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Covariant and 3 + 1 Equations for Dynamo-Chiral General Relativistic Magnetohydrodynamics

Monthly notices of the Royal Astronomical Society, 2018-09

2018

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A study of vorticity formation in high energy nuclear collisions

The European physical journal. C, Particles and fields, 2015-09, Vol.75 (9), p.1-14, Article 406

2015

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Systematic construction of upwind constrained transport schemes for MHD

Journal of computational physics, 2021-01, Vol.424, p.109748, Article 109748

2021

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A fully covariant mean-field dynamo closure for numerical 3 + 1 resistive GRMHD

Monthly notices of the Royal Astronomical Society, 2013-01, Vol.428 (1), p.71-85

2013

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General relativistic models for rotating magnetized neutron stars in conformally flat space–time

Monthly notices of the Royal Astronomical Society, 2017-09, Vol.470 (2), p.2469-2493

2017

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Fast Magnetic Reconnection: Secondary Tearing Instability and Role of the Hall Term

The Astrophysical journal, 2019-11, Vol.885 (1), p.56

2019

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Relativistic viscous hydrodynamics for heavy-ion collisions with ECHO-QGP

The European physical journal. C, Particles and fields, 2013-08, Vol.73 (8), p.1-26, Article 2524

2013

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Fast reconnection in relativistic plasmas: the magnetohydrodynamics tearing instability revisited

Monthly notices of the Royal Astronomical Society, 2016-08, Vol.460 (4), p.3753-3765

2016

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Papaloizou–Pringle instability suppression by the magnetorotational instability in relativistic accretion discs

Monthly notices of the Royal Astronomical Society, 2018-03, Vol.475 (1), p.108-120

2018

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RESISTIVE MAGNETOHYDRODYNAMICS SIMULATIONS OF THE IDEAL TEARING MODE

The Astrophysical journal, 2015-06, Vol.806 (1), p.1-8

2015

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The role of currents distribution in general relativistic equilibria of magnetized neutron stars

Monthly notices of the Royal Astronomical Society, 2015-03, Vol.447 (4), p.3278-3278

2015

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A constrained transport method for the solution of the resistive relativistic MHD equations

Monthly notices of the Royal Astronomical Society, 2019-07, Vol.486 (3), p.4252-4274

2019

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Modeling the effect of small-scale magnetic turbulence on the X-ray properties of Pulsar Wind Nebulae

Monthly notices of the Royal Astronomical Society, 2017-10, Vol.470 (4), p.4066-4074

2017

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Multi-D magnetohydrodynamic modelling of pulsar wind nebulae: recent progress and open questions

Journal of plasma physics, 2016-12, Vol.82 (6), p.141102; 112102; 056501; 012016; 105004; 235002-141102; 112102; 056501; 012016; 105004; 235002, Article 635820601

2016

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General relativistic radiation hydrodynamics of accretion flows - I. Bondi-Hoyle accretion

Monthly notices of the Royal Astronomical Society, 2011-11, Vol.417 (4), p.2899-2915

2011

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Constraints on particle acceleration sites in the Crab nebula from relativistic magnetohydrodynamic simulations

Monthly notices of the Royal Astronomical Society, 2015-05, Vol.449 (3), p.3149-3149

2015

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On the divergence-free condition in Godunov-type schemes for ideal magnetohydrodynamics: the upwind constrained transport method

Journal of computational physics, 2004-03, Vol.195 (1), p.17-48

2004

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Magnetized relativistic jets and long-duration GRBs from magnetar spin-down during core-collapse supernovae

Monthly notices of the Royal Astronomical Society, 2009-07, Vol.396 (4), p.2038-2050

2009

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Non-thermal emission from relativistic MHD simulations of pulsar wind nebulae: from synchrotron to inverse Compton

Astronomy and astrophysics (Berlin), 2008-07, Vol.485 (2), p.337-349

2008

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Fast magnetic reconnection: The ideal tearing instability in classic, Hall, and relativistic plasmas

Journal of physics. Conference series, 2018-05, Vol.1031 (1), p.12020

2018

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Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Monthly notices of the Royal Astronomical Society, 2014-04, Vol.439 (4), p.3541-3563

2014

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Simulated synchrotron emission from pulsar wind nebulae

Astronomy and astrophysics (Berlin), 2006-07, Vol.453 (2), p.621-633

2006

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The ideal tearing mode: theory and resistive MHD simulations

Journal of physics. Conference series, 2016-05, Vol.719 (1), p.12016

2016

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Creation and dissipation of magnetic fields in non-ideal GRMHD simulations

Journal of physics. Conference series, 2020-09, Vol.1623 (1), p.12004

2020

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Relativistic MHD modeling of magnetized neutron stars, pulsar winds, and their nebulae

Plasma physics and controlled fusion, 2018-01, Vol.60 (1), p.14027

2018

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Covariant and 3 + 1 Equations for Dynamo-Chiral General Relativistic Magnetohydrodynamics

A study of vorticity formation in high energy nuclear collisions

Systematic construction of upwind constrained transport schemes for MHD

A fully covariant mean-field dynamo closure for numerical 3 + 1 resistive GRMHD

General relativistic models for rotating magnetized neutron stars in conformally flat space–time

Fast Magnetic Reconnection: Secondary Tearing Instability and Role of the Hall Term

Relativistic viscous hydrodynamics for heavy-ion collisions with ECHO-QGP

Fast reconnection in relativistic plasmas: the magnetohydrodynamics tearing instability revisited

Papaloizou–Pringle instability suppression by the magnetorotational instability in relativistic accretion discs

RESISTIVE MAGNETOHYDRODYNAMICS SIMULATIONS OF THE IDEAL TEARING MODE

The role of currents distribution in general relativistic equilibria of magnetized neutron stars

A constrained transport method for the solution of the resistive relativistic MHD equations

Modeling the effect of small-scale magnetic turbulence on the X-ray properties of Pulsar Wind Nebulae

Multi-D magnetohydrodynamic modelling of pulsar wind nebulae: recent progress and open questions

General relativistic radiation hydrodynamics of accretion flows - I. Bondi-Hoyle accretion

Constraints on particle acceleration sites in the Crab nebula from relativistic magnetohydrodynamic simulations

On the divergence-free condition in Godunov-type schemes for ideal magnetohydrodynamics: the upwind constrained transport method

Magnetized relativistic jets and long-duration GRBs from magnetar spin-down during core-collapse supernovae

Non-thermal emission from relativistic MHD simulations of pulsar wind nebulae: from synchrotron to inverse Compton

Fast magnetic reconnection: The ideal tearing instability in classic, Hall, and relativistic plasmas

Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Simulated synchrotron emission from pulsar wind nebulae

The ideal tearing mode: theory and resistive MHD simulations

Creation and dissipation of magnetic fields in non-ideal GRMHD simulations

Relativistic MHD modeling of magnetized neutron stars, pulsar winds, and their nebulae

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