CREMASCHINI, Claudio and Zdeněk STUCHLÍK. KINETIC THEORY FOR GRAVITATING SYSTEMS OF COLLISIONLESS NEUTRAL MATTER. International Journal of Modern Physics D. SG - Singapurská republika, 2013, vol. 22, No 13, 24 pp. ISSN 0218-2718. Available from: https://dx.doi.org/10.1142/S0218271813500776.
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Basic information
Original name KINETIC THEORY FOR GRAVITATING SYSTEMS OF COLLISIONLESS NEUTRAL MATTER
Authors CREMASCHINI, Claudio and Zdeněk STUCHLÍK.
Edition International Journal of Modern Physics D, SG - Singapurská republika, 2013, 0218-2718.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW www
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1142/S0218271813500776
UT WoS 000326718400008
Keywords in English Kinetic theory; Equilibrium distribution function; Collisionless neutral matter; Temperature anisotropy; Dark matter
Tags UF
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 19/1/2021 13:30.
Abstract
The study of the statistical properties of collisionless systems formed by neutral particles subject to gravitational field represents an intriguing theoretical issue. In astrophysics, it directly relates to the description of collisionless gravitating dark matter (DM) halos. Structures of this type are expected to be characterized by intrinsically non-Maxwellian kinetic distribution functions (KDFs) and to exhibit temperature anisotropy, i.e. an anisotropy in the directional particle velocity dispersions. In this paper, a theoretical analysis of the issue is proposed, based on the kinetic theory developed in the framework of the Vlasov-Poisson description for nonrelativistic DM systems at equilibrium. By implementing the method of invariants, explicitsolutions for the equilibrium KDFs are constructed and expressed through generalized Gaussian distributions. A perturbative theory is developed which allows them to be cast in terms of Chapman-Enskog series representations and to evaluat
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