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Preprints of the Keldysh Institute of Applied Mathematics, 2021, 004, 40 pp.
DOI: https://doi.org/10.20948/prepr-2021-4
(Mi ipmp2922)
 

Jeans instability of the protoplanetary circumstellar disk taking into account the magnetic field and radiation in the nonextensive Tsallis kinetics

A. V. Kolesnichenko
References:
Abstract: Within the framework of the Tsallis non-extensive statistics, a derivation of the Jeans gravitational instability criteria is given for a self-gravitating protoplanetary disk, the substance of which consists of a mixture of a conducting ideal $q$-gas and modified radiation of a photon gas. The instability criteria are derived from the corresponding dispersion relations written for both neutral disk matter and magnetized plasma with modified blackbody radiation. The thermodynamics of a photon gas is constructed based on the nonextensive quantum entropy Tsallis, which depends on the deformation parameter. It is shown that blackbody radiation can stabilize the state of a nonextensive medium for a purely gaseous disk, and for an electrically conducting disk, the Jeans instability criterion is modified by a magnetic field and radiation pressure only in the transverse regime of propagation of the disturbance wave.
Keywords: Jeans criteria, protoplanetary disk, blackbody radiation, nonextensive Tsallis kinetics.
Funding agency Grant number
Ministry of Science and Higher Education of the Russian Federation 075-15-2020-780
Document Type: Preprint
Language: Russian
Citation: A. V. Kolesnichenko, “Jeans instability of the protoplanetary circumstellar disk taking into account the magnetic field and radiation in the nonextensive Tsallis kinetics”, Keldysh Institute preprints, 2021, 004, 40 pp.
Citation in format AMSBIB
\Bibitem{Kol21}
\by A.~V.~Kolesnichenko
\paper Jeans instability of the protoplanetary circumstellar disk taking into account the magnetic field and radiation in the nonextensive Tsallis kinetics
\jour Keldysh Institute preprints
\yr 2021
\papernumber 004
\totalpages 40
\mathnet{http://mi.mathnet.ru/ipmp2922}
\crossref{https://doi.org/10.20948/prepr-2021-4}
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