Abstract
AbstractThe Siegert relation relates field and intensity temporal correlations. After a historical review of the Siegert relation and the Hanbury Brown and Twiss effect, we discuss the validity of this relation in two different domains. We first show that this relation can be used in astrophysics to determine the fundamental parameters of stars, and that it is especially important for the observation with stellar emission lines. Second, we check the validity of this relation for moving quantum scatterers illuminated by a strong driving field.
Funder
Agence Nationale de la Recherche
FAPESP
CNPq
CAPES
European Research Council
Publisher
Springer Science and Business Media LLC
Subject
Atomic and Molecular Physics, and Optics
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