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Chinese Physics C> 2018, Vol. 42> Issue(10) : 103101 DOI: 10.1088/1674-1137/42/10/103101

Phenomenology of colored radiative neutrino mass model and its implications on cosmic-ray observations

  • 1.

      Center for High Energy Physics, Peking University, Beijing 100871, China

  • 2.

      School of Physics and Technology, University of Jinan, Jinan, Shandong 250022, China

  • 3.

      State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China

  • 4.

     Center for High Energy Physics, Peking University, Beijing 100871, China

  • 5.

     State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China

  • 6.

     School of Physics, Nankai University, Tianjin 300071, China

  • We extend the colored Zee-Babu model with a gauged U(1)B-L symmetry, and a scalar singlet dark matter (DM) candidate S. The spontaneous breaking of U(1)B-L leaves a residual Z2 symmetry that stabilizes the DM, and generates a tiny neutrino mass at the two-loop level with the color seesaw mechanism. After investigating the DM and flavor phenomenology of this model systematically, we further focus on its imprint on two cosmic-ray anomalies:The Fermi-LAT gamma-ray excess at the Galactic Center (GCE), and the PeV ultra-high energy (UHE) neutrino events at the IceCube. We found that the Fermi-LAT GCE spectrum can be well-fitted by DM annihilation into a pair of on-shell singlet Higgs mediators while being compatible with the constraints from the relic density, direct detections, and dwarf spheroidal galaxies, in the Milky Way. Although the UHE neutrino events at the IceCube could be accounted for by the resonance production of a TeV-scale leptoquark, the relevant Yukawa couplings have been severely limited by the current low-energy flavor experiments. We subsequently derive the IceCube limits on the Yukawa couplings by employing its latest six-year data.
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    [1] L. Goodenough and D. Hooper, arXiv:0910.2998[hep-ph]
    [2] D. Hooper and L. Goodenough, Phys. Lett. B, 697:412 (2011), arXiv:1010.2752[hep-ph]
    [3] D. Hooper and T. Linden, Phys. Rev. D, 84:123005 (2011), arXiv:1110.0006[astro-ph.HE]
    [4] K. N. Abazajian and M. Kaplinghat, Phys. Rev. D, 86:083511 (2012) Erratum:[Phys. Rev. D, 87:129902 (2013)], arXiv:1207.6047[astro-ph.HE]
    [5] C. Gordon and O. Macias, Phys. Rev. D, 88(8):083521 (2013); Erratum:[Phys. Rev. D, 89(4):049901 (2014)], arXiv:1306.5725[astro-ph.HE]
    [6] K. N. Abazajian, N. Canac, S. Horiuchi, and M. Kaplinghat, Phys. Rev. D, 90(2):023526 (2014), arXiv:1402.4090[astroph.HE]
    [7] T. Daylan, D. P. Finkbeiner, D. Hooper, T. Linden, S. K. N. Portillo, N. L. Rodd, and T. R. Slatyer, Phys. Dark Univ., 12:1 (2016), arXiv:1402.6703[astro-ph.HE]
    [8] F. Calore, I. Cholis and C. Weniger, JCAP, 1503:038 (2015), arXiv:1409.0042[astro-ph.CO]
    [9] Q. Yuan and B. Zhang, JHEAp, 3-4:1 (2014), arXiv:1404.2318[astro-ph.HE]
    [10] R. Bartels, S. Krishnamurthy, and C. Weniger, Phys. Rev. Lett., 116(5):051102 (2016), arXiv:1506.05104[astroph.HE]
    [11] S. K. Lee, M. Lisanti, B. R. Safdi, T. R. Slatyer, and W. Xue, Phys. Rev. Lett., 116(5):051103 (2016), arXiv:1506.05124[astro-ph.HE]
    [12] M. Ackermann et al (Fermi-LAT Collaboration), Astrophys. J., 840(1):43 (2017), arXiv:1704.03910[astro-ph.HE]
    [13] M. Ajello et al (Fermi-LAT Collaboration), arXiv:1705.00009[astro-ph.HE]
    [14] D. Haggard, C. Heinke, D. Hooper, and T. Linden, JCAP, 1705(5):056 (2017), arXiv:1701.02726[astro-ph.HE]
    [15] R. Bartels, D. Hooper, T. Linden, S. Mishra-Sharma, N. L. Rodd, B. R. Safdi, and T. R. Slatyer, arXiv:1710.10266[astro-ph.HE]
    [16] P. Agrawal, B. Batell, P. J. Fox, and R. Harnik, JCAP, 1505:011 (2015), arXiv:1411.2592[hep-ph]
    [17] J. M. Cline, G. Dupuis, Z. Liu, and W. Xue, Phys. Rev. D, 91(11):115010 (2015), arXiv:1503.08213[hep-ph]
    [18] G. Elor, N. L. Rodd, and T. R. Slatyer, Phys. Rev. D, 91:103531 (2015), arXiv:1503.01773[hep-ph]
    [19] F. Calore, I. Cholis, C. McCabe, and C. Weniger, Phys. Rev. D, 91(6):063003 (2015), arXiv:1411.4647[hep-ph]
    [20] M. Cirelli, D. Gaggero, G. Giesen, M. Taoso, and A. Urbano, JCAP, 1412(12):045 (2014), arXiv:1407.2173[hep-ph]
    [21] P. A. R. Ade et al (Planck Collaboration), arXiv:1502.01589[astro-ph.CO]
    [22] T. R. Slatyer, arXiv:1506.03811[hep-ph]
    [23] B. Dutta, Y. Gao, T. Ghosh, and L. E. Strigari, Phys. Rev. D, 92(7):075019 (2015), arXiv:1508.05989[hep-ph]
    [24] A. Berlin, D. Hooper, and S. D. McDermott, Phys. Rev. D, 89(11):115022 (2014), arXiv:1404.0022[hep-ph]
    [25] A. Alves, S. Profumo, F. S. Queiroz, and W. Shepherd, Phys. Rev. D, 90(11):115003 (2014), arXiv:1403.5027[hep-ph]
    [26] P. Agrawal, B. Batell, D. Hooper, and T. Lin, Phys. Rev. D, 90(6):063512 (2014), arXiv:1404.1373[hep-ph]
    [27] M. Abdullah, A. DiFranzo, A. Rajaraman, T. M. P. Tait, P. Tanedo, and A. M. Wijangco, Phys. Rev. D, 90:035004 (2014), arXiv:1404.6528[hep-ph]
    [28] A. Martin, J. Shelton, and J. Unwin, Phys. Rev. D, 90(10):103513 (2014), arXiv:1405.0272[hep-ph]
    [29] A. Berlin, P. Gratia, D. Hooper, and S. D. McDermott, Phys. Rev. D, 90(1):015032 (2014), arXiv:1405.5204[hep-ph]
    [30] T. Mondal and T. Basak, Phys. Lett. B, 744:208 (2015), arXiv:1405.4877[hep-ph]
    [31] J. M. Cline, G. Dupuis, Z. Liu, and W. Xue, JHEP, 1408:131 (2014), arXiv:1405.7691[hep-ph]
    [32] C. Cheung, M. Papucci, D. Sanford, N. R. Shah, and K. M. Zurek, Phys. Rev. D, 90(7):075011 (2014), arXiv:1406.6372[hep-ph]
    [33] P. Ko and Y. Tang, JCAP, 1501:023 (2015), arXiv:1407.5492[hep-ph]
    [34] M. Cahill-Rowley, J. Gainer, J. Hewett, and T. Rizzo, JHEP, 1502:057 (2015), arXiv:1409.1573[hep-ph]
    [35] M. Freytsis, D. J. Robinson, and Y. Tsai, Phys. Rev. D, 91(3):035028 (2015), arXiv:1410.3818[hep-ph]
    [36] M. Kaplinghat, T. Linden, and H. B. Yu, Phys. Rev. Lett., 114(21):211303 (2015), arXiv:1501.03507[hep-ph]
    [37] C. H. Chen and T. Nomura, Phys. Lett. B, 746:351 (2015), arXiv:1501.07413[hep-ph]
    [38] T. Gherghetta, B. von Harling, A. D. Medina, M. A. Schmidt, and T. Trott, Phys. Rev. D, 91:105004 (2015), arXiv:1502.07173[hep-ph]
    [39] J. Cao, L. Shang, P. Wu, J. M. Yang, and Y. Zhang, JHEP, 1510:030 (2015), arXiv:1506.06471[hep-ph]
    [40] K. Freese, A. Lopez, N. R. Shah, and B. Shakya, JHEP, 1604:059 (2016), arXiv:1509.05076[hep-ph]
    [41] M. Duerr, P. Fileviez P..??rez and J. Smirnov, JHEP, 1606:008 (2016), arXiv:1510.07562[hep-ph]
    [42] Y. Cai and A. P. Spray, JHEP, 1606:156 (2016), arXiv:1511.09247[hep-ph]
    [43] Y. L. Tang and S. h. Zhu, JHEP, 1603:043 (2016), arXiv:1512.02899[hep-ph]
    [44] R. Ding, Z. L. Han, Y. Liao, and W. P. Xie, JHEP, 1605:030 (2016), arXiv:1601.06355[hep-ph]
    [45] M. E. Krauss, T. Opferkuch, F. Staub, and M. W. Winkler, Phys. Dark Univ., 14:29 (2016), arXiv:1605.05327[hep-ph]
    [46] M. Escudero, S. J. Witte, and D. Hooper, arXiv:1709.07002[hep-ph]
    [47] M. G. Aartsen et al (IceCube Collaboration), arXiv:1510.05223[astro-ph.HE]
    [48] M. G. Aartsen et al (IceCube Collaboration), Phys. Rev. Lett., 111:021103 (2013), arXiv:1304.5356[astro-ph.HE]
    [49] M. G. Aartsen et al (IceCube Collaboration), Science, 342:1242856 (2013), arXiv:1311.5238[astro-ph.HE]
    [50] M. G. Aartsen et al (IceCube Collaboration), Phys. Rev. Lett., 113:101101 (2014), arXiv:1405.5303[astro-ph.HE]
    [51] M. G. Aartsen et al (IceCube Collaboration), arXiv:1710.01191[astro-ph.HE]
    [52] I. Cholis and D. Hooper, JCAP, 1306:030 (2013), arXiv:1211.1974[astro-ph.HE]
    [53] L. A. Anchordoqui et al, JHEAp, 1-2:1 (2014), arXiv:1312.6587[astro-ph.HE]
    [54] K. Murase, AIP Conf. Proc., 1666:040006 (2015), arXiv:1410.3680[hep-ph]
    [55] B. Feldstein, A. Kusenko, S. Matsumoto, and T. T. Yanagida, Phys. Rev. D, 88(1):015004 (2013), arXiv:1303.7320[hepph]
    [56] A. Esmaili and P. D. Serpico, JCAP, 1311:054 (2013), arXiv:1308.1105[hep-ph]
    [57] Y. Ema, R. Jinno and T. Moroi, Phys. Lett. B, 733:120 (2014), arXiv:1312.3501[hep-ph]
    [58] A. Bhattacharya, M. H. Reno, and I. Sarcevic, JHEP, 1406:110 (2014), arXiv:1403.1862[hep-ph]
    [59] T. Higaki, R. Kitano, and R. Sato, JHEP, 1407:044 (2014), arXiv:1405.0013[hep-ph]
    [60] C. Rott, K. Kohri, and S. C. Park, Phys. Rev. D, 92(2):023529 (2015), arXiv:1408.4575[hep-ph]
    [61] A. Esmaili, S. K. Kang, and P. D. Serpico, JCAP, 1412(12):054 (2014), arXiv:1410.5979[hep-ph]
    [62] C. S. Fong, H. Minakata, B. Panes, and R. Zukanovich Funchal, JHEP, 1502:189 (2015), arXiv:1411.5318[hep-ph]
    [63] K. Murase, R. Laha, S. Ando, and M. Ahlers, Phys. Rev. Lett., 115(7):071301 (2015), arXiv:1503.04663[hep-ph]
    [64] C. El Aisati, M. Gustafsson, and T. Hambye, Phys. Rev. D, 92(12):123515 (2015), arXiv:1506.02657[hep-ph]
    [65] S. M. Boucenna, M. Chianese, G. Mangano, G. Miele, S. Morisi, O. Pisanti, and E. Vitagliano, JCAP, 1512(12):055 (2015), arXiv:1507.01000[hep-ph]
    [66] P. Ko and Y. Tang, Phys. Lett. B, 751:81 (2015), arXiv:1508.02500[hep-ph]
    [67] M. Re Fiorentin, V. Niro, and N. Fornengo, JHEP, 1611:022 (2016), arXiv:1606.04445[hep-ph]
    [68] P. S. B. Dev, D. Kazanas, R. N. Mohapatra, V. L. Teplitz, and Y. Zhang, JCAP, 1608(8):034 (2016), arXiv:1606.04517[hep-ph]
    [69] M. Chianese and A. Merle, arXiv:1607.05283[hep-ph]
    [70] T. Cohen, K. Murase, N. L. Rodd, B. R. Safdi, and Y. Soreq, arXiv:1612.05638[hep-ph]
    [71] M. Dhuria and V. Rentala, arXiv:1712.07138[hep-ph]
    [72] Y. Bai, R. Lu and J. Salvado, JHEP, 1601:161 (2016), arXiv:1311.5864[hep-ph]
    [73] K. Griest and M. Kamionkowski, Phys. Rev. Lett., 64:615 (1990)
    [74] L. Hui, Phys. Rev. Lett., 86:3467 (2001),[astro-ph/0102349]
    [75] M. A. Doncheski and R. W. Robinett, Phys. Rev. D, 56:7412 (1997),[hep-ph/9707328]
    [76] L. A. Anchordoqui, C. A. Garcia Canal, H. Goldberg, D. Gomez Dumm, and F. Halzen, Phys. Rev. D, 74:125021 (2006),[hep-ph/0609214]
    [77] I. Alikhanov, JHEP, 1307:093 (2013), arXiv:1305.2905[hepph]
    [78] V. Barger and W. Y. Keung, Phys. Lett. B, 727:190 (2013), arXiv:1305.6907[hep-ph]
    [79] B. Dutta, Y. Gao, T. Li, C. Rott, and L. E. Strigari, Phys. Rev. D, 91:125015 (2015), arXiv:1505.00028[hep-ph]
    [80] U. K. Dey and S. Mohanty, JHEP, 1604:187 (2016), arXiv:1505.01037[hep-ph]
    [81] N. Mileo, A. de la Puente, and A. Szynkman, JHEP, 1611:124 (2016), arXiv:1608.02529[hep-ph]
    [82] P. S. B. Dev, D. K. Ghosh, and W. Rodejohann, Phys. Lett. B, 762:116 (2016), arXiv:1605.09743[hep-ph]
    [83] K. S. Babu and C. N. Leung, Nucl. Phys. B, 619:667 (2001),[hep-ph/0106054]
    [84] W. Rodejohann and C. E. Yaguna, JCAP, 1512(12):032 (2015), arXiv:1509.04036[hep-ph]
    [85] A. Biswas, S. Choubey, and S. Khan, JHEP, 1608:114 (2016), arXiv:1604.06566[hep-ph]
    [86] M. Klasen, F. Lyonnet, and F. S. Queiroz, arXiv:1607.06468[hep-ph]
    [87] J. C. Montero and V. Pleitez, Phys. Lett. B, 675:64 (2009), arXiv:0706.0473[hep-ph]
    [88] W. Wang and Z. L. Han, Phys. Rev. D, 92:095001 (2015), arXiv:1508.00706[hep-ph]
    [89] S. Patra, W. Rodejohann, and C. E. Yaguna, arXiv:1607.04029[hep-ph]
    [90] W. Wang, R. Wang, Z. L. Han, and J. Z. Han, Eur. Phys. J. C, 77(12):889 (2017), arXiv:1705.00414[hep-ph]
    [91] D. Nanda and D. Borah, arXiv:1709.08417[hep-ph]
    [92] Z. L. Han, W. Wang and R. Ding, arXiv:1712.05722[hep-ph]
    [93] J. M. Arnold, B. Fornal, and M. B. Wise, Phys. Rev. D, 88:035009 (2013), arXiv:1304.6119[hep-ph]
    [94] W. F. Chang, S. C. Liou, C. F. Wong, and F. Xu, JHEP, 1610:106 (2016), arXiv:1608.05511[hep-ph]
    [95] G. Cacciapaglia, C. Csaki, G. Marandella, and A. Strumia, Phys. Rev. D, 74:033011 (2006),[hep-ph/0604111]
    [96] M. Aaboud et al (ATLAS Collaboration), arXiv:1707.02424[hep-ex]
    [97] The ATLAS collaboration (ATLAS Collaboration), ATLASCONF-2016-045. G. Aad et al (ATLAS Collaboration), Phys. Rev. D, 90(5):052005 (2014), arXiv:1405.4123[hep-ex]
    [98] CMS Collaboration (CMS Collaboration), CMS-PAS-EXO-16-031; CMS Collaboration (CMS Collaboration), CMS-PASEXO-12-061
    [99] N. Okada and S. Okada, Phys. Rev. D, 93(7):075003 (2016), arXiv:1601.07526[hep-ph]
    [100] N. Okada and S. Okada, Phys. Rev. D, 95(3):035025 (2017), arXiv:1611.02672[hep-ph]
    [101] V. De Romeri, E. Fernandez-Martinez, J. Gehrlein, P. A. N. Machado, and V. Niro, arXiv:1707.08606[hep-ph]
    [102] V. Khachatryan et al (CMS Collaboration), Phys. Rev. D, 93(3):032004 (2016), arXiv:1509.03744[hep-ex] CMS Collaboration (CMS Collaboration), CMS-PAS-EXO-12-041
    [103] CMS Collaboration (CMS Collaboration), CMS-PAS-EXO-16-007; (CMS Collaboration), CMS-PAS-EXO-12-042
    [104] V. Khachatryan et al (CMS Collaboration), arXiv:1612.01190[hep-ex] A. M. Sirunyan et al (CMS Collaboration), JHEP, 1707:121 (2017), arXiv:1703.03995[hep-ex]
    [105] M. Aaboud et al (ATLAS Collaboration), New J. Phys., 18(9):093016 (2016), arXiv:1605.06035[hep-ex]
    [106] G. Aad et al (ATLAS Collaboration), Phys. Lett. B, 709:158 (2012) Erratum:[Phys. Lett. B, 711:442 (2012)], arXiv:1112.4828[hep-ex]
    [107] G. Aad et al (ATLAS Collaboration), Eur. Phys. J. C, 72:2151 (2012), arXiv:1203.3172[hep-ex]
    [108] G. Aad et al (ATLAS Collaboration), JHEP, 1306:033 (2013), arXiv:1303.0526[hep-ex]
    [109] G. Aad et al (ATLAS Collaboration), Eur. Phys. J. C, 76(1):5 (2016), arXiv:1508.04735[hep-ex]
    [110] V. Khachatryan et al (CMS Collaboration), Phys. Rev. Lett., 116(7):071801 (2016), arXiv:1512.01224[hep-ex]
    [111] M. Aaboud et al (ATLAS Collaboration), Phys. Rev. D, 96(5):052004 (2017), arXiv:1703.09127[hep-ex]
    [112] G. Aad et al (ATLAS Collaboration), Phys. Lett. B, 716:1 (2012), arXiv:1207.7214[hep-ex]
    [113] S. Chatrchyan et al (CMS Collaboration), Phys. Lett. B, 716:30 (2012), arXiv:1207.7235[hep-ex]
    [114] G. Aad et al (ATLAS and CMS Collaborations], Phys. Rev. Lett., 114:191803 (2015), arXiv:1503.07589[hep-ex]
    [115] V. Barger, P. Langacker, and G. Shaughnessy, Phys. Rev. D, 75:055013 (2007),[hep-ph/0611239]
    [116] V. Barger, P. Langacker, M. McCaskey, M. J. Ramsey-Musolf, and G. Shaughnessy, Phys. Rev. D, 77:035005 (2008), arXiv:0706.4311[hep-ph]
    [117] T. Robens and T. Stefaniak, Eur. Phys. J. C, 75:104 (2015), arXiv:1501.02234[hep-ph]
    [118] T. Robens and T. Stefaniak, Eur. Phys. J. C, 76(5):268 (2016), arXiv:1601.07880[hep-ph]
    [119] P. P. Giardino, K. Kannike, I. Masina, M. Raidal, and A. Strumia, JHEP, 1405:046 (2014), arXiv:1303.3570[hep-ph]
    [120] G. Aad et al (ATLAS and CMS Collaborations], JHEP, 1608:045 (2016), arXiv:1606.02266[hep-ex]
    [121] J. Abdallah et al (DELPHI Collaboration), Eur. Phys. J. C, 38:1 (2004),[hep-ex/0410017]
    [122] K. L. McDonald and B. H. J. McKellar, hep-ph/0309270
    [123] K. S. Babu and C. Macesanu, Phys. Rev. D, 67:073010 (2003),[hep-ph/0212058]
    [124] M. Nebot, J. F. Oliver, D. Palao, and A. Santamaria, Phys. Rev. D, 77:093013 (2008), arXiv:0711.0483[hep-ph]
    [125] J. A. Casas and A. Ibarra, Nucl. Phys. B, 618:171 (2001),[hep-ph/0103065] A. Ibarra and G. G. Ross, Phys. Lett. B, 591:285 (2004),[hep-ph/0312138]
    [126] Y. Liao and J. Y. Liu, Phys. Rev. D, 81:013004 (2010), arXiv:0911.3711[hep-ph]
    [127] M. Kohda, H. Sugiyama, and K. Tsumura, Phys. Lett. B, 718:1436 (2013), arXiv:1210.5622[hep-ph]
    [128] M. Carpentier and S. Davidson, Eur. Phys. J. C, 70:1071 (2010), arXiv:1008.0280[hep-ph]
    [129] T. Nomura and H. Okada, Phys. Rev. D, 94:075021 (2016), arXiv:1607.04952[hep-ph]
    [130] S. Y. Guo, Z. L. Han, B. Li, Y. Liao, and X. D. Ma, arXiv:1707.00522[hep-ph]
    [131] I. Dorsner, S. Fajfer, A. Greljo, J. F. Kamenik, and N. Kosnik, Phys. Rept., 641:1 (2016), arXiv:1603.04993[hep-ph]
    [132] A. M. Baldini et al (MEG Collaboration), Eur. Phys. J. C, 76(8):434 (2016), arXiv:1605.05081[hep-ex] J. Adam et al (MEG Collaboration), Phys. Rev. Lett., 110:201801 (2013), arXiv:1303.0754[hep-ex]
    [133] B. Aubert et al (BaBar Collaboration), Phys. Rev. Lett., 104:021802 (2010), arXiv:0908.2381[hep-ex]
    [134] D. Chakraverty, D. Choudhury, and A. Datta, Phys. Lett. B, 506:103 (2001),[hep-ph/0102180]
    [135] K. m. Cheung, Phys. Rev. D, 64:033001 (2001),[hepph/0102238]
    [136] G. F. Giudice, P. Paradisi, and M. Passera, JHEP, 1211:113 (2012), arXiv:1208.6583[hep-ph]
    [137] G. W. Bennett et al (Muon g-2 Collaboration), Phys. Rev. D, 73:072003 (2006),[hep-ex/0602035]
    [138] M. Bauer and M. Neubert, Phys. Rev. Lett., 116(14):141802 (2016), arXiv:1511.01900[hep-ph]
    [139] J. Baron et al (ACME Collaboration), Science, 343:269 (2014), arXiv:1310.7534[physics.atom-ph]
    [140] M. Bona et al (UTfit Collaboration), JHEP, 0803:049 (2008), arXiv:0707.0636[hep-ph]
    [141] N. D. Christensen and C. Duhr, Comput. Phys. Commun., 180:1614 (2009), arXiv:0806.4194[hep-ph]; A. Alloul, N. D. Christensen, C. Degrande, C. Duhr, and B. Fuks, Comput. Phys. Commun., 185:2250 (2014), arXiv:1310.1921[hep-ph]
    [142] A. Belyaev, N. D. Christensen, and A. Pukhov, Comput. Phys. Commun., 184:1729 (2013), arXiv:1207.6082[hepph]
    [143] G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, Comput. Phys. Commun., 192:322 (2015), arXiv:1407.6129[hepph]
    [144] P. A. R. Ade et al (Planck Collaboration), Astron. Astrophys., 571:A16 (2014), arXiv:1303.5076[astro-ph.CO]
    [145] D. S. Akerib et al (LUX Collaboration), Phys. Rev. Lett., 118(2):021303 (2017), arXiv:1608.07648[astro-ph.CO]
    [146] E. Aprile et al (XENON Collaboration), Phys. Rev. Lett., 119(18):181301 (2017), arXiv:1705.06655[astro-ph.CO]
    [147] X. Cui et al (PandaX-Ⅱ Collaboration), Phys. Rev. Lett., 119(18):181302 (2017), arXiv:1708.06917[astro-ph.CO]
    [148] J. M. Cline, K. Kainulainen, P. Scott, and C. Weniger, Phys. Rev. D, 88:055025 (2013) Erratum:[Phys. Rev. D, 92(3):039906 (2015)], arXiv:1306.4710[hep-ph]
    [149] J. F. Navarro, C. S. Frenk, and S. D. M. White, Astrophys. J., 462:563 (1996),[astro-ph/9508025]
    [150] M. Cirelli et al, JCAP, 1103:051 (2011) Erratum:[JCAP, 1210:E01 (2012)], arXiv:1012.4515[hep-ph]
    [151] S. J. Clark, B. Dutta, and L. E. Strigari, arXiv:1709.07410[astro-ph.HE]
    [152] A. Geringer-Sameth and S. M. Koushiappas, Phys. Rev. Lett., 107:241303 (2011), arXiv:1108.2914[astro-ph.CO]
    [153] M. Ackermann et al (Fermi-LAT Collaboration), Phys. Rev. Lett., 107:241302 (2011), arXiv:1108.3546[astro-ph.HE]
    [154] M. Ackermann et al (Fermi-LAT Collaboration), Phys. Rev. D, 89:042001 (2014), arXiv:1310.0828[astro-ph.HE]
    [155] A. Geringer-Sameth, S. M. Koushiappas, and M. G. Walker, Phys. Rev. D, 91:no. 8, 083535 (2015), arXiv:1410.2242[astro-ph.CO]
    [156] M. Ackermann et al (Fermi-LAT Collaboration), Phys. Rev. Lett., 115(23):231301 (2015), arXiv:1503.02641[astroph.HE]
    [157] M. Aguilar et al (AMS Collaboration), Phys. Rev. Lett. 117(23):231102 (2016),
    [158] M. G. Aartsen et al (IceCube Collaboration), arXiv:1701.03731[astro-ph.HE]
    [159] R. Gandhi, C. Quigg, M. H. Reno, and I. Sarcevic, Astropart. Phys., 5:81 (1996),[hep-ph/9512364]
    [160] C. Y. Chen, P. S. Bhupal Dev, and A. Soni, Phys. Rev. D, 89(3):033012 (2014), arXiv:1309.1764[hep-ph]
    [161] S. L. Glashow, Phys. Rev., 118:316 (1960),
    [162] R. D. Ball et al, Nucl. Phys. B, 867:244 (2013), arXiv:1207.1303[hep-ph]
    [163] T. A. Gabriel, D. E. Groom, P. K. Job, N. V. Mokhov, and G. R. Stevenson, Nucl. Instrum. Meth. A, 338:336 (1994),
    [164] M. P. Kowalski, Search for neutrino induced cascades with the AMANDA-Ⅱ detector
    [165] R. Gandhi, C. Quigg, M. H. Reno, and I. Sarcevic, Phys. Rev. D, 58:093009 (1998),[hep-ph/9807264]
    [166] M. Ahlers and F. Halzen, Rept. Prog. Phys., 78(12):126901 (2015)
    [167] M. G. Aartsen et al (IceCube Collaboration), Astrophys. J., 809(1):98 (2015), arXiv:1507.03991[astro-ph.HE]
    [168] M. G. Aartsen et al (IceCube Collaboration), Phys. Rev. D, 91(2):022001 (2015), arXiv:1410.1749[astro-ph.HE]

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Ran Ding, Zhi-Long Han, Li Huang and Yi Liao. Phenomenology of colored radiative neutrino mass model and its implications on cosmic-ray observations[J]. Chinese Physics C, 2018, 42(10): 103101. doi: 10.1088/1674-1137/42/10/103101
Ran Ding, Zhi-Long Han, Li Huang and Yi Liao. Phenomenology of colored radiative neutrino mass model and its implications on cosmic-ray observations[J]. Chinese Physics C, 2018, 42(10): 103101.  doi: 10.1088/1674-1137/42/10/103101 shu
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Received: 2018-05-28
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    Supported by the NSFC (11575089, 11025525), the National Key Research and Development Program of China (2017YFA0402200) and the CAS Center for Excellence in Particle Physics (CCEPP).

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Phenomenology of colored radiative neutrino mass model and its implications on cosmic-ray observations

  • 1.  Center for High Energy Physics, Peking University, Beijing 100871, China
  • 2.  School of Physics and Technology, University of Jinan, Jinan, Shandong 250022, China
  • 3.  State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China
  • 4. Center for High Energy Physics, Peking University, Beijing 100871, China
  • 5. State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China
  • 6. School of Physics, Nankai University, Tianjin 300071, China
  • Received Date: 2018-05-28
  • Available Online: 2018-10-05
Fund Project:  Supported by the NSFC (11575089, 11025525), the National Key Research and Development Program of China (2017YFA0402200) and the CAS Center for Excellence in Particle Physics (CCEPP).

Abstract: We extend the colored Zee-Babu model with a gauged U(1)B-L symmetry, and a scalar singlet dark matter (DM) candidate S. The spontaneous breaking of U(1)B-L leaves a residual Z2 symmetry that stabilizes the DM, and generates a tiny neutrino mass at the two-loop level with the color seesaw mechanism. After investigating the DM and flavor phenomenology of this model systematically, we further focus on its imprint on two cosmic-ray anomalies:The Fermi-LAT gamma-ray excess at the Galactic Center (GCE), and the PeV ultra-high energy (UHE) neutrino events at the IceCube. We found that the Fermi-LAT GCE spectrum can be well-fitted by DM annihilation into a pair of on-shell singlet Higgs mediators while being compatible with the constraints from the relic density, direct detections, and dwarf spheroidal galaxies, in the Milky Way. Although the UHE neutrino events at the IceCube could be accounted for by the resonance production of a TeV-scale leptoquark, the relevant Yukawa couplings have been severely limited by the current low-energy flavor experiments. We subsequently derive the IceCube limits on the Yukawa couplings by employing its latest six-year data.

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