2022
DOI: 10.48550/arxiv.2205.08141
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Decays of a bino-like particle in the low-mass regime

Abstract: We study the phenomenology associated with a light bino-like neutralino with mass ă " m τ in the context of the R-parity violating Minimal Supersymmetric Standard Model. This is a well-motivated example of scenarios producing potentially light and long-lived exotic particles, which might be testable in far-detector experiments, such as the FASER experiment at the Large Hadron Collider. A quantitative assessment of the discovery potential or the extraction of limits run through a detailed understanding of the i… Show more

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Cited by 4 publications
(8 citation statements)
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“…See ref. [30] for a recent study on the low-energy phenomenomology of a bino-like neutralino lighter than the tau lepton.…”
Section: Introductionmentioning
confidence: 99%
“…See ref. [30] for a recent study on the low-energy phenomenomology of a bino-like neutralino lighter than the tau lepton.…”
Section: Introductionmentioning
confidence: 99%
“…They have been studied extensively for various present and future experiments including SHiP [59,60], ATLAS [59], far detectors at the LHC [61][62][63][64], Belle II [65], Super-Kamiokande [66], and future lepton colliders [67,68]. These works mostly consider the signature of a neutralino decay into a charged lepton plus a meson, induced by LQ D operators [69], while the production can result from decays of either mesons, τ leptons, or Z-boson.…”
Section: Jhep02(2023)120mentioning
confidence: 99%
“…The dominant decay mode of the neutralino is dictated by the relative sizes of the RPV couplings, as well as the neutralino mass [69]. For m χ0 1 O (4.5) GeV, the neutralino can decay into a meson and a lepton via an LQ D operator, if kinematically allowed.…”
Section: Neutralino Decaymentioning
confidence: 99%
“…1 can be as light as a GeV or even lighter [14][15][16][17][18][19][20][21][22][23], in which case its production in decays of τ lepton or heavy mesons is kinematically allowed. Such a light neutralino should be dominantly Bino according to current bounds [21][22][23][24][25]. In addition, it has to decay, e.g., via RPV couplings so as to avoid overclosing the Universe [26][27][28][29].…”
mentioning
confidence: 99%
“…We focus on the case in which only λ 113 or λ 123 is non-zero and there is no squark mixing. The decay of such a light neutralino is suppressed, so that it appears as missing energy at the detector level [25]. We propose to probe λ 113 via the decay mode B + → p χ0…”
mentioning
confidence: 99%