Effect of the toroidal magnetic field on the runaway instability of relativistic tori

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F13%3A00393329" target="_blank" >RIV/67985815:_____/13:00393329 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201321500" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201321500</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201321500" target="_blank" >10.1051/0004-6361/201321500</a>

Result language
angličtina
Original language name
Effect of the toroidal magnetic field on the runaway instability of relativistic tori
Original language description
Runaway instability operates in fluid tori around black holes. It affects systems close to the critical (cusp overflowing) configuration. The runaway effect depends on the radial profile l(R) of the angular momentum distribution of the fluid, on the dimension-less spin a of the central black hole (|a| 1), and other factors, such as self-gravity.
Czech name
—
Czech description
—

Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
—

Project
<a href="/en/project/GC13-00070J" target="_blank" >GC13-00070J: Accretion process in strong gravity of Galactic Center</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Similar results(10)