2021
DOI: 10.1007/jhep05(2021)191
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Neutrino beam-dump experiment with FASER at the LHC

Abstract: The neutrino physics program at the LHC, which will soon be initiated by the FASER experiment, will provide unique opportunities for precision studies of neutrino interaction vertices at high energies. This will also open up the possibility to search for beyond the standard model (BSM) particles produced in such interactions in the specific high-energy neutrino beam-dump experiment. In this study, we illustrate the prospects for such searches in models with the dipole or Z′ portal to GeV-scale heavy neutral le… Show more

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Cited by 48 publications
(32 citation statements)
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References 93 publications
(177 reference statements)
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“…Other studies include considerations of solar neutrinos [4][5][6], atmospheric neutrinos in IceCube [7], or short-baseline experiments [8][9][10][11][12][13]. The HNL dipole portal can be explored also at dedicated experiment for long-lived particle searches such as SHiP [14], FASER [15,16], or MATHUSLA [17,18].…”
Section: Jhep07(2021)200mentioning
confidence: 99%
“…Other studies include considerations of solar neutrinos [4][5][6], atmospheric neutrinos in IceCube [7], or short-baseline experiments [8][9][10][11][12][13]. The HNL dipole portal can be explored also at dedicated experiment for long-lived particle searches such as SHiP [14], FASER [15,16], or MATHUSLA [17,18].…”
Section: Jhep07(2021)200mentioning
confidence: 99%
“…[86,87], and dipole interactions have been considered in Ref. [88]. In addition, other portals between fermionic BSM states and the SM have also been investigated, including in supersymmetric models with light neutralinos [84,89], which are a promising solution to the hierarchy problem, and in effective field [4,31,50,91] and references therein.…”
Section: Dark Photon Massmentioning
confidence: 99%
“…A scenario that has been well studied in the literature consists of a Z and a HNL [95][96][97], which could also explain the MiniBooNE anomaly [98]. In addition to its usual neutrino-mixing based production modes, the HNL could be produced through Z → N N decays [99], or via the upscattering of SM neutrinos, νp → N p [88]. If the HNL is produced in neutrino scattering in the upstream rock, it could also be detected via a multiple coincident muon signature traversing the FPF experiments [100].…”
Section: Dark Photon Massmentioning
confidence: 99%
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“…Searches for other types of physics beyond the Standard Model in FASER have previously been discussed in refs. [36][37][38][39][40][41][42][43][44][45][46][47][48][49], while refs. [50][51][52][53] have focused specifically on FASERν.…”
Section: Introductionmentioning
confidence: 99%