2013/05/31 by P. S. Bhupal Dev, Srubabati Goswami, Sreetama Goswami +2 · 107 citations
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Double beta decay #Neutrino #Neutrino Physics Research #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Seesaw molecular geometry #hep-ex #hep-ph #nucl-ex #nucl-th
paper · pdf · doi:10.1103/physrevd.88.091301
published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 88(9) (American Physical Society) · 6 pages, 4 figures, 3 tables; updated version including GERDA results; Figure 4 and Tables II and III added
arxiv created 2013/07/17 · openalex publication_date 2013/11/22 · arxiv updated 2013/11/27 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We study the implications of the recent results on neutrinoless double beta decay (0\ensuremathν\ensuremathβ\ensuremathβ) from GERDA-I (76Ge) and KamLAND\mathrm\text\ensuremath-Zen+EXO\mathrm\text\ensuremath-200 (136Xe) and the upper limit on the sum of light neutrino masses from Planck. We show that the upper limits on the effective neutrino mass from 136Xe are stronger than those from 76Ge for most of the recent calculations of the nuclear matrix elements (NMEs). We also analyze the compatibility of these limits with the claimed observation in 76Ge and show that while the updated claim value is still compatible with the recent GERDA limit as well as the individual 136Xe limits for a few NME calculations, it is inconsistent with the combined 136Xe limit for all but one NME. Imposing the most stringent limit from Planck, we find that the canonical light neutrino contribution cannot saturate the current limit, irrespective of the NME uncertainties. Saturation can be reached by inclusion of the right-handed (RH) neutrino contributions in TeV-scale left-right symmetric models with type-II seesaw. This imposes a lower limit on the lightest neutrino mass. Using the 0\ensuremathν\ensuremathβ\ensuremathβ bounds, we also derive correlated constraints in the RH sector, complimentary to those from direct searches at the LHC.