Hung Yi Chou National Yang Ming University Taipei Nymu General relativistic magnetohydrodynamic (grmhd) flows along magnetic fields threading a black hole can be divided into inflow and outflow parts, according to the result of the competition between the black hole gravity and magneto centrifugal forces along the field line. The m87 jet is extensively examined by utilizing general relativistic magnetohydrodynamic (grmhd) simulations, as well as the steady axisymmetric force free electrodynamic (ffe) solution.
Grmhd Hung Yi Pu We have confirmed that, at large distance, the grmhd jet solutions are in good agreement with the previously known trans fast special relativistic magnetohydrodynamic (srmhd) jet properties, as expected. Odyssey is a public, gpu based general relativistic radiative transfer (grrt) code for computing images and or spectra in kerr metric, which described the spacetime aroung a rotating black hole. Abstract general relativistic magnetohydrodynamic (grmhd) flows along magnetic fields threading a black hole can be divided into inflow and outflow parts, according to the result of the competition between the black hole gravity and magneto centrifugal forces along the field line. Title: the first images of a black hole and general relativistic magnetohydrodynamical (grmhd) accretion jet : achievements and challenges speaker: prof. hung yi pu.
Grmhd Hung Yi Pu Abstract general relativistic magnetohydrodynamic (grmhd) flows along magnetic fields threading a black hole can be divided into inflow and outflow parts, according to the result of the competition between the black hole gravity and magneto centrifugal forces along the field line. Title: the first images of a black hole and general relativistic magnetohydrodynamical (grmhd) accretion jet : achievements and challenges speaker: prof. hung yi pu. In this paper, we focus on the pfd grmhd flow in the funnel region, including both the inflow and outflow parts. for comparison, let us quickly consider the case when the grmhd flow becomes fluid dominated. As an intriguing alternative, we present an semi analytical approach to model black hole grmhd flow along the many ordered and large scale magnetic field lines distributed near the black hole rotational axis. General relativistic magnetohydrodynamic (grmhd) flows along magnetic fields threading a black hole can be divided into inflow and outflow parts, according to the result of the competition between the black hole gravity and magneto centrifugal forces along the field line. Dive into the research topics where hung yi pu is active. these topic labels come from the works of this person. together they form a unique fingerprint.
Pt Hung Yi Indonesia In this paper, we focus on the pfd grmhd flow in the funnel region, including both the inflow and outflow parts. for comparison, let us quickly consider the case when the grmhd flow becomes fluid dominated. As an intriguing alternative, we present an semi analytical approach to model black hole grmhd flow along the many ordered and large scale magnetic field lines distributed near the black hole rotational axis. General relativistic magnetohydrodynamic (grmhd) flows along magnetic fields threading a black hole can be divided into inflow and outflow parts, according to the result of the competition between the black hole gravity and magneto centrifugal forces along the field line. Dive into the research topics where hung yi pu is active. these topic labels come from the works of this person. together they form a unique fingerprint.
Pt Hung Yi Indonesia General relativistic magnetohydrodynamic (grmhd) flows along magnetic fields threading a black hole can be divided into inflow and outflow parts, according to the result of the competition between the black hole gravity and magneto centrifugal forces along the field line. Dive into the research topics where hung yi pu is active. these topic labels come from the works of this person. together they form a unique fingerprint.
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