Rotating Stars in Relativity
arXiv:1612.03050 · doi:10.1007/s41114-017-0008-x
Abstract
Rotating relativistic stars have been studied extensively in recent years, both theoretically and observationally, because of the information they might yield about the equation of state of matter at extremely high densities and because they are considered to be promising sources of gravitational waves. The latest theoretical understanding of rotating stars in relativity is reviewed in this updated article. The sections on equilibrium properties and on nonaxisymmetric oscillations and instabilities in -modes and -modes have been updated. Several new sections have been added on equilibria in modified theories of gravity, approximate universal relationships, the one-arm spiral instability, on analytic solutions for the exterior spacetime, rotating stars in LMXBs, rotating strange stars, and on rotating stars in numerical relativity including both hydrodynamic and magnetohydrodynamic studies of these objects.
174 pages, 40 figures, accepted by Living Reviews in Relativity, matches published version
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- Radial oscillations and stability of compact stars in gravity
- GW190814: On the properties of the secondary component of the binary
- Fast Rotating Relativistic Stars: Spectra and Stability without Approximation
- On the dynamical bar-mode instability in spinning bosonic stars
- Effects of the equation of state on the bulk properties of maximally-rotating neutron stars
- Spectral classification of gravitational-wave emission and equation of state constraints in binary neutron star mergers
- PIC methods in astrophysics: Simulations of relativistic jets and kinetic physics in astrophysical systems
- Binary neutron star mergers: Effects of spin and post-merger dynamics
- Rapidly rotating -resonance-admixed hypernuclear compact stars
- Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
- Gyrohydrodynamics: Relativistic spinful fluid with strong vorticity
- Universal relations for differentially rotating relativistic stars at the threshold to collapse
- Maximum mass and universal relations of rotating relativistic hybrid hadron-quark stars
- Evolution of Highly Eccentric Binary Neutron Stars Including Tidal Effects
- Hot neutron stars with microscopic equations of state
- How to search for gravitational waves from -modes of known pulsars
- Differentially rotating neutron stars in scalar-tensor theories of gravity
- Rotating neutron stars with quark cores
- Anisotropic quark stars in gravity
- New code for equilibriums and quasiequilibrium initial data of compact objects. IV. Rotating relativistic stars with mixed poloidal and toroidal magnetic fields
- Effect of spin on the inspiral of binary neutron stars
- Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations
- Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and radius determination
- The surface of rapidly-rotating neutron stars: implications to neutron star parameter estimation
- Effects of -meson on properties of hyperon stars in density dependent relativistic mean field model
- Gravitational Waves from Core-Collapse Supernovae
- Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data
- Radial oscillations and tidal Love numbers of dark energy stars
- Speed of sound constraints on maximally rotating neutron stars
- Deformed black hole in Sagittarius A
- Universal relations for the Keplerian sequence of rotating neutron stars
- Hadron matter in neutron stars in view of gravitational wave observations
- Equilibrium sequences of differentially rotating stars with post-merger-like rotational profiles
- Black hole-neutron star coalescence: effects of the neutron star spin on jet launching and dynamical ejecta mass
- Universal and approximate relations for the gravitational-wave damping timescale of -modes in neutron stars
- Fast Rotating Neutron Stars: Oscillations and Instabilities
- Characterizing the breakdown of quasi-universality in the post-merger gravitational waves from binary neutron star mergers
- On the dynamical stability of quasi-toroidal differentially rotating neutron stars
- Black Hole Formation from the Collision of Plane-Fronted Gravitational Waves
- Pasta properties of the neutron star within effective relativistic mean-field model
- Revisiting the maximum mass of differentially rotating neutron stars in general relativity: Übermassive stars with realistic equations of state
- Effect of Inner Crust EoS on Neutron star properties
- Calculation of multipole moments of axistationary electrovacuum spacetimes
- Initial data for general relativistic simulations of multiple electrically charged black holes with linear and angular momenta
- Crustal properties of a neutron star within an effective relativistic mean-field model
- Models of binary neutron star remnants with tabulated equations of state
- Dense matter equation of state for neutron star mergers
- New code for equilibriums and quasiequilibrium initial data of compact objects. II. Convergence tests and comparisons of binary black hole initial data
- On the Maximum Mass of General Relativistic Uniformly Rotating White Dwarfs
- Quantifying uncertainties in general relativistic magnetohydrodynamic codes
- Quasinormal modes of supersymmetric microstate geometries from the D1-D5 CFT
- Tidal deformability and radial oscillations of anisotropic polytropic spheres
- Universal relations for innermost stable circular orbits around rapidly rotating neutron stars
- Merger-inspired rotation laws and the low-T/W instability in neutron stars
- The fate of twin stars on the unstable branch: implications for the formation of twin stars
- Gravitational Waves from Disks Around Spinning Black Holes: Simulations in Full General Relativity
- Improving the convergence order of binary neutron star merger simulations in the Baumgarte-Shapiro-Shibata-Nakamura formulation
- Epicyclic oscillations in the Hartle-Thorne external geometry
- Non-radial oscillations and global stellar properties of anisotropic compact stars using realistic equations of state
- Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
- Search for gravitational waves emitted from SN 2023ixf
- Nonlinear dynamics of oscillating neutron stars in scalar-tensor gravity
- I-Love-Q to the extreme
- Massive relativistic compact stars from SU(3) symmetric quark models
- Universal Relations for rapidly rotating neutron stars using supervised machine-learning techniques
- On the asymptotic behavior of static perfect fluids
- Magnetised neutron star crust within effective relativistic mean-field model
- Finite-temperature effects in dynamical-spacetime binary neutron star merger simulations: Validation of the parametric approach
- Nonlinear Fluctuations in Relativistic Causal Fluids
- Numerical Relativity and High Energy Physics: Recent Developments
- Rapidly spinning dark matter-admixed neutron stars
- Fundamental physics with neutron stars
- Impact of rotation on the evolution of convective vortices in collapsing stars
- Chiral symmetry breaking in accelerating and rotating frames
- Hyperonization in compact stars
- Hyperons and 's in rotating protoneutron stars: Global properties
- Neutron Stars in Palatini and Theories
- Slowly rotating Tolman VII solution
- Relating Braking Indices of Young Pulsars to the Dynamics of Superfluid Cores
- Astrophysics with the Laser Interferometer Space Antenna
- Neutron and quark stars: constraining the parameters for simple EoS using the GW170817
- Modeling matter(s) in SEOBNRv5THM: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars
- Rotating Neutron Stars with the Relativistic Ab Initio Calculations
- Ridges in rotating neutron-star properties due to first order phase transitions
- On the minimum spin period of accreting pulsars
- Effects of nucleon-nucleon short-range correlation and symmetry energy on the evolution of newly born magnetars
- Neutron stars and the cosmological constant problem
- Methods for relativistic self-gravitating fluids: From binary neutron stars to black hole-disks and magnetized rotating neutron stars
- Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
- Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?
- Structure of Polytropic Stars in General Relativity
- Testing merging of Dark Exotic Stars from Gravitational Waves in the Multi-messenger approach
- Vortex pinning in the superfluid core of relativistic neutron stars
- Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement
- Emergent spin polarization from meson condensation in rotating hadronic matter
- Shear viscosity and electrical conductivity of rotating quark matter in Nambu--Jona-Lasinio Model
- Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
- General relativistic self-gravitating equilibrium disks around rotating neutron stars
- Maximal mass of the neutron star with a deconfined quark core
- Probing the parameters of a Schwarzschild black hole surrounded by quintessence and cloud of strings through four standard astrophysical tests
- Impact of ultralight bosonic dark matter on the dynamical bar-mode instability of rotating neutron stars
- Shear Viscosity and Electrical Conductivity of Rotating Nuclear Medium in Hadron Resonance Gas and Nambu-Jona Lasinio Models
- Relativistic excitation of compact stars
- Rotating charged fluids: Theorems and results for Weyl-type systems
- Gravitational wave interactions with a viscous fluid: Core collapse supernova, binary neutron star merger, and accretion around a black hole merger
- Accuracy and Applicability of the Hartle-Thorne and Komatsu-Eriguchi-Hachisu Methods for Modeling Rotating Neutron Stars
- Luminosity of accretion disks in compact objects with quadrupole
- Slowly rotating condensate dark stars beyond the mean-field approximation
- Sudden discharge of young charged magnetars as a new model for FRBs
- Unified nonparametric equation-of-state inference from the neutron-star crust to perturbative-QCD densities
- Systematic study for the surface properties of neutron star