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Showing 1 to 11 of 11 for “"GRMHD"”.

  1. GRMHD simulations and analysis of polarized emission from black hole accretion systems

    Submission original under an indefinite embargo labeled 'Open Access'. The submission was exported from vireo on 2023-04-12 without embargo terms

    uiuc Repository record for GRMHD simulations and analysis of polarized emission from black hole accretion systems (opens in a new tab)

  2. Black Hole Astrophysics : Magnetohydrodynamics on the Kerr Geometry

    … of General Relativistic Magnetohydrodynamics (GRMHD). The behavior of non-radiative accretion flows and outflows on the Kerr space-time is analyzed. Basic equations of conservative GRMHD and aspects of numerical schemes are presented. Relativistic codes and astrophysical simulations validate …

    heid-diss Repository record for Black Hole Astrophysics : Magnetohydrodynamics on the Kerr Geometry (opens in a new tab)

  3. Black Hole Accretion Systems

    … (MHD), and general relativistic MHD (GRMHD) equations of motion, which are integrated numerically. I wrote the VHD and nonrelativistic MHD numerical codes, and coauthored the GRMHD code (Gammie et al., 2003). I first studied VHD accretion disk models, such as those studied by …

    uiuc Repository record for Black Hole Accretion Systems (opens in a new tab)

  4. On Stability and Evolution of Solutions in General Relativity

    … of general relativistic magnetohydrodynamics (GRMHD). We compute the eigenvalues and eigenvectors of GRMHD and establish degeneracy conditions. Finally, we consider the initial value problem for axisymmetric GRMHD. We formulate the general Einstein and MHD equations under the assumption of a …

    byu Repository record for On Stability and Evolution of Solutions in General Relativity (opens in a new tab)

  5. Self-consistent dynamical and radiative models of low-luminosity active galactic nuclei

    … on general relativistic magnetohydrodynamic (GRMHD) simulations. Before proceeding, we noted, as others have before us, that global disk simulations model transient accretion flows in the sense that the numerical values for, e.g., the density decay with time as the initial disk drains into the …

    uiuc Repository record for Self-consistent dynamical and radiative models of low-luminosity active galactic nuclei (opens in a new tab)

  6. General-relativistic magnetohydrodynamics simulations of black hole accretion disks: dynamics and radiative properties

    … general relativistic magnetohydrodynamics (GRMHD), to construct a realistic dynamical and radiation model of accretion disks. Our simulations are for black holes in low luminous regimes that probably possesses a hot and thick accretion disk. Flows in this regime are called radiatively …

    uiuc Repository record for General-relativistic magnetohydrodynamics simulations of black hole accretion disks: dynamics and radiative properties (opens in a new tab)

  7. General relativistic radiation magnetohydrodynamics, with applications to black hole accretion disks

    … for general relativistic magnetohydrodynamics (GRMHD). However, even the local details of MRI-driven turbulence simulations are still not completely understood. Along the way, this work considers a central issue with modeling the MRI: whether the resulting stress is independent of the numerics …

    uiuc Repository record for General relativistic radiation magnetohydrodynamics, with applications to black hole accretion disks (opens in a new tab)

  8. General relativistic magnetohydrodynamic simulations of binary neutron star mergers

    … fully general relativistic magnetohydrodynamic (GRMHD) binary neutron star merger (BNS) simulations, conducted by using the numerical code "Whisky" under various conditions, such as, different Equation of State (EOS) for neutron matter (APR4, Ideal fluid and H4 EOSs), masses (with equal/unequal …

    trento Repository record for General relativistic magnetohydrodynamic simulations of binary neutron star mergers (opens in a new tab)

  9. Relativistic Radiative Hydrodynamics Calculation of Accretion Flow into Supermassive Black Hole

    … with general relativistic magnetohydrodynamic (GRMHD) simulation of accretion flow simulation. We are able to use the models to constrain observational parameters of Sgr A*. We also compute the synchrotron emissivity and absorptivity from first principles, in order to verify improved approximate …

    uiuc Repository record for Relativistic Radiative Hydrodynamics Calculation of Accretion Flow into Supermassive Black Hole (opens in a new tab)

  10. Dissipative heating and nonthermal distributions in black hole accretion flaring events

    … using general relativistic magnetohydrodynamics (GRMHD) and radiative transfer calculations with a nonthermal kappa distribution function (which effectively adds a power-law tail to the thermal distribution) for electrons accelerated by resistive heating in reconnecting current sheets. This …

    uiuc Repository record for Dissipative heating and nonthermal distributions in black hole accretion flaring events (opens in a new tab)

  11. Statistical methods for assisting computational models for the event horizon telescope

    Submission original under an indefinite embargo labeled 'Open Access'. The submission was exported from vireo on 2025-03-28 without embargo terms

    uiuc Repository record for Statistical methods for assisting computational models for the event horizon telescope (opens in a new tab)