Abstract
After the successful investigation and confirmation of non zero \(\theta _{13}^{PMNS}\) by various experiments, we are standing at a square where we still encounter a number of issues, which are to be settled. In this paper, we have extended our recent work towards a precise prediction of the \(\theta _{23}^{PMNS}\) mixing angle, taking into account the neutrino mass hierarchy. We parameterize the non-trivial correlation between quark (CKM) and lepton (PMNS) mixing matrices in quark-lepton complementarity (QLC) model as \(V_{c}= U_{CKM}. \psi . U_{PMNS}\), where \(\psi \) is a diagonal phase matrix. Monte Carlo simulations are used to estimate the texture of \(V_{c}\) and compare the results with the standard Tri-Bi-Maximal (TBM) and Bi-Maximal (BM) structures of neutrino mixing matrix. We have predicted the value of \(\theta _{23}^{PMNS} \) for normal and inverted neutrino mass hierarchies. The value of \(\theta _{23}^{PMNS}\) obtained for two cases are about \(1.3\sigma \) away from each other, implying the better precision can give us a strong hint for the type of neutrino mass hierarchy.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Similar content being viewed by others
References
J. Beringer et al., (Particle Data Group), Phys. Rev. D 28, 010001 (2012); A. Ceccucci, Z. Ligeti, Y. Sakai, PDG (2014). http://pdg.lbl.gov/2014/reviews/
F. An et al., [Daya Bay Collaboration], Phys. Rev. Lett. 108, 171803 (2012); J. Ahn et al., [RENO Collaboration], Phys. Rev. Lett. 108, 191802 (2012); K. Abe et al., [T2K Collaboration], Phys. Rev. Lett. 107, 041801 (2011); P. Adamson et al., [MINOS Collaboration], Phys. Rev. Lett. 107, 181802 (2011); Y. Abe et al., [Double Chooz Collaboration], Phys. Rev. D 86, 052008 (2012)
H. Georgi, C. Jarlskog, Phys. Lett. B 86, 297 (1979); H. Minakata, A.Y. Smirnov, Phys. Rev. D 70, 073009 (2004); W. Rodejohann, Phys. Rev. D 69, 033005 (2004); K.A. Hochmuth, W. Rodejohann, Phys. Rev. D 75, 073001 (2007); S.K. Agarwalla, M.K. Parida, R. N. Mohapatra, G. Rajasekaran, Phys. Rev. D 75, 033007 (2007)
Z.z. Xing, Phys. Lett. B 618,141 (2005); A. Dighe, S. Goswami, P. Roy, Phys. Rev. D 73, 071301 (2006); A.Y. Smirnov, arXiv:hep-ph/0604213; P.H. Frampton, S.T. Petcov, W. Rodejohann, Nucl. Phys. B 687, 31 (2004); A. Datta, L. Everett, P. Ramond, Phys. Lett. B 620, 42 (2005); J. Harada, Europhys. Lett. 75, 248 (2006); J. Harada, Europhys. Lett. 103, 21001 (2013); M. Picariello, B.C. Chauhan, J. Pulido, E. Torrente-Lujan, Mod. Phys. Lett. A 22, 5860 (2008)
B.C. Chauhan, M. Picariello, J. Pulido, E. Torrente-Lujan, Eur. Phys. J. C 50, 573 (2007)
G.G. Ross, Grand Unified Theories (Westview Press, Reading, MA, 1985)
F. Björkeroth et al., Testing constrained sequential dominance models of neutrinos, arXiv:1412.6996 [hep-ph] (2015)
G. Sharma, B.C. Chauhan, JHEP 1607, 075 (2016)
Acknowledgements
B.C. Chauhan and all the other authors acknowledge the financial support provided by University Grants Commission(UGC), Government of India vide Grant No. UGC MRP-MAJOR-PHYS-2013-12281.
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2018 Springer International Publishing AG, part of Springer Nature
About this paper
Cite this paper
Sharma, G., Bhardwaj, S., Chauhan, B.C., Verma, S. (2018). Quark-Lepton Complementarity Model Based Predictions for \(\theta _{23}^{PMNS}\) with Neutrino Mass Hierarchy. In: Naimuddin, M. (eds) XXII DAE High Energy Physics Symposium . Springer Proceedings in Physics, vol 203. Springer, Cham. https://doi.org/10.1007/978-3-319-73171-1_57
Download citation
DOI: https://doi.org/10.1007/978-3-319-73171-1_57
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-319-73170-4
Online ISBN: 978-3-319-73171-1
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)