Open AccessRadiatively driven plasma jets around compact objects
Author(s) -
Chattopadhyay Indranil,
Chakrabarti Sandip K.
Publication year - 2002
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2002.05424.x
Subject(s) - physics , drag , plasma , photon , radiation , shock (circulatory) , radiation pressure , electron , flow velocity , astrophysics , terminal velocity , flow (mathematics) , mechanics , optics , nuclear physics , medicine
Matter accreting on to black holes may develop shocks due to the centrifugal barrier. Some of the inflowing matter in the post‐shock flow is deflected along the axis in the form of jets. Post‐shock flow which behaves like a Compton cloud has ‘hot’ electrons emitting high‐energy photons. We study the effect of these ‘hot’ photons on the outflowing matter. Radiation from this region could accelerate the outflowing matter, but radiation pressure should also slow it down. We show that the radiation drag restricts the flow from attaining a very high velocity. We introduce the concept of an ‘equilibrium velocity’ ( v eq ∼0.5 c ) , which sets the upper limit of the terminal velocity achieved by a cold plasma due to radiation deposition force in the absence of gravity. If the injection energy is E in , then we find that the terminal velocity v ∞ satisfies a relation .