Home > Publications database > Neutrino Detection without Neutrino Detectors: Discovering Collider Neutrinos at FASER with Electronic Signals Only > print

001     479195
005     20230510113815.0
024 7 _ |a Arakawa:2022rmp
|2 INSPIRETeX
024 7 _ |a inspire:2098400
|2 inspire
024 7 _ |a arXiv:2206.09932
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2022-02929
|2 datacite_doi
037 _ _ |a PUBDB-2022-02929
041 _ _ |a English
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 J.Arakawa.1
|b 0
|e Corresponding author
245 _ _ |a Neutrino Detection without Neutrino Detectors: Discovering Collider Neutrinos at FASER with Electronic Signals Only
260 _ _ |c 2022
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1656057753_3188
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
500 _ _ |a Will be submitted to journal.
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 $10^4$ collider neutrinos using its emulsion-based neutrino detector FASER$\nu$. In this study, we show that, even without processing the emulsion data, low-level input provided by the electronic detector components of FASER and FASER$\nu$ will be able to establish a $5\sigma$ discovery of collider neutrinos with as little as $5~\text{fb}^{-1}$ 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
588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |a neutrino, detector
|2 INSPIRE
650 _ 7 |a neutrino, production
|2 INSPIRE
650 _ 7 |a 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
700 1 _ |a Waterbury, Michael
|0 M.Waterbury.1
|b 4
856 4 _ |u https://bib-pubdb1.desy.de/record/479195/files/HTML-Approval_of_scientific_publication.html
856 4 _ |u https://bib-pubdb1.desy.de/record/479195/files/PDF-Approval_of_scientific_publication.pdf
856 4 _ |y OpenAccess
|u https://bib-pubdb1.desy.de/record/479195/files/2206.09932v1.pdf
856 4 _ |y OpenAccess
|x pdfa
|u https://bib-pubdb1.desy.de/record/479195/files/2206.09932v1.pdf?subformat=pdfa
909 C O |o oai:bib-pubdb1.desy.de:479195
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910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 3
|6 P:(DE-H253)PIP1097110
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-611
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Fundamental Particles and Forces
|x 0
914 1 _ |y 2022
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Creative Commons Attribution CC BY 4.0
|0 LIC:(DE-HGF)CCBY4
|2 HGFVOC
915 _ _ |a Published
|0 StatID:(DE-HGF)0580
|2 StatID
920 1 _ |0 I:(DE-H253)T-20120731
|k T
|l Theorie-Gruppe
|x 0
980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)T-20120731
980 1 _ |a FullTexts

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