Journal
EUROPEAN PHYSICAL JOURNAL D
Volume 76, Issue 12, Pages -Publisher
SPRINGER
DOI: 10.1140/epjd/s10053-022-00558-5
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Funding
- French National Research Agency [ANR19-CE47-0014-01, ANR-20-CE31-0003]
- Sao Paulo Research Foundation (FAPESP) [2018/15554-5, 2019/13143-0, 2017/09390-7, 2021/026739]
- National Council for Scientific and Technological Development (CNPq) [313886/2020-2]
- project STIC-AmSud [Ph879-17/CAPES 88887.521971/20 20-00]
- CAPES-STINT project [88887.649265/2021-00]
- Doeblin Federation
- Region PACA (project I2C)
- European project ANDLICA, ERC [832219]
- French government, through the UCAJEDI Investments in the Future project [ANR-15-IDEX-01]
- UCA-JEDI project [ANR-15-IDEX-01]
- OPTIMAL platform
- European Research Council (ERC) [832219] Funding Source: European Research Council (ERC)
- Agence Nationale de la Recherche (ANR) [ANR-20-CE31-0003] Funding Source: Agence Nationale de la Recherche (ANR)
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This paper discusses the relationship between the Siegert relation and the intensity temporal correlations, and examines the validity of this relation in the fields of astrophysics and quantum scattering.
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 check the validity of this relation for moving quantum scatterers illuminated by a strong driving field.
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