2001
DOI: 10.1007/s100500170022
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Latest results from the HEIDELBERG-MOSCOW double beta decay experiment

Abstract: Abstract. New results for the double beta decay of76 Ge are presented. They are extracted from Data obtained with the Heidelberg-Moscow experiment, which operates five enriched 76 Ge detectors in an extreme low-level environment in the Gran Sasso underground laboratory. The two neutrino accompanied double beta decay is evaluated for the first time for all five detectors with a statistical significance of 47.7 kg y resulting in a half life of T

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Cited by 619 publications
(462 citation statements)
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References 26 publications
(10 reference statements)
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“…Optimal ββ(0ν) sensitivities have been reached in a series of experiments based on the calorimetric approach. In particular, the best limit on ββ(0ν) comes from the Heidelberg-Moscow (HM) experiment [37] on 76 Ge (Fig. 3) even if similar results have been obtained also by the IGEX experiment [38] (Tab.…”
Section: Present and Past Experimentsmentioning
confidence: 59%
“…Optimal ββ(0ν) sensitivities have been reached in a series of experiments based on the calorimetric approach. In particular, the best limit on ββ(0ν) comes from the Heidelberg-Moscow (HM) experiment [37] on 76 Ge (Fig. 3) even if similar results have been obtained also by the IGEX experiment [38] (Tab.…”
Section: Present and Past Experimentsmentioning
confidence: 59%
“…In general, due to smallness of the 1-3 mixing the contribution of ν 3 is very small: If the Heidelberg-Moscow positive result [3,4,5,6,7] is confirmed, either our approach, at least in its present form, is not correct or another mechanism, different from the Majorana mass of the light neutrinos gives main contribution to the decay rate.…”
Section: A 1-3 Mixingmentioning
confidence: 83%
“…The results reported in [21] will be checked in the currently running and forthcoming NDB experiments. There are a large number of projects such as CUORICINO [23], CUORE [24], GERDA [25], MAJORANA [26], SuperNEMO [27], EXO [28], GENIUS [29] which aim to achieve a sensitivity upto 0.01eV for M ee . Cosmological observations put an upper bound on the sum of neutrino masses…”
Section: Numerical Resultsmentioning
confidence: 99%