Observables sensitive to absolute neutrino masses. II

By G. Fogli, E. Lisi, A. Marrone, A. Melchiorri, A. Palazzo, A. M. Rotunno, P. Serra, J. Silk, A. Slosar. 2008

156 citations recorded by the source corpus.

In this followup to Phys. Rev. D 75, 053001 (2007) , we report updated constraints on neutrino mass-mixing parameters, in light of recent neutrino oscillation data (KamLAND, SNO, and MINOS) and cosmological observations (WMAP 5-year and other data). We discuss their interplay with the final 0{nu}2{beta} decay results in {sup 76}Ge claimed by part of the Heidelberg-Moscow Collaboration, using recent evaluations of the corresponding nuclear matrix elements, and their uncertainties. We also comment on the 0{nu}2{beta} limits in {sup 130}Te recently set by Cuoricino and on prospective limits or signals from the Karlsruhe tritium neutrino experiment.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/f3429e4389715b3a735fb3a5632b83b7ef7bf240

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In Nuclear and High Energy Physics

1. A. Marrone
2. E. Lisi
3. A. Palazzo
4. Francesco Capozzi
5. S. Pastor
6. O. Mena
7. E. di Valentino
8. A. Melchiorri

Citations in the corpus

• Evidence of $\theta_{13}$>0 from global neutrino data analysis (2011, methodology): “Our atmospheric ν analysis is restricted to the two CP-conserving cases cos δ = ±1 [2, 6]; we plan to remove such restriction in the future, so as to analyze both atmospheric and long-baseline accelerator data with unconstrained δ (see [13] for a previous analysis of this kind).”
• Global constraints on absolute neutrino masses and their ordering (2017, methodology): “[23] G.”
• Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects (2018, methodology): “We refer the reader to the seminal works of Croft et al. (1999), Seljak et al. (2005), Goobar et al. (2006), Seljak et al. (2006), Gratton et al. (2008), Fogli et al. (2008), and Viel et al. (2010).”
• Global analysis of neutrino masses, mixings and phases: entering the era of leptonic CP violation searches (2012, background): “We also show updated oscillation constraints on the main absolute mass observables [44, 45], namely, the effective electron neutrino mass mβ (probed in β decay), the effective Majorana mass (probed in 0ν2β decay searches), and the sum of neutrino masses Σ, which can be probed by precision cosmology.”
• Neutrino Mass from Cosmology (2012, background): “phases. Thus cosmological results are complementary to terrestrial experiments. The interested reader can nd the allowed regions in the parameter space dened by any pair of parameters ( P ;m ;m ) in [21, 49, 50]. The two cases involving P are shown in Fig. 6. Now we can nd the possible present value”