| Home > Publications database > Neutrino Detection without Neutrino Detectors:Discovering Collider Neutrinos at FASER with Electronic Signals Only > print |
| 001 | 479596 | ||
| 005 | 20250715175806.0 | ||
| 024 | 7 | _ | |a 10.1103/PhysRevD.106.052011 |2 doi |
| 024 | 7 | _ | |a Arakawa:2022rmp |2 INSPIRETeX |
| 024 | 7 | _ | |a inspire:2098400 |2 inspire |
| 024 | 7 | _ | |a 0556-2821 |2 ISSN |
| 024 | 7 | _ | |a 1089-4918 |2 ISSN |
| 024 | 7 | _ | |a 1538-4500 |2 ISSN |
| 024 | 7 | _ | |a 1550-2368 |2 ISSN |
| 024 | 7 | _ | |a 1550-7998 |2 ISSN |
| 024 | 7 | _ | |a 2470-0010 |2 ISSN |
| 024 | 7 | _ | |a 2470-0029 |2 ISSN |
| 024 | 7 | _ | |a arXiv:2206.09932 |2 arXiv |
| 024 | 7 | _ | |a 10.3204/PUBDB-2022-03159 |2 datacite_doi |
| 024 | 7 | _ | |a altmetric:130030563 |2 altmetric |
| 024 | 7 | _ | |a WOS:000894544800002 |2 WOS |
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| 037 | _ | _ | |a PUBDB-2022-03159 |
| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 530 |
| 088 | _ | _ | |a UCI-TR-2022-09 |2 Other |
| 088 | _ | _ | |a DESY-22-101 |2 DESY |
| 088 | _ | _ | |a arXiv:2206.09932 |2 arXiv |
| 100 | 1 | _ | |a Arakawa, Jason |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 245 | _ | _ | |a Neutrino Detection without Neutrino Detectors:Discovering Collider Neutrinos at FASER with Electronic Signals Only |
| 260 | _ | _ | |a Melville, NY |c 2022 |b Inst. |
| 264 | _ | 1 | |3 online |2 Crossref |b American Physical Society (APS) |c 2022-09-29 |
| 264 | _ | 1 | |3 print |2 Crossref |b American Physical Society (APS) |c 2022-09-01 |
| 336 | 7 | _ | |a article |2 DRIVER |
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| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 520 | _ | _ | |a The detection of collider neutrinos will provide new insights about neutrino production, propagation, and interactions at TeV energies, the highest human-made energies ever observed. During run 3 of the LHC, the FASER experiment is expected to detect roughly 104 collider neutrinos using its emulsion-based neutrino detector FASERν. In this study, we show that, even without processing the emulsion data, low-level input provided by the electronic detector components of FASER and FASERν will be able to establish a 5σ discovery of collider neutrinos with as little as 5 fb-1 of integrated luminosity. These results foreshadow the possible early discovery of collider neutrinos in LHC run 3. |
| 536 | _ | _ | |a 611 - Fundamental Particles and Forces (POF4-611) |0 G:(DE-HGF)POF4-611 |c POF4-611 |f POF IV |x 0 |
| 536 | _ | _ | |a DFG project 390833306 - EXC 2121: Quantum Universe (390833306) |0 G:(GEPRIS)390833306 |c 390833306 |x 1 |
| 542 | _ | _ | |i 2022-09-29 |2 Crossref |u https://creativecommons.org/licenses/by/4.0/ |
| 588 | _ | _ | |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de |
| 650 | _ | 7 | |a neutrino: detector |2 INSPIRE |
| 650 | _ | 7 | |a neutrino: production |2 INSPIRE |
| 650 | _ | 7 | |a interpretation of experiments: CERN LHC Coll |2 INSPIRE |
| 650 | _ | 7 | |a propagation |2 INSPIRE |
| 650 | _ | 7 | |a TeV |2 INSPIRE |
| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 0 |
| 700 | 1 | _ | |a Feng, Jonathan L. |0 Jonathan.L.Feng.1 |b 1 |
| 700 | 1 | _ | |a Ismail, Ahmed |b 2 |
| 700 | 1 | _ | |a Kling, Felix |0 P:(DE-H253)PIP1097110 |b 3 |u desy |
| 700 | 1 | _ | |a Waterbury, Michael |0 M.Waterbury.1 |b 4 |
| 773 | 1 | 8 | |a 10.1103/physrevd.106.052011 |b American Physical Society (APS) |d 2022-09-29 |n 5 |p 052011 |3 journal-article |2 Crossref |t Physical Review D |v 106 |y 2022 |x 2470-0010 |
| 773 | _ | _ | |a 10.1103/PhysRevD.106.052011 |g Vol. 106, no. 5, p. 052011 |0 PERI:(DE-600)2844732-3 |n 5 |p 052011 |t Physical review / D |v 106 |y 2022 |x 2470-0010 |
| 787 | 0 | _ | |a Arakawa, Jason et.al. |d 2022 |i IsParent |0 PUBDB-2022-02929 |r UCI-TR-2022-09 ; DESY-22-101 |t Neutrino Detection without Neutrino Detectors:Discovering Collider Neutrinos at FASER with Electronic Signals Only |
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| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/479596/files/Scintillator_Neutrinos.pdf |y OpenAccess |
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