Scientific objectives of Einstein Telescope

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; Bassiri R; Beker M; Beveridge N; Bizouard M; Bond C; Bose S; Bosi L; Braccini S; Bradaschia C; Britzger M; Brueckner F; Bulik T; Bulten HJ; Burmeister O; Calloni E; Campsie P; Carbone L; Cella G; Chalkley E; Chassande Mottin E; Chelkowski S; Chincarini A; Di Cintio A; Clark J; Coccia E; Colacino CN; Colas J; Colla A; Corsi A; Cumming A; Cunningham L; Cuoco E; Danilishin S; Danzmann K; Daw E; De Salvo R; DEL POZZO, WALTER; Dent T; De Rosa R; Di Fiore L; Emilio MD; Di Virgilio A; Dietz A; Doets M; Dueck J; Edwards M; Fafone V; Fairhurst S; Falferi P; Favata M; Ferrari V; Ferrini 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 DI; Jones G; Kamaretsos I; Mishra CK; Kawazoe F; Khalili F; Kley B; Kokeyama K; Kokkotas K; Kroker S; Kumar R; Kuroda K; Lagrange B; Lastzka N; Li TGF; 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; Shaughnessy RO; Ott CD; Palomba C; Paoli A; Parguez G; Pasqualetti A; Passuello D; Perciballi M; Piergiovanni F; Pinard L; Pitkin M; Plastino W; Plissi M; Popolizio P; Porter E; Prato M; Prodi G; Punturo M; Puppo P; Rabeling D; Racz I; Rapagnani P; Re V; Read J; Regimbau T; Rehbein H; Reid S; Ricci F; Richard F; Robinson C; Rocchi A; Romano R; Rowan S; Rudiger A; Samblowski A; Santamaria L; Sassolas B; Schilling R; Schmidt P; Schnabel R; Schutz B; Schwarz C; Scott J; Seidel P; Sintes AM; Somiya K; Sopuerta CF; Sorazu B; Speirits F; Storchi L; Strain K; Strigin S; Sutton P; Tarabrin S; Taylor B; Thurin A; Tokmakov K; Tournefier H; Vaccarone R; Vahlbruch H; van den Brand JFJ; Van den Broeck C; van der 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.; FIDECARO, FRANCESCO; PASSAQUIETI, ROBERTO; POGGIANI, ROSA; TONELLI, MAURO

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oai:arpi.unipi.it:11568/154306

Scientific objectives of Einstein Telescope

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
Bassiri R
Beker M
Beveridge N
Bizouard M
Bond C
Bose S
Bosi L
Braccini S
Bradaschia C
Britzger M
Brueckner F
Bulik T
Bulten HJ
Burmeister O
Calloni E
Campsie P
Carbone L
Cella G
Chalkley E
Chassande Mottin E
Chelkowski S
Chincarini A
Di Cintio A
Clark J
Coccia E
Colacino CN
Colas J
Colla A
Corsi A
Cumming A
Cunningham L
Cuoco E
Danilishin S
Danzmann K
Daw E
De Salvo R
WALTER DEL POZZO
Dent T
De Rosa R
Di Fiore L
Emilio MD
Di Virgilio A
Dietz A
Doets M
Dueck J
Edwards M
Fafone V
Fairhurst S
Falferi P
Favata M
Ferrari V
Ferrini 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 DI
Jones G
Kamaretsos I
Mishra CK
Kawazoe F
Khalili F
Kley B
Kokeyama K
Kokkotas K
Kroker S
Kumar R
Kuroda K
Lagrange B
Lastzka N
Li TGF
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
Shaughnessy RO
Ott CD
Palomba C
Paoli A
Parguez G
Pasqualetti A
Passuello D
Perciballi M
Piergiovanni F
Pinard L
Pitkin M
Plastino W
Plissi M
Popolizio P
Porter E
Prato M
Prodi G
Punturo M
Puppo P
Rabeling D
Racz I
Rapagnani P
Re V
Read J
Regimbau T
Rehbein H
Reid S
Ricci F
Richard F
Robinson C
Rocchi A
Romano R
Rowan S
Rudiger A
Samblowski A
Santamaria L
Sassolas B
Schilling R
Schmidt P
Schnabel R
Schutz B
Schwarz C
Scott J
Seidel P
Sintes AM
Somiya K
Sopuerta CF
Sorazu B
Speirits F
Storchi L
Strain K
Strigin S
Sutton P
Tarabrin S
Taylor B
Thurin A
Tokmakov K
Tournefier H
Vaccarone R
Vahlbruch H
van den Brand JFJ
Van den Broeck C
van der 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.
FRANCESCO FIDECARO
ROBERTO PASSAQUIETI
ROSA POGGIANI
MAURO TONELLI
Publication date: 1 January 2012
Publisher
Doi

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. RI Santamaria, Lucia/A-7269-2012; Gemme, Gianluca/C-7233-2008; prodi, giovanni/B-4398-2010; Hild, Stefan/A-3864-2010; Punturo, Michele/I-3995-201

info:eu-repo/semantics/article

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Archivio della Ricerca - Università di Pisa

oai:arpi.unipi.it:11568/154306

Last time updated on 13/04/2017

This paper was published in Archivio della Ricerca - Università di Pisa.

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