Transonic structure of slowly rotating accretion flows with shocks around black holes

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00484766" target="_blank" >RIV/67985815:_____/17:00484766 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S1743921316012953" target="_blank" >http://dx.doi.org/10.1017/S1743921316012953</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S1743921316012953" target="_blank" >10.1017/S1743921316012953</a>

Result language
angličtina
Original language name
Transonic structure of slowly rotating accretion flows with shocks around black holes
Original language description
We present recent results of the studies of low angular momentum accretion of matter onto Schwarzschild black hole using fully relativistic numerical simulations. We compare the resulting 2D structure of transonic flows with results of 1D pseudo-Newtonian computations of non-magnetized flow. The research has observable consequences on black holes on the whole mass scale, in particular it is related to the time-scale and shape of luminosity flares in Sgr A* or to the evolution of QPO frequency during outbursts of microquasars.
Czech name
—
Czech description
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Project
<a href="/en/project/GB14-37086G" target="_blank" >GB14-37086G: Albert Einstein Center for Gravitation and Astrophysics</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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