Non-local tails in radiation in odd dimensions
M. Khlopunov

TL;DR
This paper investigates how non-local tail effects in odd-dimensional spacetimes influence radiation from localized sources, revealing unique temporal and spectral features in scalar radiation within a three-dimensional model.
Contribution
It demonstrates the presence of tail signals in radiation in odd dimensions and derives their impact on radiation power and spectral distribution, extending understanding of wave propagation beyond four dimensions.
Findings
Tail signals cause shifts in radiation power extremum points.
Radiation in 3D occurs mainly in lower harmonics.
Spectral distribution differs from 4D, favoring higher harmonics in higher dimensions.
Abstract
Huygens principle violation in a spacetime of odd dimensions leads to the fact that the retarded massless fields of localised sources depend on their history of motion preceding the retarded time. This non-local character of retarded fields should result into the formation of tail signals in the radiation of localised sources. In particular, in gravity theories with odd number of extra spacetime dimensions the gravitational radiation of binary systems should contain the tail terms. In this work, we demonstrate the presence of tail signal in radiation within a simple model of scalar field interacting with the point charge moving on elliptical orbit in three dimensions. We find that the tail term results into the characteristic dependence of radiation power of the charge on time. In particular, its extremum points do not correspond to the moments when the charge passes the pericenter and…
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations
