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Volumn 46, Issue 26, 2007, Pages 6648-6654

Generation of a flat-top laser beam for gravitational wave detectors by means of a nonspherical Fabry-Perot resonator

Author keywords

[No Author keywords available]

Indexed keywords

DETECTORS; GRAVITY WAVES; INTERFEROMETRY; RESONATORS; SENSITIVITY ANALYSIS; THERMAL NOISE;

EID: 34548139504     PISSN: 1559128X     EISSN: 15394522     Source Type: Journal    
DOI: 10.1364/AO.46.006648     Document Type: Article
Times cited : (45)

References (18)
  • 1
    • 0010305170 scopus 로고    scopus 로고
    • Advanced LIGO systems design
    • LIGO Tech. Note T-010075-00-D
    • P. Fritschel, "Advanced LIGO systems design," LIGO Tech. Note T-010075-00-D, http://docuserv.ligo.caltech.edu/.
    • Fritschel, P.1
  • 2
    • 84975574819 scopus 로고
    • Optical resonators using gradedphase mirrors
    • P. A. Belanger and C. Paré, "Optical resonators using gradedphase mirrors," Opt. Lett. 16, 1057-1059 (1991).
    • (1991) Opt. Lett , vol.16 , pp. 1057-1059
    • Belanger, P.A.1    Paré, C.2
  • 4
    • 36749008284 scopus 로고    scopus 로고
    • Reducing thermoelastic noise in gravitational-wave interferometers by flattening the light beams
    • gr-qc/0409075
    • 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, 2004, http://arxiv.org/archive/ gr-qc.
    • (2004) arXiv.org e-Print archive
    • D'Ambrosio, E.1    O'Shaughnessy, R.2    Strigin, S.3    Thorne, K.S.4    Vyatchanin, S.5
  • 5
    • 84894009234 scopus 로고    scopus 로고
    • R. O'Shaughnessy, S. Strigin, and S. Vyatchanin, The implications of Mexican-hat mirrors: calculations of thermoelastic noise and interferometer sensitivity to perturbation for the Mexican-hat-mirror proposal for advanced LIGO, arXiv.org e-Print archive, gr-qc/0409050, 2004, http://arxiv.org/archive/ gr-qc.
    • R. O'Shaughnessy, S. Strigin, and S. Vyatchanin, "The implications of Mexican-hat mirrors: calculations of thermoelastic noise and interferometer sensitivity to perturbation for the Mexican-hat-mirror proposal for advanced LIGO," arXiv.org e-Print archive, gr-qc/0409050, 2004, http://arxiv.org/archive/ gr-qc.
  • 7
    • 84894011810 scopus 로고    scopus 로고
    • J. Agresti and R. DeSalvo, Flat beam profile to depress thermal noise, presented at Aspen Winter Conference on Gravitational Waves, Gravitational Wave Advanced Detectors Workshop (GWADW), Aspen, Colo, USA, 16-22 January 2005, e-Print LIGO-G050041-00-Z, http://docuserv.ligo.caltech. edu/.
    • J. Agresti and R. DeSalvo, "Flat beam profile to depress thermal noise," presented at Aspen Winter Conference on Gravitational Waves, Gravitational Wave Advanced Detectors Workshop (GWADW), Aspen, Colo, USA, 16-22 January 2005, e-Print LIGO-G050041-00-Z, http://docuserv.ligo.caltech. edu/.
  • 8
    • 17044368738 scopus 로고    scopus 로고
    • Mirror thermal noise in flat-beam cavities for advanced gravitational wave interferometers
    • J.-Y. Vinet, "Mirror thermal noise in flat-beam cavities for advanced gravitational wave interferometers," Class. Quantum Grav. 22, 1395-1404 (2005).
    • (2005) Class. Quantum Grav , vol.22 , pp. 1395-1404
    • Vinet, J.-Y.1
  • 9
    • 33645500444 scopus 로고    scopus 로고
    • J. Agresti, E. D'Ambrosio, R. DeSalvo, D. Forest, B. Lagrange, J. M. Mackowski, C. Michel, J. L. Montorio, N. Morgado, L. Pinard, A. Remillieux, B. Simoni, M. Tarallo, and P. Willems, Design and construction of a prototype of a flat top beam interferometer and initial tests, J. Phys.: Conf. Ser. 32, 301-308 (2006).
    • J. Agresti, E. D'Ambrosio, R. DeSalvo, D. Forest, B. Lagrange, J. M. Mackowski, C. Michel, J. L. Montorio, N. Morgado, L. Pinard, A. Remillieux, B. Simoni, M. Tarallo, and P. Willems, "Design and construction of a prototype of a flat top beam interferometer and initial tests," J. Phys.: Conf. Ser. 32, 301-308 (2006).
  • 11
    • 17044412316 scopus 로고    scopus 로고
    • Non-spherical mirrors to reduce thermoelastic noise in advanced gravity wave interferometers
    • E. D'Ambrosio, "Non-spherical mirrors to reduce thermoelastic noise in advanced gravity wave interferometers," Phys. Rev. D 67, 102004 (2003).
    • (2003) Phys. Rev. D , vol.67 , pp. 102004
    • D'Ambrosio, E.1
  • 12
    • 33750183289 scopus 로고    scopus 로고
    • Cavity with a deformable mirror for tailoring the shape of the eigenmode
    • P. Beyersdorf, S. Zappe, M. M. Fejer, and M. Burkhardt, "Cavity with a deformable mirror for tailoring the shape of the eigenmode," Appl. Opt. 45, 6723-6728 (2006).
    • (2006) Appl. Opt , vol.45 , pp. 6723-6728
    • Beyersdorf, P.1    Zappe, S.2    Fejer, M.M.3    Burkhardt, M.4
  • 15
    • 84893990689 scopus 로고    scopus 로고
    • M. G. Tarallo, Experimental study of a non Gaussian optical resonator to reduce mirror thermal noise for graviatational waves detectors, Ph.D. disseration (University of Pisa, 2005), e-Print LIGO-P050032-00-R, http://docuserv.ligo. caltech.edu/.
    • M. G. Tarallo, "Experimental study of a non Gaussian optical resonator to reduce mirror thermal noise for graviatational waves detectors," Ph.D. disseration (University of Pisa, 2005), e-Print LIGO-P050032-00-R, http://docuserv.ligo. caltech.edu/.
  • 16
    • 0019543440 scopus 로고
    • Intracavity adaptive optics. 1: Astigmatism correction performance
    • J. M. Spinhirne, D. Anafl, R. H. Freeman, and H. R. Garcia, "Intracavity adaptive optics. 1: Astigmatism correction performance," Appl. Opt. 20, 976-984 (1981).
    • (1981) Appl. Opt , vol.20 , pp. 976-984
    • Spinhirne, J.M.1    Anafl, D.2    Freeman, R.H.3    Garcia, H.R.4
  • 17
    • 0032651367 scopus 로고    scopus 로고
    • Solid-state laser resonators with diffractive optic thermal aberration correction
    • S. Makki and J. Leger, "Solid-state laser resonators with diffractive optic thermal aberration correction," IEEE J. Quantum Electron. 35, 1075-1085 (1999).
    • (1999) IEEE J. Quantum Electron , vol.35 , pp. 1075-1085
    • Makki, S.1    Leger, J.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.