SuperB Technical Design Report
In this Technical Design Report (TDR) we describe the SuperB detector that was to be installed on the SuperB e+e- high luminosity collider. The SuperB asymmetric collider, which was to be constructed on the Tor Vergata campus near the INFN Frascati National Laboratory, was designed to operate both a...
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| creator | Sapor, M Diacono, D Gargano, F Loddo, F Manzari, V Mazziotta, M. N Nappi, E Sgura, I Zalieckas, J Boldini, M Di Sipio, R Gabrielli, A Montanari, A Tosi, N Travaglini, R Mattison, T. S Barnyakov, M. Yu Levichev, E. B Cheng, C. H Flood, K Ongmongkolkul, P Zhu, R. Y Randazzo, N Zheng, Y Campos, P Pushpawela, B Polania, G. A. Calderon Szybinski, B Harezlak, D Radecki, M Andreotti, M Baldini, W Carassiti, V Luppi, E Manzali, M Munerato, M Santoro, V Tomassetti, L Peruzzi, I Rama, M Fabbricatore, P Michalowski, J Zawiejski, L Zdybal, M Ustynov, A Brossard, J Burmistrov, L Chaumat, V Stocchi, A Variola, A Grancagnolo, F Cenci, R Roberts, D Twedt, E. W Cheaib, R Lindemann, D Citterio, M Fiorini, C Liberali, V Berra, A Lietti, D Maino, M Pessina, G Simard, M Giordano, R Russo, G Sciacca, C Bellato, M Crescente, A Michelotto, M Montecassiano, F Morandin, M Manazza, A Lubrano, P Papi, A Forti, F Giorgi, M Lilli, L Paoloni, E Téllez, A. Fernández Lunadei, R Zullo, A Di Ciaccio, A Spiriti, E Millan-Almaraz, J. R Aston, D Jackson, P. D Leith, D. W. G. S Sullivan, M Wienands, U Wisniewski, W Bezshyyko, O Soffer, A Bianchi, F Marcello, S Auriemma, G Vidal, F. Martinez de Cos, J. Mazorra Dejong, S Franta, J |
| description | In this Technical Design Report (TDR) we describe the SuperB detector that
was to be installed on the SuperB e+e- high luminosity collider. The SuperB
asymmetric collider, which was to be constructed on the Tor Vergata campus near
the INFN Frascati National Laboratory, was designed to operate both at the
Upsilon(4S) center-of-mass energy with a luminosity of 10^{36} cm^{-2}s^{-1}
and at the tau/charm production threshold with a luminosity of 10^{35}
cm^{-2}s^{-1}. This high luminosity, producing a data sample about a factor 100
larger than present B Factories, would allow investigation of new physics
effects in rare decays, CP Violation and Lepton Flavour Violation. This
document details the detector design presented in the Conceptual Design Report
(CDR) in 2007. The R&D and engineering studies performed to arrive at the full
detector design are described, and an updated cost estimate is presented.
A combination of a more realistic cost estimates and the unavailability of
funds due of the global economic climate led to a formal cancelation of the
project on Nov 27, 2012. |
| doi_str_mv | 10.48550/arxiv.1306.5655 |
| format | Article |
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was to be installed on the SuperB e+e- high luminosity collider. The SuperB
asymmetric collider, which was to be constructed on the Tor Vergata campus near
the INFN Frascati National Laboratory, was designed to operate both at the
Upsilon(4S) center-of-mass energy with a luminosity of 10^{36} cm^{-2}s^{-1}
and at the tau/charm production threshold with a luminosity of 10^{35}
cm^{-2}s^{-1}. This high luminosity, producing a data sample about a factor 100
larger than present B Factories, would allow investigation of new physics
effects in rare decays, CP Violation and Lepton Flavour Violation. This
document details the detector design presented in the Conceptual Design Report
(CDR) in 2007. The R&D and engineering studies performed to arrive at the full
detector design are described, and an updated cost estimate is presented.
A combination of a more realistic cost estimates and the unavailability of
funds due of the global economic climate led to a formal cancelation of the
project on Nov 27, 2012.</description><identifier>DOI: 10.48550/arxiv.1306.5655</identifier><language>eng</language><subject>Physics - High Energy Physics - Experiment ; Physics - Instrumentation and Detectors</subject><creationdate>2013-06</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/1306.5655$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.1306.5655$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Sapor, M</creatorcontrib><creatorcontrib>Diacono, D</creatorcontrib><creatorcontrib>Gargano, F</creatorcontrib><creatorcontrib>Loddo, F</creatorcontrib><creatorcontrib>Manzari, V</creatorcontrib><creatorcontrib>Mazziotta, M. 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Mazorra</creatorcontrib><creatorcontrib>Dejong, S</creatorcontrib><creatorcontrib>Franta, J</creatorcontrib><title>SuperB Technical Design Report</title><description>In this Technical Design Report (TDR) we describe the SuperB detector that
was to be installed on the SuperB e+e- high luminosity collider. The SuperB
asymmetric collider, which was to be constructed on the Tor Vergata campus near
the INFN Frascati National Laboratory, was designed to operate both at the
Upsilon(4S) center-of-mass energy with a luminosity of 10^{36} cm^{-2}s^{-1}
and at the tau/charm production threshold with a luminosity of 10^{35}
cm^{-2}s^{-1}. This high luminosity, producing a data sample about a factor 100
larger than present B Factories, would allow investigation of new physics
effects in rare decays, CP Violation and Lepton Flavour Violation. This
document details the detector design presented in the Conceptual Design Report
(CDR) in 2007. The R&D and engineering studies performed to arrive at the full
detector design are described, and an updated cost estimate is presented.
A combination of a more realistic cost estimates and the unavailability of
funds due of the global economic climate led to a formal cancelation of the
project on Nov 27, 2012.</description><subject>Physics - High Energy Physics - Experiment</subject><subject>Physics - Instrumentation and Detectors</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzjsPgjAYheEuDgbdnQh_AOyF0jIqXhMSE2UnH6VVEkRS1Oi_F9TlnO3Ng9CM4CCUnOM52Ff1DAjDUcAjzsfIPT1abZdeptWlqRTU3kp31bnxjrq92fsEjQzUnZ7-30HZZp0lOz89bPfJIvWhr_hGaMGh31iWRkhjdCSN4gpTSoAwkESwgsZKQckJxSEFWkgW61AxyUoRMwe5v-zXl7e2uoJ954MzH5zsA6LlNpY</recordid><startdate>20130624</startdate><enddate>20130624</enddate><creator>Sapor, M</creator><creator>Diacono, D</creator><creator>Gargano, F</creator><creator>Loddo, F</creator><creator>Manzari, V</creator><creator>Mazziotta, M. N</creator><creator>Nappi, E</creator><creator>Sgura, I</creator><creator>Zalieckas, J</creator><creator>Boldini, M</creator><creator>Di Sipio, R</creator><creator>Gabrielli, A</creator><creator>Montanari, A</creator><creator>Tosi, N</creator><creator>Travaglini, R</creator><creator>Mattison, T. S</creator><creator>Barnyakov, M. Yu</creator><creator>Levichev, E. B</creator><creator>Cheng, C. H</creator><creator>Flood, K</creator><creator>Ongmongkolkul, P</creator><creator>Zhu, R. Y</creator><creator>Randazzo, N</creator><creator>Zheng, Y</creator><creator>Campos, P</creator><creator>Pushpawela, B</creator><creator>Polania, G. A. 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W</creatorcontrib><creatorcontrib>Cheaib, R</creatorcontrib><creatorcontrib>Lindemann, D</creatorcontrib><creatorcontrib>Citterio, M</creatorcontrib><creatorcontrib>Fiorini, C</creatorcontrib><creatorcontrib>Liberali, V</creatorcontrib><creatorcontrib>Berra, A</creatorcontrib><creatorcontrib>Lietti, D</creatorcontrib><creatorcontrib>Maino, M</creatorcontrib><creatorcontrib>Pessina, G</creatorcontrib><creatorcontrib>Simard, M</creatorcontrib><creatorcontrib>Giordano, R</creatorcontrib><creatorcontrib>Russo, G</creatorcontrib><creatorcontrib>Sciacca, C</creatorcontrib><creatorcontrib>Bellato, M</creatorcontrib><creatorcontrib>Crescente, A</creatorcontrib><creatorcontrib>Michelotto, M</creatorcontrib><creatorcontrib>Montecassiano, F</creatorcontrib><creatorcontrib>Morandin, M</creatorcontrib><creatorcontrib>Manazza, A</creatorcontrib><creatorcontrib>Lubrano, P</creatorcontrib><creatorcontrib>Papi, A</creatorcontrib><creatorcontrib>Forti, F</creatorcontrib><creatorcontrib>Giorgi, M</creatorcontrib><creatorcontrib>Lilli, L</creatorcontrib><creatorcontrib>Paoloni, E</creatorcontrib><creatorcontrib>Téllez, A. Fernández</creatorcontrib><creatorcontrib>Lunadei, R</creatorcontrib><creatorcontrib>Zullo, A</creatorcontrib><creatorcontrib>Di Ciaccio, A</creatorcontrib><creatorcontrib>Spiriti, E</creatorcontrib><creatorcontrib>Millan-Almaraz, J. R</creatorcontrib><creatorcontrib>Aston, D</creatorcontrib><creatorcontrib>Jackson, P. D</creatorcontrib><creatorcontrib>Leith, D. W. G. S</creatorcontrib><creatorcontrib>Sullivan, M</creatorcontrib><creatorcontrib>Wienands, U</creatorcontrib><creatorcontrib>Wisniewski, W</creatorcontrib><creatorcontrib>Bezshyyko, O</creatorcontrib><creatorcontrib>Soffer, A</creatorcontrib><creatorcontrib>Bianchi, F</creatorcontrib><creatorcontrib>Marcello, S</creatorcontrib><creatorcontrib>Auriemma, G</creatorcontrib><creatorcontrib>Vidal, F. Martinez</creatorcontrib><creatorcontrib>de Cos, J. Mazorra</creatorcontrib><creatorcontrib>Dejong, S</creatorcontrib><creatorcontrib>Franta, J</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Sapor, M</au><au>Diacono, D</au><au>Gargano, F</au><au>Loddo, F</au><au>Manzari, V</au><au>Mazziotta, M. N</au><au>Nappi, E</au><au>Sgura, I</au><au>Zalieckas, J</au><au>Boldini, M</au><au>Di Sipio, R</au><au>Gabrielli, A</au><au>Montanari, A</au><au>Tosi, N</au><au>Travaglini, R</au><au>Mattison, T. S</au><au>Barnyakov, M. Yu</au><au>Levichev, E. B</au><au>Cheng, C. H</au><au>Flood, K</au><au>Ongmongkolkul, P</au><au>Zhu, R. Y</au><au>Randazzo, N</au><au>Zheng, Y</au><au>Campos, P</au><au>Pushpawela, B</au><au>Polania, G. A. Calderon</au><au>Szybinski, B</au><au>Harezlak, D</au><au>Radecki, M</au><au>Andreotti, M</au><au>Baldini, W</au><au>Carassiti, V</au><au>Luppi, E</au><au>Manzali, M</au><au>Munerato, M</au><au>Santoro, V</au><au>Tomassetti, L</au><au>Peruzzi, I</au><au>Rama, M</au><au>Fabbricatore, P</au><au>Michalowski, J</au><au>Zawiejski, L</au><au>Zdybal, M</au><au>Ustynov, A</au><au>Brossard, J</au><au>Burmistrov, L</au><au>Chaumat, V</au><au>Stocchi, A</au><au>Variola, A</au><au>Grancagnolo, F</au><au>Cenci, R</au><au>Roberts, D</au><au>Twedt, E. W</au><au>Cheaib, R</au><au>Lindemann, D</au><au>Citterio, M</au><au>Fiorini, C</au><au>Liberali, V</au><au>Berra, A</au><au>Lietti, D</au><au>Maino, M</au><au>Pessina, G</au><au>Simard, M</au><au>Giordano, R</au><au>Russo, G</au><au>Sciacca, C</au><au>Bellato, M</au><au>Crescente, A</au><au>Michelotto, M</au><au>Montecassiano, F</au><au>Morandin, M</au><au>Manazza, A</au><au>Lubrano, P</au><au>Papi, A</au><au>Forti, F</au><au>Giorgi, M</au><au>Lilli, L</au><au>Paoloni, E</au><au>Téllez, A. Fernández</au><au>Lunadei, R</au><au>Zullo, A</au><au>Di Ciaccio, A</au><au>Spiriti, E</au><au>Millan-Almaraz, J. R</au><au>Aston, D</au><au>Jackson, P. D</au><au>Leith, D. W. G. S</au><au>Sullivan, M</au><au>Wienands, U</au><au>Wisniewski, W</au><au>Bezshyyko, O</au><au>Soffer, A</au><au>Bianchi, F</au><au>Marcello, S</au><au>Auriemma, G</au><au>Vidal, F. Martinez</au><au>de Cos, J. Mazorra</au><au>Dejong, S</au><au>Franta, J</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>SuperB Technical Design Report</atitle><date>2013-06-24</date><risdate>2013</risdate><abstract>In this Technical Design Report (TDR) we describe the SuperB detector that
was to be installed on the SuperB e+e- high luminosity collider. The SuperB
asymmetric collider, which was to be constructed on the Tor Vergata campus near
the INFN Frascati National Laboratory, was designed to operate both at the
Upsilon(4S) center-of-mass energy with a luminosity of 10^{36} cm^{-2}s^{-1}
and at the tau/charm production threshold with a luminosity of 10^{35}
cm^{-2}s^{-1}. This high luminosity, producing a data sample about a factor 100
larger than present B Factories, would allow investigation of new physics
effects in rare decays, CP Violation and Lepton Flavour Violation. This
document details the detector design presented in the Conceptual Design Report
(CDR) in 2007. The R&D and engineering studies performed to arrive at the full
detector design are described, and an updated cost estimate is presented.
A combination of a more realistic cost estimates and the unavailability of
funds due of the global economic climate led to a formal cancelation of the
project on Nov 27, 2012.</abstract><doi>10.48550/arxiv.1306.5655</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.1306.5655 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_1306_5655 |
| source | arXiv.org |
| subjects | Physics - High Energy Physics - Experiment Physics - Instrumentation and Detectors |
| title | SuperB Technical Design Report |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-19T16%3A49%3A14IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=SuperB%20Technical%20Design%20Report&rft.au=Sapor,%20M&rft.date=2013-06-24&rft_id=info:doi/10.48550/arxiv.1306.5655&rft_dat=%3Carxiv_GOX%3E1306_5655%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |