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Conferences > EQEC > 1994 > QWD > QWD38
  • European Quantum Electronics Conference
  • Technical Digest Series (Optica Publishing Group, 1994),
  • paper QWD38

Dependence of the sensitivity of interferometric gravitational antennas on laser correlation functions

R. Romano, F. Barone, L. Di Fiore, M. A. Man'ko, V. I. Man'ko, S. Solimeno, and F. Zaccaria

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Abstract

Aim of this communication is to discuss the role of the correlation functions of the light sources in setting up the Standard Noise Limit (SNL) of interferometric GW antennae. Extending the analyses of a previous paper,1 we will discuss an algebraic model for analyzing the sensitivity of interferometers, using mirrors suspended to multiple pendula and limited by radiation pressure and photon noise.

© 1994 IEEE

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