Physical Review D, ISSN 2470-0010, 2018, Volume 98, Issue 10, p. 104039

We present the first numerical models of differentially rotating stars in alternative theories of gravity. We chose a particular class of scalar-tensor...

GENERAL RELATIVISTIC STARS | THRESHOLD | EQUATION-OF-STATE | STABILITY | ASTRONOMY & ASTROPHYSICS | MAXIMUM MASS | PHYSICS, PARTICLES & FIELDS | Neutron stars | Gravitation | Stars | Relativity | Neutrons | Stellar evolution | Rotation | Tensors | Binary stars | Angular momentum | Stellar rotation | Mathematical models | Theory of relativity

GENERAL RELATIVISTIC STARS | THRESHOLD | EQUATION-OF-STATE | STABILITY | ASTRONOMY & ASTROPHYSICS | MAXIMUM MASS | PHYSICS, PARTICLES & FIELDS | Neutron stars | Gravitation | Stars | Relativity | Neutrons | Stellar evolution | Rotation | Tensors | Binary stars | Angular momentum | Stellar rotation | Mathematical models | Theory of relativity

Journal Article

Astronomy and Astrophysics, ISSN 0004-6361, 2002, Volume 381, Issue 3, pp. L49 - L52

A new spectral code for constructing general-relativistic models of rapidly rotating stars with an unprecedented accuracy is presented. As a first application,...

Gravitation | Stars: neutron | Relativity | Methods: numerical | Stars: rotation | stars : rotation | GENERAL RELATIVISTIC STARS | stars : neutron | STABILITY | PULSAR | GRAVITATIONAL-FIELD | NUMERICAL APPROACH | POLYTROPES | gravitation | MODELS | relativity | ASTRONOMY & ASTROPHYSICS | methods : numerical | FLUID BODIES | EQUATION | DISK

Gravitation | Stars: neutron | Relativity | Methods: numerical | Stars: rotation | stars : rotation | GENERAL RELATIVISTIC STARS | stars : neutron | STABILITY | PULSAR | GRAVITATIONAL-FIELD | NUMERICAL APPROACH | POLYTROPES | gravitation | MODELS | relativity | ASTRONOMY & ASTROPHYSICS | methods : numerical | FLUID BODIES | EQUATION | DISK

Journal Article

Reports on Mathematical Physics, ISSN 0034-4877, 2009, Volume 64, Issue 1, pp. 257 - 269

Investigation of general-relativistic spherically symmetric steady accretion of self-gravitating perfect fluid onto compact objects reveals the existence of...

general-relativistic hydrodynamics | accretion | SELFGRAVITATION | HYDRODYNAMICS | SPHERICAL ACCRETION | DEGENERATE NEUTRON CORES | PHYSICS, MATHEMATICAL | Fluid dynamics | Analysis | Fluids | Approximation | Stability | Computational fluid dynamics | Perturbation methods | Mathematical analysis | Fluid flow | Mathematical models | Physics - General Relativity and Quantum Cosmology

general-relativistic hydrodynamics | accretion | SELFGRAVITATION | HYDRODYNAMICS | SPHERICAL ACCRETION | DEGENERATE NEUTRON CORES | PHYSICS, MATHEMATICAL | Fluid dynamics | Analysis | Fluids | Approximation | Stability | Computational fluid dynamics | Perturbation methods | Mathematical analysis | Fluid flow | Mathematical models | Physics - General Relativity and Quantum Cosmology

Journal Article

Computer Physics Communications, ISSN 0010-4655, 2005, Volume 168, Issue 1, pp. 1 - 24

We present a hierarchical algorithm for the adaptation of numerical solvers in high energy astrophysics. This approach is based on clustering the entries of...

Computational methods in fluid dynamics | Magnetohydrodynamics | Physical processes | Radiation transfer | JET FORMATION | magnetohydrodynamics | physical processes | HYDRODYNAMICS | COMPTONIZATION | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | PHYSICS, MATHEMATICAL | ACCRETION DISKS | SCHEME | CODE | COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS | radiation transfer | MAGNETIC-FIELD | SYNCHROTRON EMISSION | computational methods in fluid dynamics | ROTATIONAL ENERGY | Models | Algorithms

Computational methods in fluid dynamics | Magnetohydrodynamics | Physical processes | Radiation transfer | JET FORMATION | magnetohydrodynamics | physical processes | HYDRODYNAMICS | COMPTONIZATION | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | PHYSICS, MATHEMATICAL | ACCRETION DISKS | SCHEME | CODE | COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS | radiation transfer | MAGNETIC-FIELD | SYNCHROTRON EMISSION | computational methods in fluid dynamics | ROTATIONAL ENERGY | Models | Algorithms

Journal Article

Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN 0556-2821, 12/2004, Volume 70, Issue 12, pp. 1 - 123004

We have constructed models of uniformly rotating compact stars including hyperons, Bose-Einstein condensates of antikaons, and quarks. First order phase...

GENERAL RELATIVISTIC STARS | 3RD FAMILY | DENSE | RX J185635-3754 | MODELS | NUMERICAL-METHOD | PHASE-TRANSITIONS | ASTRONOMY & ASTROPHYSICS | NEUTRON-STARS | CONDENSATION | POLYTROPES | PHYSICS, PARTICLES & FIELDS | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies

GENERAL RELATIVISTIC STARS | 3RD FAMILY | DENSE | RX J185635-3754 | MODELS | NUMERICAL-METHOD | PHASE-TRANSITIONS | ASTRONOMY & ASTROPHYSICS | NEUTRON-STARS | CONDENSATION | POLYTROPES | PHYSICS, PARTICLES & FIELDS | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies

Journal Article

Astronomy and Astrophysics, ISSN 0004-6361, 2003, Volume 405, Issue 2, pp. 405 - 408

Using a multi domain spectral method, we investigate systematically the general-relativistic model for axisymmetric uniformly rotating, homogeneous fluid...

Gravitation | Relativity | Methods: numerical | Stars: rotation | stars : rotation | GENERAL RELATIVISTIC STARS | NUMERICAL-METHOD | NEUTRON-STARS | PULSAR | POLYTROPES | gravitation | MODELS | relativity | ASTRONOMY & ASTROPHYSICS | methods : numerical | EQUILIBRIUM | FLUID BODIES | FIGURES | MACLAURIN SPHEROIDS

Gravitation | Relativity | Methods: numerical | Stars: rotation | stars : rotation | GENERAL RELATIVISTIC STARS | NUMERICAL-METHOD | NEUTRON-STARS | PULSAR | POLYTROPES | gravitation | MODELS | relativity | ASTRONOMY & ASTROPHYSICS | methods : numerical | EQUILIBRIUM | FLUID BODIES | FIGURES | MACLAURIN SPHEROIDS

Journal Article

Physical Review D, ISSN 2470-0010, 01/2016, Volume 93, Issue 2

We study the general relativistic collapse of neutron star (NS) models in spherical symmetry. Our initially stable models are driven to collapse by the...

CORES | GRAVITATIONAL COLLAPSE | RADIATION FLUID | ASTRONOMY & ASTROPHYSICS | GENERAL-RELATIVISTIC HYDRODYNAMICS | FIELD-EQUATIONS | DYNAMICS | STELLAR COLLAPSE | CRITICAL-BEHAVIOR | SCALAR FIELD | SIMILARITY | PHYSICS, PARTICLES & FIELDS | Neutron stars | Amplitudes | Stars | Gravitational collapse | Scalars | Mathematical models | Boundaries | Density

CORES | GRAVITATIONAL COLLAPSE | RADIATION FLUID | ASTRONOMY & ASTROPHYSICS | GENERAL-RELATIVISTIC HYDRODYNAMICS | FIELD-EQUATIONS | DYNAMICS | STELLAR COLLAPSE | CRITICAL-BEHAVIOR | SCALAR FIELD | SIMILARITY | PHYSICS, PARTICLES & FIELDS | Neutron stars | Amplitudes | Stars | Gravitational collapse | Scalars | Mathematical models | Boundaries | Density

Journal Article

ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 11/1994, Volume 291, Issue 1, pp. 155 - 170

A new and precise numerical code for computing equilibrium configurations of relativistic rotating bodies has been used to construct ''realistic'' rotating...

GENERAL RELATIVISTIC STARS | NUCLEAR | NUMERICAL-METHOD | STARS, NEUTRON ROTATION PULSARS EVOLUTION | MILLISECOND PULSAR | FIELD-THEORETICAL-MODEL | ASTRONOMY & ASTROPHYSICS | SPIN-UP | FLUID BODIES | EQUATIONS OF STATE | ANGULAR-MOMENTUM LOSS | EQUATION | RELATIVITY | DENSE MATTER

GENERAL RELATIVISTIC STARS | NUCLEAR | NUMERICAL-METHOD | STARS, NEUTRON ROTATION PULSARS EVOLUTION | MILLISECOND PULSAR | FIELD-THEORETICAL-MODEL | ASTRONOMY & ASTROPHYSICS | SPIN-UP | FLUID BODIES | EQUATIONS OF STATE | ANGULAR-MOMENTUM LOSS | EQUATION | RELATIVITY | DENSE MATTER

Journal Article

The Astrophysical Journal, ISSN 0004-637X, 08/2004, Volume 611, Issue 2 I, pp. 977 - 995

Some active galactic nuclei, microquasars, and gamma-ray bursts may be powered by the electromagnetic braking of a rapidly rotating black hole. We investigate...

Galaxies: active | Hydrodynamics | Turbulence | Accretion, accretion disks | Black hole physics | accretion, accretion disks | ELECTRODYNAMICS | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | MAGNETOSPHERES | ENERGY EXTRACTION | black hole physics | DRIVEN ACCRETION FLOWS | DISKS | ASTRONOMY & ASTROPHYSICS | MARGINALLY STABLE ORBIT | SPIN EVOLUTION | MAGNETIC-FIELD | galaxies : active | hydrodynamics turbulence | ROTATIONAL ENERGY | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies

Galaxies: active | Hydrodynamics | Turbulence | Accretion, accretion disks | Black hole physics | accretion, accretion disks | ELECTRODYNAMICS | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | MAGNETOSPHERES | ENERGY EXTRACTION | black hole physics | DRIVEN ACCRETION FLOWS | DISKS | ASTRONOMY & ASTROPHYSICS | MARGINALLY STABLE ORBIT | SPIN EVOLUTION | MAGNETIC-FIELD | galaxies : active | hydrodynamics turbulence | ROTATIONAL ENERGY | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 9/2000, Volume 317, Issue 3, pp. 550 - 562

We study the mathematical character of the angular moment equations of radiative transfer in spherical symmetry and conclude that the system is hyperbolic for...

methods: numerical | radiative transfer | Radiative transfer | Methods: numerical | RIEMANN SOLVERS | LOCAL CHARACTERISTIC APPROACH | MODEL | TRANSPORT | II SUPERNOVAE | STELLAR CORE COLLAPSE | ASTRONOMY & ASTROPHYSICS | methods : numerical | GENERAL-RELATIVISTIC HYDRODYNAMICS | DIFFUSION | CONSERVATION-LAWS | SCHEMES | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies

methods: numerical | radiative transfer | Radiative transfer | Methods: numerical | RIEMANN SOLVERS | LOCAL CHARACTERISTIC APPROACH | MODEL | TRANSPORT | II SUPERNOVAE | STELLAR CORE COLLAPSE | ASTRONOMY & ASTROPHYSICS | methods : numerical | GENERAL-RELATIVISTIC HYDRODYNAMICS | DIFFUSION | CONSERVATION-LAWS | SCHEMES | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies

Journal Article

The Astrophysical Journal, ISSN 0004-637X, 01/2002, Volume 564, Issue 2 I, pp. 909 - 913

As a rapidly rotating neutron star spins down due to the loss of its angular momentum, its central density increases and the nuclear matter in its core...

Dense matter | Stars: interiors | Stars: evolution | Stars: neutron | Stars: rotation | stars : rotation | GENERAL RELATIVISTIC STARS | SPIN-DOWN | NUMERICAL-METHOD | stars : neutron | PULSAR | STATE | stars : interiors | POLYTROPES | KAON CONDENSATION | MODELS | dense matter | ASTRONOMY & ASTROPHYSICS | stars : evolution | QUARK MATTER | EQUATION

Dense matter | Stars: interiors | Stars: evolution | Stars: neutron | Stars: rotation | stars : rotation | GENERAL RELATIVISTIC STARS | SPIN-DOWN | NUMERICAL-METHOD | stars : neutron | PULSAR | STATE | stars : interiors | POLYTROPES | KAON CONDENSATION | MODELS | dense matter | ASTRONOMY & ASTROPHYSICS | stars : evolution | QUARK MATTER | EQUATION

Journal Article

Pramana, ISSN 0304-4289, 11/1991, Volume 37, Issue 5, pp. 395 - 403

We construct a formula for the energy released when a spherical shell of charged matter disperses in the presence of a dyon core. Reasons for such a...

gamma ray bursts | Dyon | 04.90 | general relativistic stability | GENERAL RELATIVISTIC STABILITY | PHYSICS | DYON | GAMMA-RAY BURSTS

gamma ray bursts | Dyon | 04.90 | general relativistic stability | GENERAL RELATIVISTIC STABILITY | PHYSICS | DYON | GAMMA-RAY BURSTS

Journal Article

Journal of Mathematical Physics, ISSN 0022-2488, 01/1973, Volume 14, Issue 1, pp. 104 - 118

The Schwarzchild manifold of general relativity theory is unsatisfactory as a particle model because the singularity at the origin makes it geodesically...

Journal Article

Astrophysical Journal, ISSN 0004-637X, 07/2016, Volume 825, Issue 1, pp. 6 - 6

We present self-consistent, axisymmetric core-collapse supernova simulations performed with the PROMETHEUS-VERTEX code for 18 pre-supernova models in the range...

Supernovae: general | Hydrodynamics | Instabilities | Neutrinos | MASSIVE STARS | neutrinos | GENERAL-RELATIVISTIC SIMULATIONS | ACCRETION-SHOCK | hydrodynamics | SPHERICAL-SYMMETRY | 3 DIMENSIONS | instabilities | supernovae: general | RADIATION-HYDRODYNAMICS | CIRCLE-DOT STAR | EQUATION-OF-STATE | ADVECTIVE-ACOUSTIC CYCLE | ASTRONOMY & ASTROPHYSICS | HYDRODYNAMICS SIMULATIONS | Axisymmetric | Accretion | Computer simulation | Supernovae | Progenitors (astrophysics) | Luminosity | Explosions | LUMINOSITY | AXIAL SYMMETRY | INSTABILITY | NEUTRONS | NEUTRON STARS | APPROXIMATIONS | RESOLUTION | HEATING | HYDRODYNAMICS | SIMULATION | SUPERNOVAE | LAYERS | DENSITY | EXPLOSIONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | EXPANSION | ADVECTION | INTERFACES | NEUTRINOS

Supernovae: general | Hydrodynamics | Instabilities | Neutrinos | MASSIVE STARS | neutrinos | GENERAL-RELATIVISTIC SIMULATIONS | ACCRETION-SHOCK | hydrodynamics | SPHERICAL-SYMMETRY | 3 DIMENSIONS | instabilities | supernovae: general | RADIATION-HYDRODYNAMICS | CIRCLE-DOT STAR | EQUATION-OF-STATE | ADVECTIVE-ACOUSTIC CYCLE | ASTRONOMY & ASTROPHYSICS | HYDRODYNAMICS SIMULATIONS | Axisymmetric | Accretion | Computer simulation | Supernovae | Progenitors (astrophysics) | Luminosity | Explosions | LUMINOSITY | AXIAL SYMMETRY | INSTABILITY | NEUTRONS | NEUTRON STARS | APPROXIMATIONS | RESOLUTION | HEATING | HYDRODYNAMICS | SIMULATION | SUPERNOVAE | LAYERS | DENSITY | EXPLOSIONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | EXPANSION | ADVECTION | INTERFACES | NEUTRINOS

Journal Article

Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN 1550-7998, 2003, Volume 68, Issue 10

In this paper, we develop an iterative scheme to enable the explicit calculation of an arbitrary post-Newtonian order for a relativistic body that reduces to...

GENERAL RELATIVISTIC STARS | NUMERICAL-METHODS | ROTATING POLYTROPES | MODELS | EQUILIBRIUM | PHYSICS, PARTICLES & FIELDS | Physics - General Relativity and Quantum Cosmology

GENERAL RELATIVISTIC STARS | NUMERICAL-METHODS | ROTATING POLYTROPES | MODELS | EQUILIBRIUM | PHYSICS, PARTICLES & FIELDS | Physics - General Relativity and Quantum Cosmology

Journal Article

Physical Review D, ISSN 0556-2821, 11/2001, Volume 64, Issue 10, p. 26

Gravitational waves from binary neutron stars in quasiequilibrium circular orbits are computed using an approximate method which we propose in this paper. In...

ORDER | MODELS | ASTRONOMY & ASTROPHYSICS | EQUATIONS | SYSTEMS | FORMALISM | QUASI-EQUILIBRIUM CONFIGURATIONS | BLACK-HOLE | COMPACT BINARIES | GENERAL-RELATIVISTIC SIMULATION | RADIATION | PHYSICS, PARTICLES & FIELDS | Physics - General Relativity and Quantum Cosmology

ORDER | MODELS | ASTRONOMY & ASTROPHYSICS | EQUATIONS | SYSTEMS | FORMALISM | QUASI-EQUILIBRIUM CONFIGURATIONS | BLACK-HOLE | COMPACT BINARIES | GENERAL-RELATIVISTIC SIMULATION | RADIATION | PHYSICS, PARTICLES & FIELDS | Physics - General Relativity and Quantum Cosmology

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2009, Volume 400, Issue 1, pp. 100 - 122

We employ cosmological hydrodynamical simulations to study the growth of massive black holes (BHs) at high redshifts subject to BH merger recoils from...

black hole physics | methods: numerical | cosmology: theory | Methods: Numerical | Cosmology: Theory | Black hole physics | GRAVITATIONAL RECOIL | HIGH-REDSHIFT QUASARS | Z-GREATER-THAN-5.7 QUASARS | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | ADDITIONAL QUASARS | SUPERMASSIVE BLACK-HOLES | ACTIVE GALACTIC NUCLEI | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | GALAXY FORMATION | PARTICLE HYDRODYNAMICS SIMULATIONS | Growth | Analysis | Astronomy | Quasars | Astrophysics | Simulation | Black holes

black hole physics | methods: numerical | cosmology: theory | Methods: Numerical | Cosmology: Theory | Black hole physics | GRAVITATIONAL RECOIL | HIGH-REDSHIFT QUASARS | Z-GREATER-THAN-5.7 QUASARS | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | ADDITIONAL QUASARS | SUPERMASSIVE BLACK-HOLES | ACTIVE GALACTIC NUCLEI | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | GALAXY FORMATION | PARTICLE HYDRODYNAMICS SIMULATIONS | Growth | Analysis | Astronomy | Quasars | Astrophysics | Simulation | Black holes

Journal Article

Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 01/2011, Volume 410, Issue 1, pp. L37 - L41

ABSTRACT In a realistic model of magneto‐elastic oscillations in magnetars, we find that crustal shear oscillations, often invoked as an explanation of...

stars: flare | MHD | stars: magnetars | stars: magnetic field | stars: oscillations | stars: neutron | Stars: magnetic field | Stars: flare | Stars: neutron | Stars: magnetars | Stars: oscillations | APPROXIMATION | QPOS | NUCLEON MATTER | GIANT-FLARE | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | X-RAY OSCILLATIONS | EQUATION-OF-STATE | TORSIONAL OSCILLATIONS | ASTRONOMY & ASTROPHYSICS | MAGNETIZED NEUTRON-STARS | QUASI-PERIODIC OSCILLATIONS | Earth | Crust | Magnetic fields | Analysis

stars: flare | MHD | stars: magnetars | stars: magnetic field | stars: oscillations | stars: neutron | Stars: magnetic field | Stars: flare | Stars: neutron | Stars: magnetars | Stars: oscillations | APPROXIMATION | QPOS | NUCLEON MATTER | GIANT-FLARE | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | X-RAY OSCILLATIONS | EQUATION-OF-STATE | TORSIONAL OSCILLATIONS | ASTRONOMY & ASTROPHYSICS | MAGNETIZED NEUTRON-STARS | QUASI-PERIODIC OSCILLATIONS | Earth | Crust | Magnetic fields | Analysis

Journal Article

Physical Review D, ISSN 0556-2821, 2002, Volume 65, Issue 4, p. 16

We study the equilibrium sequences of close binary systems in circular orbits and composed of different mass stars with a polytropic equation of state in...

TESTS | MODELS | POLYTROPIC STARS | COALESCENCE | ASTRONOMY & ASTROPHYSICS | NEUTRON-STARS | HYDRODYNAMICS | PULSAR | QUASI-EQUILIBRIUM | GENERAL-RELATIVISTIC SIMULATION | CONFIGURATIONS | PHYSICS, PARTICLES & FIELDS

TESTS | MODELS | POLYTROPIC STARS | COALESCENCE | ASTRONOMY & ASTROPHYSICS | NEUTRON-STARS | HYDRODYNAMICS | PULSAR | QUASI-EQUILIBRIUM | GENERAL-RELATIVISTIC SIMULATION | CONFIGURATIONS | PHYSICS, PARTICLES & FIELDS

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2018, Volume 478, Issue 2, pp. 1875 - 1883

We study model images and polarization maps of Sagittarius A* at 230 GHz. We post-process general relativistic magnetohydrodynamic simulations and perform a...

Polarization | Accretion | Galaxy: centre | Accretion discs | Black hole physics | MHD | Radiative transfer | ADVECTION-DOMINATED ACCRETION | GRMHD SIMULATIONS | accretion discs | radiative transfer | MHD-polarization | EVENT-HORIZON | LINEAR-POLARIZATION | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | MAGNETIC-FIELD STRUCTURE | ELECTRON THERMODYNAMICS | SGR-A-ASTERISK | accretion | black hole physics | ASTRONOMY & ASTROPHYSICS | GALACTIC-CENTER | EMISSION | Physics - High Energy Astrophysical Phenomena

Polarization | Accretion | Galaxy: centre | Accretion discs | Black hole physics | MHD | Radiative transfer | ADVECTION-DOMINATED ACCRETION | GRMHD SIMULATIONS | accretion discs | radiative transfer | MHD-polarization | EVENT-HORIZON | LINEAR-POLARIZATION | GENERAL-RELATIVISTIC MAGNETOHYDRODYNAMICS | MAGNETIC-FIELD STRUCTURE | ELECTRON THERMODYNAMICS | SGR-A-ASTERISK | accretion | black hole physics | ASTRONOMY & ASTROPHYSICS | GALACTIC-CENTER | EMISSION | Physics - High Energy Astrophysical Phenomena

Journal Article