Evaluation of the performance of polished mirror surfaces for the TAMA gravitational wave detector by use of a wave-front tracing simulation

Applied Optics

Volumn 41, Issue 28, 2002, Pages 5913-5920

  Tomaru, Takayuki ^a,b   Miyoki, Shinji ^a   Ohashi, Masatake ^a   Kuroda, Kazuaki ^a   Uchiyama, Takashi ^c   Suzuki, Toshikazu ^c   Yamamoto, Akira ^c   Shintomi, Takakazu ^c   Ueda, Akitoshi ^c   Tatsumi, Daisuke ^c   Sato, Shuichi ^c   Arai, Koji ^c   Ando, Masaki ^a   Watanabe, Koji ^d   Nakamura, Kenji ^d   Watanabe, Masahiko ^d   Ito, Kazuhiko ^d   Kataoka, Izumi ^d   Yamamoto, Hiroaki ^e   Bochner, Brett ^f   Hefetz, Yaron ^g   more..

^a UNIVERSITY OF TOKYO   (Japan)

^b HIGH ENERGY ACCELERATOR RESEARCH ORGANIZATION KEK   (Japan)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^d Japan Aviat Electron Indust   (Japan)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f HOFSTRA UNIVERSITY   (United States)

^g Hofstra University ^*  (Israel)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0036794056     PISSN: 1559128X     EISSN: 21553165     Source Type: Journal    
DOI: 10.1364/AO.41.005913     Document Type: Article

References (21)

1. K. Tsubono, “300-m laser interferometer gravitational wave detector (TAMA300) in Japan,” in Proceedings of the First Edoardo Amaldi Conference on Gravitational Wave Experiments (World Scientific, Singapore, 1995), pp. 112-114.
2. K. Kuroda, Y. Kozai, M. Fujimoto, M. Ohashi, R. Takahashi, T. Yamazaki, M. A. Barton, N. Kanda, Y. Saito, N. Kamikubota, Y. Ogawa, T. Suzuki, N. Kawashima, E. Mizuno, K. Tsubono, K. Kawabe, N. Mio, S. Moriwaki, A. Araya, K. Ueda, K. Nakagawa, T. Nakamura, and members of TAMA group, “Status of TAMA,” in Proceedings of the International Conference on Gravitational Waves: Source and Detectors (World Scientific, Singapore, 1997), pp. 100-107.
3. M. Ando, K. Arai, R. Takahashi, G. Heinzel, S. Kawamura, D. Tatsumi, N. Kanda, H. Tagoshi, A. Araya, H. Asada, Y. Aso, M. A. Barton, M. Fujimoto, M. Fukushima, T. Futamase, K. Hayama, G. Horikoshi, H. Ishizuka, N. Kamikubota, K. Kaw-abe, N. Kawashima, Y. Kobayashi, Y. Kojima, K. Kondo, Y. Kozai, K. Kuroda, N. Matsuda, N. Mio, K. Miura, O. Miy-akawa, S. M. Miyama, S. Miyoki, S. Moriwaki, M. Musha, S. Nagano, K. Nakagawa, T. Nakamura, K. Nakao, K. Numata, Y. Ogawa, M. Ohashi, N. Ohishi, S. Okutomi, K. Oohara, S. Otsuka, Y. Saito, M. Sasaki, S. Sato, A. Sekiya, M. Shibata, K. Somiya, T. Suzuki, A. Takamori, T. Tanaka, S. Taniguchi, S. Telada, K. Tochikubo, T. Tomaru, K. Tsubono, N. Tsuda, T. Uchiyama, A. Ueda, K. Ueda, K. Waseda, Y. Watanabe, H. Yakura, K. Yamamoto, and T. Yamazaki, “Stable operation of a 300-m laser interferometer with sufficient sensitivity to detect gravitational-wave events within our galaxy,” Phys. Rev. Lett. 86, 3950-3954 (2001).
4. H. Tagoshi, N. Kanda, T. Tanaka, D. Tatsumi, S. Telada, M. Ando, K. Arai, A. Araya, H. Asada, M. A. Barton, M. Fujimoto, M. Fukushima, T. Futamase, G. Heinzel, G. Horikoshi, H. Ishizuka, N. Kamikubota, K. Kawabe, S. Kawamura, N. Kawashima, Y. Kojima, Y. Kozai, K. Kuroda, N. Matsuda, S. Matsumura, S. Miki, N. Mio, O. Miyakawa, S. Miyama, S. Miyoki, E. Mizuno, S. Moriwaki, M. Musha, S. Nagano, K. Nakagawa, T. Nakamura, K. Nakao, K. Numata, Y. Ogawa, M. Ohashi, N. Ohishi, A. Okutomi, K. Oohara, S. Otsuka, Y. Saito, M. Sasaki, S. Sato, A. Sekiya, M. Shibata, K. Shirakata, K. Somiya, T. Suzuki, R. Takahashi, A. Takamori, S. Taniguchi, K. Tochikubo, T. Tomaru, K. Tsubono, N. Tsuda, T. Uchiyama, A. Ueda, K. Ueda, K. Ueda, K. Waseda, Y. Watanabe, H. Yakura, K. Yamamoto, and T. Yamazaki, “First search for gravitational waves from inspiraling compact binaries using TAMA300 data,” Phys. Rev. D 63, 062001, 1-5 (2001).
5. A. Abramovici, W. E. Althouse, R. W. P. Drever, Y. Gursel, S. Kawamura, F. J. Raab, D. Shoemaker, L. Sievers, R. E. Spero, K. S. Thorne, R. E. Vogt, R. Weiss, S. E. Whitcomb, and M. E. Zucker, “LIGO: the Laser Interferometer Gravitational-Wave Observatory,” Science 256, 325-333 (1992).
6. The VIRGO Collaboration, “VIRGO Final Design Report,” VIR-TRE-1000-13 (1997).
7. K. Danzmann, H. Luck, A. Rüdiger, R. Schilling, M. Schrem-pel, W. Winkler, J. Hough, G. P. Newton, N. A. Robertson, H. Ward, A. M. Campbell, J. E. Logan, D. I. Robertson, K. A. Strain, J. R. J. Bennett, V. Kose, M. Kühne, B. F. Schutz, D. Nicholson, J. Shuttleworth, H. Welling, P. Aufmuth, R. Rinkleff, A. Tunnermann, and B. Willke, “GEO 600: a 600-m laser interferometric gravitational wave antenna,” in Proceedings of the First Edoardo Amaldi Conference on Gravitational Wave Experiments (World Scientific, Singapore, 1995), pp. 100-111.
8. R. W. P. Drever, “Fabry-Perot cavity gravity-wave detectors,” in The Detection of Gravitational Wave, D. G. Blair, ed. (Cambridge U. Press, Cambridge, UK, 1991), pp. 306-328.
9. P. Hello and J. Y. Vinet, “Numerical model of transient thermal effect in high power optical resonators,” J. Phys. (Paris) I 3, 717-732 (1993).
10. B. Bochner, “Modeling the performance of interferometric gravitational-wave detectors with realistically imperfect optics,” Ph.D. thesis (Massachusetts Institute of Technology, Cambridge, Mass., 1998).
11. P. Saha, “Fast estimation of transverse fields in high-finesse optical cavities,” J. Opt. Soc. Am. A 14, 2195-2202 (1997).
12. 6level at 1064 nm,” Opt. Lett. 20, 530-532 (1995).
13. A. Ueda, K. Uehara, K. Uchisawa, K. Ueda, H. Sekiguchi, T. Mitake, K. Nakamura, N. Kitajima, and I. Kataoka, “Ultrahigh quality cavity with 1.5 ppm loss at 1064 nm,” Opt. Rev. 3, 369-372 (1996).
14. C. J. Walsh, A. J. Leistner, and B. F. Oreb, “Power spectral density analysis of optical substrates for gravitational-wave interferometry,” Appl. Opt. 38, 4790 -4801 (1999).
15. J. M. Elson and J. M. Benett, “Calculation of the power spectral density from surface profile data,” Appl. Opt. 34, 201-208 (1995).
16. M. V. Berry, “Diffractals,” J. Phys. A: Math. Gen. 12, 781-797 (1979).
17. M. Born and E. Wolf, Principles of Optics, 5th ed. (Pergamon, New York, 1974).
18. S. Sato, S. Miyoki, M. Ohashi, M. Fujimoto, T. Yamazaki, M. Fukushima, A. Ueda, K. Ueda, K. Watanabe, K. Nakamura, K. Etoh, N. Kitajima, K. Ito, and I. Kataoka, “Loss factors of mirrors for a gravitational wave antenna,” Appl. Opt. 38, 2880-2885 (1999).
19. K. Kuroda, M. Ohashi, S. Miyoki, D. Tatsumi, S. Sato, H. Ishizuka, M. Fujimoto, S. Kawamura, R. Takahashi, T. Yamazaki, K. Arai, M. Fukushima, K. Waseda, S. Telada, A. Ueda, T. Shintomi, A. Yamamoto, T. Suzuki, Y. Saito, T. Ha-ruyama, N. Sato, K. Tsubono, K. Kawabe, M. Ando, K. Ueda, H. Yoneda, M. Musha, N. Mio, S. Moriwaki, A. Araya, N. Kanda, and M. E. Tobar, “Large-scale cryogenic gravitational wave telescope,” Int. J. Mod. Phys. D 8, 557-579 (1999).
20. D. Shoemaker, “Advanced LIGO 2002-2006,” presented at the 2001 Aspen Winter Conference on Gravitational Waves and Their Detection, Aspen, Colo., 4-10 February 2001, http:// www.ligo.caltech.edu/docs/G/G010020-00.pdf
21. W. H. Press, S. A. Teukolsky, W. T. Vetterling, and B. P. Flannery, “Numerical recipes in Fortran 77,” (Cambridge U. Press, Cambridge, Mass., 1986).