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Advanced Virgo

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Part of the book series: Springer Theses ((Springer Theses))

Abstract

Ground-based GW detectors are very complex optical systems and for this reason they are divided in different subsystems. Each of them takes care of a different topic but of course there are strong interactions between them.

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Notes

  1. 1.

    The waist is the point with the smallest size in a Gaussian beam.

  2. 2.

    A wedge in an optic element consists on introducing an angle between its two surfaces.

  3. 3.

    The baffles are mechanical elements coated with a particular material which absorbs light.

References

  1. The Virgo Collaboration, Advanced Virgo Technical Design Report, Internal note, Virgo, VIR-0128-12 (2012)

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  2. A. Freise et al., Frequency domain interferometer simulation with higher-order spatial modes. Class. Quantum Grav. 21(5) (2004)

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  3. Optickle website: https://github.com/optickle/optickle

  4. B. Bhawal, M. Evans, E. Maros, M. Rahman, H. Yamamoto, Overview of End-to-End Model, Technical note, LIGO, https://labcit.ligo.caltech.edu/~e2e/ (1997)

  5. F. Acernese et al., Measurements of superattenuator seismic isolation by Virgo interferometer. Astropart. Phys. 33 (2010)

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  6. G. Pillant, E. Genin, ISYS Training Session, Presentation, Virgo, VIR-0215A-17 (2017)

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Correspondence to Julia Casanueva Diaz .

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Casanueva Diaz, J. (2018). Advanced Virgo. In: Control of the Gravitational Wave Interferometric Detector Advanced Virgo. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-96014-2_4

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