1998
DOI: 10.1007/s100520050149
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An upper limit on the

Abstract: An upper limit on the neutrino mass from three-and ve-prong tau decays. The ALEPH CollaborationAbstract A bound on the tau neutrino mass is established using the data collected from 1991 to 1995 at p s ' m Z with the ALEPH detector. Two separate limits are derived by tting the distribution of visible energy vs invariant mass in ! 2 + and ! 3 2 + ( 0 ) decays. The two results are combined to obtain a 95% condence level upper limit of 18:2 MeV=c 2 on the mass of the tau neutrino.

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Cited by 52 publications
(4 citation statements)
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“…The observation of neutrino oscillations demonstrated the existence of non-zero neutrino masses, allowing the π 0 → νν decay via Z-boson exchange. The direct experimental limit on the tau neutrino mass, m ντ < 18.2 MeV/c 2 at 95% confidence level (CL) [3], corresponds to a branching ratio (BR) for π 0 → νν below 5 × 10 −10 at 90% CL. A more stringent limit is set by cosmological constraints on the sum of the neutrino masses: Σm ν 1 eV/c 2 , implying BR(π 0 → νν) < 10 −24 , which is well below the current experimental sensitivity.…”
Section: Introductionmentioning
confidence: 99%
“…The observation of neutrino oscillations demonstrated the existence of non-zero neutrino masses, allowing the π 0 → νν decay via Z-boson exchange. The direct experimental limit on the tau neutrino mass, m ντ < 18.2 MeV/c 2 at 95% confidence level (CL) [3], corresponds to a branching ratio (BR) for π 0 → νν below 5 × 10 −10 at 90% CL. A more stringent limit is set by cosmological constraints on the sum of the neutrino masses: Σm ν 1 eV/c 2 , implying BR(π 0 → νν) < 10 −24 , which is well below the current experimental sensitivity.…”
Section: Introductionmentioning
confidence: 99%
“…The upper limit for the mass of the lightest neutrino flavor v e was obtained from experiments for measurement of the high-energy part of the tritium βspectrum and recent experiments yield 2 eV upper limit (Weinheimer et al, 1999;Lobashev et al, 1999). As a result of the recent experiments, the upper mass limits of v µ and v τ were found to be 170 KeV (Assamagan et al, 1996) and 18.2 MeV (Barate et al, 1998), respectively. The Solar and atmospheric neutrino experiments allow to find the square mass differences 2 2 2 12 2 1 m m m ∆ = − and 2 2 2 23 3 2 m m m ∆ = − , but not the absolute values of the neutrino masses.…”
Section: Introductionmentioning
confidence: 99%
“…The most sensitive bounds on the mass of the ν τ can be derived from the analysis of the invariant-mass spectrum of semi-hadronic τ decays, e.g. the present best limit of m ν τ < 18.2 MeV=c 2 (95% confidence level) was based on the kinematics of 2939 (52) events of τ − → 2π − π þ ν τ (τ − → 3π − 2π þ ðπ − Þν τ ) [8]. This method depends on a determination of the kinematic end point of the mass spectrum; thus high precision on m τ is needed.…”
Section: Introductionmentioning
confidence: 99%