Browsing by Subject "gravitational wave detection"

Browsing by Subject "gravitational wave detection"

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  • Loriani Fard, Sina Leon (Hannover : Institutionelles Repositorium der Leibniz Universität Hannover, 2020)
    The search for a fundamental, self-consistent theoretical framework to cover phenomena over all energy scales is possibly the most challenging quest of contemporary physics. Approaches to reconcile quantum mechanics and ...
  • Loriani, S.; Schlippert, D.; Schubert, C.; Abend, Sven; Ahlers, H.; Ertmer, Wolfgang; Rudolph, J.; Hogan, J.M.; Kasevich, M.A.; Rasel, E.M.; Gaaloul, N. (Bristol : Institute of Physics Publishing, 2019)
    Recent proposals for space-borne gravitational wave detectors based on atom interferometry rely on extremely narrow single-photon transition lines as featured by alkaline-earth metals or atomic species with similar electronic ...
  • Krüger, Christoph; Heinert, Daniel; Khalaidovski, Alexander; Steinlechner, Jessica; Nawrodt, Ronny; Schnabel, Roman; Lück, Harald (London : Institute of Physics Publishing, 2015)
    Crystalline silicon has been proposed as a new test mass material in third generation gravitational wave detectors such as the Einstein telescope (ET). Birefringence can reduce the interferometric contrast and can produce ...
  • Bode, Nina (Hannover : Institutionelles Repositorium der Leibniz Universität Hannover, 2023)
    Current and future gravitational wave detectors (GWDs) require high power and low noise laser systems at a wavelength of 1064nm in the continuous wave regime, with excellent spatial beam quality. These systems are highly ...
  • Mehmet, M.; Vahlbruch, H. (Bristol : Institute of Physics Publishing, 2019)
    The engineering of strongly squeezed vacuum states of light is a key technology for the reduction of quantum noise in gravitational wave detectors. We report on the observation of up to 12.0 dB squeezed vacuum states of ...
  • LISA Pathfinder Collaboration; Audley, H.; Born, M.; Danzmann, K.; Diepholz, I.; Heinzel, G.; Hewitson, M.; Karnesis, N.; Kaune, B.; Korsakova, N.; Paczkowski, S.; Reiche, J.; Troebs, M.; Wanner, G.; Wissel, L.; Wittchen, A.; et al. (London : Institute of Physics, 2017)
    This paper describes a methodology to analyze, in the frequency domain, the steady-state control performances of the LISA Pathfinder mission. In particular, it provides a technical framework to give a comprehensive ...
  • LISA Pathfinder Collaboration; Audley, H.; Born, M.; Danzmann, K.; Diepholz, I.; Heinzel, G.; Hewitson, M.; Karnesis, N.; Kaune, B.; Korsakova, N.; Paczkowsk, S.; Reiche, J.; Troebs, M.; Wanner, G.; Wissel, L.; Wittchen, A.; et al. (London : Institute of Physics, 2017)
    LISA Pathfinder, the European Space Agency's technology demonstrator mission for future spaceborne gravitational wave observatories, was launched on 3 December 2015, from the European space port of Kourou, French Guiana. ...
  • Bischof, Lea (Hannover : Institutionelles Repositorium der Leibniz Universität Hannover, 2023)
    The Laser Interferometer Space Antenna (LISA) will be a future gravitational wave observatory in space. It will consist of three spacecraft forming a triangular constellation using laser links. The angles of the constellation ...
  • Kirchhoff, R.; Mow-Lowry, C.M.; Bergmann, G.; Hanke, M.M.; Koch, P.; Köhlenbeck, S.M.; Leavey, S.; Lehmann, J.; Oppermann, P.; Wöhler, J.; Wu, D.S.; Lück, H.; Strain, K.A. (Bristol : IOP Publ., 2020)
    High precision measurements in various applications rely on active seismic isolation to decouple the experiment from seismic motion; therefore, closed feed-back control techniques such as sensor blending and sensor correction ...
  • Bergmann, G.; Mow-Lowry, C.M.; Adya, V.B.; Bertolini, A.; Hanke, M.M.; Kirchhoff, R.; Köhlenbeck, S.M.; Kühn, G.; Oppermann, P.; Wanner, A.; Westphal, T.; Wöhler, J.; Wu, D.S.; Lück, H.; Strain, K.A.; Danzmann, Karsten (Bristol : Institute of Physics Publishing, 2017)
    The 10 m prototype facility at the Albert-Einstein-institute (AEI) in Hanover, Germany, employs three large seismic attenuation systems to reduce mechanical motion. The AEI seismic-attenuation-system (AEI-SAS) uses mechanical ...
  • Isleif, Katharina-Sophie; Bischof, Lea; Ast, Stefan; Penkert, Daniel; Schwarze, Thomas S.; Barranco, German Fernandez; Zwetz, Max; Veith, Sonja; Hennig, Jan-Simon; Tröbs, Michael; Reiche, Jens; Gerberding, Oliver; Danzmann, Karsten; Heinzel, Gerhard (Bristol : Institute of Physics Publishing, 2018)
    LISA is a proposed space-based laser interferometer detecting gravitational waves by measuring distances between free-floating test masses housed in three satellites in a triangular constellation with laser links in-between. ...
  • Kranzhoff, S.L.; Lehmann, J.; Kirchhoff, R.; Carlassara, M.; Cooper, S.J.; Koch, P.; Leavey, S.; Lück, H.; Mow-Lowry, C.M.; Wöhler, J.; von Wrangel, J.; Wu, D.S. (Bristol : IOP Publ., 2022)
    High precision interferometers such as gravitational-wave detectors require complex seismic isolation systems in order to decouple the experiment from unwanted ground motion. Improved inertial sensors for active isolation ...