The Einstein Telescope: a third-generation gravitational wave observatory

By M. Punturo, L. Fiore, B. Allen, M. Granata, J. Colas, P. Wolfango, B. Barr, R. Rosa, K. Yamamoto, A. Pasqualetti and 125 more. 2010

2,132 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics

View Paper: https://www.semanticscholar.org/paper/2f302189c82a47afa8fe3ec7728f7ded86e30773

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In Astronomy and Astrophysics

1. Paolo Pani
2. Marek Lewicki
3. V. Cardoso
4. B. Carr
5. C. Caprini
6. V. Vaskonen
7. Juan García-Bellido
8. John Ellis

In Atomic and Molecular Physics, and Optics

1. Marek Lewicki
2. John Ellis
3. Paolo Pani
4. Ilya Mandel
5. M. Volonteri
6. J. No
7. V. Cardoso
8. M. Maggiore

Citations in the corpus

• Dark halos around neutron stars and gravitational waves (2018, background): “However, we note that third generation GW detectors such as the Einstein telescope [52] capable of detecting thousands of BNS mergers within a few years motivate looking for variability in neutron star merger properties.”
• A Review of Gravitational Waves from Cosmic Domain Walls (2017, background): “In Europe, the more advanced ground-based observatory, Einstein Telescope (ET) [127], is planned with the aim of achieving further improvement in sensitivity.”
• Two populations of LIGO-Virgo black holes (2020, methodology): “Right panel: expected sensitivities of Einstein Telescope (ET) [113], AION/MAGIS [114, 115], AEDGE [116], and LISA [117], and the design sensitivity of LIGO [118] on equal mass BH binaries of total mass M at signal-to-noise ratio larger than 8.”
• On the maximal strength of a first-order electroweak phase transition and its gravitational wave signal (2018, background): “the current and future sensitivities (see also [88]) of the European Pulsar Timing Array (EPTA) [89] and LIGO [90{92], as well as the projected sensitivities of LISA [93], the Einstein Telescope (ET) [94,95], the Cosmic Explorer (CE) [96], and the Square Kilometre Array (SKA) [97]. Finally, we also ”
• Challenges and opportunities of gravitational-wave searches at MHz to GHz frequencies (2020, background): “This sensitivity should be achieved by the third generation terrestrial GW detectors that are anticipated to come online in the later half of the 2030s [195, 196].”
• Solar-mass primordial black holes explain NANOGrav hint of gravitational waves (2020, methodology): “Future prospects of various GW observations are also shown: SKA [61], LISA [103], TianQin [104, 105], BBO [106], DECIGO [107], AION [108], AEDGE [109], Advanced LIGO Hanford and Livingston [110] combined with Advanced Virgo [111] as well as LIGO India [112, 113] and KAGRA [114, 115] (HLVIK), and Ein”
• Expected properties of the first gravitational wave signal detected with pulsar timing arrays (2015, background): “…GW astronomy are potentially so revolutionary that the design of a third generation of GBDs –the Einstein telescope (ET)– is now being investigated (Punturo et al. 2010), and the European Space Agency (ESA) has selected The Gravitational Universe science theme (eLISA Consortium 2013) for the L3…”
• Gravitational wave energy budget in strongly supercooled phase transitions (2019, methodology): “compare the produced GW signal to the sensitivities of dierent phases of LIGO [71{73], as well as the projected experiments LISA [74], MAGIS [75,76] and AION [77] 12. and the Einstein Telescope (ET) [78,79]. We also show the envisioned sensitivities of the proposed future missions DECIGO [80] and Bi”
• Probing the pre-BBN universe with gravitational waves from cosmic strings (2018, background): “f the cosmos. Indeed, GWs emitted as far back as in ation could potentially be detected by LIGO/Virgo [31] or proposed future detectors such as LISA [32], BBO/DECIGO [33], the Einstein Telescope (ET) [34,35], and Cosmic Explorer (CE) [36]. A stable and predictable source of primordial GWs is needed ”