Cavity with a deformable mirror for tailoring the shape of the eigenmode

Applied Optics

Volumn 45, Issue 26, 2006, Pages 6723-6728

  Beyersdorf, Peter T ^a   Zappe, Stephan ^b   Fejer, M M ^b   Burkhardt, Mark ^b  

^a SAN JOSE STATE UNIVERSITY   (United States)

^b STANFORD UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EIGENVALUES AND EIGENFUNCTIONS; GAUSSIAN NOISE (ELECTRONIC); INTERFEROMETERS; OPTICAL SYSTEMS;

DEFORMABLE MIRRORS; FLATTOP SPATIAL PROFILE; GAUSSIAN PROFILE; SPHERICAL MIRRORS;

MIRRORS;

EID: 33750183289     PISSN: 1559128X     EISSN: 15394522     Source Type: Journal    
DOI: 10.1364/AO.45.006723     Document Type: Article

References (4)

1. P. Fritschel, "The second generation LIGO interferometers," AIP Conf. Proc. 575, 15-23 (2001).
2. Y. T. Liu and K. S. Thorne, "Thermoelastic noise and homoge neous thermal noise in finite sized gravitational-wave test masses," Phys. Rev. D 62, 122002 (2000).
3. E. D'Ambrosio, R. O'Shaughnessy, K. Thorne, P. Willems, S. Strigin, and S. Vyatchanin, "Advanced LIGO: non-Gaussian beams," Class. Quantum Grav. 21, S867-S873 (2004).
4. E. D'Ambrosio, R. O'Shaughnessy, S. Strigin, K. S. Thorne, and S. Vyatchanin, "Reducing thermoelastic noise in gravitational-wave interferometers by flattening the light beams," arXiv.org e-Print archive, gr-qc/0409075, 20 September 2004, http://arxiv.org/abs/gr-qc/0409075.