2019
DOI: 10.1155/2019/4863620
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Constraining the Effective Mass of Majorana Neutrino with Sterile Neutrino Mass for Inverted Ordering Spectrum

Abstract: Inspired by the experimental anomalies in neutrino physics and recent oscillation data from short baseline and another neutrino experiment, the realization of one extra neutrino flavor seem to be favoring. This extra flavor may change the observable, |m ββ | of currently data taking and next-generation (ββ)0ν -decay experiments aim to probe and possibly look the Inverted Ordering region(|m ββ | 10 −2 eV) of parameter space. This observation would allow establishing physics beyond the standard model and phenome… Show more

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Cited by 9 publications
(6 citation statements)
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“…Determination of precise CP phase value is not only important for verifying the baryon asymmetry of the universe [60] but also for explaining the sterile neutrino phenomenon [61].…”
Section: Multi-nucleon Interactions and Their Implicationsmentioning
confidence: 99%
“…Determination of precise CP phase value is not only important for verifying the baryon asymmetry of the universe [60] but also for explaining the sterile neutrino phenomenon [61].…”
Section: Multi-nucleon Interactions and Their Implicationsmentioning
confidence: 99%
“…These uncertainties cause major challenges in the determination of the CPviolating phase which is not yet constrained. Precise CP phase value is not only crucial for verifying the baryon asymmetry of the Universe, but also for explaining the physics beyond the standard model and effective mass of neutrinos [8].…”
Section: Introductionmentioning
confidence: 99%
“…This discovery can shed light on the origin of leptogenesis [4] and can be a tool to answer some of the intriguing questions like baryon asymmetry of the universe [5]. Precise CP phase value is also required for the exact absolute neutrino mass measurement in double beta decay experiments and also for explaining the sterile neutrinos phenomenon [6]. The global analysis [7] shows two sets of best fit values of neutrino oscillation parameters in 1σ and 3σ ranges that correspond to the analysis done, with and without Super-Kamiokande atmospheric neutrino data.…”
Section: Introductionmentioning
confidence: 99%