Intensity interferometry and the second-order correlation function $g^{(2)}$ in astrophysics
| Autor: | C. Foellmi |
|---|---|
| Přispěvatelé: | Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) |
| Rok vydání: | 2009 |
| Předmět: |
Quantum optics
Physics Narrabri Stellar Intensity Interferometer Cosmic microwave background Intensity interferometer Observational techniques FOS: Physical sciences Astronomy and Astrophysics Astrophysics Polarization (waves) 01 natural sciences Interferometry Space and Planetary Science 0103 physical sciences Astrophysics - Instrumentation and Methods for Astrophysics 010306 general physics Instrumentation and Methods for Astrophysics (astro-ph.IM) 010303 astronomy & astrophysics Quantum |
| Zdroj: | Astronomy and Astrophysics-A&A Astronomy and Astrophysics-A&A, EDP Sciences, 2009, 507, pp.1719. ⟨10.1051/0004-6361/200911739⟩ |
| ISSN: | 1432-0746 0004-6361 |
| DOI: | 10.1051/0004-6361/200911739 |
| Popis: | Most observational techniques in astronomy can be understood as exploiting the various forms of the first-order correlation function g^(1). As however demonstrated by the Narrabri Stellar Intensity Interferometer back in the 1960's by Hanbury Brown & Twiss, and which is the first experiment to measure the second-order correlation function g^(2), light can carry more information than simply its intensity, spectrum and polarization. Since this experiment, theoretical and laboratory studies of non-classical properties of light have become a very active field of research, namely quantum optics. Despite the variety of results in this field, astrophysics remained focused essentially on first-order coherence. In this paper, we study the possibility that quantum properties of light could be observed in cosmic sources. We provide the basic mathematical ingredients about the first and the second order correlation functions, applied to the modern context of astronomical observations. The exploitation of g^(2) is certainly richer than what a modern intensity interferometer could bring and is particularly interesting for sources of non-thermal light. We conclude by briefly presenting why microquasars in our galaxy and their extragalactic parents can represent an excellent first target in the optical/near-infrared where to observe non-thermal light, and test the use of g^(2) in astrophysical sources. 10 pages, accepted for publication in A&A. Vastly rewritten. Much more precise and (hopefully) accurate |
| Databáze: | OpenAIRE |
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