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Dark matter constraints from a cosmic refractive index

Producción científica: Conference contributionrevisión exhaustiva

Resumen

The dark-matter candidates of particle physics invariably possess electromagnetic interactions, if only at loop level. Light, in passing through dark matter, can thus exhibit frequencydependent effects, exhibiting a refractive index which deviates from its vacuum value. Its real part gives dispersive effects in propagation: such are signalled through systematic, frequency-dependent time delays in the observed light curves of cosmologically distant gamma-ray bursts. We review the theoretical framework for their analysis and use observations of gamma-ray-burst radio afterglows to set a direct limit on the electric-charge-to-mass ratio of dark matter.

Idioma originalEnglish
Título de la publicación alojadaIntersections of Particle and Nuclear Physics - Proceedings of the 10th International Conference
Páginas248-251
Número de páginas4
DOI
EstadoPublished - 2009
Evento10th International Conference on Intersections of Particle and Nuclear Physics - San Diego, CA, United States
Duración: may 26 2009may 31 2009

Serie de la publicación

NombreAIP Conference Proceedings
Volumen1182
ISSN (versión impresa)0094-243X
ISSN (versión digital)1551-7616

Conference

Conference10th International Conference on Intersections of Particle and Nuclear Physics
País/TerritorioUnited States
CiudadSan Diego, CA
Período5/26/095/31/09

ASJC Scopus subject areas

  • General Physics and Astronomy

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