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  5. Intensity landscapes in elliptical and oval billiards with a circular absorbing region
 
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Intensity landscapes in elliptical and oval billiards with a circular absorbing region
File(s)
2411.08694v2.pdf (9.68 MB)
Accepted version
Author(s)
Holmes, Katherine
Hall, Joseph
Graefe, Eva-Maria
Type
Journal Article
Abstract
Billiard models of single particles moving freely in two-dimensional regions enclosed by hard walls, have long provided ideal toy models for the investigation of dynamical systems and chaos. Recently, billiards with (semi-)permeable walls and internal holes have been used to study open systems. Here we introduce a billiard model containing an internal region with partial absorption. The absorption does not change the trajectories, but instead reduces an intensity variable associated with each trajectory. The value of the intensity can be tracked as a function of the initial configuration and the number of reflections from the wall and depicted in intensity landscapes over the Poincar'e phase space. This is similar in spirit to escape time diagrams that are often considered in dynamical systems with holes. We analyse the resulting intensity landscapes for three different geometries; a circular, elliptic, and oval billiard, respectively, all with a centrally placed circular absorbing region. The intensity landscapes feature increasingly more complex structures, organised around the sets of points in phase space that intersect the absorbing region in a given iteration, which we study in some detail. On top of these, the intensity landscapes are enriched by effects arising from multiple absorption events for a given trajectory.
Date Issued
2024-11-13
Date Acceptance
2025-06-27
Citation
Physical Review E: Statistical, Nonlinear, and Soft Matter Physics
URI
https://hdl.handle.net/10044/1/122135
DOI
https://www.dx.doi.org/10.1103/9bv6-4npn
ISSN
1539-3755
Publisher
American Physical Society
Journal / Book Title
Physical Review E: Statistical, Nonlinear, and Soft Matter Physics
Copyright Statement
Copyright This paper is embargoed until publication. Once published the author’s accepted manuscript will be made available under a CC-BY License in accordance with Imperial’s Research Publications Open Access policy (www.imperial.ac.uk/oa-policy).
License URL
https://creativecommons.org/licenses/by/4.0/
Identifier
http://arxiv.org/abs/2411.08694v2
Subjects
nlin.CD
nlin.CD
physics.class-ph
Publication Status
Accepted
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