z-logo
open-access-imgOpen Access
Signal-to-noise ratio of intensity interferometry experiments with highly asymmetric x-ray sources
Author(s) -
Y.P. Feng,
Ian McNulty,
N. Xu,
E. Gluskin
Publication year - 1995
Language(s) - English
Resource type - Reports
DOI - 10.2172/510394
Subject(s) - optics , physics , coherence (philosophical gambling strategy) , interferometry , pinhole (optics) , aperture (computer memory) , signal to noise ratio (imaging) , detector , noise (video) , signal (programming language) , coherence length , degree of coherence , beam (structure) , acoustics , artificial intelligence , computer science , image (mathematics) , programming language , superconductivity , quantum mechanics
The authors discuss the signal-to-noise ratio of an intensity interferometry experiment for a highly asymmetric x-ray source using different aperture shapes in front of the photodetectors. It is argued that, under ideal conditions using noiseless detectors and electronics, the use of slit-shaped apertures, whose widths are smaller but whose lengths are much greater than the transverse coherence widths of the beam in the corresponding directions, provides no signal-to-noise advantage over the use of pinhole apertures equal to or smaller than the coherence area. As with pinholes, the signal-to-noise ratio is determined solely by the count degeneracy parameter and the degree of coherence of the beam. This contrasts with the signal-to-noise ratio enhancement achievable using slit-shaped apertures with an asymmetric source in a Young`s experiment

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom