Implications of fermionic dark matter on recent neutrino oscillation data

Shivaramakrishna Singirala

doi:10.1088/1674-1137/41/4/043102

Chinese Physics C> 2017, Vol. 41> Issue(4) : 043102 DOI: 10.1088/1674-1137/41/4/043102

Implications of fermionic dark matter on recent neutrino oscillation data

Shivaramakrishna Singirala

1.
School of Physics, University of Hyderabad, Hyderabad-500046, India

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Abstract：
We investigate flavor phenomenology and dark matter in the context of the scotogenic model. In this model, the neutrino masses are generated through radiative corrections at the one-loop level. Considering the neutrino mixing matrix to be of tri-bimaximal form with additional perturbations to accommodate the recently observed non-zero value of the reactor mixing angle θ₁₃, we obtain the relation between various neutrino oscillation parameters and the model parameters. Working in a degenerate heavy neutrino mass spectrum, we obtain light neutrino masses obeying the normal hierarchy and also study the relic abundance of fermionic dark matter candidates, including coannihilation effects. A viable parameter space is thus obtained, consistent with neutrino oscillation data, relic abundance and various lepton flavor violating decays such as l_α→l_βγ and l_α→3l_β.
- dark matter ,
- neutrino mixing ,
- lepton flavor violation

References

[1]	P. Minkowski, Phys. Lett. B, 67:421 (1977); R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett., 44:912 (1980); M. Gell-Mann, P. Ramond, and R. Slansky (1980), print-80-0576 (CERN); J. Schechter and J. W. F. Valle, Phys. Rev. D, 22:2227 (1980)
[2]	R. N. Mohapatra and G. Senjanovic, Phys. Rev. D, 23:165 (1981); G. Lazarides, Q. Shafi, and C. Wetterich, Nucl. Phys. B, 181:287 (1981); C. Wetterich, Nucl. Phys. B, 187:343 (1981); B. Brahmachari and R. N. Mohapatra, Phys. Rev. D, 58:015001 (1998); S. Antusch and S. F. King, Phys. Lett. B, 597:199 (2004); R. N. Mohapatra, Nucl. Phys. Proc. suppl., 138:257 (2005)
[3]	R. Foot, H. Lew, X. G. He et al, Z. Phys. C, 44:441 (1989)
[4]	E. Ma, Phys. Rev. D, 73:077301 (2006), arXiv:hepph/0601225
[5]	B. Pontecorvo, Sov. Phys. JETP, 7:172 (1958); Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys., 28:870 (1962)
[6]	F. P. An et al (DAYA-BAY Collaboration), Phys. Rev. Lett., 108:171803 (2012), arXiv:1203.1669
[7]	F. P. An et al (DAYA-BAY Collaboration), Chin. Phys. C, 37:011001 (2013), arXiv:1210.6327
[8]	J. K. Ahn et al (RENO Collaboration), Phys. Rev. Lett., 108:191802 (2012), arXiv:1204.0626
[9]	K. Abe et al (T2K Collaboration), Phys. Rev. D, 88:032002 (2013), arXiv:1304.0841
[10]	D. Forero, M. Tortela, and J. Valle, Phys. Rev. D, 90:093006 (2014), arXiv:1405.7540
[11]	P. A. R. Ade et al (Planck Collaboration), Astron. Astrophys., 571:A1 (2014), arXiv:1303.5062
[12]	L. Lepoz Honorez, E.Nezri, J. F. Oliver et al, JCAP, 02:28 (2007), arXiv:hep-ph/0612275
[13]	R. Barbieri, L. E. Hall, and V. S. Rychkov, Phys. Rev. D, 74:015007 (2006), arXiv:hep-ph/0603188
[14]	M. Gustafsson, PoS CHARGED, 2010:030 (2010), arXiv:1106.1719
[15]	Daijiro Suematsu, Takashi Toma, Tetsuro Yoshida, Phys. Rev. D, 79:093004 (2009), arXiv:0903.0287
[16]	D. Schmidt, T Schwetz, and T. Toma, Phys. Rev. D, 85:073009 (2012), arXiv:1201.0906
[17]	T. Toma and A. Vicente, JHEP, 01:160 (2014), arXiv:1312.2840
[18]	A. Vicente, C E. Yaguna, JHEP, 02:144 (2015), arXiv:1412.2545
[19]	G. Altarelli, F. Ferugilo, Rev. Mod. Phys., 82:2701 (2010); G. Altarelli, F. Ferugilo, L. Merlo, and E. Stamou, JHEP, 08:021 (2012), arXiv:1205.4670; S. F. King and C. Luhn, Rept. Prog. Phys., 76:056201 (2013), arXiv:1301.1340; S. F. King, A. Merle, S. Morisi et al, New Journ. Phys., 16:045018 (2014); H. Isimori et al, Prog. Theor. Phys. Suppl., 183:1 (2010)
[20]	P. F. Harrison, D. H. Perkins, and W.G. Scott, Phys. Lett. B, 458:79 (1999); Phys. Lett. B, 530:167 (2002); Z. Z. Xing, Phys. Lett. B, 533:85 (2002); P. F. Harrison and W. G. Scott, Phys. Lett. B, 535:163 (2002); Phys. Lett. B, 557:76 (2003); X.-G. He and A. Zee, Phys. Lett. B, 560:87 (2003); L. Wolfenstein, Phys. Rev. D, 18:958 (1978); Y. Yamanaka, H. Sugawara, and S. Pakvasa, Phys. Rev. D, 25:1895 (1982); D, 29:2135(E) (1984); N. Li and B.-Q. Ma, Phys. Rev. D, 71:017302 (2005), arXiv:hep-ph/0412126
[21]	M. Sruthilaya, C. Soumya, K.N. Deepthi et al, New J. Phys., 17:083028 (2015), arXiv:1408.4392
[22]	K. Griest and D. Seckel, Phys. Rev. D, 43:3191 (1991)
[23]	K. A. Olive et al, Particle Data Group Collaboration, Chin. Phys. C, 38:090001 (2014)

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Shivaramakrishna Singirala. Implications of fermionic dark matter on recent neutrino oscillation data[J]. Chinese Physics C, 2017, 41(4): 043102. doi: 10.1088/1674-1137/41/4/043102

Shivaramakrishna Singirala. Implications of fermionic dark matter on recent neutrino oscillation data[J]. Chinese Physics C, 2017, 41(4): 043102. doi: 10.1088/1674-1137/41/4/043102 shu

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Received: 2016-07-14
Revised: 2016-11-23

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This work is supported by DST-Inspire Fellowship division-IF130927

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沈阳化工大学材料科学与工程学院沈阳 110142

Implications of fermionic dark matter on recent neutrino oscillation data

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