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Spacetime symmetries and geometric diffusion
KTH, School of Industrial Engineering and Management (ITM), Energy Technology, Applied Thermodynamics and Refrigeration.ORCID iD: 0000-0002-0121-8162
Univ Granada, Fac Educ Econ & Tecnol Ceuta, Dept Algebra, Cortadura Valle S-N, Ceuta 51001, Spain.;Univ Granada, Inst Carlos I Fis Teor & Computac, E-18071 Granada, Spain.;Univ Granada, Nanoparticles Trapping Lab, Granada, Spain..
Univ Pontificia Comillas, Dept Matemat Aplicada, Grp Dinam No Lineal, C Alberto Aguilera 25, Madrid 28015, Spain.;Univ Pontificia Comillas, Inst Invest Tecnol IIT, Madrid 28015, Spain..
Univ Pontificia Comillas, Inst Invest Tecnol IIT, Madrid 28015, Spain..ORCID iD: 0000-0002-6524-4298
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2024 (English)In: Journal of Physics A: Mathematical and Theoretical, ISSN 1751-8113, E-ISSN 1751-8121, Vol. 57, no 28, article id 285204Article in journal (Refereed) Published
Abstract [en]

We examine relativistic diffusion through the frame and observer bundles associated with a Lorentzian manifold (M, g). Our focus is on spacetimes with a non-trivial isometry group, and we detail the conditions required to find symmetric solutions of the relativistic diffusion equation. Additionally, we analyze the conservation laws associated with the presence of Killing vector fields on (M, g) and their implications for the expressions of the geodesic spray and the vertical Laplacian on both the frame and the observer bundles. Finally, we present several relevant examples of symmetric spacetimes.

Place, publisher, year, edition, pages
IOP Publishing , 2024. Vol. 57, no 28, article id 285204
Keywords [en]
diffusion Lorentzian manifolds, covariant Fokker-Planck equation, spacetime symmetries
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-350521DOI: 10.1088/1751-8121/ad5a57ISI: 001257347100001Scopus ID: 2-s2.0-85197454525OAI: oai:DiVA.org:kth-350521DiVA, id: diva2:1884293
Note

QC 20240715

Available from: 2024-07-15 Created: 2024-07-15 Last updated: 2024-07-15Bibliographically approved

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Basquens, Marc

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