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Field and intensity correlations: the Siegert relation from stars to quantum emitters

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Pierre Lassègues
  • Function : Author
  • PersonId : 1163759
Martial Morisse
  • Function : Author
  • PersonId : 1163761
André Cidrim
  • Function : Author
  • PersonId : 1163762
Nolan Matthews
  • Function : Author
  • PersonId : 1130754
Guillaume Labeyrie
  • Function : Author
  • PersonId : 1112283
Jean-Pierre Rivet
Farrokh Vakili
  • Function : Author
  • PersonId : 1037946
Robin Kaiser
William Guerin
Mathilde Hugbart

Abstract

The 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 verify the validity of this relation for moving quantum scatterers illuminated by a strong driving field.
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Dates and versions

hal-03775390 , version 1 (13-09-2022)

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Pierre Lassègues, Mateus Antônio Fernandes Biscassi, Martial Morisse, André Cidrim, Nolan Matthews, et al.. Field and intensity correlations: the Siegert relation from stars to quantum emitters. 2022. ⟨hal-03775390⟩
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