Strong thermal SO(10)-inspired leptogenesis in the light of recent results from long-baseline neutrino experiments
Strong thermal SO(10)-inspired leptogenesis in the light of recent results from long-baseline neutrino experiments
We confront recent experimental results on neutrino mixing parameters with the requirements from strong thermal SO(10)-inspired leptogenesis, where the asymmetry is produced from next-to-lightest right-handed neutrinos N2 independently of the initial conditions. There is a nice agreement with latest global analyses supporting sin δ < 0 and normal ordering at ∼ 95% C.L. On the other hand, the more stringent experimental lower bound on the atmospheric mixing angle starts to corner strong thermal SO(10)-inspired leptogenesis. Prompted and encouraged by this rapid experimental advance, we obtain a precise determination of the allowed region in the plane δ versus θ23. We confirm that for the benchmark case α2 ≡ mD2/mcharm = 5 , where mD2 is the intermediate neutrino Dirac mass setting the N2 mass, and initial pre-existing asymmetry N B − L p,i = 10− 3, the bulk of solutions lies in the first octant. Though most of the solutions are found outside the 95% C.L. experimental region, there is still a big allowed fraction that does not require a too fine-tuned choice of the Majorana phases so that the neutrinoless double beta decay effective neutrino mass allowed range is still mee ≃ [10, 30] meV. We also show how the constraints depend on N B − L p,i and α2. In particular, we show that the current best fit, (θ23, δ) ≃ (47°, −130°), can be reproduced for N B − L p,i = 10− 3 and α2 = 6. Such large values for α2 have been recently obtained in a few realistic fits within SO(10)-inspired models. Finally, we also obtain that current neutrino data rule out N B − L p,i ≳ 0.1 for α2 ≲ 4.7.
1-19
Di Bari, Pasquale
3fe21e59-0eff-41bc-8faa-fdd817146418
Chianese, Marco
4cef572a-0a80-41f4-b835-b9792d41ba4e
May 2018
Di Bari, Pasquale
3fe21e59-0eff-41bc-8faa-fdd817146418
Chianese, Marco
4cef572a-0a80-41f4-b835-b9792d41ba4e
Di Bari, Pasquale and Chianese, Marco
(2018)
Strong thermal SO(10)-inspired leptogenesis in the light of recent results from long-baseline neutrino experiments.
Journal of High Energy Physics, 2018 (73), .
(doi:10.1007/JHEP05(2018)073).
Abstract
We confront recent experimental results on neutrino mixing parameters with the requirements from strong thermal SO(10)-inspired leptogenesis, where the asymmetry is produced from next-to-lightest right-handed neutrinos N2 independently of the initial conditions. There is a nice agreement with latest global analyses supporting sin δ < 0 and normal ordering at ∼ 95% C.L. On the other hand, the more stringent experimental lower bound on the atmospheric mixing angle starts to corner strong thermal SO(10)-inspired leptogenesis. Prompted and encouraged by this rapid experimental advance, we obtain a precise determination of the allowed region in the plane δ versus θ23. We confirm that for the benchmark case α2 ≡ mD2/mcharm = 5 , where mD2 is the intermediate neutrino Dirac mass setting the N2 mass, and initial pre-existing asymmetry N B − L p,i = 10− 3, the bulk of solutions lies in the first octant. Though most of the solutions are found outside the 95% C.L. experimental region, there is still a big allowed fraction that does not require a too fine-tuned choice of the Majorana phases so that the neutrinoless double beta decay effective neutrino mass allowed range is still mee ≃ [10, 30] meV. We also show how the constraints depend on N B − L p,i and α2. In particular, we show that the current best fit, (θ23, δ) ≃ (47°, −130°), can be reproduced for N B − L p,i = 10− 3 and α2 = 6. Such large values for α2 have been recently obtained in a few realistic fits within SO(10)-inspired models. Finally, we also obtain that current neutrino data rule out N B − L p,i ≳ 0.1 for α2 ≲ 4.7.
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Chianese Bari 2018 Article Strong Thermal SO10 inspired
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Submitted date: 2018
Accepted/In Press date: 30 April 2018
e-pub ahead of print date: 10 May 2018
Published date: May 2018
Identifiers
Local EPrints ID: 418854
URI: http://eprints.soton.ac.uk/id/eprint/418854
ISSN: 1029-8479
PURE UUID: 52be42ee-6078-497d-b279-fafab90d8289
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Date deposited: 23 Mar 2018 17:30
Last modified: 15 Mar 2024 18:56
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Author:
Marco Chianese
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