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

Ran Ding; Zhi-Long Han; Li Huang; Yi Liao

doi:10.1088/1674-1137/42/10/103101

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

Ran Ding ¹ ,
Zhi-Long Han ² ,
Li Huang ³ ,
Yi Liao ^1,3,4

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

Abstract
HTML
Reference
Related

PDF

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.
- neutrino mass models ,
- gamma-ray excess at galactic center ,
- IceCube neutrinos ,
- dark matter

References

[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]

[1]	Ming-Jie Zhang , Shu-Min Zhao , Xing-Xing Dong , Zhong-Jun Yang , Tai-Fu Feng . Scalar neutrino dark matter in the BLMSSM. Chinese Physics C, 2021, 45(9): 093106. doi: 10.1088/1674-1137/ac0c0e
[2]	Lian-Bao Jia , Tong Li . Interpretation of the Galactic gamma-ray excess with the dark matter indicated by ⁸Be and ⁴He anomalous transitions. Chinese Physics C, 2021, 45(6): 063101. doi: 10.1088/1674-1137/abeda6
[3]	Wen Yin . Dark matter, neutrino mass, cutoff for cosmic-ray neutrino, and the Higgs boson invisible decay from a neutrino portal interaction. Chinese Physics C, 2019, 43(4): 045101. doi: 10.1088/1674-1137/43/4/045101
[4]	Ran Ding , Zhi-Long Han , Lei Feng , Bin Zhu . Confronting the DAMPE excess with the scotogenictype-II seesaw model. Chinese Physics C, 2018, 42(8): 083104. doi: 10.1088/1674-1137/42/8/083104
[5]	Kun Wang , Fei Wang , Jingya Zhu , Quanlin Jie . The semi-constrained NMSSM in light of muon g-2, LHC, anddark matter constraints. Chinese Physics C, 2018, 42(10): 103109. doi: 10.1088/1674-1137/42/10/103109
[6]	Yi Zhao , Xiao-Jun Bi , Peng-Fei Yin , Xinmin Zhang . Searching for γ-ray emission from Reticulum Ⅱ by Fermi-LAT. Chinese Physics C, 2018, 42(2): 025102. doi: 10.1088/1674-1137/42/2/025102
[7]	Rui-Yun Guo , Jing-Fei Zhang , Xin Zhang . Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter. Chinese Physics C, 2018, 42(9): 095103. doi: 10.1088/1674-1137/42/9/095103
[8]	Andrea Addazi , Antonino Marcianò . Gravitational waves from dark first order phase transitions and dark photons. Chinese Physics C, 2018, 42(2): 023107. doi: 10.1088/1674-1137/42/2/023107
[9]	Wen Yin . Fixed point and anomaly mediation in partial N=2 supersymmetric standard models. Chinese Physics C, 2018, 42(1): 013104. doi: 10.1088/1674-1137/42/1/013104
[10]	Guoli Liu , Fei Wang , Wenyu Wang , Jin-Min Yang . Explaining DAMPE results by dark matter with hierarchical lepton-specific Yukawa interactions. Chinese Physics C, 2018, 42(3): 035101. doi: 10.1088/1674-1137/42/3/035101
[11]	Andrea Addazi , Stephon Alexander , Yi-Fu Cai , Antonino Marcianó . Dark matter and baryogenesis in the Fermi-bounce curvaton mechanism. Chinese Physics C, 2018, 42(6): 065101. doi: 10.1088/1674-1137/42/6/065101
[12]	Peyman Zakeri , Mohammad Moosavi , Mohammadreza Zakeri , Yaser Ayazi . A minimal model for two-component FIMP dark matter: A basic search. Chinese Physics C, 2018, 42(7): 073101. doi: 10.1088/1674-1137/42/7/073101
[13]	Andrea Addazi , Pietro Donà , Antonino Marcianò . Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions. Chinese Physics C, 2018, 42(7): 075102. doi: 10.1088/1674-1137/42/7/075102
[14]	Liuyuan Shen , Yicen Mou , Yunlong Zheng , Mingzhe Li . Direct couplings of mimetic dark matter and their cosmological effects. Chinese Physics C, 2018, 42(1): 015101. doi: 10.1088/1674-1137/42/1/015101
[15]	Shivaramakrishna Singirala . Implications of fermionic dark matter on recent neutrino oscillation data. Chinese Physics C, 2017, 41(4): 043102. doi: 10.1088/1674-1137/41/4/043102
[16]	Yi-Ming Hu , Jin Chang , Deng-Yi Chen , Jian-Hua Guo , Yun-Long Zhang , Chang-Qing Feng . Environmental test of the BGO calorimeterfor DArk Matter Particle Explorer. Chinese Physics C, 2016, 40(11): 116003. doi: 10.1088/1674-1137/40/11/116003
[17]	S. A. Alavi , F. S. Kazemian . Photonic dark matter portal and quantum physics. Chinese Physics C, 2016, 40(2): 025101. doi: 10.1088/1674-1137/40/2/025101
[18]	KANG Ke-Jun , YUE Qian , WU Yu-Cheng et al. (CDEX collaboration) and (TEXONO collaboration) . CDEX-1 1 kg point-contact germanium detector for low mass dark matter searches. Chinese Physics C, 2013, 37(12): 126002. doi: 10.1088/1674-1137/37/12/126002
[19]	TANG Zhi-Cheng , YUAN Qiang , BI Xiao-Jun , CHEN Guo-Ming . On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays. Chinese Physics C, 2011, 35(8): 725-734. doi: 10.1088/1674-1137/35/8/006
[20]	YUAN Qiang , BI Xiao-Jun , ZHANG Juan . Perspective of Galactic dark matter subhalo detection on Fermi from the EGRET observation. Chinese Physics C, 2009, 33(10): 826-833. doi: 10.1088/1674-1137/33/10/002

Access

Get Citation

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

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2018-05-28

Fund

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).

Article Metric

Article Views(1568)
PDF Downloads(27)
Cited by(0)

Policy on re-use

To reuse of Open Access content published by CPC, for content published under the terms of the Creative Commons Attribution 3.0 license (“CC CY”), the users don’t need to request permission to copy, distribute and display the final published version of the article and to create derivative works, subject to appropriate attribution.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

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

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

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

HTML

目录