in relativistic mean-field models with isoscalar- and isovector-meson mixing
• Quasi-normal g-modes of neutron stars with quarks
• A long optical plateau in the afterglow of the Extended Emission short GRB 150424A: Evidence for energy injection by a magnetar?
• Effects of nuclear symmetry energy and equation of state on neutron star properties
• Three Additional Quiescent Low-Mass X-ray Binary Candidates in 47 Tucanae
• Holographic approach to compact stars and their binary mergers
• Twin Stars within the SU(3) Chiral Quark-Meson Model
• Neutron Skin in CsI and Low-Energy Effective Weak Mixing Angle from COHERENT Data
• Nuclear Masses and Neutron Stars
• Predicting Ranges for Pulsars' Braking Indices
• The relativistic entrainment matrix of a superfluid nucleon-hyperon mixture. II. Effect of finite temperatures
• Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
• Static Neutron Stars Perspective of Quadratic and Induced Inflationary Attractor Scalar-tensor Theories
• Pulsars probe the low-frequency gravitational sky: Pulsar Timing Arrays basics and recent results
• The neutron/proton ratio of squeezed-out nucleons and the high density behavior of the nuclear symmetry energy
• Higher order bulk characteristic parameters of asymmetric nuclear matter
• Toward Realistic and Practical No-Hair Relations for Neutron Stars in the Non-Relativistic Limit
• Origin of symmetry energy in finite nuclei and density dependence of nuclear matter symmetry energy from measured alpha-decay energies
• Probing the Nuclear Symmetry Energy with Heavy-Ion Reactions Induced by Neutron-Rich Nuclei
• Anomalous thermodynamics and phase transitions of neutron-star matter
• Phase Transitions In Compact Stars
• Constraining properties of rapidly rotating neutron stars using data from heavy-ion collisions
• Strange Quark Matter in Stars: A General Overview
• Probing the high-density behavior of symmetry energy with gravitational waves
• Timescale of twin-peak quasi-periodic oscillations and mass of accreting neutron stars
• Microscopically constrained mean field models from chiral nuclear thermodynamics
• Magnetic Fields and Afterglows of BdHNe: Inferences from GRB 130427A, GRB 160509A, GRB 160625B, GRB 180728A and GRB 190114C
• Neutron-proton effective mass splitting and thermal evolution in neutron rich matter
• Magnetars from Neutron Star--White Dwarf Mergers: Application to Fast Radio Bursts
• The Birth of Quark Stars: Photon-driven Supernovae?
• An improved single particle potential for transport model simulations of nuclear reactions induced by rare isotope beams
• Dilute neutron matter on the lattice at next-to-leading order in chiral effective field theory
• Using Light Charged Particles to Probe the Asymmetry Dependence of the Nuclear Caloric Curve
• Numerically Fitting The Electron Fermi Energy and The Electron Fraction in A Neutron Star
• Constraining the nuclear symmetry energy and properties of neutron star from GW170817 by Bayesian analysis
• Effect of spin on the inspiral of binary neutron stars
• Formation of Sub-millisecond Pulsars and Possibility of Detection
• Extended quark mean-field model for neutron stars
• Symmetry energy systematics and its high density behavior
• Stability and gravitational collapse of neutron stars with realistic equations of state
• Ruling out the supersoft high-density symmetry energy from the discovery of PSR J0740+6620 with mass $2.14_{-0.09}^{+0.10}{M}_{\odot }$
• Thermodynamic properties and shear viscosity over entropy density ratio of nuclear fireball in a quantum-molecular dynamics model
• Oscillations of Rapidly Rotating Superfluid Stars
• Clusterized nuclear matter in the (proto-)neutron star crust and the symmetry energy
• Charge Exchange Spin-Dipole Excitations of 90Zr and 208Pb and Neutron Matter Equation of State
• Cross-checking the symmetry energy at high densities
• Pulsar slow glitches in a solid quark star model
• Modeling pion production in heavy-ion collisions at intermediate energies
• Nuclear limits on gravitational waves from elliptically deformed pulsars
• Imprints of the nuclear symmetry energy on gravitational waves from the axial w-modes of neutron stars
• Consistent Skyrme parametrizations constrained by GW170817
• Normal or abnormal isospin-fractionation as a qualitative probe of nuclear symmetry energy at supradensities
• Warm dense matter and cooling of supernovae remnants
• Measuring Neutron Star Mass and Radius with Three Mass-Radius Relations
• Hybrid stars with sequential phase transitions: the emergence of the g${}_2$ mode
• Isovector properties of quark matter and quark stars in an isospin-dependent confining model
• Properties of the redback millisecond pulsar binary 3FGL J0212.1+5320
• Magnetohydrodynamic Rebound Shocks of Supernovae
• Dynamic Evolution of a Quasi-Spherical General Polytropic Magnetofluid with Self-Gravity
• Effects of pion potential and nuclear symmetry energy on the ${\pi }^{-}/{\pi }^{+}$ ratio in heavy-ion collisions at beam energies around the pion production threshold
• Properties of the remnant disk and the dynamical ejecta produced in low-mass black hole-neutron star mergers
• Lorentz covariant nucleon self-energy decomposition of the nuclear symmetry energy
• X-ray Spectral Identification of Three Candidate Quiescent Low-Mass X-ray Binaries in the Globular Cluster NGC 6304
• Equation of state of isospin-asymmetric nuclear matter in relativistic mean-field models with chiral limits
• Constraining a possible time variation of the gravitational constant G with terrestrial nuclear laboratory data
• Momentum dependent mean-field dynamics of compressed nuclear matter and neutron stars
• Correlations between the nuclear breathing mode energy and properties of asymmetric nuclear matter
• Impact of massive neutron star radii on the nature of phase transitions in dense matter
• Isospin dependence of nucleon emission and radial flow in heavy-ion collisions induced by high energy radioactive beams
• Bag model and quark star
• The pasta phase and its consequences on neutrino opacities
• Extended Skyrme interactions for transport model simulations of heavy-ion collisions
• Rotation at 1122 Hz and the neutron star structure
• Gravitational Wave Signatures of Highly Magnetized Neutron Stars
• A novel determination of density, temperature and symmetry energy for nuclear multi-fragmentation through primary fragment yield reconstruction
• Dense Matter in Neutron Stars with eXTP
• Optical spectroscopy of the quiescent counterpart to EXO 0748-676
• Searches for Shapiro delay in seven binary pulsars using the MeerKAT telescope
• Sensitivity of neutron to proton ratio toward the high density behavior of symmetry energy in heavy-ion collisions
• Neutron-proton bremsstrahlung from intermediate energy heavy-ion reactions as a probe of the nuclear symmetry energy?
• From the crust to the core of Neutron Stars on a microscopic basis
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• A family of well behaved charge analogues of Durgapal's perfect fluid exact solution in general relativity
• Universal relations for the Keplerian sequence of rotating neutron stars
• On attributes of a Rotating Neutron star with a Hyperon core
• Solution to the hyperon puzzle using dark matter
• LOFAR early-time search for coherent radio emission from Short GRB 181123B
• Unified description of astrophysical properties of neutron stars independent of the equation of state
• Calculation of the Structure Properties of a Strange Quark Star in the Presence of Strong Magnetic Field Using a Density Dependent Bag Constant
• Holographic Symmetry Energy of the Nuclear Matter
• Neutron star cooling - a challenge to the nuclear mean field
• The Low Quiescent X-Ray Luminosity of the Transient X-Ray Burster EXO 1747-214
• Pulsar kicks by anisotropic neutrino emission from quark matter
• CREX- and PREX-II-motivated relativistic interactions and their implications for the bulk properties of nuclear matter and neutron stars
• Nuclear Matter and Neutron Stars from Relativistic Brueckner-Hartree-Fock Theory
• Folding model study of the charge-exchange scattering to the isobaric analog state and implication for the nuclear symmetry energy
• Universal relations for compact stars with heavy baryons
• Asymmetric Nuclear Matter and Neutron Star Properties in Relativistic ab initio Theory in the Full Dirac Space
• Toward relativistic mean-field description of $\bar{\text{N}}$-nucleus reactions
• Nuclear matter fourth-order symmetry energy in non-relativistic mean-field models
• Constraining a neutron star merger origin for localized fast radio bursts
• Effects of a weakly interacting light U boson on the nuclear equation of state and properties of neutron stars in relativistic models
• Generation of the magnetic helicity in a neutron star driven by the electroweak electron-nucleon interaction
• Delineating effects of tensor force on the density dependence of nuclear symmetry energy
• Microkelvin thermometry with Bose-Einstein condensates of magnons and applications to studies of the AB interface in superfluid ${}^3$He
• Fallback accretion on to a newborn magnetar: long GRBs with giant X-ray flares
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Critical parameters of liquid-gas phase transition in thermal symmetric and asymmetric nuclear matter
• Gravitational wave asteroseismology for low-mass neutron stars
• Isoscaling behavior in the Isospin dependent Quantum Molecular Dynamics model
• Mean-field study of hot beta-stable protoneutron star matter: Impact of the symmetry energy and nucleon effective mass
• Neutron skins as laboratory constraints on properties of neutron stars and on what we can learn from heavy ion fragmentation reactions
• Relativistic Mean Field Model parameterizations in the light of GW170817, GW190814, and PSR J0740 + 6620
• Influence of the single-particle structure on the nuclear surface and the neutron skin
• Neutron-skin thickness of finite nuclei in relativistic mean-field models with chiral limits
• Study on anisotropic strange stars in $f(\mathbb{T},\mathcal{T})$ gravity
• Search for the chiral magnetic effect in collisions between two isobars with deformed and neutron-rich nuclear structures
• Anisotropic Dark Matter Stars
• Stellar Hydrostatic Equilibrium Compact Structures in $f(\mathcal{G},T)$ Gravity
• Nuclear symmetry energy effects on neutron stars properties
• Confronting a set of Skyrme and ${\chi }_{EFT}$ predictions for the crust of neutron stars
• Symmetry energy extracted from the S$\pi$RIT pion data in Sn+Sn systems
• Observational evidence for stellar-mass black holes
• Effects of nuclear symmetry energy on eta meson production and its rare decay to the dark U-boson in heavy-ion reactions
• Empirical information on nuclear matter fourth-order symmetry energy from an extended nuclear mass formula
• Differential isospin-fractionation in dilute asymmetric nuclear matter
• Isospin-asymmetric nuclear matter
• A new statistical method for the structure of the inner crust of neutron stars
• Massive Hybrid Quark Stars with Strong Magnetic Field
• Low density nuclear matter with light clusters in a generalized nonlinear relativistic mean-field model
• Hadron-quark phase transition in the SU(3) local Nambu-Jona-Lasinio (NJL) model with vector interaction
• Indirect methods in nuclear astrophysics with relativistic radioactive beams
• Links Between Heavy Ion and Astrophysics
• Experimental reconstruction of primary hot isotopes and characteristic properties of the fragmenting source in the heavy ion reactions near the Fermi energy
• Quark mean-field model for nuclear matter with or without bag
• To probe into pulsar's interior through gravitational waves
• Understanding the symmetry energy using data from the ALADIN-2000 Collaboration taken at the GSI Large Neutron Detector
• Isospin effects and symmetry energy studies with INDRA
• Masses of Neutron Stars in High-Mass X-ray Binaries with Optical Astrometry
• Triton/${}^3$He ratio as an observable for neutron skin thickness
• Inequality between size and angular momentum for bodies
• Central Speed of Sound, Trace Anomaly and Observables of Neutron Stars from Perturbative Analyses of Scaled TOV Equations
• Runaway Relaxion from Finite Density
• Axisymmetric deformations of neutron stars and gravitational-wave astronomy
• Effect of the momentum dependence of nuclear symmetry potential on pion-/pion+ ratio in heavy-ion collisions
• Parameterized non-relativistic limit of stellar structure equations in Ricci-based gravity theories
• Hydrodynamic simulations of pulsar glitch recovery
• Application of density dependent parametrization models to asymmetric nuclear matter
• Neutron Stars in frames of $R^2$-gravity and Gravitational Waves
• Constraining the equation of state of hybrid stars using recent information from multidisciplinary physics
• Density-dependent van der Waals model under the GW170817 constraint
• Tidal heating as a direct probe of strangeness inside neutron stars
• On the change of old neutron star masses with galactocentric distance
• Nuclear collective dynamics in the lattice Hamiltonian Vlasov method
• Superfluidity and excitations at unitarity
• Effects of the density dependence of nuclear symmetry energy on properties of superheavy nuclei
• Comparison between the Thomas-Fermi and Hartree-Fock-Bogoliubov Methods in the Inner Crust of a Neutron Star: The Role of Pairing Correlations
• Exploring universal characteristics of neutron star matter with relativistic \textit{ab initio} equations of state
• A phenomenological equation of state for isospin asymmetric nuclear matter
• Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque
• A direct probe of the in-medium pn scattering cross section
• Relativistic approach for the determination of nuclear and neutron star properties in consideration of PREX-II results
• Model dependence of isospin sensitive observables at high densities
• Effective interactions of hyperons and mass-radius relation of neutron stars
• Impact of The Newly Revised Gravitational Redshift of X-ray Burster GS 1826-24 on The Equation of State of Supradense Neutron-Rich Matter
• Dense nuclear matter and symmetry energy in strong magnetic fields
• Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars
• Effect of nucleon effective mass and symmetry energy on the neutrino mean free path in a neutron star
• Decomposition of sensitivity of the symmetry energy observables
• Ensemble in-equivalence in supernova matter within a simple model
• Old neutron stars as probes of isospin-violating dark matter
• Chandra Observations of 1RXS J141256.0+792204 (Calvera)
• Binary Pulsars in Magnetic Field versus Spin Period Diagram
• Isobaric incompressibility of the isospin asymmetric nuclear matter
• Heavy-ion Collisions: Direct and indirect probes of the density and temperature dependence of Esym
• Breaking of universal relationships of axial wI-modes in hybrid stars: rapid and slow hadron-quark conversion scenarios
• Investigating Variability of Quiescent Neutron Stars in the Globular Clusters NGC 6440 and Terzan 5
• Symmetry energy and neutron star properties in the saturated Nambu-Jona-Lasinio model
• Symmetry energy at subnuclear densities deduced from nuclear masses
• Properties of neutron star described by a relativistic $abinitio$ model
• Effect of the momentum dependence of nuclear symmetry potential on the transverse and elliptic flows
• Collisionless drag for a one-dimensional two-component Bose-Hubbard model
• Nuclear collective dynamics in transport model with the lattice Hamiltonian method
• Chandra Observation of Quiescent Low-Mass X-ray Binaries in the Globular Cluster NGC 6304
• Twist-induced Magnetosphere Reconfiguration for Intermittent Pulsars
• Stability of the $\beta$-equilibrated dense matter and core-crust transition in neutron stars
• On the relativistic precession and oscillation frequencies of test particles around rapidly rotating compact stars
• Uniqueness of the Inflationary Higgs Scalar for Neutron Stars and Failure of non-inflationary Approximations
• Radio pulsar populations
• New covariant density functionals of nuclear matter for compact star simulations
• Mean free path and shear viscosity in central ${}^{129}$Xe+${}^{119}$Sn collisions below 100 MeV/nucleon
• Warm asymmetric quark matter and proto-quark stars within the confined-isospin-density-dependent mass model
• Relativistic kinetic theory for spin-1/2 particles: Conservation laws, thermodynamics, and linear waves
• Analyzing the speed of sound in neutron star with machine learning
• Thermodynamical properties of a neutral vector boson gas in a constant magnetic field
• Optical spectroscopy and Doppler tomography of Cygnus X-2
• The radiative efficiency of relativistic jet and wind: A case study of GRB 070110
• Constraining the density dependence of the nuclear symmetry energy from an X-ray bursting neutron star
• Holographic cold dense matter constrained by neutron stars
• Strange Quark Stars as Probe of Dark Matter
• Energy release from hadron-quark phase transition in neutron stars and the axial $w$-mode of gravitational waves
• Rotating hybrid stars with the Dyson-Schwinger quark model
• Effects of hadron-quark phase transition on properties of Neutron Stars
• The kinks in charge radii across $N$ = 82 and 126 revisited
• Effects of the U-boson on the inner edge of neutron star crusts
• Neutrino trapping in braneworld extremely compact stars
• Neutron Stars in Modified Teleparallel Gravity
• Radial oscillations in neutron stars from QCD
• Bayesian Inference of dense matter equation of state of neutron star with antikaon condensation
• Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations
• Effects of symmetry energy in ${}^{132}\mathrm{Sn}{+}^{124}\mathrm{Sn}$ reaction at 300 MeV/nucleon
• A new well behaved class of charge analogue of Adler's relativistic exact solution
• Reconstructed primary fragments and symmetry energy, temperature and density of the fragmenting source in ${}^{64}$Zn + ${}^{112}$Sn at 40 MeV/nucleon
• Effects of nuclear symmetry energy and in-medium NN cross section in heavy-ion collisions at beam energies below the pion production threshold
• Model Atmospheres for X-ray Bursting Neutron Stars
• Relationship between the symmetry energy and the single-nucleon potential in isospin-asymmetric nucleonic matter
• Effect of the $\sigma$-cut potential on the properties of neutron stars with or without a hyperonic core
• Early Evolution of a Newborn Magnetar with Strong Precession Motion in GRB 180620A
• Comparison of the Characteristics of Magnetars Born in Death of Massive Stars and Merger of Compact Objects With {\em Swift} Gamma-Ray Burst Data
• Hybrid stars with color superconducting cores in an extended FCM model
• The evolution of low mass, close binary systems with a neutron star component: a detailed grid
• Production of cascade hypernuclei via the (K-,K+) reaction within a quark-meson coupling model
• Parity Violation in Astrophysics
• Skyrmion Stars: Astrophysical motivations and implications
• Spherically symmetric elastic bodies in general relativity
• Role of the symmetry energy slope in neutron stars: exploring the model-dependency
• Tidal Deformability of Strange Quark Planets and Strange Dwarfs
• On the role of strong gravity in polarization from scattering of light in relativistic flows
• Modeling the Multi-Band Afterglow of GRB 130831A: Evidence for a Spinning-Down Magnetar Dominated by Gravitational Wave Losses?
• Neutron stars and stellar mergers as a laboratory for dense QCD matter
• Floquet Spinor Bose Gases
• Degenerate fermionic matter at N${}^3$LO: Quantum Electrodynamics
• Neutron star mass in dark matter clumps
• The newly born magnetars powering gamma-ray burst internal-plateau emission: are there strange stars?
• The Buchdahl Stability Bound in Eddington-inspired Born-Infeld Gravity
• On the Chandrasekhar Limit in Generalized Uncertainty Principles
• The ASY-EOS experiment at GSI: investigating the symmetry energy at supra-saturation densities
• Linear response study of collisionless spin drag
• Effects of Onset of Phase Transition on Binary Neutron Star Mergers
• Isotropic and anisotropic neutron star structure in 4D Einstein Gauss Bonnet Gravity
• Observation of hypertritons in Au+Au collisions at \sqrt{s_{NN}} = 200 GeV
• Symmetry energy, unstable nuclei, and neutron star crusts
• Rapid Spin Deceleration of Magnetized Proto-Neutron Stars via Asymmetric Neutrino Emission
• Properties of quark-matter cores in massive hybrid stars
• Modeling the Ionosphere with GPS and Rotation Measure Observations
• A Machine Learning Approach For Classifying Low-mass X-ray Binaries Based On Their Compact Object Nature
• Dense matter equation of state and phase transitions from a Generalized Skyrme model
• Neutron-superfluid vortices and proton-superconductor flux tubes: Development of a minimal model for pulsar glitches
• A minimal model for finite temperature superfluid dynamics
• Nucleon Effective E-Mass in Neutron-Rich Matter from the Migdal-Luttinger Jump
• Strange star equations of state revisited
• Multi-Wavelength Observations of GRB 111228A and Implications for the Fireball and its environment
• From chiral EFT to perturbative QCD: a Bayesian model mixing approach to symmetric nuclear matter
• Gravitational Collapse of Baryonic and Dark matter
• Gravitational Waves from Newborn Accreting Millisecond Magnetars
• New JWST redshifts for the host galaxies of CDF-S XT1 and XT2: understanding their nature
• Early Optical Observations of GRB 150910A: Bright Jet Optical Afterglow and X-ray Dipole Radiation from a Magnetar Central Engine
• Neutron stars within the Skyrme model
• Nuclear pasta and symmetry energy in the relativistic point-coupling model
• Braking indices of pulsars obtained in the presence of an effective force
• Neutron Skins: Weak Elastic Scattering and Neutron Stars
• Scale invariant elastic stars in General Relativity
• Constraining Palatini gravity with GR-independent equations of state for neutron stars
• Astro-quark matter: a challenge facing astroparticle physics
• Spin-down induced quark-hadron phase transition in cold isolated neutron stars
• Universal Relations For Generic Family Of Neutron Star Equations Of State
• Recalibration of the binding energy of hypernuclei measured in emulsion experiments and its implications
• The cooling, mass and radius of the neutron star in EXO 0748-676 in quiescence with XMM-Newton
• Incompressibility and Symmetry Energy of Neutron Star
• Charged pion production from Au + Au collisions at $\sqrt{s_{NN}}=2.4$ GeV in the Relativistic Vlasov-Uehling-Uhlenbeck model
• Quenched Λ spin-orbit splitting by relativistic Fock diagram in single-Λ hypernuclei
• Quark Matter Equation of State from Perturbative QCD
• The White Dwarf Companion of a 2 M_sun Neutron Star
• Nuclear symmetry energy and proton-rich reactions at intermediate energies
• Rotational parameters of strange stars in comparison with neutron stars
• High $p_t$ squeezed-out n/p ratio as a probe of $K_{\mathrm{sym}}$ of the symmetry energy
• Neutron Stars In $f(R,T)$ Theory: Slow Rotation Approximation
• Implications of Fermionic Dark Matter Interactions on Anisotropic Neutron Stars
• Spin-down of neutron stars by neutrino emission
• Black hole-neutron star mergers with massive neutron stars in numerical relativity
• Glitches due to (quasi) neutron-vortex scattering in the superfluid inner crust of a pulsar
• Relativistic self-energy decomposition of nuclear symmetry energy and equation of state of neutron matter within QCD sum rules
• Determining the density dependence of the nuclear symmetry energy using heavy-ion reactions
• Determination of the density region of the symmetry energy probed by the ${\pi }^{-}/{\pi }^{+}$ ratio
• The radius of a typical-mass neutron star and chiral effective field theory
• Investigating the role of nuclear parameters on oscillation modes in hot Neutron Stars
• Impact of strong magnetic fields on the inner crust of neutron stars
• Competition between fermions and bosons in nuclear matter at low densities and finite temperatures
• Does Sub-millisecond Pulsar XTE J1739-285 Contain a Low Magnetic Neutron Star or Quark Star ?
• Role of isospin physics in supernova matter and neutron stars
• Observable form of pulses emitted from relativistic collapsing objects
• Hadron-quark phase transition in neutron star by combining the relativistic Brueckner-Hartree-Fock theory and Dyson-Schwinger equation approach
• Probing the density dependence of the symmetry energy by nucleon flow
• Supernova Neutrinos as a Precise Probe of Nuclear Neutron Skin
• Improving Pulsar Timing Precision with Single Pulses
• Pasta phases in neutron stars under strong magnetic fields
• $f$-mode oscillations of dark matter admixed quarkyonic neutron star
• Approximative Analytic Study of Fermions in Magnetar's Crust; Ultra-relativistic Plane Waves, Heun and Mathieu Solutions and Beyond
• Geometric creation of quantum vorticity
• Equation of state and hybrid star properties with the weakly interacting light U-boson in relativistic models
• A key factor to the spin parameter of uniformly rotating compact stars: crust structure
• The Auxiliary Field Diffusion Monte Carlo Method for Nuclear Physics and Nuclear Astrophysics
• Describing the speed of sound peak of isospin-asymmetric cold strongly interacting matter using effective models
• SWIFT J1749.4-2807: A neutron or quark star?
• Binary evolution leading to the formation of the very massive neutron star in the J0740+6620 binary system
• Phase Diagrams of Antiferromagnetic Spin-1 Bosons on Square Optical Lattice with the Quadratic Zeeman Effect
• Moments of inertia of neutron stars in relativistic mean field theory: the role of the isovector scalar channel
• Symmetry energy softening in nuclear matter with non-nucleonic constituents
• Initialization effect in heavy-ion collisions at intermediate energies
• Approximate Spacetime for Neutron Stars
• The Mass Spectrum of X-Ray Binaries
• Pulsar PSR B0943+10 as an isotropic Vaidya-Tikekar type compact star : A comprehensive study
• Improved Analytic Love-C Relations for Neutron Stars
• The electromagnetic and gravitational-wave radiations of X-ray transient CDF-S XT2
• Multipolar Electromagnetic Emission of Newborn Magnetar
• Multimessenger signal from phase transition of neutron star to quark star
• Time-dependent nuclear energy-density functional theory toolkit for neutron star crust: Dynamics of a nucleus in a neutron superfluid
• Probing dense matter in compact star cores with radio pulsar data
• Noncyclic geometric phases and helicity transitions for neutrino oscillations in a magnetic field
• Boundary conditions for star matter and other periodic fermionic systems
• Neutron and quark stars: constraining the parameters for simple EoS using the GW170817
• Rotating Neutron Stars with the Relativistic Ab Initio Calculations
• Statistical analysis of experimental multifragmentation events in ${}^{64}$Zn + ${}^{112}$Sn at 40 MeV/nucleon
• Effects of ${\varphi }_0$-meson on the EOS of hyperon star in the relativistic mean field model
• Astrophysical Quark Matter
• Quark deconfinement in neutron star cores and the ground state of neutral matter
• Towards a unified hadron-quark equation of state for neutron stars within the relativistic mean-field model
• Insights Into Neutron Stars From Gravitational Redshifts and Universal Relations
• Phase diagram of neutron-rich nuclear matter and its impact on astrophysics
• Disentangling effects of collision geometry and symmetry energy in U+U collisions
• Superfluid effects on gauging core temperatures of neutron stars in low-mass X-ray binaries
• Letter of Intent: the NA60+ experiment
• Investigation of neutron density distribution of ${}^{208}$Pb nucleus when the proton density is constrained to its experimental distribution
• Anti-de Sitter neutron stars in the theory of gravity with nonminimal derivative coupling
• Can the nuclear symmetry potential at supra-saturation densities be negative?
• r-mode instability of neutron stars in low-mass X-ray binaries: effects of Fermi surface depletion and superfluidity of dense matter
• On the minimum spin period of accreting pulsars
• Dark Matter Influence on Quarkyonic Stars: A Relativistic Mean Field Analysis
• Tidal dissipation in binary neutron star inspirals from hyperon bulk viscosity: Phase modeling and parameter estimation bias
• Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers
• Color superconductivity in the Nambu Jona-Lasinio model complemented by a Polyakov loop
• Novel technique to extract experimental symmetry free energy information of nuclear matter
• Neutron stars as probes of extreme energy density matter
• A Search for Rapidly Spinning Pulsars and Fast Transients in Unidentified Radio Sources with the NRAO 43-Meter Telescope
• Symmetry potentials and in-medium nucleon-nucleon cross sections within the Nambu-Jona-Lasinio model in relativistic impulse approximation
• Distinguishing Bare Quark Stars from Neutron Stars
• Triton-3He relative and differential flows and the high density behavior of nuclear symmetry energy
• Compositional Freeze-Out of Neutron Star Crusts
• QCD Corrections to QED Vacuum Polarization
• Recent astrophysical and accelerator based results on the Hadronic Equation of State
• Possible evidence that pulsars are quark stars
• Detections of millisecond pulsars with the Fermi Large Area Telescope
• Pygmy resonances and symmetry energy
• VLT/FORS2 observations of the optical counterpart of the isolated neutron star RBS 1774
• Testing the Accretion-induced Field-decay and Spin-up Model for Recycled Pulsars
• Pairing effects on neutron matter equation of state and symmetry energy at subsaturation densities
• Suitable resolution for EOS tables in neutron star investigation
• Sensitivity of deexcitation energies of superdeformed secondary minima to the density dependence of symmetry energy with the relativistic mean-field theory
• Gap-bridging enhancement of modified Urca processes in nuclear matter
• Distinct Classes of Compact Stars Based On Geometrically Deduced Equations of State
• Neutron Star Radius-to-mass Ratio from Partial Accretion Disc Occultation as Measured through Fe K$\alpha$ Line Profiles
• Blind spots of probing the high-density symmetry energy in heavy-ion collisions
• Searching for Sub-Second Stellar Variability with Wide-Field Star Trails and Deep Learning
• A Pseudo-Photon in Non-Trivial Background Fields
• Study of hybrid stars with nonstrange quark matter cores
• Constraining the Skyrme effective interactions and the neutron skin thickness of nuclei using isospin diffusion data from heavy ion collisions
• Nuclear collision in strong magnetic field
• Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?
• Slowly rotating neutron stars and hadronic stars in chiral SU(3) quark mean field model
• Gravitomagnetism in superconductors and compact stars
• Neutron Stars and Black Holes in Star Clusters
• Impact of Neutrino Flavor Conversions on Neutron Star Merger Dynamics, Ejecta, Nucleosynthesis, and Multi-Messenger Signals
• Neutron matter within QCD sum rules
• Three-body force effect on neutrino emissivities of neutron stars within the framework of the Brueckner-Hartree-Fock approach
• The Possible Electromagnetic Counterparts of the First High-Probability NSBH Merger LIGO/Virgo S190814bv
• How do mirror charge radii constrain density dependence of the symmetry energy?
• Microscopic constraints for the equation of state and structure of neutron stars: a Bayesian model mixing framework
• Quark matter and the astrophysics of neutron stars
• Direct Inference of Nuclear Equation-of-State Parameters from Gravitational-Wave Observations
• $f$-mode oscillations in hot Neutron Stars: Effect of hyperons and neutrino trapping
• Properties of glitching pulsars in the Skyrme-Hartree-Fock framework
• The Impact of $f(\mathcal{G},T)$ Gravity on the Evolution of Cavity in the Cluster of Stars
• Novel halos in light kaonic nuclei as an indicator of nuclear equation of state at supra-normal densities
• Constraining the Hadron-Quark Phase Transition Chemical Potential via Astronomical Observation
• Search for Redshifted 2.2 MeV Neutron Capture Line From A0535+262 in Outburst
• Charmed hypernuclei within density-dependent relativistic mean-field theory
• Single-Particle Spectrum of Pure Neutron Matter
• Mass Distribution and "Mass Gap" of Compact Stellar Remnants in Binary Systems
• Effect of liquid drop model parameters on nuclear liquid gas phase transition
• On the Formation of SMC X-1: the Effect of Mass and Orbital Angular Momentum Loss
• Symmetry energy from fragment observables in the canonical thermodynamic model
• Neutron star under homotopy perturbation method
• Correlation between the curvature and some properties of the neutron star
• The origin of the elements and other implications of gravitational wave detection for nuclear physics
• Probing the symmetry energy with isospin ratio from nucleons to fragments
• Note on neutron star equation of state in the light of GW170817
• The kHz QPOs of Neutron Stars and Millisecond Pulsars and Implications
• Measurement of $p$-${\Xi }^{-}$ ($\bar{p}$-${\bar{\Xi }}^{+}$) Correlation Function in Isobar and Au+Au Collisions at $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV with the STAR Detector
• Probing $\Lambda$ potential via its $v_2$ flow in hypernuclei-induced reaction
• A deep search for radio pulsations from the 1.3 M${}_{\odot }$ compact-object binary companion of young pulsar PSR J1906+0746
• Recent progress on superstrange dynamics
• Stellar Evolution in Close Binaries: Processes and Outcomes
• New solution to the hyperon puzzle of neutron stars: Quantum many-body effects
• Vacuum fluctuation effects on asymmetric nuclear matter
• Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement
• Some aspects of the phase diagram of nuclear matter relevant to compact stars
• Theoretical constraints on properties of low-mass neutron stars from EOS of inner crust matters
• Applications of the Octet Baryon Quark-Meson Coupling Model to Hybrid Stars
• Plasma Instabilities Dominate Radioactive Transients Magnetic Fields: The self-confinement of leptons in Type Ia and Core-Collapse Supernovae, and Kilonovae
• Dipole Polarizability of Finite Nuclei as a Probe of Neutron Stars
• Characterization of the inner edge of the neutron star crust
• Isospin Asymmetry in Nuclei, Neutron Stars, and Heavy-Ion Collisions
• Gravitational wave signatures of phase transition from hadronic to quark matter in isolated neutron stars and binaries
• Neutron Star as a Mirror for Gravitational Waves
• Constraining properties of neutron stars with heavy-ion reactions in terrestrial laboratories
• BPS Skyrme neutron stars in generalized gravity
• Freeze-out and thermalization in relativistic heavy ion collisions
• Properties of rotating neutron stars in light of binary compact object mergers
• Neutron-rich nuclei and the equation of state of stellar matter
• Schwinger-Keldysh approach to tunneling transport at a hadron-quark interface
• Phase Structure of Compact Star in Modified Quark-Meson Coupling Model
• Constraining the relative inclinations of the planets B and C of the millisecond pulsar PSR B1257+12
• Magnetic coupling through flux branching of adjacent type-I and -II superconductors in a neutron star
• True Unicorns and False Positives: Simulated Probabilities of Dark Massive Companions to Bright Stars
• Landau parameters and entrainment matrix of cold stellar matter: effect of the symmetry energy and strong magnetic fields
• Neutron Star News and Puzzles
• Transition Density and Pressure at the Inner Edge of Neutron Star Crusts
• ${\Omega }^{-}$ production as a probe of equation of state of dense matter near the QCD phase transition in relativistic heavy-ion collisions
• Microlensing pulsars
• The first extragalactic ultra-compact X-ray binary : a candidate black hole-white dwarf system
• Degeneracy, the virial theorem, and stellar collapse
• Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars?
• Axial Gravitational Normal Modes of Uniform Density Star in Anti-de Sitter Spacetime
• Primordial black holes versus their impersonators at gravitational wave observatories
• High-density Skyrmion matter and Neutron Stars
• Neutron tunneling: A new mechanism to power explosive phenomena in neutron stars, magnetars, and neutron star mergers
• Slowly rotating condensate dark stars beyond the mean-field approximation
• Triaxial instabilities in rapidly rotating Neutron Stars
• Searching For Strange Quark Planets
• Maximum mass limit of strange stars in quadratic curvature-matter coupled gravity
• Baryons in the Nambu Jona-Lasinio models
• Impact of Anisotropy on Neutron Star Structure and Curvature
• On Modeling Anisotropic Quark Stars: The Role of Anisotropy in Radial Oscillation Spectra
• Universal relation between dipole polarizability of finite nuclei and neutron-star compactness
• Constraining the parameterized neutron star equation of state with astronomical observations
• Probing the density dependence of symmetry energy at subsaturation density with HICs
• Compact elastic objects in general relativity
• Incompressibility of asymmetric nuclear matter
• Structural Properties of Magnetized Neutron Stars under f (R, T ) Gravity Framework
• Astrometric microlensing probes of the isolated neutron star population with Roman
• Classification of $g$-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars
• The Low-Frequency Spectra of Radio Pulsars
• Flux tube clustering from magnetic coupling of adjacent type-I and -II superconductors in a neutron star: persistent gravitational radiation
• Performance of the prototype beam drift chamber for LAMPS at RAON with proton and Carbon-12 beams
• Isospin blocking and its effects in heavy-ion collisions
• Search for gravitational-wave bursts in LIGO data at the Schenberg antenna sensitivity range
• Basic quantities of the Equation of State in isospin asymmetric nuclear matter
• Realistic Equations of State Informing Neutron Star Post-Merger Gravitational-Wave Frequencies
• Constraining Hamiltonians from chiral effective field theory with neutron-star data
• Prompt and Afterglow Constraints on the Central Engine of GRB 240825A
• On the desert between neutron star and black hole remnants
• Vortex Retention Mediated Turbulent Transitions in Self-Gravitating Bosonic and Axionic Condensates
• The Relativistic Gravitational Field of a Spherically Symmetric Extended Body
• Fully general relativistic description of rapidly-rotating axially-symmetric neutron stars for constraining nuclear matter equations of state
• Tidal Love numbers and the dynamical instability of AdS bubbles
• Unified nonparametric equation-of-state inference from the neutron-star crust to perturbative-QCD densities
• Can a supernova bang twice?
• Formation of large chunk of nuclear matter in heavy-ion collisions
• Radial oscillations of quark stars in light of current astrophysical constraints: A comparative study
• Hyperstars - Main Origin of Short Gamma Ray Bursts?
• Structure of Anisotropic Magnetized Neutron Stars in f(R,T) Gravity with Realistic Equation of State