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Neutron Stars

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lightbulbAbout this topic
Neutron stars are extremely dense remnants of massive stars that have undergone supernova explosions. Composed primarily of neutrons, they exhibit strong gravitational and magnetic fields, and possess rapid rotation rates. Their study provides insights into fundamental physics, including nuclear interactions and the behavior of matter under extreme conditions.
lightbulbAbout this topic
Neutron stars are extremely dense remnants of massive stars that have undergone supernova explosions. Composed primarily of neutrons, they exhibit strong gravitational and magnetic fields, and possess rapid rotation rates. Their study provides insights into fundamental physics, including nuclear interactions and the behavior of matter under extreme conditions.

Key research themes

1. How does the presence and nature of quark matter affect the equation of state and observable properties of neutron stars?

This research area focuses on understanding the transition from hadronic matter to quark matter inside neutron stars, the corresponding changes in the equation of state (EoS), and how these changes influence neutron star maximum mass, radius, tidal deformability, and gravitational wave signatures. It is crucial for interpreting observations from X-ray missions, gravitational wave detectors, and multimessenger astronomy to constrain dense matter physics beyond nuclear saturation density.

Key finding: Presents unified equations of state incorporating a crossover transition from hadronic to quark matter (QHC18 EoS), showing that large repulsive density-density and attractive diquark pairing interactions are favored by... Read more
Key finding: Using a hybrid EoS between a model-independent Taylor expansion for hadronic matter and a Nambu-Jona-Lasinio (NJL) model for quark matter, the study finds large quark cores (up to half the star mass) possible if the... Read more
Key finding: Demonstrates that gravitational wave emission from postmerger phase is sensitive to the presence of a quark-hadron crossover transition in the neutron star EoS, with the QHC19 EOS showing longer-duration and shifted peak... Read more
Key finding: Combines a density-dependent relativistic mean-field model including hyperons with a color superconducting three-flavor NJL model for quark matter to construct hybrid star EoSs meeting the 2 M☉ mass constraint. Shows stable... Read more
Key finding: By applying realistic equations of state across neutron star layers (including crust) in the framework of modified gravity (f(R,T) theory), the work finds that modifications slightly increase maximum mass (<1%) and restrict... Read more

2. What do neutron star mass distributions and maximum mass constraints imply about the dense matter equation of state?

This theme investigates neutron star mass measurements from radio pulsars, binary systems, and gravitational wave detections to infer the shape of the underlying mass distribution and the existence of a maximum stable neutron star mass. Establishing the maximum mass informs nuclear and quark matter EoS stiffness, constrains sound speeds in dense matter, and affects interpretations of mergers and gamma-ray bursts.

Key finding: Using a Gaussian mixture model and Bayesian model selection on neutron star masses in binaries, the study finds strong evidence for a bimodal mass distribution with a sharp high-mass cutoff between 2.0 and 2.6 M☉ (90%... Read more
Key finding: By jointly modeling the NS mass distribution and spin dependence in NS–BH mergers, and including the possibility of rapid NS rotation increasing maximum mass up to ~20%, the paper infers maximum nonspinning NS mass around... Read more
Key finding: Analyzing a catalogue of 56 young neutron stars associated with supernova remnants, the authors find distributions of initial spin periods and magnetic fields are well described by lognormal distributions with means... Read more
Key finding: Modeling accretion disks around neutron and quark stars, the study shows that electromagnetic emission properties (energy flux, temperature distribution, spectrum) differ depending on the underlying EoS and type of compact... Read more

3. How do high magnetic fields and alternative gravity theories alter neutron star maximum mass limits and structural properties?

This research area examines the impact of strong magnetic fields, presence of hyperons, and modifications to General Relativity on neutron star structure and maximum mass. By extending gravity theories (e.g., f(R), f(R,T)) and incorporating magnetic pressure contributions, these studies explore how to reconcile observations of massive neutron stars exceeding 2 M☉ with theoretical models including exotic matter.

Key finding: By incorporating cubic and quadratic corrections in f(R) and f(G) gravity models alongside strong magnetic fields up to 6–8 ×10¹⁸ G, the paper shows that maximum neutron star masses can exceed 3-4 M☉, with stable stars... Read more
Key finding: Employing realistic nuclear matter EoSs and f(R,T) gravity with R+2λT form, the work constrains λ to be |λ| ≲ 0.02 due to effects on the low sound speed in neutron star crusts. The modifications can increase maximum neutron... Read more
Key finding: Using a unified approach with a consistent EoS (Brueckner-Hartree-Fock) and microscopic superfluid gaps for nucleons, and accounting for direct Urca processes occurring at low NS masses (~1.1 M☉), the study finds that proton... Read more

All papers in Neutron Stars

The Strathprints institutional repository () is a digital archive of University of Strathclyde research outputs. It has been developed to disseminate open access research outputs, expose data about those outputs, and enable the management... more
Phase 12 extends the Unified Loop Framework from the cosmic scale of Phase 11 to the full stellar and compact-object lifecycle. The framework's atomic primitive, a figure-8 with paired black-hole-mode and white-hole-mode lobes, is shown... more
Cosmic Gravitational Depth Theory (CGDT) proposes that gravity is not merely an attractive interaction between masses but the observable manifestation of a deeper multidimensional process. According to this framework, all matter exists... more
We present a unified, observationally grounded framework showing that stored rotational energy (E rot ) is the missing gravitational component that explains galactic rotation curves without dark matter. We further show how the same... more
[59] This paper explores a speculative geometric framework — the “0-Sphere model” — that attempts to reinterpret microscopic gravitational structure through trajectory-based internal dynamics rather than conventional local field... more
General relativity defines horizons through coordinate geometry, without a strictly local, coordinateindependent scalar criterion. This Letter demonstrates that within the C(r) information-carrying capacity framework [1], the condition C̃... more
We describe directed searches for continuous gravitational waves in data from the sixth LIGO science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with... more
This paper presents a unified cosmological model proposing that our observable universe exists within the event horizon of a parent singularity. We hypothesize that the birth of a universe is a 'Quantum-Dark' event, where the collapse of... more
Standard astrophysical models fail to reconcile the mass-radius relationship of massive neutron stars like PSR J0740+6620 without invoking exotic states of matter. This paper proposes a deterministic solution based on the Fabric... more
We present a numerical demonstration of the duality between the geometric Lagrangian L_geo = 4·ḋ² + (1/R)·d² + (1/4)·√(R²-d²) (describing an oscillating circle of radius R = π) and the Polyakov Lagrangian for a bosonic string compactified... more
This hypothesis proposes a model of galactic dynamics that replaces the dark matter (DM) postulate with the interaction of Coulomb forces arising from charge asymmetry in astrophysical plasma. The central engine of the system is a... more
Preamble: Context and Motivation This document develops, in full, the following integrated thesis, connecting the deepest structures of the Riemann zeta function to observable gravitational, astrophysical, and electroweak phenomena. The... more
We present the dτ-Aperiodic Structural Model (dτ-ASM), a deterministic quasicrystalline framework derived from the prime-logarithmic spectral grid and a τ-symmetric cut-and-project construction. The resulting structure is a... more
Contemporary astrophysics models mass loss prior to a supernova explosion primarily through the phenomenological hydrodynamics of hot gases and radiationdriven stellar winds. However, these models fail to causally explain exact mass cuts... more
We apply the Recursive Harmonic Coherence Model (RHCM) φ-shell framework to 243 compact binary coalescence events from the LIGO, Virgo, and KAGRA catalogues (O1-O5 partial), spanning binary black hole (BBH), binary neutron star (BNS), and... more
by A H
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst... more
In this work, we offer a new exact solution to the Einstein-Maxwell field equations that describe a charged anisotropic compact star that is spherically symmetric, static, and subject to a quadratic equation of state. By adopting a... more
In this paper, we construct the Schwarzschild-de Sitter metric as the spherically symmetric static exact solution of the vacuum Einstein equation G µν + Λ g µν = 0 (Λ = 3/R 2) derived in the preceding paper [1]. This exact solution is... more
In previous papers discussing the concept of Combined Gravitational Action (CGA), we have laid the theoretical foundations for CGA as an alternative theory of gravity based solely on Euclidean geometry, the Galilean relativity principle,... more
We report on observations of the polarization of optical and γ -ray photons from the Crab nebula and pulsar system using the Galway Astronomical Stokes Polarimeter (GASP), the Hubble Space Telescope, Advanced Camera for Surveys and the... more
The Infinity galaxy black hole sits between two merging galaxies with no stellar seed. PUH says Planck Stars form wherever SPF density reaches the Planck threshold — no stellar precursor required, no particular location required. A merger... more
The standard model of physics treats the universe as a single continuous arena governed by four known forces. This paper proposes the Layered Universe Hypothesis (LUH): the universe is organised into three nested structural layers-the... more
A fundamental relationship has been hidden in the mathematics of physics for over 300 years. The mechanics of Newton, the atomic model of Bohr, the field equations of Einstein, the geometry of Schwarzschild, and the cosmology of Friedmann... more
The observable universe has a conventional compactness Cconv = GM/(Rc²) ≈ 0.17, placing it inside its own gravitational closure threshold of Cconv = 1/4. Inside a gravitational closure, field energy cannot propagate beyond the boundary.... more
The maximum compactness of stable baryonic matter is Ccrit = GM/(Rc²) = 1/4. General Relativity places a weaker bound at the Buchdahl limit C ≤ 4/9 ≈ 0.44, yet every observed neutron star with a directly measured mass and radius satisfies... more
The CCEGA framework contains a single free parameter, the critical density ρ c , at which the modulus eld ϕ exits its vacuum and the eective gravitational coupling G eff begins to fall below G. In Papers 1617 this parameter was xed... more
The Ramesh Theory of Everything (Ramesh TOE) replaces the concept of fundamental rest mass with purely dynamic/kinetic energy stored in stable soliton excitations of a single density layer (ρ ≈ ρ 0 = 1.39) under absolute universal time T.... more
The Spacetime Wave Theory of Lewis requires the electron orbital wave to execute 36,863 wavelengths before phase closure, with 96.5 wavelengths per orbit and 382 orbits, all derived from the Balmer formula. The geometric field closure... more
Brocco's Threshold identifies a single geometric constant — s_crit = 1/(4π) ≈ 0.0796 — that predicts the onset of coherent emission in every class of accreting system tested, from white dwarfs at 0.6 solar masses to supermassive black... more
In this Review we study the nuclear pastas as they are expected to be formed in neutron star cores. We start with a study of the pastas formed in nuclear matter (composed of protons and neutrons), we follow with the role of the electron... more
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst... more
We present the set of deep Neutron Star Interior Composition Explorer (NICER) X-ray timing observations of the nearby rotation-powered millisecond pulsars PSRsJ0437-4715, J0030+0451, J1231-1411, and J2124-3358, selected as targets for... more
A single equation governs self-confinement from quarks to galactic black holes. When the compactness of a confined field system reaches the square of its coupling constant, the field catches its own tail and cannot extend further. It... more
Results are presented from a semi-coherent search for continuous gravitational waves from the brightest low-mass X-ray binary, Scorpius X-1, using data collected during the first Advanced LIGO observing run (O1). The search combines a... more
We describe directed searches for continuous gravitational waves in data from the sixth LIGO science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with... more
We present a unified framework for pulsar glitches and magnetar giant flares as confinement stability events governed by an action density limit at gravitational compactness C = GM/Rc2 = 1/4. This limit is the point at which the... more
We present a dynamical treatment of gravitational curvature as a propagating field sourced by mass-energy in Schwarzschild geometry. A mass M continuously sources curvature that propagates outward at the locally measured speed of light v... more
We propose that gravitational, electromagnetic, and strong force confinement are instances of a single geometric mechanism: a propagating field structure achieves self-closure when its dimensionless confinement compactness-the ratio of... more
The ROSE postulate (Randomly Organized Structural Entities) proposes a topology-first account of structural realism: what is most invariant in nature is not the specific catalogue of forces used to model localized phenomena, but a limited... more
We investigate long Gamma-Ray Bursts (GRB) which manifest a sharp linear rise followed by an exponential decay in their γ-ray prompt emission observed with the BAT instrument on board the Swift satellite. We offer a simple electrodynamic... more
We derive an empirical relation between neutron star mass and radius using compactness as the primary variable. Fitting to 58 neutron stars with well-constrained measurements, we obtain a quadratic compactness-mass law achieving R 2 =... more
Background: Thyroid Nodules (TN) are the most common endocrine disorder worldwide. Etiology and pathogenesis of thyroid benign and malignant nodules (TBN and TMN, respectively) are still not enough understood. The present study was... more
Studying the effect of magnetic fields on particle emission from the surface of neutron stars is vital for advancing our understanding of neutron star physics and high-energy astrophysical processes. One of the main topics in pulsar... more
Neutron stars provide a unique laboratory for studying matter at extreme pressures and densities. While there is no direct way to explore their interior structure, X-rays emitted from these stars can indirectly provide clues to the... more
Neutron stars provide a unique laboratory for studying matter at extreme pressures and densities. While there is no direct way to explore their interior structure, X-rays emitted from these stars can indirectly provide clues to the... more
We define a monotone scalar envelope functional that compresses neutron star compactness and tidal deformability posterior samples into a single dimensionless load variable L = C + k √ Λ ,
Physical theory provides powerful tools for predicting instability, turbulence, and collapse, yet offers no unified account of why many systems persist far beyond their nominal failure thresholds. Across fluids, plasmas, gravitating... more
We have performed detailed temporal and time-integrated spectral analysis of 286 bursts from SGR J1550 -5418 detected with the Fermi Gamma-ray Burst Monitor (GBM) in January 2009, resulting in the largest uniform sample of temporal and... more
We present the discovery of a variable optical counterpart to the unidentified gamma-ray source 3FGL J0212.1+5320 and argue that this is a new compact binary millisecond pulsar (MSP) candidate. We show 3FGL J0212.1+5320 hosts a... more
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