Prospects of higher-order Laguerre Gauss modes in future gravitational wave detectors

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

12 pages, 8 figures

Scientific paper

10.1103/PhysRevD.79.122002

The application of higher-order Laguerre Gauss (LG) modes in large-scale gravitational wave detectors has recently been proposed. In comparison to the fundamental mode, some higher-order Laguerre Gauss modes can significantly reduce the contribution of coating Brownian noise. Using frequency domain simulations we give a detailed analysis of the longitudinal and angular control signals derived with a LG33 mode in comparison to the fundamental TEM00 mode. The performance regarding interferometric sensing and control of the LG33 mode is found to be similar, if not even better in all aspects of interest. In addition, we evaluate the sensitivity gain of the implementation of LG33 modes into the Advanced Virgo instrument. Our analysis shows that the application of the LG33 mode results in a broadband improvement of the Advanced Virgo sensitivity, increasing the potential detection rate of binary neutron star inspirals by a factor 2.1.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Prospects of higher-order Laguerre Gauss modes in future gravitational wave detectors does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Prospects of higher-order Laguerre Gauss modes in future gravitational wave detectors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Prospects of higher-order Laguerre Gauss modes in future gravitational wave detectors will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-425272

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.