2006
DOI: 10.1088/1475-7516/2006/07/005
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Long-lived staus at neutrino telescopes

Abstract: Abstract. We perform an exhaustive study of the role neutrino telescopes could play in the discovery and exploration of supersymmetric extensions of the Standard Model with a long-lived stau next-to-lightest superparticle. These staus are produced in pairs by cosmic neutrino interactions in the Earth matter. We show that the background of stau events to the standard muon signal is negligible and plays no role in the determination of the cosmic neutrino flux. On the other hand, one can expect up to 50 pair even… Show more

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Cited by 48 publications
(94 citation statements)
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“…Also direct a production at colliders is strongly suppressed. Nevertheless, (quasi-) stable τ 1 's could appear in collider detectors (and neutrino telescopes [344]) as a possible signature of the a LSP. However, since the M P measurement at colliders [351], which would have been a decisive test of the G LSP, seems cosmologically disfavored in most of the parameter space of R-parity conserving SUSY models, it may very well be a challenge to distinguish between the a LSP and the G LSP.…”
Section: Experimental Prospectsmentioning
confidence: 99%
“…Also direct a production at colliders is strongly suppressed. Nevertheless, (quasi-) stable τ 1 's could appear in collider detectors (and neutrino telescopes [344]) as a possible signature of the a LSP. However, since the M P measurement at colliders [351], which would have been a decisive test of the G LSP, seems cosmologically disfavored in most of the parameter space of R-parity conserving SUSY models, it may very well be a challenge to distinguish between the a LSP and the G LSP.…”
Section: Experimental Prospectsmentioning
confidence: 99%
“…Various aspects of this scenario were further considered in Refs. [5,6,7]. In principle one could think that cosmic rays could be an even better source of supersymmetric events, and ultimately of NLSPs.…”
Section: Introductionmentioning
confidence: 99%
“…It also implies that ℓ (1) can be produced by the interactions of high energy neutrinos with the earth and propagate through it until reaching a detector, in very close analogy to the case of NLSP sleptons studied in Refs. [9,10,11,12,13]. We will show that interactions of high energy neutrinos (E ν > 10 5 GeV) with nucleons in the Earth will produce pairs of NLKPs.…”
Section: Introductionmentioning
confidence: 90%