Velocity Distribution of a Homogeneously Cooling Granular Gas.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
22 May 2020
Historique:
revised: 27 11 2019
received: 26 07 2019
accepted: 23 04 2020
entrez: 6 6 2020
pubmed: 6 6 2020
medline: 6 6 2020
Statut: ppublish

Résumé

In contrast to molecular gases, granular gases are characterized by inelastic collisions and require therefore permanent driving to maintain a constant kinetic energy. The kinetic theory of granular gases describes how the average velocity of the particles decreases after the driving is shut off. Moreover, it predicts that the rescaled particle velocity distribution will approach a stationary state with overpopulated high-velocity tails as compared to the Maxwell-Boltzmann distribution. While this fundamental theoretical result was reproduced by numerical simulations, an experimental confirmation is still missing. Using a microgravity experiment that allows the spatially homogeneous excitation of spheres via magnetic fields, we confirm the theoretically predicted exponential decay of the tails of the velocity distribution.

Identifiants

pubmed: 32501095
doi: 10.1103/PhysRevLett.124.208007
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

208007

Auteurs

Peidong Yu (P)

Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt (DLR), 51170 Cologne, Germany.
Institut für Theoretische Physik, Universität zu Köln, 50937 Cologne, Germany.

Matthias Schröter (M)

Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt (DLR), 51170 Cologne, Germany.

Matthias Sperl (M)

Institut für Materialphysik im Weltraum, Deutsches Zentrum für Luft- und Raumfahrt (DLR), 51170 Cologne, Germany.
Institut für Theoretische Physik, Universität zu Köln, 50937 Cologne, Germany.

Classifications MeSH