@article{altenmuller_arenz_baek_beck_beglarian_behrens_bergmann_berlev_besserer_blaum_et al._2020, title={High-resolution spectroscopy of gaseous Kr-83m conversion electrons with the KATRIN experiment}, volume={47}, ISSN={["1361-6471"]}, DOI={10.1088/1361-6471/ab8480}, abstractNote={Abstract}, number={6}, journal={JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS}, author={Altenmuller, K. and Arenz, M. and Baek, W-J and Beck, M. and Beglarian, A. and Behrens, J. and Bergmann, T. and Berlev, A. and Besserer, U. and Blaum, K. and et al.}, year={2020}, month={Jun} }
 @article{aalseth_adles_anderson_avignone_barabash_bowyer_brodzinski_brudanin_champangne_collar_et al._2003, title={The Majorana Ge-76 double-beta decay project}, volume={124}, ISSN={0920-5632}, DOI={10.1016/S0920-5632(03)02116-9}, abstractNote={The interest and relevance of next-generation 0v ββ-decay experiments is increasing. Even with nonzero neutrino mass strongly suggested by solar and atmospheric neutrino experiments sensitive to δm2, 0v ββ-decay experiments are still the only way to establish the Dirac or Majorana nature of neutrinos by measuring the effective electron neutrino mass, 〈mv〉. In addition, the atmospheric neutrino oscillation experiments imply that at least one neutrino has a mass greater than about 50 meV. The Majorana Experiment expects to probe an effective neutrino mass near this critical value. Majorana is a next-generation 76Ge double-beta decay search. It will employ 500 kg of Ge, isotopically enriched to 86% in 76Ge, in the form of ∼ 200 detectors in a close-packed array. Each crystal will be electronically segmented and each segment fitted with pulse-shape analysis electronics. This combination of segmentation and pulse-shape analysis significantly improves our ability to discriminate neutrinoless double beta-decay from internal cosmogenic 68Ge and 60Co. The half-life sensitivity is estimated to be 4.2 × 1027 y corresponding to a 〈mv〉 range of ≤ 20 − 70 meV, depending on the nuclear matrix elements used to interpret the data.}, journal={NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS}, author={Aalseth, CE and Adles, E and Anderson, D and Avignone, FT and Barabash, A and Bowyer, TW and Brodzinski, RL and Brudanin, V and Champangne, A and Collar, JI and et al.}, year={2003}, month={Jul}, pages={247–252} }
 @misc{adelberger_austin_bahcall_balantekin_bogaert_brown_buchmann_cecil_champagne_braeckeleer_et al._1998, title={Solar fusion cross sections}, volume={70}, ISSN={["1539-0756"]}, DOI={10.1103/RevModPhys.70.1265}, abstractNote={We review and analyze the available information on the nuclear-fusion cross sections that are most important for solar energy generation and solar neutrino production. We provide best values for the low-energy cross-section factors and, wherever possible, estimates of the uncertainties. We also describe the most important experiments and calculations that are required in order to improve our knowledge of solar fusion rates.}, number={4}, journal={REVIEWS OF MODERN PHYSICS}, author={Adelberger, EG and Austin, SM and Bahcall, JN and Balantekin, AB and Bogaert, G and Brown, LS and Buchmann, L and Cecil, FE and Champagne, AE and Braeckeleer, L and et al.}, year={1998}, month={Oct}, pages={1265–1291} }