\begin{document}$U(1)_{B-L}$\end{document} symmetry already present in the Standard Model. In addition, we propose a general framework in which the \begin{document}$U(1)_{B-L}$\end{document} symmetry is spontaneously broken into an even \begin{document}${\cal{Z}}_{2n}$\end{document} subgroup, setting the general conditions for neutrinos to be Majorana and for dark matter stability to exist in terms of the residual \begin{document}${\cal{Z}}_{2n}$\end{document}. As an example, under this general framework, we build a class of simple models where, in a scotogenic manner, the dark matter candidate is the lightest particle running inside the mass loop of a neutrino. The global \begin{document}$U(1)_{B-L}$\end{document} symmetry in our framework, being anomaly free, can also be gauged in a straightforward manner leading to a richer phenomenology."> Scotogenic dark symmetry as a residual subgroup of Standard Model symmetries -
  • [1]

    CMS Collaboration, S. Chatrchyanet al., Phys. Lett. B,716: 30-61 (2012), arXiv:1207.7235[hep-ex

  • [2]

    ATLAS Collaboration, G. Aadet al., Phys. Lett. B,716: 1-29 (2012), arXiv:1207.7214[hep-ex

  • [3]

    LUX Collaboration, D. S. Akeribet al., Phys. Rev. Lett.,118(2): 021303 (2017), arXiv:1608.07648 [astro-ph.CO

  • [4]

    XENON Collaboration, E. Aprileet al., Phys. Rev. Lett.,121(11): 111302 (2018), arXiv:1805.12562 [astro-ph.CO

  • [5]

    Planck Collaboration, N. Aghanimet al., arXiv: 1807.06209[astro-ph.CO]

  • [6]

    A. B. McDonald, Rev. Mod. Phys.,88(3): 030502 (2016)

  • [7]

    T. Kajita, Rev. Mod. Phys.,88(3): 030501 (2016)

  • [8]

    Daya Bay Collaboration, F. P. Anet al., Phys. Rev. Lett.,108: 171803 (2012), arXiv:1203.1669 [hep-ex

  • [9]

    T2K Collaboration, K. Abeet al., Phys. Rev. Lett.,118(15): 151801 (2017), arXiv:1701.00432 [hep-ex

  • [10]

    P. F. De Salas, S. Gariazzo, O. Menaet al., Front. Astron. Space Sci.,5: 36 (2018), arXiv:1806.11051[hep-ph

  • [11]

    P. F. de Salas, D. V. Forero, C. A. Terneset al., Phys. Lett. B,782: 633-640 (2018), arXiv:1708.01186[hep-ph

  • [12]

    E. Ma, Phys. Rev. Lett.,81: 1171-1174 (1998), arXiv:hep-ph/9805219[hep-ph

  • [13]

    S. Centelles Chuliá, R. Srivastava, and J. W. F. Valle, Phys. Lett. B,781: 122-128 (2018), arXiv:1802.05722[hep-ph

  • [14]

    P. Minkowski, Phys. Lett. B,67: 421-428 (1977)

  • [15]

    T. Yanagida,Horizontal symmetry and masses of neutrinos, Workshop on the baryon number of the Universe and unified theories, O. Sawada and A. Sugamoto, eds. (1979) 95

  • [16]

    R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett.,44: 912 (1980)

  • [17]

    J. Schechter and J. W. F. Valle, Phys. Rev. D,25: 774 (1982)

  • [18]

    J. Schechter and J. Valle, Phys. Rev. D,22: 2227 (1980)

  • [19]

    R. Foot, H. Lew, X. G. Heet al., Z. Phys. C,44: 441 (1989)

  • [20]

    A. Zee, Phys. Lett. B,93: 389 (1980)

  • [21]

    K. S. Babu, Phys. Lett. B,203: 132-136 (1988)

  • [22]

    E. Ma, Phys. Rev. D,73: 077301 (2006), arXiv:hep-ph/0601225[hep-ph

  • [23]

    F. Bonnet, M. Hirsch, T. Otaet al., JHEP,07: 153 (2012), arXiv:1204.5862[hep-ph

  • [24]

    E. Ma, Phys. Rev. Lett.,112: 091801 (2014), arXiv:1311.3213[hep-ph

  • [25]

    D. Aristizabal Sierra, A. Degee, L. Dorameet al., JHEP,03: 040 (2015), arXiv:1411.7038 [hep-ph

  • [26]

    E. Ma, Phys. Rev. Lett.,115(1): 011801 (2015), arXiv:1502.02200[hep-ph

  • [27]

    A. E. Cárcamo Hernández, S. Kovalenko, and I. Schmidt, JHEP,02: 125 (2017), arXiv:1611.09797[hep-ph

  • [28]

    R. Cepedello, M. Hirsch, and J. Helo, JHEP,1707: 079 (2017), arXiv:1705.01489[hep-ph

  • [29]

    N. Bernal, A. E. Cárcamo Hernández, I. de Medeiros Varzielaset al., JHEP,05: 053 (2018), arXiv:1712.02792[hep-ph

  • [30]

    R. Cepedello, R. M. Fonseca, and M. Hirsch, JHEP,1810: 197 (2018), arXiv:1807.00629 [hep-ph

  • [31]

    G. Anamiati, O. Castillo-Felisola, R. M. Fonsecaet al., JHEP,12: 066 (2018), arXiv:1806.07264[hep-ph

  • [32]

    A. E. Cárcamo Hernández, S. Kovalenko, R. Pasechniket al., arXiv: 1901.02764[hep-ph]

  • [33]

    M. Hirsch, R. Srivastava, and J. W. F. Valle, Phys. Lett. B,781: 302-305 (2018), arXiv:1711.06181[hep-ph

  • [34]

    C. Bonilla, S. Centelles Chuliá, R. Cepedelloet al., arXiv: 1812.01599 [hep-ph]

  • [35]

    S. Centelles Chuliá, E. Ma, R. Srivastava, and J. W. F. Valle, Phys. Lett. B,767: 209-213 (2017), arXiv:1606.04543[hep-ph

  • [36]

    J. C. Montero and V. Pleitez, Phys. Lett. B,675: 64-68 (2009), arXiv:0706.0473[hep-ph

  • [37]

    E. Ma and R. Srivastava, Phys. Lett. B,741: 217-222 (2015), arXiv:1411.5042 [hep-ph

  • [38]

    E. Ma, N. Pollard, R. Srivastavaet al., Phys. Lett. B,750: 135-138 (2015), arXiv:1507.03943[hep-ph

  • [39]

    E. Ma and R. Srivastava, Mod. Phys. Lett. A,30(26): 1530020 (2015), arXiv:1504.00111[hep-ph

  • [40]

    S.-Y. Ho, T. Toma, and K. Tsumura, Phys. Rev. D,94(3): 033007 (2016), arXiv:1604.07894[hep-ph

  • [41]

    E. Ma, N. Pollard, O. Popovet al., Mod. Phys. Lett. A,31(27): 1650163 (2016), arXiv:1605.00991[hep-ph

  • [42]

    S. Patra, W. Rodejohann, and C. E. Yaguna, JHEP,09: 076 (2016), arXiv:1607.04029[hep-ph

  • [43]

    W. Wang and Z.-L. Han, arXiv: 1611.03240[hep-ph]. [JHEP04, 166(2017)]

  • [44]

    W. Wang, R. Wang, Z.-L. Hanet al., Eur. Phys. J. C,77(23): 889 (2017), arXiv:1705.00414[hep-ph

  • [45]

    D. Nanda and D. Borah, Phys. Rev. D,96(11): 115014 (2017), arXiv:1709.08417[hep-ph

  • [46]

    Z.-L. Han and W. Wang, Eur. Phys. J. C,78(10): 839 (2018), arXiv:1805.02025[hep-ph

  • [47]

    S. K. Kang and O. Popov, Phys. Rev. D,98(11): 115025 (2018), arXiv:1807.07988[hep-ph

  • [48]

    T. Modak, S. Sadhukhan, and R. Srivastava, Phys. Lett. B,756: 405-412 (2016), arXiv:1601.00836[hep-ph

  • [49]

    S. Singirala, R. Mohanta, and S. Patra, Eur. Phys. J. Plus,133(11): 477 (2018), arXiv:1704.01107[hep-ph

  • [50]

    V. De Romeri, E. Fernandez-Martinez, J. Gehrleinet al., JHEP,10: 169 (2017), arXiv:1707.08606[hep-ph

  • [51]

    T. Nomura and H. Okada, Eur. Phys. J. C,78(3): 189 (2018), arXiv:1708.08737[hep-ph

  • [52]

    A. Das, N. Okada, and D. Raut, Eur. Phys. J. C,78(9): 696 (2018), arXiv:1711.09896[hep-ph

  • [53]

    N. Okada, S. Okada, and D. Raut, arXiv: 1811.11927[hep-ph]

  • [54]

    J. Calle, D. Restrepo, C. E. Yagunaet al., arXiv: 1812.05523[hep-ph]

  • [55]

    F. Bazzocchi, M. Lattanzi, S. Riemer-Sørensenet al., JCAP,08: 013 (2008), arXiv:0805.2372[astro-ph

  • [56]

    M. Lattanzi, S. Riemer-Sorensen, M. Tortolaet al., Phys. Rev. D,88(6): 063528 (2013), arXiv:1303.4685[astro-ph.HE

  • [57]

    M. Lattanzi, S. Riemer-Sørensen, M. Tortolaet al., Nucl. Instrum. Meth. A,742: 154-157 (2014)

  • [58]

    C. Bonilla, J. W. F. Valle, and J. C. Romão, Phys. Rev. D,91(11): 113015 (2015), arXiv:1502.01649[hep-ph

  • [59]

    J.-L. Kuo, M. Lattanzi, K. Cheunget al., JCAP,12: 026 (2018), arXiv:1803.05650[astro-ph.CO

  • [60]

    T. Brune and H. Päs, Phys. Rev. D,99(9): 096005 (2019), arXiv:1808.08158[hep-ph

  • [61]

    D. Fontes, J. C. Romao, and J. W. Valle, JHEP,10: 245 (2019), arXiv:1908.09587[hep-ph

  • [62]

    G. Passarino and M. J. G. Veltman, Nucl. Phys. B,160: 151-207 (1979)

Baidu
map