Scientific Results

Scientific objectives of Einstein Telescope

Year: 2012

Authors: Sathyaprakash B.; Abernathy M.; Acernese F.; Ajith P.; Allen B.; Amaro-Seoane P.; Andersson N.; Aoudia S., Arun K.; Astone P., Krishnan B.; Barack L.; Barone F.; Barr B.; Barsuglia M.; Bassan M.; Bssiri R.; Beker M.; Beveridge N.; Bizouard M.; Bond C.; Bose S.; Bosi L.; Braccini S.; Bradaschia C.; Britzger M.; Brueckner F.; Bulik T.; Bulten H.J.; Burmeister O.; Calloni E.; Campsie P.; Carbone L.; Cella G.; Chalkley E.; Chassandre-Mottin E.; Chelkowski S.; Chincarini A.; Di Cintio A.; Clark J.; Coccia E.; Colacino C.; Colas J.; Colla A.; Corsi A.; Cumming A.; Cunningham L.; Cuoco E.; Danilishin S.; Danzmann K.; Daw E.; De Salvo R.; Del Pozzo W.; Dent T.; De Rosa R.; Di Fiore L.; Di Paolo Emilio M.; Di Virgilio A.; Dietz A.; Doets M.; Dueck J.; Edwards M.; Fafone V.; Fairhurst S.; Falferi P.; Favata M.; Ferrari V.; Ferrini F., Fidecaro F.; Flaminio R.; Franc J.; Frasconi F.; Freise A.; Friedrich D.; Fulda P.; Gair J.; Galimberti M.; Gemme G.; Genin E.; Gennai A.; Giazotto A.; Glampedakis K.; Gossan S.; Gouaty R.; Graef C.; Graham W.; Granata M.; Grote H.; Guidi G.; Hallam J.; Hammond G.; Hannam M.; Harms J.; Haughian K.; Hawke I.; Heinert D.; Hendry M.; Heng I.; Hennes E.; Hild S.; Hough J.; Huet D.; Husa S.; Huttner S.; Iyer B.; Jones D.I.; Jones G.; Kamaretsos I.; Kant Mishra C.; Kawazoe F.; Khalili F.; Kley B.; Kokeyama K.; Kokkotas K.; Kroker S.; Kumar R.; Kuroda K.; Lagrange B.; Lastzka N.; Li T.G.F.; Lorenzini M.; Losurdo G.; Luck H.; Majorana E.; Malvezzi V.; Mandel I.; Mandic V.; Marka S.; Marin F.; Marion F.; Marque J.; Martin I.; Mc Leod D.; Mckechan D.; Mehmet M.; Michel C.; Minenkov Y.; Morgado N.; Morgia A.; Mosca S.; Moscatelli L.; Mours B.; Muller-Ebhardt H.; Murray P.; Naticchioni L.; Nawrodt R.; Nelson J.; O’Shaughnessy R.; Ott C. D.; Palomba C.; Paoli A.; Parguez G.; Pasqualetti A.; Passaquieti R.; Passuello D.; Perciballi M.; Piergiovanni F.; Pinard L.; Pitkin M.; Plastino W.; Poggiani R.; Popolizio P.; Porter E.; Prato M.; Prodi G.; Punturo M.; Puppo P.; Rabeling D.; Rapagnani P.; Racz I.; Re V.; Read J.; Regimbau T.; Rehbein H.; Reid S.; Ricci F.; Richard F.; Robinson C.; Rocchi A.; Romano E.; Rowan S.; Ruediger A.; Samblowski A.; Santamaria L.; Sassolas B.; Schmidt P.; Schnabel R.; Schutz B.; Schwarz C.; Scott J.; Seidel P.; Sintes A.; Somiya K.; Sopuerta C. F.; Sorazu B.; Speirits F.; Storchi L.; Strain K.; Strigin S.; Sutton P.; Tarabrin S.; Taylor B.; Thurin A.; Tokmakov K.; Tonelli M.; Tournefier H.; Vaccarone R.; Vahlbruch H.; van den Brand J.; van den Broeck C.; van den Putten S.; van Veggel M.; Vecchio A.; Veitch J.; Vetrano F.; Vicere A.; Vyatchanin S.; Wessels P.; Willke B.; Winkler W.; Woan G.; Woodcraft A.; Yamamoto K.

Autors Affiliation: Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales; Univ Glasgow, Dept Phys & Astron, Glasgow G12 8QQ, Lanark, Scotland; Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy; Univ Salerno, I-84084 Salerno, Italy; Caltech CaRT, Pasadena, CA 91125 USA; Leibniz Univ Hannover, D-30167 Hannover, Germany; Max Planck Inst Gravitat Phys, D-30167 Hannover, Germany; Max Planck Inst Gravitat Phys, D-14476 Potsdam, Germany; Inst Ciencies Espai, ES-08193 Barcelona, Spain; Univ Southampton, Southampton SO17 1BJ, Hants, England; Chennai Math Inst, Siruseri 603103, India; Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy; Univ Roma La Sapienza, I-00185 Rome, Italy; Univ Paris Diderot, CNRS IN2P3, CEA DSM IRFU, Lab AstroParticule & Cosmol APC,Observ Paris, F-75013 Paris, France; Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy; Univ Roma Tor Vergata, I-00133 Rome, Italy; Nikhef, Amsterdam, Netherlands; Univ Paris 11, LAL, CNRS, IN2P3, F-91898 Orsay, France; Univ Birmingham, Birmingham B15 2TT, W Midlands, England; Washington State Univ, Pullman, WA 99164 USA; Ist Nazl Fis Nucl, Sez Perugia, Milan, Italy; Ist Nazl Fis Nucl, Sez Pisa, Milan, Italy; EGO, I-56021 Cascina, Pi, Italy; Friedrich Schiller Univ Jena PF 07737 Jena, Jena, Germany; Univ Warsaw, Astron Observ, PL-00478 Warsaw, Poland; Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands; Univ Naples Federico II, I-80126 Naples, Italy; Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy; Moscow MV Lomonosov State Univ, Moscow 119992, Russia; Univ Sheffield, Sheffield S10 2TN, S Yorkshire, England; Univ Sannio, Benevento, Italy; Univ Savoie, CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France; Fdn Bruno Kessler, CNR, Ist Foton & Nanotecnol, I-38123 Povo, Trento, Italy; Ist Nazl Fis Nucl, Grp Collegato Trento, Milan, Italy; Univ Pisa, Dipartimento Fis, Pisa, Italy; Univ Lyon 1, CNRS, IN2P3, LMA, F-69622 Villeurbanne, Lyon, France; Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England; Univ Tubingen, Theoret Astrophys TAT, D-72076 Tubingen, Germany; Ist Nazl Fis Nucl, Sez Firenze, I-50019 Sesto Fiorentino, Italy; Univ Urbino Carlo Bo, I-61029 Urbino, Italy; Univ Illes Balears, Dept Fis, E-07122 Palma De Mallorca, Spain; Raman Res Inst, Bangalore 560080, Karnataka, India; Moscow MV Lomonosov State Univ, Moscow 119992, Russia; Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba, Japan; MIT Kavli Inst, Cambridge, MA 02139 USA; Univ Minnesota, Minneapolis, MN 55455 USA; Columbia Univ, Dept Phys, New York, NY 10027 USA; Penn State Univ, University Pk, PA 16802 USA; Ist Nazl Fis Nucl, Sez Roma Tre, I-00146 Rome, Italy; Univ Roma Tre, Dipartimento Fis, I-00146 Rome, Italy; Univ Trento, Trento, Italy; KFKI Res Inst Particle & Nucl Phys, Budapest, Hungary; Univ Mississippi, Dept Phys & Astron, University, MS 38677 USA; Univ Nice Sophia Antipolis, CNRS, Observ Cote dAzur, F-06304 Nice, France; CALTECH, LIGO, Pasadena, CA 91125 USA; Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan; CSIC IEEC, Inst Space Sci, Barcelona 08193, Spain; Laser Zentrum Hannover eV, D-30419 Hannover, Germany; Royal Observ, Greenwich SE10 8XJ, England; Ist Nazl Fis Nucl, Sez Padova, Milan, Italy

Abstract: The advanced interferometer network will herald a new era in observational astronomy. There is a very strong science case to go beyond the advanced detector network and build detectors that operate in a frequency range from 1 Hz to 10 kHz, with sensitivity a factor 10 better in amplitude. Such detectors will be able to probe a range of topics in nuclear physics, astronomy, cosmology and fundamental physics, providing insights into many unsolved problems in these areas.

Journal/Review: CLASSICAL AND QUANTUM GRAVITY

Volume: 29 (12)      Pages from: 124013  to: 124013

More Information: This work was supported by the European Commission under the Framework Programme 7 (FP7) \’Capacities\’, project Einstein Telescope (ET) design study (Grant Agreement 211743), http://www.et-gw.eu/. We thank Drs Asad Ali and Evan Ochsner for comments.
KeyWords: gravitational waves; ET Telescope; gravitational waves observations; gamma-ray bursts; black-hole
DOI: 10.1088/0264-9381/29/12/124013

Citations: 274
data from “WEB OF SCIENCE” (of Thomson Reuters) are update at: 2022-01-23
References taken from IsiWeb of Knowledge: (subscribers only)
Connecting to view paper tab on IsiWeb: Click here
Connecting to view citations from IsiWeb: Click here

gdpr-image
This site uses cookies. If you decide to continue browsing we consider that you accept their use. For more information about cookies and how to delete them please read our Info Policy on cookies use.
Read more