Thermal noise reduction in interferometric gravitational wave antennas: using high order TEM modes

Details Thermal noise reduction in interferometric gravitational wave antennas: using high order TEM modes Thermal noise reduction in interferometric gravitational wave antennas: using high order TEM modes

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cqgra..23.5777m&link_type=abstract

Classical and Quantum Gravity, Volume 23, Issue 20, pp. 5777-5784 (2006).

Computer Science

22

Scientific paper

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.

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