Scientific objectives of Einstein Telescope

B. Sathyaprakash; M. Abernathy; F. Acernese; P. Ajith; B. Allen; P. Amaro-Seoane; N. Andersson; S. Aoudia; K. Arun; P. Astone; B. Krishnan; L. Barack; F. Barone; B. Barr; M. Barsuglia; M. Bassan; R. Bassiri; M. Beker; N. Beveridge; M. Bizouard; C. Bond; S. Bose; L. Bosi; S. Braccini; C. Bradaschia; M. Britzger; F. Brueckner; T. Bulik; H. J. Bulten; O. Burmeister; E. Calloni; P. Campsie; L. Carbone; G. Cella; E. Chalkley; E. Chassande-Mottin; S. Chelkowski; A. Chincarini; A. Di Cintio; J. Clark; E. Coccia; C. N. Colacino; J. Colas; A. Colla; A. Corsi; A. Cumming; L. Cunningham; E. Cuoco; S. Danilishin; K. Danzmann; E. Daw; R. De Salvo; W. Del Pozzo; T. Dent; R. De Rosa; L. Di Fiore; M. Di Paolo Emilio; A. Di Virgilio; A. Dietz; M. Doets; J. Dueck; M. Edwards; V. Fafone; S. Fairhurst; P. Falferi; M. Favata; V. Ferrari; F. Ferrini; F. Fidecaro; R. Flaminio; J. Franc; F. Frasconi; A. Freise; D. Friedrich; P. Fulda; J. Gair; M. Galimberti; G. Gemme; E. Genin; A. Gennai; A. Giazotto; K. Glampedakis; S. Gossan; R. Gouaty; C. Graef; W. Graham; M. Granata; H. Grote; G. Guidi; J. Hallam; G. Hammond; M. Hannam; J. Harms; K. Haughian; I. Hawke; D. Heinert; M. Hendry; I. Heng; E. Hennes; S. Hild; J. Hough; D. Huet; S. Husa; S. Huttner; B. Iyer; D. I. Jones; G. Jones; I. Kamaretsos; C. Kant Mishra; F. Kawazoe; F. Khalili; B. Kley; K. Kokeyama; K. Kokkotas; S. Kroker; R. Kumar; K. Kuroda; B. Lagrange; N. Lastzka; T. G.F. Li; M. Lorenzini; G. Losurdo; H. Lück; E. Majorana; V. Malvezzi; I. Mandel; V. Mandic; S. Marka; F. Marin; F. Marion; J. Marque; I. Martin; D. Mc Leod; D. McKechan; M. Mehmet; C. Michel; Y. Minenkov; N. Morgado; A. Morgia; S. Mosca; L. Moscatelli; B. Mours; H. Müller-Ebhardt; P. Murray; L. Naticchioni; R. Nawrodt; J. Nelson; R. O. Shaughnessy; C. D. Ott; C. Palomba; A. Paoli; G. Parguez; A. Pasqualetti; R. Passaquieti; D. Passuello; M. Perciballi; F. Piergiovanni; L. Pinard; M. Pitkin; W. Plastino; M. Plissi; R. Poggiani; P. Popolizio; E. Porter; M. Prato; G. Prodi; M. Punturo; P. Puppo; D. Rabeling; I. Racz; P. Rapagnani; V. Re; J. Read; T. Regimbau; H. Rehbein; S. Reid; F. Ricci; F. Richard; C. Robinson; A. Rocchi; R. Romano; S. Rowan; A. Rüdiger; A. Samblowski; L. Santamaría; B. Sassolas; R. Schilling; P. Schmidt; R. Schnabel; B. Schutz; C. Schwarz; J. Scott; P. Seidel; A. M. Sintes; K. Somiya; C. F. Sopuerta; B. Sorazu; F. Speirits; L. Storchi; K. Strain; S. Strigin; P. Sutton; S. Tarabrin; B. Taylor; A. Thürin; K. Tokmakov; M. Tonelli; H. Tournefier; R. Vaccarone; H. Vahlbruch; J. F.J. Van Den Brand; C. Van Den Broeck; S. Van Der Putten; M. Van Veggel; A. Vecchio; J. Veitch; F. Vetrano; A. Vicere; S. Vyatchanin; P. Weels; B. Willke; W. Winkler; G. Woan; A. Woodcraft; K. Yamamoto

doi:10.1088/0264-9381/29/12/124013

Scientific objectives of Einstein Telescope

B. Sathyaprakash, M. Abernathy, F. Acernese, P. Ajith, B. Allen, P. Amaro-Seoane, N. Andersson, S. Aoudia, K. Arun, P. Astone, B. Krishnan, L. Barack, F. Barone, B. Barr, M. Barsuglia, M. Bassan, R. Bassiri, M. Beker, N. Beveridge, M. BizouardC. Bond, S. Bose, L. Bosi, S. Braccini, C. Bradaschia, M. Britzger, F. Brueckner, T. Bulik, H. J. Bulten, O. Burmeister, E. Calloni, P. Campsie, L. Carbone, G. Cella, E. Chalkley, E. Chassande-Mottin, S. Chelkowski, A. Chincarini, A. Di Cintio, J. Clark, E. Coccia, C. N. Colacino, J. Colas, A. Colla, A. Corsi, A. Cumming, L. Cunningham, E. Cuoco, S. Danilishin, K. Danzmann, E. Daw, R. De Salvo, W. Del Pozzo, T. Dent, R. De Rosa, L. Di Fiore, M. Di Paolo Emilio, A. Di Virgilio, A. Dietz, M. Doets, J. Dueck, M. Edwards, V. Fafone, S. Fairhurst, P. Falferi, M. Favata, V. Ferrari, F. Ferrini, F. Fidecaro, R. Flaminio, J. Franc, F. Frasconi, A. Freise, D. Friedrich, P. Fulda, J. Gair, M. Galimberti, G. Gemme, E. Genin, A. Gennai, A. Giazotto, K. Glampedakis, S. Gossan, R. Gouaty, C. Graef, W. Graham, M. Granata, H. Grote, G. Guidi, J. Hallam, G. Hammond, M. Hannam, J. Harms, K. Haughian, I. Hawke, D. Heinert, M. Hendry, I. Heng, E. Hennes, S. Hild, J. Hough, D. Huet, S. Husa, S. Huttner, B. Iyer, D. I. Jones, G. Jones, I. Kamaretsos, C. Kant Mishra, F. Kawazoe, F. Khalili, B. Kley, K. Kokeyama, K. Kokkotas, S. Kroker, R. Kumar, K. Kuroda, B. Lagrange, N. Lastzka, T. G.F. Li, M. Lorenzini, G. Losurdo, H. Lück, E. Majorana, V. Malvezzi, I. Mandel, V. Mandic, S. Marka, F. Marin, F. Marion, J. Marque, I. Martin, D. Mc Leod, D. McKechan, M. Mehmet, C. Michel, Y. Minenkov, N. Morgado, A. Morgia, S. Mosca, L. Moscatelli, B. Mours, H. Müller-Ebhardt, P. Murray, L. Naticchioni, R. Nawrodt, J. Nelson, R. O. Shaughnessy, C. D. Ott, C. Palomba, A. Paoli, G. Parguez, A. Pasqualetti, R. Passaquieti, D. Passuello, M. Perciballi, F. Piergiovanni, L. Pinard, M. Pitkin, W. Plastino, M. Plissi, R. Poggiani, P. Popolizio, E. Porter, M. Prato, G. Prodi, M. Punturo, P. Puppo, D. Rabeling, I. Racz, P. Rapagnani, V. Re, J. Read, T. Regimbau, H. Rehbein, S. Reid, F. Ricci, F. Richard, C. Robinson, A. Rocchi, R. Romano, S. Rowan, A. Rüdiger, A. Samblowski, L. Santamaría, B. Sassolas, R. Schilling, P. Schmidt, R. Schnabel, B. Schutz, C. Schwarz, J. Scott, P. Seidel, A. M. Sintes, K. Somiya, C. F. Sopuerta, B. Sorazu, F. Speirits, L. Storchi, K. Strain, S. Strigin, P. Sutton, S. Tarabrin, B. Taylor, A. Thürin, K. Tokmakov, M. Tonelli, H. Tournefier, R. Vaccarone, H. Vahlbruch, J. F.J. Van Den Brand, C. Van Den Broeck, S. Van Der Putten, M. Van Veggel, A. Vecchio, J. Veitch, F. Vetrano, A. Vicere, S. Vyatchanin, P. Weels, B. Willke, W. Winkler, G. Woan, A. Woodcraft, K. Yamamoto

Research output: Contribution to journal › Article › peer-review

428 Scopus citations

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 1Hz to 10kHz, 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.

Original language	English (US)
Article number	124013
Journal	Classical and Quantum Gravity
Volume	29
Issue number	12
DOIs	https://doi.org/10.1088/0264-9381/29/12/124013
State	Published - Jun 21 2012

All Science Journal Classification (ASJC) codes

Physics and Astronomy (miscellaneous)

Access to Document

10.1088/0264-9381/29/12/124013

Cite this

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., ... Yamamoto, K. (2012). Scientific objectives of Einstein Telescope. Classical and Quantum Gravity, 29(12), Article 124013. https://doi.org/10.1088/0264-9381/29/12/124013

@article{7ec32145fcca45298a17b20afc5b867b,

title = "Scientific objectives of Einstein Telescope",

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 1Hz to 10kHz, 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.",

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

year = "2012",

month = jun,

day = "21",

doi = "10.1088/0264-9381/29/12/124013",

language = "English (US)",

volume = "29",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing Ltd.",

number = "12",

}

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, Cintio, AD, 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, Pozzo, WD, Dent, T, De Rosa, R, Fiore, LD, Emilio, MDP, Virgilio, AD, 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, 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, Lück, H, Majorana, E, Malvezzi, V, Mandel, I, Mandic, V, Marka, S, Marin, F, Marion, F, Marque, J, Martin, I, Leod, DM, McKechan, D, Mehmet, M, Michel, C, Minenkov, Y, Morgado, N, Morgia, A, Mosca, S, Moscatelli, L, Mours, B, Müller-Ebhardt, H, Murray, P, Naticchioni, L, Nawrodt, R, Nelson, J, Shaughnessy, RO, Ott, CD, Palomba, C, Paoli, A, Parguez, G, Pasqualetti, A, Passaquieti, R, Passuello, D, Perciballi, M, Piergiovanni, F, Pinard, L, Pitkin, M, Plastino, W, Plissi, M, Poggiani, R, 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, Rüdiger, A, Samblowski, A, Santamaría, 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, Thürin, A, Tokmakov, K, Tonelli, M, 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, Weels, P, Willke, B, Winkler, W, Woan, G, Woodcraft, A & Yamamoto, K 2012, 'Scientific objectives of Einstein Telescope', Classical and Quantum Gravity, vol. 29, no. 12, 124013. https://doi.org/10.1088/0264-9381/29/12/124013

TY - JOUR

T1 - Scientific objectives of Einstein Telescope

AU - Sathyaprakash, B.

AU - Abernathy, M.

AU - Acernese, F.

AU - Ajith, P.

AU - Allen, B.

AU - Amaro-Seoane, P.

AU - Andersson, N.

AU - Aoudia, S.

AU - Arun, K.

AU - Astone, P.

AU - Krishnan, B.

AU - Barack, L.

AU - Barone, F.

AU - Barr, B.

AU - Barsuglia, M.

AU - Bassan, M.

AU - Bassiri, R.

AU - Beker, M.

AU - Beveridge, N.

AU - Bizouard, M.

AU - Bond, C.

AU - Bose, S.

AU - Bosi, L.

AU - Braccini, S.

AU - Bradaschia, C.

AU - Britzger, M.

AU - Brueckner, F.

AU - Bulik, T.

AU - Bulten, H. J.

AU - Burmeister, O.

AU - Calloni, E.

AU - Campsie, P.

AU - Carbone, L.

AU - Cella, G.

AU - Chalkley, E.

AU - Chassande-Mottin, E.

AU - Chelkowski, S.

AU - Chincarini, A.

AU - Cintio, A. Di

AU - Clark, J.

AU - Coccia, E.

AU - Colacino, C. N.

AU - Colas, J.

AU - Colla, A.

AU - Corsi, A.

AU - Cumming, A.

AU - Cunningham, L.

AU - Cuoco, E.

AU - Danilishin, S.

AU - Danzmann, K.

AU - Daw, E.

AU - De Salvo, R.

AU - Pozzo, W. Del

AU - Dent, T.

AU - De Rosa, R.

AU - Fiore, L. Di

AU - Emilio, M. Di Paolo

AU - Virgilio, A. Di

AU - Dietz, A.

AU - Doets, M.

AU - Dueck, J.

AU - Edwards, M.

AU - Fafone, V.

AU - Fairhurst, S.

AU - Falferi, P.

AU - Favata, M.

AU - Ferrari, V.

AU - Ferrini, F.

AU - Fidecaro, F.

AU - Flaminio, R.

AU - Franc, J.

AU - Frasconi, F.

AU - Freise, A.

AU - Friedrich, D.

AU - Fulda, P.

AU - Gair, J.

AU - Galimberti, M.

AU - Gemme, G.

AU - Genin, E.

AU - Gennai, A.

AU - Giazotto, A.

AU - Glampedakis, K.

AU - Gossan, S.

AU - Gouaty, R.

AU - Graef, C.

AU - Graham, W.

AU - Granata, M.

AU - Grote, H.

AU - Guidi, G.

AU - Hallam, J.

AU - Hammond, G.

AU - Hannam, M.

AU - Harms, J.

AU - Haughian, K.

AU - Hawke, I.

AU - Heinert, D.

AU - Hendry, M.

AU - Heng, I.

AU - Hennes, E.

AU - Hild, S.

AU - Hough, J.

AU - Huet, D.

AU - Husa, S.

AU - Huttner, S.

AU - Iyer, B.

AU - Jones, D. I.

AU - Jones, G.

AU - Kamaretsos, I.

AU - Mishra, C. Kant

AU - Kawazoe, F.

AU - Khalili, F.

AU - Kley, B.

AU - Kokeyama, K.

AU - Kokkotas, K.

AU - Kroker, S.

AU - Kumar, R.

AU - Kuroda, K.

AU - Lagrange, B.

AU - Lastzka, N.

AU - Li, T. G.F.

AU - Lorenzini, M.

AU - Losurdo, G.

AU - Lück, H.

AU - Majorana, E.

AU - Malvezzi, V.

AU - Mandel, I.

AU - Mandic, V.

AU - Marka, S.

AU - Marin, F.

AU - Marion, F.

AU - Marque, J.

AU - Martin, I.

AU - Leod, D. Mc

AU - McKechan, D.

AU - Mehmet, M.

AU - Michel, C.

AU - Minenkov, Y.

AU - Morgado, N.

AU - Morgia, A.

AU - Mosca, S.

AU - Moscatelli, L.

AU - Mours, B.

AU - Müller-Ebhardt, H.

AU - Murray, P.

AU - Naticchioni, L.

AU - Nawrodt, R.

AU - Nelson, J.

AU - Shaughnessy, R. O.

AU - Ott, C. D.

AU - Palomba, C.

AU - Paoli, A.

AU - Parguez, G.

AU - Pasqualetti, A.

AU - Passaquieti, R.

AU - Passuello, D.

AU - Perciballi, M.

AU - Piergiovanni, F.

AU - Pinard, L.

AU - Pitkin, M.

AU - Plastino, W.

AU - Plissi, M.

AU - Poggiani, R.

AU - Popolizio, P.

AU - Porter, E.

AU - Prato, M.

AU - Prodi, G.

AU - Punturo, M.

AU - Puppo, P.

AU - Rabeling, D.

AU - Racz, I.

AU - Rapagnani, P.

AU - Re, V.

AU - Read, J.

AU - Regimbau, T.

AU - Rehbein, H.

AU - Reid, S.

AU - Ricci, F.

AU - Richard, F.

AU - Robinson, C.

AU - Rocchi, A.

AU - Romano, R.

AU - Rowan, S.

AU - Rüdiger, A.

AU - Samblowski, A.

AU - Santamaría, L.

AU - Sassolas, B.

AU - Schilling, R.

AU - Schmidt, P.

AU - Schnabel, R.

AU - Schutz, B.

AU - Schwarz, C.

AU - Scott, J.

AU - Seidel, P.

AU - Sintes, A. M.

AU - Somiya, K.

AU - Sopuerta, C. F.

AU - Sorazu, B.

AU - Speirits, F.

AU - Storchi, L.

AU - Strain, K.

AU - Strigin, S.

AU - Sutton, P.

AU - Tarabrin, S.

AU - Taylor, B.

AU - Thürin, A.

AU - Tokmakov, K.

AU - Tonelli, M.

AU - Tournefier, H.

AU - Vaccarone, R.

AU - Vahlbruch, H.

AU - Van Den Brand, J. F.J.

AU - Van Den Broeck, C.

AU - Van Der Putten, S.

AU - Van Veggel, M.

AU - Vecchio, A.

AU - Veitch, J.

AU - Vetrano, F.

AU - Vicere, A.

AU - Vyatchanin, S.

AU - Weels, P.

AU - Willke, B.

AU - Winkler, W.

AU - Woan, G.

AU - Woodcraft, A.

AU - Yamamoto, K.

PY - 2012/6/21

Y1 - 2012/6/21

N2 - 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 1Hz to 10kHz, 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.

AB - 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 1Hz to 10kHz, 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.

UR - http://www.scopus.com/inward/record.url?scp=84862295488&partnerID=8YFLogxK

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U2 - 10.1088/0264-9381/29/12/124013

DO - 10.1088/0264-9381/29/12/124013

M3 - Article

AN - SCOPUS:84862295488

SN - 0264-9381

VL - 29

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 12

M1 - 124013

ER -

Scientific objectives of Einstein Telescope

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