arXiv · gr-qc/0301095
Self-interacting gas in a gravitational wave field
Abstract
We investigate a relativistic self-interacting gas in the field of an external {\it pp} gravitational wave. Based on symmetry considerations we ask for those forces which are able to compensate the imprint of the gravitational wave on the macroscopic 4-acceleration of the gaseous fluid. We establish an exactly solvable toy model according to which the stationary states which characterize such a situation have negative entropy production and are accompanied by instabilities of the microscopic particle motion. These features are similar to those which one encounters in phenomena of self-organization in many-particle systems.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Alexander B. Balakin, Winfried Zimdahl. 2003-01-23. Self-interacting gas in a gravitational wave field. https://doi.org/10.1023/a%3A1022966118594
Cite the original work for its findings. Save a collection to share your selection of sources.