activity
20002011
most citedEquation of State in Numerical Relativistic Hydrodynamics

95 citations · 241 across the 14 of their papers we have counts for

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9 papers · 1 filter

astro-ph200833 cited

Computation of mass loss from viscous accretion disc in presence of cooling

Santabrata Das, Indranil Chattopadhyay

Rotating accretion flow may undergo centrifugal pressure mediated shock transition even in presence of various dissipative processes, such as viscosity and cooling mechanism. The e…

astro-ph200642 cited

Massloss from viscous advective disc

Indranil Chattopadhyay, Santabrata Das

Rotating transonic flows are long known to admit standing or oscillating shocks and that the excess thermal energy in the post shock flow drives a part of the infalling matter as b…

astro-ph200695 cited

Equation of State in Numerical Relativistic Hydrodynamics

Dongsu Ryu, Indranil Chattopadhyay, Eunwoo Choi

Relativistic temperature of gas raises the issue of the equation of state (EoS) in relativistic hydrodynamics. We study the EoS for numerical relativistic hydrodynamics, and propos…

astro-ph2004

Radiatively Driven Jets around Black Holes

Indranil Chattopadhyay, Sandip K. Chakrabarti

The hot, puffed up, post-shock region of an advective disc is the source of high energy photons and also the jets and outflows. We study the relativistic equations of motion of jet…

astro-ph2004

Radiatively driven rotating pair-plasma jets from two component accretion flows

Indranil Chattopadhyay

Centrifugal pressure of matter spiralling onto black holes, have long been known to produce standing or oscillating shocks. The post-shock disc puffs up in the form of a torus, whi…

astro-ph2004

Computation of outflow rates from accretion disks around black holes

Santabrata Das, Indranil Chattopadhyay, A. Nandi +1

We self-consistently estimate the outflow rate from the accretion rates of an accretion disk around a black hole in which both the Keplerian and the sub-Keplerian matter flows simu…