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Effect of plasma composition on accretion on to black holes
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Effect of plasma composition on accretion on to black holes
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Matter makes a transition from non-relativistic to relativistic regime, as it falls onto a black hole. We employ a relativistic equation of state, abbreviated as RC, to study multi-species fluid flow around black holes. We show that pair-plasma fluid around a black hole is thermally not relativistic. In order to make it relativistic, a finite baryon loading is necessary. As a consequence of this, pair-plasma flow do not suffer centrifugal pressure driven shock in accretion. However, fluid with finite baryon content may undergo shock transition.
Forward citations
Cited by 2 Pith papers
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Outflow Behavior from the Transonic Advective Disks: A Hydrodynamical Simulation Study
In 2D hydro simulations, colder transonic accretion disks launch faster, lower-density, more energetic bipolar outflows than hotter disks, and outflow strength rises with viscosity.
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Outflow Behavior from the Transonic Advective Disks: A Hydrodynamical Simulation Study
In viscous hydro simulations, colder transonic advective disks drive faster, higher kinetic-energy and momentum bipolar outflows than hotter disks, and outflow strength increases with viscosity.
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