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Technical Proposal: FASERnu

FASERnu is a proposed small and inexpensive emulsion detector designed to detect collider neutrinos for the first time and study their properties. FASERnu will be located directly in front of FASER, 480 m from the ATLAS interaction point along the beam collision axis in the unused service tunnel TI...

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Autores principales: Abreu, Henso, Andreini, Marco, Antel, Claire, Ariga, Akitaka, Ariga, Tomoko, Bertone, Caterina, Boyd, Jamie, Buckley, Andy, Cadoux, Franck, Casper, David W., Cerutti, Francesco, Chen, Xin, Coccaro, Andrea, Danzeca, Salvatore, Dougherty, Liam, Dozen, Candan, Denton, Peter B., Favre, Yannick, Fellers, Deion, Feng, Jonathan L., Ferrere, Didier, Gall, Jonathan, Galon, Iftah, Gibson, Stephen, Gonzalez-Sevilla, Sergio, Hsu, Shih-Chieh, Hu, Zhen, Iacobucci, Giuseppe, Jakobsen, Sune, Jansky, Roland, Kajomovitz, Enrique, Kling, Felix, Kose, Umut, Kuehn, Susanne, Lamont, Mike, Lefebvre, Helena, Levinson, Lorne, Li, Ke, McFayden, Josh, Meehan, Sam, Mladenov, Dimitar, Nakamura, Mitsuhiro, Nakano, Toshiyuki, Nessi, Marzio, Neuhaus, Friedemann, Osborne, John, Otono, Hidetoshi, Pelletier, Serge, Petersen, Brian, Pietropaolo, Francesco, Queitsch-Maitland, Michaela, Resnati, Filippo, Sabaté-Gilarte, Marta, Salfeld-Nebgen, Jakob, Sanchez Galan, Francisco, Diaz, Pablo Santos, Sato, Osamu, Scampoli, Paola, Schmieden, Kristof, Schott, Matthias, Schulz, Holger, Sfyrla, Anna, Shively, Savannah, Smolinsky, Jordan, Soffa, Aaron M., Takubo, Yosuke, Torrence, Eric, Trojanowski, Sebastian, Tufanli, Serhan, Zhang, Dengfeng, Zhang, Gang
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:http://cds.cern.ch/record/2702868
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author Abreu, Henso
Andreini, Marco
Antel, Claire
Ariga, Akitaka
Ariga, Tomoko
Bertone, Caterina
Boyd, Jamie
Buckley, Andy
Cadoux, Franck
Casper, David W.
Cerutti, Francesco
Chen, Xin
Coccaro, Andrea
Danzeca, Salvatore
Dougherty, Liam
Dozen, Candan
Denton, Peter B.
Favre, Yannick
Fellers, Deion
Feng, Jonathan L.
Ferrere, Didier
Gall, Jonathan
Galon, Iftah
Gibson, Stephen
Gonzalez-Sevilla, Sergio
Hsu, Shih-Chieh
Hu, Zhen
Iacobucci, Giuseppe
Jakobsen, Sune
Jansky, Roland
Kajomovitz, Enrique
Kling, Felix
Kose, Umut
Kuehn, Susanne
Lamont, Mike
Lefebvre, Helena
Levinson, Lorne
Li, Ke
McFayden, Josh
Meehan, Sam
Mladenov, Dimitar
Nakamura, Mitsuhiro
Nakano, Toshiyuki
Nessi, Marzio
Neuhaus, Friedemann
Osborne, John
Otono, Hidetoshi
Pelletier, Serge
Petersen, Brian
Pietropaolo, Francesco
Queitsch-Maitland, Michaela
Resnati, Filippo
Sabaté-Gilarte, Marta
Salfeld-Nebgen, Jakob
Sanchez Galan, Francisco
Diaz, Pablo Santos
Sato, Osamu
Scampoli, Paola
Schmieden, Kristof
Schott, Matthias
Schulz, Holger
Sfyrla, Anna
Shively, Savannah
Smolinsky, Jordan
Soffa, Aaron M.
Takubo, Yosuke
Torrence, Eric
Trojanowski, Sebastian
Tufanli, Serhan
Zhang, Dengfeng
Zhang, Gang
author_facet Abreu, Henso
Andreini, Marco
Antel, Claire
Ariga, Akitaka
Ariga, Tomoko
Bertone, Caterina
Boyd, Jamie
Buckley, Andy
Cadoux, Franck
Casper, David W.
Cerutti, Francesco
Chen, Xin
Coccaro, Andrea
Danzeca, Salvatore
Dougherty, Liam
Dozen, Candan
Denton, Peter B.
Favre, Yannick
Fellers, Deion
Feng, Jonathan L.
Ferrere, Didier
Gall, Jonathan
Galon, Iftah
Gibson, Stephen
Gonzalez-Sevilla, Sergio
Hsu, Shih-Chieh
Hu, Zhen
Iacobucci, Giuseppe
Jakobsen, Sune
Jansky, Roland
Kajomovitz, Enrique
Kling, Felix
Kose, Umut
Kuehn, Susanne
Lamont, Mike
Lefebvre, Helena
Levinson, Lorne
Li, Ke
McFayden, Josh
Meehan, Sam
Mladenov, Dimitar
Nakamura, Mitsuhiro
Nakano, Toshiyuki
Nessi, Marzio
Neuhaus, Friedemann
Osborne, John
Otono, Hidetoshi
Pelletier, Serge
Petersen, Brian
Pietropaolo, Francesco
Queitsch-Maitland, Michaela
Resnati, Filippo
Sabaté-Gilarte, Marta
Salfeld-Nebgen, Jakob
Sanchez Galan, Francisco
Diaz, Pablo Santos
Sato, Osamu
Scampoli, Paola
Schmieden, Kristof
Schott, Matthias
Schulz, Holger
Sfyrla, Anna
Shively, Savannah
Smolinsky, Jordan
Soffa, Aaron M.
Takubo, Yosuke
Torrence, Eric
Trojanowski, Sebastian
Tufanli, Serhan
Zhang, Dengfeng
Zhang, Gang
author_sort Abreu, Henso
collection CERN
description FASERnu is a proposed small and inexpensive emulsion detector designed to detect collider neutrinos for the first time and study their properties. FASERnu will be located directly in front of FASER, 480 m from the ATLAS interaction point along the beam collision axis in the unused service tunnel TI12. From 2021-23 during Run 3 of the 14 TeV LHC, roughly 1,300 $\nu_e$, 20,000 $\nu_{\mu}$, and 20 $\nu_{\tau}$ will interact in FASERnu with TeV-scale energies. With the ability to observe these interactions, reconstruct their energies, and distinguish flavors, FASERnu will probe the production, propagation, and interactions of neutrinos at the highest man-made energies ever recorded. The FASERnu detector will be composed of 1000 emulsion layers interleaved with tungsten plates. The total volume of the emulsion and tungsten is $25cm \times 25cm \times 1.35m$, and the tungsten target mass is 1.2 tonnes. From 2021-23, 7 sets of emulsion layers will be installed, with replacement roughly every $20-50~fb^{-1}$ in planned Technical Stops. In this document, we summarize FASERnu's physics goals and discuss the estimates of neutrino flux and interaction rates. We then describe the FASERnu detector in detail, including plans for assembly, transport, installation, and emulsion replacement, and procedures for emulsion readout and analyzing the data. We close with cost estimates for the detector components and infrastructure work and a timeline for the experiment.
id cern-2702868
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2019
record_format invenio
spelling cern-27028682023-04-22T03:38:22Zhttp://cds.cern.ch/record/2702868engAbreu, HensoAndreini, MarcoAntel, ClaireAriga, AkitakaAriga, TomokoBertone, CaterinaBoyd, JamieBuckley, AndyCadoux, FranckCasper, David W.Cerutti, FrancescoChen, XinCoccaro, AndreaDanzeca, SalvatoreDougherty, LiamDozen, CandanDenton, Peter B.Favre, YannickFellers, DeionFeng, Jonathan L.Ferrere, DidierGall, JonathanGalon, IftahGibson, StephenGonzalez-Sevilla, SergioHsu, Shih-ChiehHu, ZhenIacobucci, GiuseppeJakobsen, SuneJansky, RolandKajomovitz, EnriqueKling, FelixKose, UmutKuehn, SusanneLamont, MikeLefebvre, HelenaLevinson, LorneLi, KeMcFayden, JoshMeehan, SamMladenov, DimitarNakamura, MitsuhiroNakano, ToshiyukiNessi, MarzioNeuhaus, FriedemannOsborne, JohnOtono, HidetoshiPelletier, SergePetersen, BrianPietropaolo, FrancescoQueitsch-Maitland, MichaelaResnati, FilippoSabaté-Gilarte, MartaSalfeld-Nebgen, JakobSanchez Galan, FranciscoDiaz, Pablo SantosSato, OsamuScampoli, PaolaSchmieden, KristofSchott, MatthiasSchulz, HolgerSfyrla, AnnaShively, SavannahSmolinsky, JordanSoffa, Aaron M.Takubo, YosukeTorrence, EricTrojanowski, SebastianTufanli, SerhanZhang, DengfengZhang, GangTechnical Proposal: FASERnuDetectors and Experimental TechniquesParticle Physics - ExperimentParticle Physics - PhenomenologyFASERnu is a proposed small and inexpensive emulsion detector designed to detect collider neutrinos for the first time and study their properties. FASERnu will be located directly in front of FASER, 480 m from the ATLAS interaction point along the beam collision axis in the unused service tunnel TI12. From 2021-23 during Run 3 of the 14 TeV LHC, roughly 1,300 $\nu_e$, 20,000 $\nu_{\mu}$, and 20 $\nu_{\tau}$ will interact in FASERnu with TeV-scale energies. With the ability to observe these interactions, reconstruct their energies, and distinguish flavors, FASERnu will probe the production, propagation, and interactions of neutrinos at the highest man-made energies ever recorded. The FASERnu detector will be composed of 1000 emulsion layers interleaved with tungsten plates. The total volume of the emulsion and tungsten is $25cm \times 25cm \times 1.35m$, and the tungsten target mass is 1.2 tonnes. From 2021-23, 7 sets of emulsion layers will be installed, with replacement roughly every $20-50~fb^{-1}$ in planned Technical Stops. In this document, we summarize FASERnu's physics goals and discuss the estimates of neutrino flux and interaction rates. We then describe the FASERnu detector in detail, including plans for assembly, transport, installation, and emulsion replacement, and procedures for emulsion readout and analyzing the data. We close with cost estimates for the detector components and infrastructure work and a timeline for the experiment.FASERnu is a proposed small and inexpensive emulsion detector designed to detect collider neutrinos for the first time and study their properties. FASERnu will be located directly in front of FASER, 480 m from the ATLAS interaction point along the beam collision axis in the unused service tunnel TI12. From 2021-23 during Run 3 of the 14 TeV LHC, roughly 1,300 electron neutrinos, 20,000 muon neutrinos, and 20 tau neutrinos will interact in FASERnu with TeV-scale energies. With the ability to observe these interactions, reconstruct their energies, and distinguish flavors, FASERnu will probe the production, propagation, and interactions of neutrinos at the highest human-made energies ever recorded. The FASERnu detector will be composed of 1000 emulsion layers interleaved with tungsten plates. The total volume of the emulsion and tungsten is 25cm x 25cm x 1.35m, and the tungsten target mass is 1.2 tonnes. From 2021-23, 7 sets of emulsion layers will be installed, with replacement roughly every 20-50 1/fb in planned Technical Stops. In this document, we summarize FASERnu's physics goals and discuss the estimates of neutrino flux and interaction rates. We then describe the FASERnu detector in detail, including plans for assembly, transport, installation, and emulsion replacement, and procedures for emulsion readout and analyzing the data. We close with cost estimates for the detector components and infrastructure work and a timeline for the experiment.arXiv:2001.03073CERN-LHCC-2019-017LHCC-P-015UCI-TR-2019-25LHCC-P-015oai:cds.cern.ch:27028682019-11-27
spellingShingle Detectors and Experimental Techniques
Particle Physics - Experiment
Particle Physics - Phenomenology
Abreu, Henso
Andreini, Marco
Antel, Claire
Ariga, Akitaka
Ariga, Tomoko
Bertone, Caterina
Boyd, Jamie
Buckley, Andy
Cadoux, Franck
Casper, David W.
Cerutti, Francesco
Chen, Xin
Coccaro, Andrea
Danzeca, Salvatore
Dougherty, Liam
Dozen, Candan
Denton, Peter B.
Favre, Yannick
Fellers, Deion
Feng, Jonathan L.
Ferrere, Didier
Gall, Jonathan
Galon, Iftah
Gibson, Stephen
Gonzalez-Sevilla, Sergio
Hsu, Shih-Chieh
Hu, Zhen
Iacobucci, Giuseppe
Jakobsen, Sune
Jansky, Roland
Kajomovitz, Enrique
Kling, Felix
Kose, Umut
Kuehn, Susanne
Lamont, Mike
Lefebvre, Helena
Levinson, Lorne
Li, Ke
McFayden, Josh
Meehan, Sam
Mladenov, Dimitar
Nakamura, Mitsuhiro
Nakano, Toshiyuki
Nessi, Marzio
Neuhaus, Friedemann
Osborne, John
Otono, Hidetoshi
Pelletier, Serge
Petersen, Brian
Pietropaolo, Francesco
Queitsch-Maitland, Michaela
Resnati, Filippo
Sabaté-Gilarte, Marta
Salfeld-Nebgen, Jakob
Sanchez Galan, Francisco
Diaz, Pablo Santos
Sato, Osamu
Scampoli, Paola
Schmieden, Kristof
Schott, Matthias
Schulz, Holger
Sfyrla, Anna
Shively, Savannah
Smolinsky, Jordan
Soffa, Aaron M.
Takubo, Yosuke
Torrence, Eric
Trojanowski, Sebastian
Tufanli, Serhan
Zhang, Dengfeng
Zhang, Gang
Technical Proposal: FASERnu
title Technical Proposal: FASERnu
title_full Technical Proposal: FASERnu
title_fullStr Technical Proposal: FASERnu
title_full_unstemmed Technical Proposal: FASERnu
title_short Technical Proposal: FASERnu
title_sort technical proposal: fasernu
topic Detectors and Experimental Techniques
Particle Physics - Experiment
Particle Physics - Phenomenology
url http://cds.cern.ch/record/2702868
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