Abstract

The second generation of ground-based interferometric gravitational wave detectors are currently being built and installed. They are designed to be better in strain sensitivity by about a factor 10 with respect to the first generation. Light originating from the laser and following unintended paths, called stray light, has been a major problem during the commissioning of all of the first generation detectors. Indeed, stray light carries information about the phase of the emitting object. Therefore, in the next generation all the optics will be suspended in the vacuum in order to mitigate their associated stray light displacement noise. Despite this additional precaution, the challenging target sensitivity at low frequency which is partially limited by quantum radiation pressure combined with up-conversion effects, requires more detailed investigation. In this paper, we turn our attention to stray light originating from auxiliary optical benches. We use a dedicated formalism to compute the re-coupling of back-reflected and back-scattered light. We show, in particular, how much care should be taken in designing and setting requirements for the input bench optics.

© 2013 OSA

PDF Article

References

  • View by:
  • |
  • |
  • |

  1. P. G. Nelson, “An analysis of scattered light in reflecting and refracting primary objectives for coronagraphs,” Coronal Solar Magnetism Observatory Technical Note 4, http://www.cosmo.ucar.edu/publications/nelson_tech4_10-06.pdf .
  2. The LIGO Scientific Collaboration, “LIGO: the laser interferometer gravitational-wave observatory,” Rep. Prog. Phys.72, 076901 (2009).
  3. The Virgo Collaboration, “The Virgo 3 km interferometer for gravitational wave detection,” J. Opt. A: Pure Appl. Opt.10, (2008).
  4. R. Schilling, L. Schnupp, W. Winkler, H. Billing, K. Maischberger, and A. Rudiger, “A method to blot out scattered light effects and its application to a gravitational wave detector,” J. Phys. E: Sci. Instrum.14(65), (1981).
    [CrossRef]
  5. E. Flanagan and K. S. Thorne, “Noise due to backscatter off baffles, the nearby wall and objects at the far end of the beam tube; and recommended actions,” LIGO Technical Report, LIGO-T940063-00 (1994).
  6. J-Y. Vinet, V. Brisson, and S. Braccini, “Scattered light noise in gravitational wave interferometric detectors: coherent effects,” Phys. Rev. D54, 1276 (1996).
    [CrossRef]
  7. J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
    [CrossRef]
  8. A. Spector and G. Mueller, “Back-reflection from a Cassegrain telescope for space-based interferometric gravitational-wave detectors,” Class. Quantum Grav.29, 205005 (2012).
    [CrossRef]
  9. D. J. Ottaway, P. Fritschel, and S. J. Waldman, “Impact of upconverted scattered light on advanced interferometric gravitational wave detectors,” Opt. Express20, 8329–8336 (2012), http://dx.doi.org/10.1364/OE.20.008329 .
    [CrossRef] [PubMed]
  10. S. Hild, “Beyond the first generation: extending the science range of the gravitational wave detector GEO600,” PhD Thesis, (2006).
  11. The Virgo Collaboration, “Noise studies during the first Virgo science run and after,” Class. Quantum Grav.25, 184003 (2008).
  12. The Virgo Collaboration, “Noise from scattered light in the Virgos second science run data,” Class. Quantum Grav.27, 194011 (2010).
  13. R. Takahashi, K. Arai, S. Kawamura, and M.R. Smith, “Direct measurement of the scattered light effect on the, sensitivity in TAMA300,” Phys. Rev. D70, 062003 (2004).
    [CrossRef]
  14. B. Canuel and E. Genin, “Determination of back scattering and direct reflection recoupling from single optics - application to the end benches,” Virgo internal document VIR-0375A-10 (2010), https://tds.ego-gw.it/ql/?c=7570 .
  15. The Virgo Collaboration, “Advanced Virgo technical design report,” Virgo internal document VIR-0128A-12 (2012), https://tds.ego-gw.it/ql/?c=8940 .
  16. P. Meystre, E. M. Wright, J. D. McCullen, and E. Vignes, “Theory of radiation-pressure-driven interferometers,” JOSA B2 (11), 1830–1840 (1985).
    [CrossRef]
  17. G. Muller, T. Delker, D. B. Tanner, and D. Reitze, “Dual-recycled cavity-enhanced Michelson interferometer for gravitational-wave detection,” Appl. Opt.42, 1257 (2003).
    [CrossRef] [PubMed]
  18. The Virgo Collaboration, “Laser with an in-loop relative frequency stability of 1.0 × 10−21on a 100-ms time scale for gravitational-wave detection,” Physical Review A79, 053824 (2009).
  19. S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
    [CrossRef]
  20. E. Tournefier, “Back-scattering by the optical benches: results from Virgo and constraints for AdV,” Virgo internal document VIR-0070A-08 (2008), https://tds.ego-gw.it/ql/?c=2083 .
  21. B. Canuel, I. Fiori, J. Marque, and E. Tournefier, “Diffused light mitigation in Virgo and constraints for Virgo+ and AdV,” Virgo internal document VIR-0792A-09 (2009), https://tds.ego-gw.it/ql/?c=7118 .
  22. Optickle home-page, http://ilog.ligo-wa.caltech.edu:7285/advligo/ISC_Modeling_Software .
  23. M. Smith, “Baffling requirements for the 4K and 2K IFO,” working note of the LIGO Project, LIGO-T980027-00 (1998).
  24. M. Barsuglia, C. Buy, B. Canuel, R. Day, E. Genin, and G. Vajente, “AdV INJ: mode matching telescope configuration choice for the ITF input telescope,” Virgo internal document VIR-0010A-12 (2011) https://tds.ego-gw.it/ql/?c=8812 .
  25. J. C. Stover, “Optical scattering measurement and analysis,” SPIE Press, Bellingham, WA, 2nd Edition (1995).
  26. E. L. Church, “Fractal surface finish,” Appl. Opt.27, 1518–1526 (1988), http://dx.doi.org/10.1364/AO.38.002870 .
    [CrossRef] [PubMed]
  27. 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) http://dx.doi.org/10.1364/AO.38.004790 .
    [CrossRef]
  28. C. J. Walsh, A. J. Leistner, J. Secko, B. F. Oreb, and D. I. Farrant, “Fabrication and measurement of optics for the laser interferometer gravitational wave observatory,” Appl. Opt.38, 2870–2879 (1999), http://dx.doi.org/10.1364/AO.38.002870 .
    [CrossRef]
  29. A. Duparré, J. Ferre-Borrull, S. Gliech, G. Notni, J. Steinert, and J. M. Bennett, “Surface characterization techniques for determining the root-mean-square roughness and power spectral densities of optical components,” Appl. Opt.41, 154–171 (2002) http://dx.doi.org/10.1364/AO.41.000154 .
    [CrossRef] [PubMed]
  30. The Virgo collaboration, “Characterization of the Virgo seismic environment,” Class. Quantum Grav.29, 025005 (2012).
  31. LosurdoG. , “Inertial control of the mirror suspensions of the VIRGO interferometer for gravitational wave detection,” Rev. Sci. Instrum.72, 3653 (2001).
    [CrossRef]
  32. The Virgo collaboration, “Virgo: a laser interferometer to detect gravitational waves,” Journal of Instrumentation7, P03012 (2012).

2012 (4)

A. Spector and G. Mueller, “Back-reflection from a Cassegrain telescope for space-based interferometric gravitational-wave detectors,” Class. Quantum Grav.29, 205005 (2012).
[CrossRef]

The Virgo collaboration, “Characterization of the Virgo seismic environment,” Class. Quantum Grav.29, 025005 (2012).

The Virgo collaboration, “Virgo: a laser interferometer to detect gravitational waves,” Journal of Instrumentation7, P03012 (2012).

D. J. Ottaway, P. Fritschel, and S. J. Waldman, “Impact of upconverted scattered light on advanced interferometric gravitational wave detectors,” Opt. Express20, 8329–8336 (2012), http://dx.doi.org/10.1364/OE.20.008329 .
[CrossRef] [PubMed]

2010 (1)

The Virgo Collaboration, “Noise from scattered light in the Virgos second science run data,” Class. Quantum Grav.27, 194011 (2010).

2009 (4)

The LIGO Scientific Collaboration, “LIGO: the laser interferometer gravitational-wave observatory,” Rep. Prog. Phys.72, 076901 (2009).

The Virgo Collaboration, “Laser with an in-loop relative frequency stability of 1.0 × 10−21on a 100-ms time scale for gravitational-wave detection,” Physical Review A79, 053824 (2009).

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

B. Canuel, I. Fiori, J. Marque, and E. Tournefier, “Diffused light mitigation in Virgo and constraints for Virgo+ and AdV,” Virgo internal document VIR-0792A-09 (2009), https://tds.ego-gw.it/ql/?c=7118 .

2008 (2)

The Virgo Collaboration, “The Virgo 3 km interferometer for gravitational wave detection,” J. Opt. A: Pure Appl. Opt.10, (2008).

The Virgo Collaboration, “Noise studies during the first Virgo science run and after,” Class. Quantum Grav.25, 184003 (2008).

2006 (1)

S. Hild, “Beyond the first generation: extending the science range of the gravitational wave detector GEO600,” PhD Thesis, (2006).

2004 (1)

R. Takahashi, K. Arai, S. Kawamura, and M.R. Smith, “Direct measurement of the scattered light effect on the, sensitivity in TAMA300,” Phys. Rev. D70, 062003 (2004).
[CrossRef]

2003 (1)

2002 (1)

2001 (1)

LosurdoG. , “Inertial control of the mirror suspensions of the VIRGO interferometer for gravitational wave detection,” Rev. Sci. Instrum.72, 3653 (2001).
[CrossRef]

1999 (2)

1997 (1)

J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
[CrossRef]

1996 (1)

J-Y. Vinet, V. Brisson, and S. Braccini, “Scattered light noise in gravitational wave interferometric detectors: coherent effects,” Phys. Rev. D54, 1276 (1996).
[CrossRef]

1988 (1)

1985 (1)

P. Meystre, E. M. Wright, J. D. McCullen, and E. Vignes, “Theory of radiation-pressure-driven interferometers,” JOSA B2 (11), 1830–1840 (1985).
[CrossRef]

1981 (1)

R. Schilling, L. Schnupp, W. Winkler, H. Billing, K. Maischberger, and A. Rudiger, “A method to blot out scattered light effects and its application to a gravitational wave detector,” J. Phys. E: Sci. Instrum.14(65), (1981).
[CrossRef]

Arai, K.

R. Takahashi, K. Arai, S. Kawamura, and M.R. Smith, “Direct measurement of the scattered light effect on the, sensitivity in TAMA300,” Phys. Rev. D70, 062003 (2004).
[CrossRef]

Bennett, J. M.

Billing, H.

R. Schilling, L. Schnupp, W. Winkler, H. Billing, K. Maischberger, and A. Rudiger, “A method to blot out scattered light effects and its application to a gravitational wave detector,” J. Phys. E: Sci. Instrum.14(65), (1981).
[CrossRef]

Bondu, F.

J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
[CrossRef]

Braccini, S.

J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
[CrossRef]

J-Y. Vinet, V. Brisson, and S. Braccini, “Scattered light noise in gravitational wave interferometric detectors: coherent effects,” Phys. Rev. D54, 1276 (1996).
[CrossRef]

Brisson, V.

J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
[CrossRef]

J-Y. Vinet, V. Brisson, and S. Braccini, “Scattered light noise in gravitational wave interferometric detectors: coherent effects,” Phys. Rev. D54, 1276 (1996).
[CrossRef]

Canuel, B.

B. Canuel, I. Fiori, J. Marque, and E. Tournefier, “Diffused light mitigation in Virgo and constraints for Virgo+ and AdV,” Virgo internal document VIR-0792A-09 (2009), https://tds.ego-gw.it/ql/?c=7118 .

Chelkowski, S.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Church, E. L.

Danzmann, K.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Degallaix, J.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Delker, T.

Duparré, A.

Farrant, D. I.

Ferrante, I.

J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
[CrossRef]

Ferre-Borrull, J.

Fiori, I.

B. Canuel, I. Fiori, J. Marque, and E. Tournefier, “Diffused light mitigation in Virgo and constraints for Virgo+ and AdV,” Virgo internal document VIR-0792A-09 (2009), https://tds.ego-gw.it/ql/?c=7118 .

Flanagan, E.

E. Flanagan and K. S. Thorne, “Noise due to backscatter off baffles, the nearby wall and objects at the far end of the beam tube; and recommended actions,” LIGO Technical Report, LIGO-T940063-00 (1994).

Freise, A.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Fritschel, P.

Gliech, S.

Grote, H.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Hewitson, M.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Hild, S.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

S. Hild, “Beyond the first generation: extending the science range of the gravitational wave detector GEO600,” PhD Thesis, (2006).

Hough, J.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Kawamura, S.

R. Takahashi, K. Arai, S. Kawamura, and M.R. Smith, “Direct measurement of the scattered light effect on the, sensitivity in TAMA300,” Phys. Rev. D70, 062003 (2004).
[CrossRef]

Leistner, A. J.

Lück, H.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Maischberger, K.

R. Schilling, L. Schnupp, W. Winkler, H. Billing, K. Maischberger, and A. Rudiger, “A method to blot out scattered light effects and its application to a gravitational wave detector,” J. Phys. E: Sci. Instrum.14(65), (1981).
[CrossRef]

Marque, J.

B. Canuel, I. Fiori, J. Marque, and E. Tournefier, “Diffused light mitigation in Virgo and constraints for Virgo+ and AdV,” Virgo internal document VIR-0792A-09 (2009), https://tds.ego-gw.it/ql/?c=7118 .

McCullen, J. D.

P. Meystre, E. M. Wright, J. D. McCullen, and E. Vignes, “Theory of radiation-pressure-driven interferometers,” JOSA B2 (11), 1830–1840 (1985).
[CrossRef]

Meystre, P.

P. Meystre, E. M. Wright, J. D. McCullen, and E. Vignes, “Theory of radiation-pressure-driven interferometers,” JOSA B2 (11), 1830–1840 (1985).
[CrossRef]

Mueller, G.

A. Spector and G. Mueller, “Back-reflection from a Cassegrain telescope for space-based interferometric gravitational-wave detectors,” Class. Quantum Grav.29, 205005 (2012).
[CrossRef]

Muller, G.

Notni, G.

Oreb, B. F.

Ottaway, D. J.

Pinard, L.

J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
[CrossRef]

Prijatelj, M.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Reitze, D.

Rudiger, A.

R. Schilling, L. Schnupp, W. Winkler, H. Billing, K. Maischberger, and A. Rudiger, “A method to blot out scattered light effects and its application to a gravitational wave detector,” J. Phys. E: Sci. Instrum.14(65), (1981).
[CrossRef]

Schilling, R.

R. Schilling, L. Schnupp, W. Winkler, H. Billing, K. Maischberger, and A. Rudiger, “A method to blot out scattered light effects and its application to a gravitational wave detector,” J. Phys. E: Sci. Instrum.14(65), (1981).
[CrossRef]

Schnupp, L.

R. Schilling, L. Schnupp, W. Winkler, H. Billing, K. Maischberger, and A. Rudiger, “A method to blot out scattered light effects and its application to a gravitational wave detector,” J. Phys. E: Sci. Instrum.14(65), (1981).
[CrossRef]

Secko, J.

Smith, J. R.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Smith, M.R.

R. Takahashi, K. Arai, S. Kawamura, and M.R. Smith, “Direct measurement of the scattered light effect on the, sensitivity in TAMA300,” Phys. Rev. D70, 062003 (2004).
[CrossRef]

Spector, A.

A. Spector and G. Mueller, “Back-reflection from a Cassegrain telescope for space-based interferometric gravitational-wave detectors,” Class. Quantum Grav.29, 205005 (2012).
[CrossRef]

Steinert, J.

Stover, J. C.

J. C. Stover, “Optical scattering measurement and analysis,” SPIE Press, Bellingham, WA, 2nd Edition (1995).

Strain, K. A.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Takahashi, R.

R. Takahashi, K. Arai, S. Kawamura, and M.R. Smith, “Direct measurement of the scattered light effect on the, sensitivity in TAMA300,” Phys. Rev. D70, 062003 (2004).
[CrossRef]

Tanner, D. B.

Thorne, K. S.

E. Flanagan and K. S. Thorne, “Noise due to backscatter off baffles, the nearby wall and objects at the far end of the beam tube; and recommended actions,” LIGO Technical Report, LIGO-T940063-00 (1994).

Tournefier, E.

B. Canuel, I. Fiori, J. Marque, and E. Tournefier, “Diffused light mitigation in Virgo and constraints for Virgo+ and AdV,” Virgo internal document VIR-0792A-09 (2009), https://tds.ego-gw.it/ql/?c=7118 .

Tournié, E.

J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
[CrossRef]

Vignes, E.

P. Meystre, E. M. Wright, J. D. McCullen, and E. Vignes, “Theory of radiation-pressure-driven interferometers,” JOSA B2 (11), 1830–1840 (1985).
[CrossRef]

Vinet, J-Y.

J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
[CrossRef]

J-Y. Vinet, V. Brisson, and S. Braccini, “Scattered light noise in gravitational wave interferometric detectors: coherent effects,” Phys. Rev. D54, 1276 (1996).
[CrossRef]

Waldman, S. J.

Walsh, C. J.

Willke, B.

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

Winkler, W.

R. Schilling, L. Schnupp, W. Winkler, H. Billing, K. Maischberger, and A. Rudiger, “A method to blot out scattered light effects and its application to a gravitational wave detector,” J. Phys. E: Sci. Instrum.14(65), (1981).
[CrossRef]

Wright, E. M.

P. Meystre, E. M. Wright, J. D. McCullen, and E. Vignes, “Theory of radiation-pressure-driven interferometers,” JOSA B2 (11), 1830–1840 (1985).
[CrossRef]

Appl. Opt. (5)

Class. Quantum Grav. (5)

The Virgo collaboration, “Characterization of the Virgo seismic environment,” Class. Quantum Grav.29, 025005 (2012).

A. Spector and G. Mueller, “Back-reflection from a Cassegrain telescope for space-based interferometric gravitational-wave detectors,” Class. Quantum Grav.29, 205005 (2012).
[CrossRef]

The Virgo Collaboration, “Noise studies during the first Virgo science run and after,” Class. Quantum Grav.25, 184003 (2008).

The Virgo Collaboration, “Noise from scattered light in the Virgos second science run data,” Class. Quantum Grav.27, 194011 (2010).

S. Hild, H. Grote, J. Degallaix, S. Chelkowski, K. Danzmann, A. Freise, M. Hewitson, J. Hough, H. Lück, M. Prijatelj, K. A. Strain, J. R. Smith, and B. Willke, “DC-readout of a signal-recycled gravitational wave detector,” Class. Quantum Grav.26, 055012 (2009).
[CrossRef]

J. Opt. A: Pure Appl. Opt. (1)

The Virgo Collaboration, “The Virgo 3 km interferometer for gravitational wave detection,” J. Opt. A: Pure Appl. Opt.10, (2008).

J. Phys. E: Sci. Instrum. (1)

R. Schilling, L. Schnupp, W. Winkler, H. Billing, K. Maischberger, and A. Rudiger, “A method to blot out scattered light effects and its application to a gravitational wave detector,” J. Phys. E: Sci. Instrum.14(65), (1981).
[CrossRef]

JOSA B (1)

P. Meystre, E. M. Wright, J. D. McCullen, and E. Vignes, “Theory of radiation-pressure-driven interferometers,” JOSA B2 (11), 1830–1840 (1985).
[CrossRef]

Journal of Instrumentation (1)

The Virgo collaboration, “Virgo: a laser interferometer to detect gravitational waves,” Journal of Instrumentation7, P03012 (2012).

Opt. Express (1)

Phys. Rev. D (3)

J-Y. Vinet, V. Brisson, and S. Braccini, “Scattered light noise in gravitational wave interferometric detectors: coherent effects,” Phys. Rev. D54, 1276 (1996).
[CrossRef]

J-Y. Vinet, V. Brisson, S. Braccini, I. Ferrante, L. Pinard, F. Bondu, and E. Tournié, “Scattered light noise in gravitational wave interferometric detectors: a statistical approach,” Phys. Rev. D56, 6085 (1997).
[CrossRef]

R. Takahashi, K. Arai, S. Kawamura, and M.R. Smith, “Direct measurement of the scattered light effect on the, sensitivity in TAMA300,” Phys. Rev. D70, 062003 (2004).
[CrossRef]

Physical Review A (1)

The Virgo Collaboration, “Laser with an in-loop relative frequency stability of 1.0 × 10−21on a 100-ms time scale for gravitational-wave detection,” Physical Review A79, 053824 (2009).

Rep. Prog. Phys. (1)

The LIGO Scientific Collaboration, “LIGO: the laser interferometer gravitational-wave observatory,” Rep. Prog. Phys.72, 076901 (2009).

Rev. Sci. Instrum. (1)

LosurdoG. , “Inertial control of the mirror suspensions of the VIRGO interferometer for gravitational wave detection,” Rev. Sci. Instrum.72, 3653 (2001).
[CrossRef]

Other (11)

P. G. Nelson, “An analysis of scattered light in reflecting and refracting primary objectives for coronagraphs,” Coronal Solar Magnetism Observatory Technical Note 4, http://www.cosmo.ucar.edu/publications/nelson_tech4_10-06.pdf .

E. Flanagan and K. S. Thorne, “Noise due to backscatter off baffles, the nearby wall and objects at the far end of the beam tube; and recommended actions,” LIGO Technical Report, LIGO-T940063-00 (1994).

S. Hild, “Beyond the first generation: extending the science range of the gravitational wave detector GEO600,” PhD Thesis, (2006).

B. Canuel and E. Genin, “Determination of back scattering and direct reflection recoupling from single optics - application to the end benches,” Virgo internal document VIR-0375A-10 (2010), https://tds.ego-gw.it/ql/?c=7570 .

The Virgo Collaboration, “Advanced Virgo technical design report,” Virgo internal document VIR-0128A-12 (2012), https://tds.ego-gw.it/ql/?c=8940 .

E. Tournefier, “Back-scattering by the optical benches: results from Virgo and constraints for AdV,” Virgo internal document VIR-0070A-08 (2008), https://tds.ego-gw.it/ql/?c=2083 .

B. Canuel, I. Fiori, J. Marque, and E. Tournefier, “Diffused light mitigation in Virgo and constraints for Virgo+ and AdV,” Virgo internal document VIR-0792A-09 (2009), https://tds.ego-gw.it/ql/?c=7118 .

Optickle home-page, http://ilog.ligo-wa.caltech.edu:7285/advligo/ISC_Modeling_Software .

M. Smith, “Baffling requirements for the 4K and 2K IFO,” working note of the LIGO Project, LIGO-T980027-00 (1998).

M. Barsuglia, C. Buy, B. Canuel, R. Day, E. Genin, and G. Vajente, “AdV INJ: mode matching telescope configuration choice for the ITF input telescope,” Virgo internal document VIR-0010A-12 (2011) https://tds.ego-gw.it/ql/?c=8812 .

J. C. Stover, “Optical scattering measurement and analysis,” SPIE Press, Bellingham, WA, 2nd Edition (1995).

Cited By

OSA participates in CrossRef's Cited-By Linking service. Citing articles from OSA journals and other participating publishers are listed here.

Alert me when this article is cited.


Metrics