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Quantum-statistical analysis of multimode far-infrared and submillimeter-wave astronomical interferometers
Stafford Withington1, Michael P Hobson, George Saklatvala
1Cavendish Laboratory, Cambridge University, Cambridge CB30 HE, UK.
Summary
We developed a quantum model for far-infrared and submillimeter-wave astronomical interferometers. This model traces quantum field properties through telescopes and detectors, enabling precise photon detection analysis.
Area of Science:
- Astronomy
- Quantum Optics
- Astrophysical Instrumentation
Background:
- Far-infrared and submillimeter-wave interferometry are crucial for astronomical observations.
- Understanding quantum effects in these instruments is vital for precise measurements.
- Existing models may not fully capture the quantum-statistical nature of the observed fields.
Purpose of the Study:
- To develop a comprehensive quantum-statistical model for multimode astronomical interferometers.
- To explicitly identify and trace optical modes throughout the interferometer system.
- To provide a framework for analyzing quantum field properties from source to detector.
Main Methods:
- Formulating a quantum-statistical model based on optical modes.
- Tracing quantum field properties through telescopes, beam combiners, and detectors.
- Deriving expressions for photon detection rates and their fluctuations.
Main Results:
- Elegant expressions for average photon detection rates in imaging arrays.
- Formulas for mean-square fluctuations in photon detection rates.
- Methods to calculate correlations between fluctuations in different detector pixels.
Conclusions:
- The presented model accurately describes quantum-statistical properties in astronomical interferometers.
- The scheme is versatile and applicable to various optical configurations.
- The model facilitates advanced analysis of photon statistics and correlations for astrophysical studies.