2019
DOI: 10.1103/physrevlett.123.081301
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Upper Bound of Neutrino Masses from Combined Cosmological Observations and Particle Physics Experiments

Abstract: We investigate the impact of prior models on the upper bound of the sum of neutrino masses, mν . Using data from large scale structure of galaxies, cosmic microwave background, type Ia supernovae, and big bang nucleosynthesis, we argue that cosmological neutrino mass and hierarchy determination should be pursued using exact models, since approximations might lead to incorrect and nonphysical bounds. We compare constraints from physically motivated neutrino mass models (i.e., ones respecting oscillation experim… Show more

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Cited by 83 publications
(62 citation statements)
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“…We can see a few features from the above results. First of all, since the neutrino mass scale is at most O(eV) [39,40], the contribution from the neutrino mass matrix is negligible for any measurable branching ratios in a collider-type experiment. Second, if we assume the Wilson coefficients associated with the dim-7 operators in SMEFT are similar in size, all of X and Y parameters will be of a similar order of magnitude.…”
Section: Matching Onto Effective Interactions In χPtmentioning
confidence: 99%
“…We can see a few features from the above results. First of all, since the neutrino mass scale is at most O(eV) [39,40], the contribution from the neutrino mass matrix is negligible for any measurable branching ratios in a collider-type experiment. Second, if we assume the Wilson coefficients associated with the dim-7 operators in SMEFT are similar in size, all of X and Y parameters will be of a similar order of magnitude.…”
Section: Matching Onto Effective Interactions In χPtmentioning
confidence: 99%
“…Now we make some numerical analysis. The values of the SM parameters are taken from the Particle Data Group [35]: [39,40], the contribution JHEP03(2020)120 11.7 from the neutrino mass matrix is negligible for any measurable branching ratios in a collidertype experiment. Second, if we assume the Wilson coefficients associated with the dim-7 operators in SMEFT are similar in size, all of X and Y parameters will be of a similar order of magnitude.…”
Section: Jhep03(2020)120mentioning
confidence: 99%
“…The atmospheric mass-squared difference, for example, dictates that at least one neutrino has to be heavier than |∆m 2 32 | 0.05 eV [27]. On the other hand, cosmic surveys limit the sum of masses of the neutrinos to be 0.26 eV [28]. For concreteness, we assume that the largest element of the neutrino mass matrix lies between m ν ∈ (0.05 − 0.…”
Section: The Effective All-singlets Operator O αβ Smentioning
confidence: 99%