Journal of High Energy Physics

, 2014:68 | Cite as

Phenomenology in supersymmetric neutrinophilic Higgs model with sneutrino dark matter

Open Access
Article

Abstract

We study a supersymmetric neutrinophilic Higgs model with large neutrino Yukawa couplings where neutrinos are Dirac particles and the lightest right-handed (RH) sneutrino is the lightest supersymmetric particle (LSP) as a dark matter candidate. Neutrinophilic Higgs bosons need to be rather heavy by the precise determination of the muon decay width and dark radiation constraints for large Yukawa couplings. From the Large Hadron Collider constraints, neutrinophilic Higgsino mass need to be heavier than several hundred GeV or close to the RH sneutrino LSP mass. The latter case is interesting because the muon anomalous magnetic dipole moment can be explained with a relatively large lightest neutrino mass, if RH sneutrino mixings are appropriately fine tuned in order to avoid stringent lepton flavor violation constraints. Dark matter is explained by asymmetric RH sneutrino dark matter in the favoured region by the muon anomalous magnetic dipole moment. In other regions, RH sneutrino could be an usual WIMP dark matter.

Keywords

Supersymmetry Phenomenology 

Notes

Open Access

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References

  1. [1]
    ATLAS collaboration, Observation of a new particle in the search for the standard model Higgs boson with the ATLAS detector at the LHC, Phys. Lett. B 716 (2012) 1 [arXiv:1207.7214] [INSPIRE].ADSGoogle Scholar
  2. [2]
    CMS collaboration, Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC, Phys. Lett. B 716 (2012) 30 [arXiv:1207.7235] [INSPIRE].ADSGoogle Scholar
  3. [3]
    T. Yanagida, Horizontal symmetry and masses of neutrinos, in Proceedings of the Workshop on the Baryon Number of the Universe and Unified Theories, Tsukuba Japan, 13-14 Feb 1979, A. Sawada and A. Sugamoto eds., pg. 95 [INSPIRE].
  4. [4]
    M. Gell-Mann, P. Ramond and R. Slansky, Complex spinors and unified theories, in Proceedings of the Supergravity Workshop, Stony Brook, New York U.S.A., 27-28 Sep 1979, P. Van Nieuwenhuizen and D.Z. Freedman eds., pg. 315 [arXiv:1306.4669] [INSPIRE].
  5. [5]
    R.N. Mohapatra and G. Senjanović, Neutrino mass and spontaneous parity violation, Phys. Rev. Lett. 44 (1980) 912 [INSPIRE].CrossRefADSGoogle Scholar
  6. [6]
    E. Ma, Naturally small seesaw neutrino mass with no new physics beyond the TeV scale, Phys. Rev. Lett. 86 (2001) 2502 [hep-ph/0011121] [INSPIRE].CrossRefADSGoogle Scholar
  7. [7]
    F. Wang, W. Wang and J.M. Yang, Split two-Higgs-doublet model and neutrino condensation, Europhys. Lett. 76 (2006) 388 [hep-ph/0601018] [INSPIRE].CrossRefADSGoogle Scholar
  8. [8]
    S. Gabriel and S. Nandi, A new two Higgs doublet model, Phys. Lett. B 655 (2007) 141 [hep-ph/0610253] [INSPIRE].CrossRefADSGoogle Scholar
  9. [9]
    K.-Y. Choi and O. Seto, A Dirac right-handed sneutrino dark matter and its signature in the gamma-ray lines, Phys. Rev. D 86 (2012) 043515 [Erratum ibid. D 86 (2012) 089904] [arXiv:1205.3276] [INSPIRE].
  10. [10]
    K.-Y. Choi and O. Seto, Light Dirac right-handed sneutrino dark matter, Phys. Rev. D 88 (2013) 035005 [arXiv:1305.4322] [INSPIRE].ADSGoogle Scholar
  11. [11]
    P. Mitropoulos, Right-handed sneutrinos as asymmetric DM and neutrino masses from neutrinophilic Higgs bosons, JCAP 11 (2013) 008 [arXiv:1307.2823] [INSPIRE].CrossRefADSGoogle Scholar
  12. [12]
    N. Haba and O. Seto, Low scale thermal leptogenesis in neutrinophilic Higgs doublet models, Prog. Theor. Phys. 125 (2011) 1155 [arXiv:1102.2889] [INSPIRE].CrossRefMATHADSGoogle Scholar
  13. [13]
    N. Haba and O. Seto, Thermal leptogenesis in a supersymmetric neutrinophilic Higgs model, Phys. Rev. D 84 (2011) 103524 [arXiv:1106.5354] [INSPIRE].ADSGoogle Scholar
  14. [14]
    N. Haba, O. Seto and Y. Yamaguchi, Resonant leptogenesis with mild degeneracy, Phys. Rev. D 87 (2013) 123540 [arXiv:1305.2484] [INSPIRE].ADSGoogle Scholar
  15. [15]
    Particle Data Group collaboration, J. Beringer et al., Review of particle physics, Phys. Rev. D 86 (2012) 010001 [INSPIRE].ADSGoogle Scholar
  16. [16]
    Planck collaboration, P.A.R. Ade et al., Planck 2013 results. XVI. Cosmological parameters, arXiv:1303.5076 [INSPIRE].
  17. [17]
    T. Fukuyama and K. Tsumura, Detecting Majorana nature of neutrinos in muon decay, arXiv:0809.5221 [INSPIRE].
  18. [18]
    W. Fetscher, H.J. Gerber and K.F. Johnson, Muon decay: complete determination of the interaction and comparison with the standard model, Phys. Lett. B 173 (1986) 102 [INSPIRE].CrossRefADSGoogle Scholar
  19. [19]
    P. Herczeg, The nature of neutrinos in muon decay and physics beyond the standard model, Los Alamos Sci. 25 (1997) 128 [INSPIRE].Google Scholar
  20. [20]
    W.J. Marciano, Fermi constants andnew physics’, Phys. Rev. D 60 (1999) 093006 [hep-ph/9903451] [INSPIRE].ADSGoogle Scholar
  21. [21]
    J. Erler and M.J. Ramsey-Musolf, Low energy tests of the weak interaction, Prog. Part. Nucl. Phys. 54 (2005) 351 [hep-ph/0404291] [INSPIRE].CrossRefADSGoogle Scholar
  22. [22]
    CHARM-II collaboration, P. Vilain et al., A precise measurement of the cross-section of the inverse muon decay ν μ + e μ + ν e, Phys. Lett. B 364 (1995) 121 [INSPIRE].CrossRefADSGoogle Scholar
  23. [23]
    S.M. Davidson and H.E. Logan, Dirac neutrinos from a second Higgs doublet, Phys. Rev. D 80 (2009) 095008 [arXiv:0906.3335] [INSPIRE].ADSGoogle Scholar
  24. [24]
    S.M. Davidson and H.E. Logan, LHC phenomenology of a two-Higgs-doublet neutrino mass model, Phys. Rev. D 82 (2010) 115031 [arXiv:1009.4413] [INSPIRE].ADSGoogle Scholar
  25. [25]
    N. Haba and K. Tsumura, ν-two Higgs doublet model and its collider phenomenology, JHEP 06 (2011) 068 [arXiv:1105.1409] [INSPIRE].CrossRefADSGoogle Scholar
  26. [26]
    LEP SUSY Working Group, ALEPH, DELPHI, L3, OPAL experiments, Notes LEPSUSYWG/01-03.1 and 04-01.1, http://lepsusy.web.cern.ch/lepsusy/Welcome.html.
  27. [27]
    P.J. Fox, R. Harnik, J. Kopp and Y. Tsai, LEP shines light on dark matter, Phys. Rev. D 84 (2011) 014028 [arXiv:1103.0240] [INSPIRE].ADSGoogle Scholar
  28. [28]
    J. Guo, Z. Kang, J. Li, T. Li and Y. Liu, Simplified supersymmetry with sneutrino LSP at 8 TeV LHC, arXiv:1312.2821 [INSPIRE].
  29. [29]
    MEG collaboration, J. Adam et al., New constraint on the existence of the μ +e +γ decay, Phys. Rev. Lett. 110 (2013) 201801 [arXiv:1303.0754] [INSPIRE].CrossRefADSGoogle Scholar
  30. [30]
    BaBar collaboration, B. Aubert et al., Searches for lepton flavor violation in the decays τ ±e ±γ and τ ±μ ±γ, Phys. Rev. Lett. 104(2010) 021802 [arXiv:0908.2381] [INSPIRE].CrossRefADSGoogle Scholar
  31. [31]
    Muon G-2 collaboration, G.W. Bennett et al., Final report of the E821 muon anomalous magnetic moment measurement at BNL, Phys. Rev. D 73 (2006) 072003 [hep-ex/0602035] [INSPIRE].ADSGoogle Scholar
  32. [32]
    K. Hagiwara, R. Liao, A.D. Martin, D. Nomura and T. Teubner, (g − 2)μ and α(M Z2) re-evaluated using new precise data, J. Phys. G 38 (2011) 085003 [arXiv:1105.3149] [INSPIRE].CrossRefADSGoogle Scholar
  33. [33]
    S.M. Barr, R.S. Chivukula and E. Farhi, Electroweak fermion number violation and the production of stable particles in the early universe, Phys. Lett. B 241 (1990) 387 [INSPIRE].CrossRefADSGoogle Scholar
  34. [34]
    S.M. Barr, Baryogenesis, sphalerons and the cogeneration of dark matter, Phys. Rev. D 44 (1991) 3062 [INSPIRE].ADSGoogle Scholar
  35. [35]
    D.B. Kaplan, A single explanation for both the baryon and dark matter densities, Phys. Rev. Lett. 68 (1992) 741 [INSPIRE].CrossRefADSGoogle Scholar
  36. [36]
    S.D. Thomas, Baryons and dark matter from the late decay of a supersymmetric condensate, Phys. Lett. B 356 (1995) 256 [hep-ph/9506274] [INSPIRE].CrossRefADSGoogle Scholar
  37. [37]
    D. Hooper, J. March-Russell and S.M. West, Asymmetric sneutrino dark matter and the Ωb /ΩDM puzzle, Phys. Lett. B 605 (2005) 228 [hep-ph/0410114] [INSPIRE].CrossRefADSGoogle Scholar
  38. [38]
    R. Kitano and I. Low, Dark matter from baryon asymmetry, Phys. Rev. D 71 (2005) 023510 [hep-ph/0411133] [INSPIRE].ADSGoogle Scholar
  39. [39]
    D.E. Kaplan, M.A. Luty and K.M. Zurek, Asymmetric dark matter, Phys. Rev. D 79 (2009) 115016 [arXiv:0901.4117] [INSPIRE].ADSGoogle Scholar
  40. [40]
    M.L. Graesser, I.M. Shoemaker and L. Vecchi, Asymmetric WIMP dark matter, JHEP 10 (2011) 110 [arXiv:1103.2771] [INSPIRE].CrossRefADSGoogle Scholar
  41. [41]
    H. Iminniyaz, M. Drees and X. Chen, Relic abundance of asymmetric dark matter, JCAP 07 (2011) 003 [arXiv:1104.5548] [INSPIRE].CrossRefADSGoogle Scholar
  42. [42]
    D.G. Cerdeño, C. Muñoz and O. Seto, Right-handed sneutrino as thermal dark matter, Phys. Rev. D 79 (2009) 023510 [arXiv:0807.3029] [INSPIRE].ADSGoogle Scholar
  43. [43]
    D.G. Cerdeño and O. Seto, Right-handed sneutrino dark matter in the NMSSM, JCAP 08 (2009) 032 [arXiv:0903.4677] [INSPIRE].CrossRefADSGoogle Scholar
  44. [44]
    D.G. Cerdeño, J.-H. Huh, M. Peiro and O. Seto, Very light right-handed sneutrino dark matter in the NMSSM, JCAP 11 (2011) 027 [arXiv:1108.0978] [INSPIRE].CrossRefADSGoogle Scholar
  45. [45]
    D.G. Cerdeño, V. Martín-Lozano and O. Seto, Displaced vertices and long-lived charged particles in the NMSSM with right-handed sneutrinos, JHEP 05 (2014) 035 [arXiv:1311.7260] [INSPIRE].CrossRefADSGoogle Scholar
  46. [46]
    D.G. Cerdeño, M. Peiró and S. Robles, Low-mass right-handed sneutrino dark matter: SuperCDMS and LUX constraints and the galactic centre gamma-ray excess, JCAP 08 (2014) 005 [arXiv:1404.2572] [INSPIRE].CrossRefADSGoogle Scholar
  47. [47]
    K.-Y. Choi, E.J. Chun and C.S. Shin, Dark matter asymmetry in supersymmetric Dirac leptogenesis, Phys. Lett. B 723 (2013) 90 [arXiv:1211.5409] [INSPIRE].MathSciNetCrossRefADSGoogle Scholar
  48. [48]
    Z. Kang, J. Li, T. Li, T. Liu and J. Yang, Asymmetric sneutrino dark matter in the NMSSM with minimal inverse seesaw, arXiv:1102.5644 [INSPIRE].
  49. [49]
    J. Guo, Z. Kang, T. Li and Y. Liu, Higgs boson mass and complex sneutrino dark matter in the supersymmetric inverse seesaw models, JHEP 02 (2014) 080 [arXiv:1311.3497] [INSPIRE].CrossRefADSGoogle Scholar
  50. [50]
    S. Kanemura, N. Machida and T. Shindou, Radiative neutrino mass, dark matter and electroweak baryogenesis from the supersymmetric gauge theory with confinement, arXiv:1405.5834 [INSPIRE].
  51. [51]
    LUX collaboration, D.S. Akerib et al., First results from the LUX dark matter experiment at the Sanford Underground Research Facility, Phys. Rev. Lett. 112 (2014) 091303 [arXiv:1310.8214] [INSPIRE].CrossRefADSGoogle Scholar
  52. [52]
    S. Profumo and L. Ubaldi, Cosmic ray-dark matter scattering: a new signature of (asymmetric) dark matter in the gamma ray sky, JCAP 08 (2011) 020 [arXiv:1106.4568] [INSPIRE].CrossRefADSGoogle Scholar
  53. [53]
    A. Aboubrahim, T. Ibrahim and P. Nath, Radiative decays of cosmic background neutrinos in extensions of MSSM with a vector like lepton generation, Phys. Rev. D 88 (2013) 013019 [arXiv:1306.2275] [INSPIRE].ADSGoogle Scholar
  54. [54]
  55. [55]
    J. Hisano, T. Moroi, K. Tobe and M. Yamaguchi, Lepton flavor violation via right-handed neutrino Yukawa couplings in supersymmetric standard model, Phys. Rev. D 53 (1996) 2442 [hep-ph/9510309] [INSPIRE].ADSGoogle Scholar
  56. [56]
    J. Hisano and K. Tobe, Neutrino masses, muon g − 2 and lepton flavor violation in the supersymmetric seesaw model, Phys. Lett. B 510 (2001) 197 [hep-ph/0102315] [INSPIRE].CrossRefADSGoogle Scholar

Copyright information

© The Author(s) 2014

Authors and Affiliations

  1. 1.Korea Astronomy and Space Science InstituteDaejonRepublic of Korea
  2. 2.Department of Life Science and TechnologyHokkai-Gakuen UniversitySapporoJapan
  3. 3.New High Energy Theory Center, Department of Physics and AstronomyRutgers UniversityPiscatawayU.S.A.

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