A
A. Gennai
Researcher at University of Birmingham
Publications - 5
Citations - 2700
A. Gennai is an academic researcher from University of Birmingham. The author has contributed to research in topics: Einstein Telescope & Gravitational-wave astronomy. The author has an hindex of 5, co-authored 5 publications receiving 1682 citations.
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Journal ArticleDOI
The Einstein Telescope: a third-generation gravitational wave observatory
M. Punturo,M. R. Abernathy,Fausto Acernese,Benjamin William Allen,Nils Andersson,K. G. Arun,Fabrizio Barone,B. Barr,M. Barsuglia,M. G. Beker,N. Beveridge,S. Birindelli,Suvadeep Bose,L. Bosi,S. Braccini,C. Bradaschia,Tomasz Bulik,Enrico Calloni,G. Cella,E. Chassande Mottin,Simon Chelkowski,Andrea Chincarini,John A. Clark,E. Coccia,C. N. Colacino,J. Colas,A. Cumming,L. Cunningham,E. Cuoco,S. L. Danilishin,Karsten Danzmann,G. De Luca,R. De Salvo,T. Dent,R. De Rosa,L. Di Fiore,A. Di Virgilio,M. Doets,V. Fafone,Paolo Falferi,R. Flaminio,J. Franc,F. Frasconi,Andreas Freise,Paul Fulda,Jonathan R. Gair,G. Gemme,A. Gennai,A. Giazotto,Kostas Glampedakis,M. Granata,Hartmut Grote,G. M. Guidi,G. D. Hammond,Mark Hannam,Jan Harms,D. Heinert,Martin Hendry,Ik Siong Heng,Eric Hennes,Stefan Hild,J. H. Hough,Sascha Husa,S. H. Huttner,Gareth Jones,F. Y. Khalili,Keiko Kokeyama,Kostas D. Kokkotas,Badri Krishnan,M. Lorenzini,Harald Lück,Ettore Majorana,Ilya Mandel,Vuk Mandic,I. W. Martin,C. Michel,Y. Minenkov,N. Morgado,Simona Mosca,B. Mours,H. Müller–Ebhardt,P. G. Murray,Ronny Nawrodt,John Nelson,Richard O'Shaughnessy,Christian D. Ott,C. Palomba,A. Paoli,G. Parguez,A. Pasqualetti,R. Passaquieti,D. Passuello,L. Pinard,Rosa Poggiani,P. Popolizio,Mirko Prato,P. Puppo,D. S. Rabeling,P. Rapagnani,Jocelyn Read,Tania Regimbau,H. Rehbein,Stuart Reid,Luciano Rezzolla,F. Ricci,F. Richard,A. Rocchi,Sheila Rowan,Albrecht Rüdiger,Benoit Sassolas,Bangalore Suryanarayana Sathyaprakash,Roman Schnabel,C. Schwarz,Paul Seidel,Alicia M. Sintes,Kentaro Somiya,Fiona C. Speirits,Kenneth A. Strain,S. E. Strigin,P. J. Sutton,S. P. Tarabrin,Andre Thüring,J. F. J. van den Brand,C. van Leewen,M. van Veggel,C. Van Den Broeck,Alberto Vecchio,John Veitch,F. Vetrano,A. Viceré,Sergey P. Vyatchanin,Benno Willke,Graham Woan,P. Wolfango,Kazuhiro Yamamoto +134 more
TL;DR: The third-generation ground-based observatory Einstein Telescope (ET) project as discussed by the authors is currently in its design study phase, and it can be seen as the first step in this direction.
Journal ArticleDOI
Sensitivity studies for third-generation gravitational wave observatories
Stefan Hild,M. R. Abernathy,Fausto Acernese,Pau Amaro-Seoane,Nils Andersson,K. G. Arun,Fabrizio Barone,B. Barr,M. Barsuglia,Mark Beker,N. Beveridge,S. Birindelli,Suvadeep Bose,L. Bosi,S. Braccini,C. Bradaschia,Tomasz Bulik,Enrico Calloni,Giancarlo Cella,E. Chassande Mottin,S. Chelkowski,Andrea Chincarini,James S. Clark,E. Coccia,C. Colacino,J. Colas,A. Cumming,L. Cunningham,E. Cuoco,S. L. Danilishin,Karsten Danzmann,R. De Salvo,T. Dent,R. De Rosa,L. Di Fiore,A. Di Virgilio,M. Doets,V. Fafone,Paolo Falferi,R. Flaminio,J. Franc,F. Frasconi,Andreas Freise,D. Friedrich,Paul Fulda,Jonathan R. Gair,Gianluca Gemme,E. Genin,A. Gennai,A. Giazotto,Kostas Glampedakis,Christian Gräf,M. Granata,Hartmut Grote,G. M. Guidi,A. Gurkovsky,G. D. Hammond,Mark Hannam,Jan Harms,D. Heinert,Martin Hendry,Ik Siong Heng,E. Hennes,J. H. Hough,Sascha Husa,S. H. Huttner,G. T. Jones,F. Y. Khalili,Keiko Kokeyama,Kostas D. Kokkotas,Badri Krishnan,Tjonnie G. F. Li,M. Lorenzini,H. Lück,Ettore Majorana,Ilya Mandel,Vuk Mandic,M. Mantovani,I. W. Martin,Christine Michel,Y. Minenkov,N. Morgado,S. Mosca,B. Mours,Helge Müller-Ebhardt,P. G. Murray,Ronny Nawrodt,Ronny Nawrodt,John Nelson,Richard O'Shaughnessy,Christian D. Ott,C. Palomba,Angela Delli Paoli,G. Parguez,A. Pasqualetti,R. Passaquieti,R. Passaquieti,D. Passuello,Laurent Pinard,Wolfango Plastino,Rosa Poggiani,Rosa Poggiani,P. Popolizio,Mirko Prato,M. Punturo,P. Puppo,D. S. Rabeling,P. Rapagnani,Jocelyn Read,Tania Regimbau,H. Rehbein,S. Reid,F. Ricci,F. Richard,A. Rocchi,Sheila Rowan,A. Rüdiger,Lucía Santamaría,Benoit Sassolas,Bangalore Suryanarayana Sathyaprakash,Roman Schnabel,C. Schwarz,Paul Seidel,Alicia M. Sintes,Kentaro Somiya,Fiona C. Speirits,Kenneth A. Strain,S. E. Strigin,P. J. Sutton,S. P. Tarabrin,Andre Thüring,J. F. J. van den Brand,M. van Veggel,C. Van Den Broeck,Alberto Vecchio,John Veitch,F. Vetrano,A. Viceré,S. P. Vyatchanin,Benno Willke,Graham Woan,Kazuhiro Yamamoto +141 more
TL;DR: In this article, a special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates, including the most relevant fundamental noise contributions.
Journal ArticleDOI
The third generation of gravitational wave observatories and their science reach
M. Punturo,M. R. Abernathy,Fausto Acernese,Benjamin William Allen,Nils Andersson,K. G. Arun,Fabrizio Barone,B. Barr,M. Barsuglia,M. G. Beker,N. Beveridge,S. Birindelli,Suvadeep Bose,L. Bosi,S. Braccini,C. Bradaschia,Tomasz Bulik,Enrico Calloni,G. Cella,E. Chassande Mottin,Simon Chelkowski,Andrea Chincarini,John A. Clark,E. Coccia,C. N. Colacino,J. Colas,A. Cumming,L. Cunningham,E. Cuoco,S. L. Danilishin,Karsten Danzmann,G. De Luca,R. De Salvo,T. Dent,R. T. DeRosa,L. Di Fiore,A. Di Virgilio,M. Doets,V. Fafone,Paolo Falferi,R. Flaminio,J. Franc,F. Frasconi,Andreas Freise,Paul Fulda,Jonathan R. Gair,G. Gemme,A. Gennai,A. Giazotto,Kostas Glampedakis,M. Granata,Hartmut Grote,G. M. Guidi,G. D. Hammond,Mark Hannam,Jan Harms,D. Heinert,Martin Hendry,Ik Siong Heng,Eric Hennes,Stefan Hild,J. H. Hough,Sascha Husa,S. H. Huttner,Gareth Jones,F. Y. Khalili,Keiko Kokeyama,Kostas D. Kokkotas,Badri Krishnan,M. Lorenzini,Harald Lück,Ettore Majorana,Ilya Mandel,Vuk Mandic,I. W. Martin,C. Michel,Y. Minenkov,N. Morgado,Simona Mosca,B. Mours,Helge Müller-Ebhardt,P. G. Murray,Ronny Nawrodt,John Nelson,Richard O'Shaughnessy,Christian D. Ott,C. Palomba,A. Paoli,G. Parguez,A. Pasqualetti,R. Passaquieti,D. Passuello,L. Pinard,Rosa Poggiani,P. Popolizio,Mirko Prato,P. Puppo,D. S. Rabeling,P. Rapagnani,Jocelyn Read,Tania Regimbau,H. Rehbein,Stuart Reid,Luciano Rezzolla,F. Ricci,F. Richard,A. Rocchi,Sheila Rowan,Albrecht Rüdiger,Benoit Sassolas,Bangalore Suryanarayana Sathyaprakash,Roman Schnabel,C. Schwarz,Paul Seidel,Alicia M. Sintes,Kentaro Somiya,Fiona C. Speirits,Kenneth A. Strain,S. E. Strigin,P. J. Sutton,S. P. Tarabrin,J. F. J. van den Brand,C. van Leewen,M. van Veggel,C. Van Den Broeck,Alberto Vecchio,John Veitch,F. Vetrano,A. Viceré,Sergey P. Vyatchanin,Benno Willke,Graham Woan,P. Wolfango,Kazuhiro Yamamoto +133 more
TL;DR: The status of the project Einstein Telescope (ET), a design study of a third-generation gravitational wave observatory, is reported in this paper, where an overview of the possible science reaches and the technological progress needed to realize a third generation observatory are discussed.
Journal ArticleDOI
Sensitivity Studies for Third-Generation Gravitational Wave Observatories
Stefan Hild,M. R. Abernathy,Fausto Acernese,Pau Amaro-Seoane,Nils Andersson,K. G. Arun,Fabrizio Barone,B. Barr,M. Barsuglia,Mark Beker,N. Beveridge,S. Birindelli,Suvadeep Bose,L. Bosi,S. Braccini,C. Bradaschia,Tomasz Bulik,Enrico Calloni,Giancarlo Cella,E. Chassande Mottin,S. Chelkowski,Andrea Chincarini,James S. Clark,E. Coccia,C. Colacino,J. Colas,A. Cumming,L. Cunningham,E. Cuoco,S. L. Danilishin,Karsten Danzmann,R. De Salvo,T. Dent,R. De Rosa,L. Di Fiore,A. Di Virgilio,M. Doets,V. Fafone,Paolo Falferi,R. Flaminio,J. Franc,F. Frasconi,Andreas Freise,D. Friedrich,Paul Fulda,Jonathan R. Gair,Gianluca Gemme,E. Genin,A. Gennai,A. Giazotto,Kostas Glampedakis,Christian Gräf,M. Granata,Hartmut Grote,G. M. Guidi,A. Gurkovsky,G. D. Hammond,Mark Hannam,Jan Harms,D. Heinert,Martin Hendry,Ik Siong Heng,E. Hennes,J. H. Hough,Sascha Husa,S. H. Huttner,G. T. Jones,F. Y. Khalili,Keiko Kokeyama,Kostas D. Kokkotas,Badri Krishnan,Tjonnie G. F. Li,M. Lorenzini,H. Lück,Ettore Majorana,Ilya Mandel,Vuk Mandic,M. Mantovani,I. W. Martin,Christine Michel,Y. Minenkov,N. Morgado,S. Mosca,B. Mours,Helge Müller-Ebhardt,P. G. Murray,Ronny Nawrodt,Ronny Nawrodt,John Nelson,Richard O'Shaughnessy,Christian D. Ott,C. Palomba,Angela Delli Paoli,G. Parguez,A. Pasqualetti,R. Passaquieti,R. Passaquieti,D. Passuello,Laurent Pinard,Wolfango Plastino,Rosa Poggiani,Rosa Poggiani,P. Popolizio,Mirko Prato,M. Punturo,P. Puppo,D. S. Rabeling,P. Rapagnani,Jocelyn Read,Tania Regimbau,H. Rehbein,S. Reid,F. Ricci,F. Richard,A. Rocchi,Sheila Rowan,A. Rüdiger,Lucía Santamaría,Benoit Sassolas,Bangalore Suryanarayana Sathyaprakash,Roman Schnabel,C. Schwarz,Paul Seidel,Alicia M. Sintes,Kentaro Somiya,Fiona C. Speirits,Kenneth A. Strain,S. E. Strigin,P. J. Sutton,S. P. Tarabrin,Andre Thüring,J. F. J. van den Brand,M. van Veggel,C. Van Den Broeck,Alberto Vecchio,John Veitch,F. Vetrano,A. Viceré,S. P. Vyatchanin,Benno Willke,Graham Woan,Kazuhiro Yamamoto +141 more
TL;DR: In this article, a special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates, including the most relevant fundamental noise contributions.
Scientific potential of Einstein Telescope
Bangalore Suryanarayana Sathyaprakash,M. R. Abernathy,Fausto Acernese,P. Amaro-Seoane,P. Amaro-Seoane,Nils Andersson,K. Arun,Fabrizio Barone,B. Barr,M. Barsuglia,M. G. Beker,N. Beveridge,S. Birindelli,Suvadeep Bose,L. Bosi,S. Braccini,C. Bradaschia,Tomasz Bulik,Enrico Calloni,G. Cella,E. Chassande-Mottin,Simon Chelkowski,Andrea Chincarini,John A. Clark,E. Coccia,C. N. Colacino,J. Colas,A. Cumming,Liam Cunningham,E. Cuoco,S. L. Danilishin,Karsten Danzmann,R. De Salvo,T. Dent,R. De Rosa,L. Di Fiore,A. Di Virgilio,M. Doets,V. Fafone,Paolo Falferi,R. Flaminio,J. Franc,F. Frasconi,Andreas Freise,D. Friedrich,Paul Fulda,Jonathan R. Gair,G. Gemme,E. Genin,A. Gennai,A. Giazotto,Kostas Glampedakis,C. Gräf,M. Granata,Hartmut Grote,G. M. Guidi,A. Gurkovsky,G. D. Hammond,Mark Hannam,Jan Harms,D. Heinert,Martin Hendry,Ik Siong Heng,Eric Hennes,Stefan Hild,J. H. Hough,Sascha Husa,S. H. Huttner,Gareth Jones,F. Y. Khalili,Keiko Kokeyama,Kostas D. Kokkotas,Badri Krishnan,Tenglin Li,M. Lorenzini,Harald Lück,Ettore Majorana,Ilya Mandel,Ilya Mandel,Vuk Mandic,M. Mantovani,I. W. Martin,C. Michel,Y. Minenkov,N. Morgado,S. Mosca,B. Mours,H. Müller-Ebhardt,P. G. Murray,Ronny Nawrodt,Ronny Nawrodt,John Nelson,Richard O'Shaughnessy,Christian D. Ott,C. Palomba,A. Paoli,G. Parguez,A. Pasqualetti,R. Passaquieti,D. Passuello,L. Pinard,Wolfango Plastino,Rosa Poggiani,P. Popolizio,Mirko Prato,M. Punturo,P. Puppo,D. S. Rabeling,István Rácz,P. Rapagnani,Jocelyn Read,T. Regimbau,H. Rehbein,Stuart Reid,Luciano Rezzolla,F. Ricci,F. Richard,A. Rocchi,Sheila Rowan,A. Rüdiger,Lucía Santamaría,B. Sassolas,Roman Schnabel,C. Schwarz,Paul Seidel,A. M. Sintes,Kentaro Somiya,F. C. Speirits,K. Speirits,K. A. Strain,S. E. Strigin,Patrick J. Sutton,S. P. Tarabrin,A. Thüring,J. F. J. van den Brand,M. van Veggel,C. Van Den Broeck,Alberto Vecchio,John Veitch,F. Vetrano,A. Viceré,Sergey P. Vyatchanin,B. Vyatchanin,Graham Woan,Kazuhiro Yamamoto +144 more
TL;DR: The advanced interferometer network will herald a new era in observational astronomy as mentioned in this paper, and 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.