Radiation Beyond Four Space-Time Dimensions

dc.creatorMironov, A.
dc.creatorMorozov, A.
dc.date2007-03-09
dc.date.accessioned2026-07-07T11:59:44Z
dc.date.available2026-07-07T11:59:44Z
dc.descriptionWe present a list of formulas describing classical radiation of the rank s tensor field from an accelerated point-like source in flat space-time of arbitrary even dimension d. This allows straightforward evaluating the total intensity and radiated momentum for any $s$ and $d$ algorithmically, by hands or with the help of a computer (e.g. with an attached MAPLE program). Practical application of formulas is limited, because, for s>1, the energy-momentum tensor for the point-like source is not conserved. This usually means that one cannot neglect contributions to radiation from tensions of the forces that cause acceleration of the source.
dc.description23 pages (8 pages + Tables and Appendix)
dc.identifierhttps://arxiv.org/abs/hep-th/0703097
dc.identifierhttp://arxiv.org/abs/hep-th/0703097
dc.identifierTheor.Math.Phys.156:1209-1217,2008
dc.identifierdoi:10.1007/s11232-008-0090-z
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206671
dc.subjectHigh Energy Physics - Theory
dc.titleRadiation Beyond Four Space-Time Dimensions
dc.typetext

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