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Impact of high-energy tails on granular gas properties

  • The velocity distribution function of granular gases in the homogeneous cooling state as well as some heated granular gases decays for large velocities as f proportional to exp(-const x nu). That is, its high-energy tail is overpopulated as compared with the Maxwell distribution. At the present time, there is no theory to describe the influence of the tail on the kinetic characteristics of granular gases. We develop an approach to quantify the overpopulated tail and analyze its impact on granular gas properties, in particular on the cooling coefficient. We observe and explain anomalously slow relaxation of the velocity distribution function to its steady state.

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Metadaten
Author details:Thorsten Poeschel, Nikolai V. BrilliantovORCiDGND, Arno FormellaORCiD
DOI:https://doi.org/10.1103/PhysRevE.74.041302
ISSN:1539-3755
ISSN:1550-2376
Pubmed ID:https://pubmed.ncbi.nlm.nih.gov/17155050
Title of parent work (English):Physical review : E, Statistical, nonlinear and soft matter physics
Publisher:The American Physical Society
Place of publishing:College Park
Publication type:Article
Language:English
Date of first publication:2006/10/19
Publication year:2006
Release date:2020/05/12
Volume:74
Issue:4
Number of pages:5
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
DDC classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Peer review:Referiert
Publishing method:Open Access
Open Access / Green Open-Access
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