Papers
Topics
Authors
Recent
Search
2000 character limit reached

A Realistic Neutrino mixing scheme arising from $A_4$ symmetry

Published 14 Apr 2023 in hep-ph | (2304.07259v3)

Abstract: We propose a unique lepton mixing scheme and its association with an exact hierarchy-philic neutrino mass matrix texture in the light of Type-I+Type-II seesaw mechanism under the framework of $A_4 \times Z_{10}$ discrete flavour symmetry. The proposed model successfully predicts the normal ordering of neutrino masses and the two Majorana phases. Additionally, the analysis extends to the effective Majorana neutrino mass, in the context of neutrinoless double beta\,($0\nu\beta\beta$)-decay.

Authors (2)
Definition Search Book Streamline Icon: https://streamlinehq.com
References (44)
  1. doi:10.1126/science.124.3212.103.
  2. arXiv:nucl-ex/0204008, doi:10.1103/PhysRevLett.89.011301.
  3. arXiv:hep-ex/0212021, doi:10.1103/PhysRevLett.90.021802.
  4. arXiv:hep-ex/9812014, doi:10.1103/PhysRevLett.82.2644.
  5. arXiv:1406.3546, doi:10.1007/JHEP07(2014)090.
  6. arXiv:hep-ph/0202074, doi:10.1016/S0370-2693(02)01336-9.
  7. arXiv:hep-ph/0511133, doi:10.1103/PhysRevD.73.057304.
  8. arXiv:0905.3534, doi:10.1016/j.nuclphysb.2009.08.018.
  9. arXiv:1909.09610, doi:10.1016/j.physrep.2020.02.001.
  10. arXiv:2211.01314, doi:10.1016/j.physletb.2023.137767.
  11. Z.-z. Xing, The μ𝜇\muitalic_μ-τ𝜏\tauitalic_τ reflection symmetry of Majorana neutrinos (10 2022). arXiv:2210.11922.
  12. arXiv:1707.05535, doi:10.1007/JHEP10(2017)102.
  13. arXiv:1512.04207, doi:10.1088/0034-4885/79/7/076201.
  14. arXiv:1505.01891, doi:10.1016/j.ppnp.2015.05.002.
  15. arXiv:1311.3846, doi:10.1038/ncomms6153.
  16. arXiv:hep-ph/0310204, doi:10.1088/0034-4885/67/2/R01.
  17. arXiv:1711.02180, doi:10.3389/fphy.2018.00040.
  18. arXiv:hep-ph/0412379, doi:10.1142/9789812702210_0003.
  19. arXiv:1301.1340, doi:10.1088/0034-4885/76/5/056201.
  20. arXiv:hep-ph/0603118, doi:10.1146/annurev.nucl.56.080805.140534.
  21. arXiv:1108.4416, doi:10.1103/PhysRevD.85.055018.
  22. arXiv:0805.3536, doi:10.1103/PhysRevD.78.015018.
  23. doi:10.1103/PhysRevD.22.2860.
  24. arXiv:2205.08531, doi:10.1016/j.physletb.2022.137354.
  25. arXiv:hep-ph/0609046, doi:10.1088/1126-6708/2007/01/043.
  26. doi:10.1143/PTP.28.870.
  27. arXiv:hep-ph/9806387, doi:10.1016/S0370-2693(98)00880-6.
  28. arXiv:1004.2798, doi:10.1140/epjc/s10052-010-1492-2.
  29. arXiv:1110.1688, doi:10.1016/j.nuclphysb.2011.12.004.
  30. arXiv:2111.03086, doi:10.3390/universe7120459.
  31. arXiv:hep-ph/0106291, doi:10.1103/PhysRevD.64.113012.
  32. arXiv:2003.01134, doi:10.1016/j.physletb.2020.135491.
  33. arXiv:2309.14769.
  34. arXiv:hep-ph/0610250, doi:10.1016/j.physletb.2006.12.006.
  35. arXiv:1002.0211, doi:10.1103/RevModPhys.82.2701.
  36. arXiv:1706.07606, doi:10.1007/JHEP11(2017)136.
  37. arXiv:1106.4269, doi:10.1103/PhysRevLett.107.061803.
  38. arXiv:1807.06209, doi:10.1051/0004-6361/201833910.
  39. doi:10.3390/universe9060290.
  40. arXiv:2202.01787, doi:10.1103/RevModPhys.95.025002.
  41. arXiv:1912.10966, doi:10.1103/PhysRevLett.124.122501.
  42. arXiv:1909.02726, doi:10.1126/science.aav8613.
  43. arXiv:1605.02889, doi:10.1103/PhysRevLett.117.082503.
  44. arXiv:2303.02358.
Citations (4)
View on Semantic Scholar

Summary

No one has generated a summary of this paper yet.

Sign Up to Summarize

Paper to Video (Beta)

No one has generated a video about this paper yet.

Sign Up to Generate All Videos Subscribe on YouTube

Whiteboard

No one has generated a whiteboard explanation for this paper yet.

Sign Up to Generate

Open Problems

We haven't generated a list of open problems mentioned in this paper yet.

Generate Now

Continue Learning

We haven't generated follow-up questions for this paper yet.

Generate Now

Collections

Sign up for free to add this paper to one or more collections.

Sign Up