Concepts and research for future detectors Summary of the Amaldi 10 C4 session

F. Acernese, F. Barone, A.S. Bell, G. Bergmann, D. Blair, M. Born, D. Brown, X. Chen, S.L. Danilishin, J. Degallaix, T. Denker, A. Di Virgilio, C. Frajuca, D. Friedrich, P. Fulda, H. Grote, S.H. Huttner, J. Kato, S. Kohlenbeck, S. LeaveyH. Luck, M. Nakano, R.N. Palmer, M. Punturo, P. Raffai, D. Schutte, D. Simakov, B.J.J. Slagmolen, K. Somiya*, J. Steinlechner, S. Steinlechner, S. Tarabrin, A.R. Wade, M. Wang, T. Westphal, C. Zhao, R.X. Adhikari, M. Adier, K. Agatsuma, B.W. Barr, R. Bassiri, J. Bauchrowitz, C. Blair, C. Bond, K. Bongs, F.S. Bortoli, G. Cagnoli, P. Calia, R. Canonico, L. Carbone, S. Hild

*Corresponding author for this work

Research output: Contribution to journal(Systematic) Review article peer-review

Abstract

Technologies, design aspects and recent progresses for future gravitational wave (GW) detectors are mentioned in this summary of the C4 session of the Amaldi 10 conference.
Original languageEnglish
Article number1700
Number of pages20
JournalGeneral Relativity and Gravitation
Volume46
Issue number5
DOIs
Publication statusPublished - 1 May 2014
Externally publishedYes

Keywords

  • Gravitational-wave detectors
  • Quantum noise
  • Seismic noise
  • Optics
  • Interferometer
  • Amaldi 10 proceedings
  • GRAVITATIONAL-WAVE DETECTORS
  • NOISE
  • PHASE
  • INTERFEROMETER
  • MODES

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