Einstein gravitational wave Telescope conceptual design study
By M. Abernathy, F. Acernese, P. Ajith, B. Allen, P. A. Seoane, N. Andersson, S. Aoudia, P. Astone, B. Krishnan, L. Barack and 162 more. 2011
269 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/3b2a5eaf0af9cc698dea9c2f845fffbfc5bdd150
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
- Juan García-Bellido
- Marco Peloso
- Daniel G. Figueroa
- N. Bartolo
- E. Belgacem
- N. Aggarwal
- M. Maggiore
- B. Carr
Citations in the corpus
- Gravitational Radiation Detection with Laser Interferometry (2013, background): “Underground detectors such as KAGRA and the Einstein Telescope should be designed to have a high degree of symmetry in the shape of the caverns around each test mass.”
- Gravitational wave detector with cosmological reach (2014, methodology): “Advanced LIGO [4] employs Fabry-Perot arm cavities with a length of 4 km, whereas Advanced VIRGO [5] and KAGRA [6] are 3 km long.”
- Proposal for gravitational-wave detection beyond the standard quantum limit through EPR entanglement (2016, methodology): “However, the narrowness of the bandwidth requires the filter cavity to be long in order to limit impact from optical losses; the current plan for Advanced LIGO is to construct a ∼ 16m filter cavity [35, 38, 39], and ∼ 300m long cavities have been studied for KAGRA [40] and for the Einstein Telecscop”
- Challenges and opportunities of gravitational-wave searches at MHz to GHz frequencies (2020, background): “To expand the detection band of Earthbound interferometers to frequencies below 10 Hz, cryogenically cooled mirrors, large beam diameters and operation underground are considered (Abernathy et al. 2011; Adhikari et al. 2020).”
- Science case for the Einstein telescope (2019, background): “Figure 6 (which is an updated version of that shown in [55]) shows the minimum detectable ellipticity (at 90% confidence level) for currently known NSs potentially emitting in the detector band, assuming two proposed ET configurations and that a full coherent matched filter analysis is done over an ”