中文
相关论文

相关论文: Combining underground and on-surface third-generat…

200 篇论文

We study the performances of a world-wide network made by a European third-generation gravitational-wave (GW) detector, together with a 40km Cosmic Explorer detector in the US, considering three scenarios for the European detector: (1)…

广义相对论与量子宇宙学 · 物理学 2025-10-10 Michele Maggiore , Francesco Iacovelli , Enis Belgacem , Michele Mancarella , Niccolò Muttoni

The Einstein Telescope (ET), the European project for a third-generation gravitational-wave detector, has a reference configuration based on a triangular shape consisting of three nested detectors with 10 km arms, where in each arm there is…

The Einstein Telescope (ET) is a proposed next-generation, underground gravitational-wave (GW) detector to be based in Europe. It will provide about an order of magnitude sensitivity increase with respect to currently operating detectors,…

We investigate the prospects for detecting a parity-violating gravitational-wave background (GWB) with third-generation ground-based detector networks. We focus on a network consisting of one Einstein Telescope (ET) and two Cosmic Explorer…

广义相对论与量子宇宙学 · 物理学 2026-02-26 Hannah Duval , Charles Badger , Mairi Sakellariadou

The upcoming European design study `Einstein gravitational-wave Telescope' represents the first step towards a substantial, international effort for the design of a third-generation interferometric gravitational wave detector. It is…

广义相对论与量子宇宙学 · 物理学 2009-11-13 A. Freise , S. Chelkowski , S. Hild , W. Del Pozzo , A. Perreca , A. Vecchio

The Einstein Telescope (ET) will be the next generation gravitational wave observatory in Europe with a sensitivity reaching beyond the CMB into the dark era of the Universe. Each corner of the triangular baseline design is the center of…

Einstein Telescope (ET) is a planned third generation gravitational waves detector located in Europe. Its design will be different from currently build interferometers, because ET will consist of three interferometers rotated by a 60 deg…

宇宙学与河外天体物理 · 物理学 2015-05-25 I. Kowalska-Leszczynska , T. Bulik

The third-generation of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer (CE), aim for an improvement in sensitivity of at least a factor of ten over a wide frequency range compared to the current…

天体物理仪器与方法 · 物理学 2022-10-05 A. Utina , A. Amato , J. Arends , C. Arina , M. de Baar , M. Baars , P. Baer , N. van Bakel , W. Beaumont , A. Bertolini , M. van Beuzekom , S. Biersteker , A. Binetti , H. J. M. ter Brake , G. Bruno , J. Bryant , H. J. Bulten , L. Busch , P. Cebeci , C. Collette , S. Cooper , R. Cornelissen , P. Cuijpers , M. van Dael , S. Danilishin , D. Dixit , S. van Doesburg , M. Doets , R. Elsinga , V. Erends , J. van Erps , A. Freise , H. Frenaij , R. Garcia , M. Giesberts , S. Grohmann , H. Van Haevermaet , S. Heijnen , J. V. van Heijningen , E. Hennes , J. -S. Hennig , M. Hennig , T. Hertog , S. Hild , H. -D. Hoffmann , G. Hoft , M. Hopman , D. Hoyland , G. A. Iandolo , C. Ietswaard , R. Jamshidi , P. Jansweijer , A. Jones , P. Jones , N. Knust , G. Koekoek , X. Koroveshi , T. Kortekaas , A. N. Koushik , M. Kraan , M. van de Kraats , S. L. Kranzhoff , P. Kuijer , K. A. Kukkadapu , K. Lam , N. Letendre , P. Li , R. Limburg , F. Linde , J. -P. Locquet , P. Loosen , H. Lueck , M. Martınez , A. Masserot , F. Meylahn , M. Molenaar , C. Mow-Lowry , J. Mundet , B. Munneke , L. van Nieuwland , E. Pacaud , D. Pascucci , S. Petit , Z. Van Ranst , G. Raskin , P. M. Recaman , N. van Remortel , L. Rolland , L. de Roo , E. Roose , J. C. Rosier , D. Ryckbosch , K. Schouteden , A. Sevrin , A. Sider , A. Singha , V. Spagnuolo , A. Stahl , J. Steinlechner , S. Steinlechner , B. Swinkels , N. Szilasi , M. Tacca , H. Thienpont , A. Vecchio , H. Verkooijen , C. H. Vermeer , M. Vervaeke , G. Visser , R. Walet , P. Werneke , C. Westhofen , B. Willke , A. Xhahi , T. Zhang

Recently, the design study `Einstein gravitational wave Telescope' (ET) has been funded within the European FP7 framework. The ambitious goal of this project is to provide a conceptual design of a detector with a hundred times better…

广义相对论与量子宇宙学 · 物理学 2008-11-24 Stefan Hild , Simon Chelkowski , Andreas Freise

The Einstein Telescope (ET), a proposed European ground-based gravitational-wave detector of third-generation, is an evolution of second-generation detectors such as Advanced LIGO, Advanced Virgo, and KAGRA which could be operating in the…

The second-generation interferometric gravitational wave detectors currently under construction are expected to make their first detections within this decade. This will firmly establish gravitational wave physics as an empirical science…

广义相对论与量子宇宙学 · 物理学 2015-06-15 Chris Van Den Broeck

Einstein Telescope (ET) is a proposed next-generation Gravitational Wave (GW) interferometer designed to detect a large number of astrophysical and cosmological sources with unprecedented sensitivity. A key target for ET is the detection of…

广义相对论与量子宇宙学 · 物理学 2025-01-17 Ilaria Caporali , Giulia Capurri , Walter Del Pozzo , Angelo Ricciardone , Lorenzo Valbusa Dall'Armi

Gravitational wave signals from compact binary coalescences offer a powerful and reliable probe of General Relativity. To date, the LIGO-Virgo-KAGRA collaboration has provided stringent consistency tests of General Relativity predictions.…

广义相对论与量子宇宙学 · 物理学 2025-11-12 Andrea Begnoni , Walter Del Pozzo , Matteo Pegorin , Joachim Pomper , Angelo Ricciardone

Einstein Telescope (ET) is a 3rd generation gravitational-wave (GW) detector that is currently undergoing a design study. ET can detect millions of compact binary mergers up to redshifts 2-8. A small fraction of mergers might be observed in…

宇宙学与河外天体物理 · 物理学 2011-08-09 B. S. Sathyaprakash , Bernard Schutz , Chris Van Den Broeck

Gravitational-wave astrophysics has the potential to be transformed by a global network of longer, colder, and thus more sensitive detectors. This network must be constructed to address a wide range of science goals, involving binary…

天体物理仪器与方法 · 物理学 2019-11-11 Evan D Hall , Matthew Evans

Over the last few years, there has been a large momentum to ensure that the third-generation era of gravitational wave detectors will find its realisation in the next decades, and numerous design studies have been ongoing for some time.…

天体物理仪器与方法 · 物理学 2023-08-02 Anna Puecher , Anuradha Samajdar , Tim Dietrich

The Einstein Telescope (ET) is the future third generation gravitational wave detector consisting of three independent interferometers arranged in a triangular configuration, with the sensitivity large enough to be able to detect stellar…

高能天体物理现象 · 物理学 2021-08-25 Neha Singh , Tomasz Bulik

Einstein gravitational-wave Telescope (ET) is a design study funded by the European Commission to explore the technological challenges of and scientific benefits from building a third generation gravitational wave detector. The three-year…

广义相对论与量子宇宙学 · 物理学 2012-06-05 B. Sathyaprakash , M. Abernathy , F. Acernese , P. Amaro-Seoane , N. Andersson , K. Arun , F. Barone , B. Barr , M. Barsuglia , M. Beker , N. Beveridge , S. Birindelli , S. Bose , L. Bosi , S. Braccini , C. Bradaschia , T. Bulik , E. Calloni , G. Cella , E. Chassande-Mottin , S. Chelkowski , A. Chincarini , J. Clark , E. Coccia , C. Colacino , J. Colas , A. Cumming , L. Cunningham , E. Cuoco , S. Danilishin , K. Danzmann , R. De. Salvo , T. Dent , R. De. Rosa , L. Di. Fiore , A. Di. Virgilio , M. Doets , V. Fafone , P. Falferi , R. Flaminio , J. Franc , F. Frasconi , A. Freise , D. Friedrich , P. Fulda , J. Gair , G. Gemme , E. Genin , A. Gennai , A. Giazotto , K. Glampedakis , C. Gräf , M. Granata , H. Grote , G. Guidi , A. Gurkovsky , G. Hammond , M. Hannam , J. Harms , D. Heinert , M. Hendry , I. Heng , E. Hennes , S. Hild , J. Hough , S. Husa , S. Huttner , G. Jones , F. Khalili , K. Kokeyama , K. Kokkotas , B. Krishnan , T. G. F. Li , M. Lorenzini , H. Lück , E. Majorana , I. Mandel , V. Mandic , M. Mantovani , I. Martin , C. Michel , Y. Minenkov , N. Morgado , S. Mosca , B. Mours , H. Müller-Ebhardt , P. Murray , R. Nawrodt , J. Nelson , R. Oshaughnessy , C. D. Ott , C. Palomba , A. Paoli , G. Parguez , A. Pasqualetti , R. Passaquieti , D. Passuello , L. Pinard , W. Plastino , R. Poggiani , P. Popolizio , M. Prato , M. Punturo , P. Puppo , D. Rabeling , I. Racz , P. Rapagnani , J. Read , T. Regimbau , H. Rehbein , S. Reid , L. Rezzolla , F. Ricci , F. Richard , A. Rocchi , S. Rowan , A. Rüdiger , L. Santamaria , B. Sassolas , R. Schnabel , C. Schwarz , P. Seidel , A. Sintes , K. Somiya , F. Speirits , K. Strain , S. Strigin , P. Sutton , S. Tarabrin , A. Thüring , J. van den Brand , M van Veggel , C. Van Den Broeck , A. Vecchio , J. Veitch , F. Vetrano , A. Vicere , S. Vyatchanin , B. Willke , G. Woan , K. Yamamoto

Einstein Telescope (ET) is conceived to be a third generation gravitational-wave observatory. Its amplitude sensitivity would be a factor ten better than advanced LIGO and Virgo and it could also extend the low-frequency sensitivity down to…

‹ 上一页 1 2 3 10 下一页 ›