Published 2006
| Version v1
Journal article
Thermal noise reduction in interferometric gravitational wave antennas: using high order TEM modes
- Creators
- Mours, B.
- Tournefier, E.
- Vinet, J.-Y.
- Others:
- Laboratoire d'Annecy de Physique des Particules (LAPP) ; Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)
- Observatoire de la Côte d'Azur (OCA) ; Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Description
We compute the low-frequency tail of the power spectral density of thermal noise in the case of an optical Fabry–Perot resonant cavity operating with Laguerre–Gauss modes of orders higher than (0, 0). We show a significant reduction of the thermal noise as the order of the mode increases. We discuss the diffraction losses.
Additional details
- URL
- https://hal.in2p3.fr/in2p3-00113125
- URN
- urn:oai:HAL:in2p3-00113125v1
- Origin repository
- UNICA