Towards gauge unified, supersymmetric hidden strong dynamics

  • We consider a class of models with extra complex scalars that are charged under both the Standard Model and a hidden strongly coupled $SU(N)_H$ gauge sector and discuss the scenarios in which the new scalars are identified as the messenger fields that mediate the spontaneously broken supersymmetries from the hidden sector to the visible sector. The new scalars are embedded into 5-plets and 10-plets of an $SU(5)_V$ gauge group that potentially unifies the Standard Model gauge groups. The Higgs bosons remain as elementary particles. In the supersymmetrized version of this class of models, vector-like fermions whose left-handed components are superpartners of the new scalars are introduced. Owing to the hidden strong force, the new low-energy scalars hadronize before decaying and thus evade the common direct searches of the supersymmetric squarks. This can be seen as a gauge mediation scenario with the scalar messenger fields forming low-energy bound states. We also discuss the possibility that in the tower of bound states formed under hidden strong dynamics (of at least the TeV scale), there exist a dark matter candidate and the collider signatures (e.g. diphoton, diboson, or dijet) of models that may show up in the near future.
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  • [1] M. Cahill-Rowley, J. Hewett, A. Ismailet al., Phys. Rev. D90(9), 095017 (2014), arXiv:1407.7021[hep-ph doi:10.1103/PhysRevD.90.095017
    [2] M. Carena, H. E. Haber, I. Lowet al., Phys. Rev. D93(3), 035013 (2016), arXiv:1510.09137[hep-ph doi:10.1103/PhysRevD.93.035013
    [3] M. Carena, J. Ellis, J. S. Leeet al., JHEP1602, 123 (2016), arXiv:1512.00437[hep-ph doi:10.1007/JHEP02(2016)123
    [4] T. Han, T. Li, S. Suet al., JHEP1311, 053 (2013), arXiv:1306.3229[hep-ph doi:10.1007/JHEP11(2013)053
    [5] N. D. Christensen, T. Han, Z. Liuet al., JHEP1308, 019 (2013), arXiv:1303.2113[hep-ph doi:10.1007/JHEP08(2013)019
    [6] N. Arkani-Hamed, A. G. Cohen, E. Katzet al., JHEP0207, 034 (2002), arXiv:hep-ph/0206021 doi:10.1088/1126-6708/2002/07/034
    [7] D. B. Kaplan and H. Georgi, Phys. Lett. B136, 183 (1984) doi:10.1016/0370-2693(84)91177-8
    [8] D. B. Kaplan, H. Georgi, and S. Dimopoulos, Phys. Lett. B136, 187 (1984) doi:10.1016/0370-2693(84)91178-X
    [9] K. Agashe, R. Contino, and A. Pomarol, Nucl. Phys. B719, 165 (2005), arXiv:hep-ph/0412089 doi:10.1016/j.nuclphysb.2005.04.035
    [10] Z. Kakushadze, G. Shiu, S. Tyeet al., Int. J. Mod. Phys. A13, 2551-2598 (1998), arXiv:9710149[hep-th
    [11] M. Cvetic, P. Langacker, and G. Shiu, Phys. Rev. D66, 066004 (2002), arXiv:0205252[hep-th
    [12] M. Cvetic, G. Shiu, and A. Uranga, Phys. Rev. Lett.87, 201801 (2001), arXiv:0107143[hep-th doi:10.1103/PhysRevLett.87.201801
    [13] M. Cvetic, G. Shiu, and A. Uranga, Nucl. Phys. B615, 3-32 (2001), arXiv:0107166[hep-th
    [14] R. Blumenhagen, M. Cvetic, P. Langackeret al., Ann. Rev. Nucl. Part. Sci.55, 71-139 (2005), arXiv:0502005[hep-th doi:10.1146/annurev.nucl.55.090704.151541
    [15] P. McGuirk, G. Shiu, and Y. Sumitomo, Phys. Rev. D81, 026005 (2010), arXiv:0911.0019[hep-th
    [16] C. Chiang, M. Ibe, and T. Yanagida, arXiv: 1512.08895 [hep-ph]
    [17] C. Chiang, H. Fukuda, K. Harigayaet al., JEHP1511, 015 (2015), arXiv:1507.02483[hepph
    [18] S. Sun, D. B. Kaplan, and A. E. Nelson, Phys. Rev. D87(12), 125036 (2013), arXiv:1303.1811[hep-ph doi:10.1103/PhysRevD.87.125036
    [19] S. Sun, arXiv: 1411.0131 [hep-ph]
    [20] S. Chang, L. J. Hall, and N. Weiner, Phys. Rev. D75, 035009 (2007), arXiv:hep-ph/0604076 doi:10.1103/PhysRevD.75.035009
    [21] M. Low and L. T. Wang, JHEP1408, 161 (2014), arXiv:1404.0682 [hep-ph
    [22] J. Bramante, N. Desai, P. Foxet al., Phys. Rev. D93(6), 063525 (2016), arXiv:1510.03460[hep-ph doi:10.1103/PhysRevD.93.063525
    [23] T. Han, Z. Liu, and S. Su, JHEP1408, 093 (2014), arXiv:1406.1181[hep-ph doi:10.1007/JHEP08(2014)093
    [24] M. Cahill-Rowley, R. Cotta, A. Drlica-Wagneret al., Phys. Rev. D91(5), 055011 (2015), arXiv:1405.6716[hep-ph doi:10.1103/PhysRevD.91.055011
    [25] R. Kitano and Y. Nomura, Phys. Rev. D73, 095004 (2006), arXiv:hepph/0602096 doi:10.1103/PhysRevD.73.095004
    [26] M. Perelstein and C. Spethmann, JHEP0704, 070 (2007), arXiv:hepph/0702038 doi:10.1088/1126-6708/2007/04/070
    [27] Y. Hamada, T. Noumi, S. Sunet al., arXiv: 1512.08984 [hep-ph]
    [28] K. Harigaya, T. Lin, and H. Lou, arXiv: 1606.00923 [hep-ph]
    [29] S. Dimopoulos, S. Raby, and F. Wilczek, Phys. Lett. B112, 133 (1982)
    [30] P. Langacker and M. Luo, Phys. Rev. D44, 817-822 (1991)
    [31] M. Carena, M. Olechowski, S. Pokorskiet al., Nucl. Phys. B426, 269-300 (1994), arXiv:9402253[hep-ph
    [32] V. Barger, M. Berger, and P. Ohmann, Phys. Rev. D47, 1093-1113 (1993), arXiv:9209232[hep-ph
    [33] P. Langacker and N. Polonsky, Phys. Rev. D47, 4028-4045 (1993), arXiv:9210235[hep-ph
    [34] J. Hisano, H. Murayama, and T. Yanagida, Nucl. Phys. B402, 46-84 (1993), arXiv:9207279[hep-ph
    [35] G. Ross and R. Roberts, Nucl. Phys. B377, 571-592 (1992)
    [36] M Carena, S. Pokorski, and C. Wagner, Nucl. Phys.406, 59-89 (1993), arXiv:9303202[hep-ph
    [37] T. Goto and T. Nihei, Phys. Rev. D59, 115009 (1999), arXiv:9808225[hep-ph
    [38] G. Giudice and A. Romanino, Nucl. Phys. B699, 65-89 (2004), arXiv:0406088[hep-ph
    [39] N. Arkani-Hamed and S. Dimopoulos, JHEP0506, 073 (2005), arXiv:hep-th/0405159 doi:10.1088/1126-6708/2005/06/073
    [40] Y. Suzukiet al.[TITAND Working Group Collaboration], arXiv: 0110005 [hep-ex]
    [41] S. Aokiet al. [JLQCD Collaboration], Phys. Rev. D62, 014506 (2000), arXiv:9911026[hep-lat
    [42] The Review of Particle Physics (2015), Chin. Phys. C,38, 090001 (2014) and 2015 update
    [43] R. Barbieri, D. Buttazzo, L. J. Hallet al., arXiv: 1603.00718 [hep-ph]
    [44] L. J. Hall, K. Harigaya, and Y. Nomura, JHEP1603, 017 (2016), arXiv:1512.07904[hep-ph doi:10.1007/JHEP03(2016)017
    [45] S. Raby, Eur. Phys. J. C59, 223-247 (2009), arXiv:0807.4921[hep-ph
    [46] W. Buchmuller, C. Ludeling, J. Schmidt, JHEP0708, 113 (2007), arXiv:0707.1651[hep-ph
    [47] S. Hamidi and C. Vafa, Nucl. Phys. B279, 465 (1987)
    [48] G. Marandella, C. Schappacher, and A. Strumia, Nucl. Phys. B715, 173 (2005), arXiv:hep-ph/0502095 doi:10.1016/j.nuclphysb.2005.03.001
    [49] K. Cheung, J. S. Lee, and P. Y. Tseng, Phys. Rev. D92(9), 095004 (2015), arXiv:1501.03552[hep-ph doi:10.1103/PhysRevD.92.095004
    [50] V. A. Novikov, L. B. Okun, M. A. Shifmanet al., Phys. Rept.41, 1 (1978)
    [51] G. Aadet al. (ATLAS Collaboration), Phys. Lett. B701, 1 (2011), arXiv:1103.1984[hep-ex doi:10.1016/j.physletb.2011.05.010
    [52] M. Fairbairn, A. C. Kraan, D. A. Milsteadet al., Phys. Rept.438, 1 (2007), arXiv:hep-ph/0611040 doi:10.1016/j.physrep.2006.10.002
    [53] A. C. Kraan, J. B. Hansen, and P. Nevski, Eur. Phys. J. C49, 623 (2007), arXiv:hepex/0511014 doi:10.1140/epjc/s10052-006-0162-x
    [54] K. Griest and M. Kamionkowski, Phys. Rev. Lett.64, 615 (1990) doi:10.1103/PhysRevLett.64.615
    [55] S. Kanemura, S. Matsumoto, T. Nabeshimaet al., Phys. Rev. D82, 055026 (2010), arXiv:1005.5651 [hep-ph doi:10.1103/PhysRevD.82.055026
    [56] R. Young and A. Thomas, Phys. Rev. D81, 014503 (2010), arXiv:0901.3310 [hep-lat
    [57] D. Akerib et al. [LUX Collaboration], arXiv: 1512.03506 [astro-ph.CO]
    [58] D. Akerib et al. [LZ Collaboration], arXiv: 1509.02910 [physics.ins-det]
    [59] Z. Yu, J. Zheng, X. Biet al., Nucl. Phys. B860, 115-151 (2012)
    [60] V. Khachatryanet al. [CMS Collaboration], Phys. Lett. B749, 560-582 (2015), arXiv:1503.04114[hepex doi:10.1016/j.physletb.2015.08.047
    [61] CMS Collaboration [CMS Collaboration], CMS-PAS-HIG-14-006
    [62] G. Aadet al. [ATLAS Collaboration], Phys. Rev. D92(3), 032004 (2015), arXiv:1504.05511 [hep- ex
    [63] V. Khachatryanet al. [CMS Collaboration], JHEP1510, 144 (2015), arXiv:1504.00936 [hep-ex
    [64] G. Aadet al. [ATLAS Collaboration], arXiv:1509.00389 [hep-ex]
    [65] G. Aadet al. [ATLAS Collaboration], arXiv:1507.05930 [hep-ex]
    [66] G. Aadet al. [ATLAS Collaboration], Phys. Lett. B738, 428 (2014), arXiv:1407.8150 [hep-ex
    [67] G. Aadet al. [ATLAS Collaboration], Phys. Rev. D91(5), 052007 (2015), arXiv:1407.1376 [hep-ex
    [68] CMS Collaboration [CMS Collaboration], CMS-PAS-EXO-14-005
    [69] M. Aaboudet al. [ATLAS Collaboration], CERN-EP-2017-042 , [arXiv:1703.09127 [hep-ex]]
    [70] CMS Collaboration [CMS Collaboration], CMS-PAS-B2G-16-023
    [71] ATLAS Collaboration [ATLAS Collaboration], ATLAS-CONF-2016-074
    [72] CMS Collaboration [CMS Collaboration], CMS-PAS-EXO-17-005
    [73] V. Khachatryanet al. [CMS Collaboration], Phys. Rev. D91(5), 052009 (2015), arXiv:1501.04198 [hep-ex
    [74] J. Kamenik and M. Redi, arXiv:1603.07719 [hep-ph]
    [75] A. G. Cohen, D. B. Kaplan, and A. E. Nelson, Phys. Lett. B412, 301 (1997), arXiv:hep-ph/9706275 doi:10.1016/S0370-2693(97)00995-7
    [76] M. A. Luty, Phys. Rev. D57, 1531 (1998), arXiv:hep-ph/9706235 doi:10.1103/PhysRevD.57.1531
    [77] A. D. Martin, W. J. Stirling, R. S. Thorneet al., Eur. Phys. J. C63, 189 (2009), arXiv:0901.0002 [hep-ph doi:10.1140/epjc/s10052-009-1072-5
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Cheng-Wei Chiang, Sichun Sun and Fang Ye. Towards gauge unified, supersymmetric hidden strong dynamics[J]. Chinese Physics C. doi: 10.1088/1674-1137/abc0ce
Cheng-Wei Chiang, Sichun Sun and Fang Ye. Towards gauge unified, supersymmetric hidden strong dynamics[J]. Chinese Physics C. doi:10.1088/1674-1137/abc0ce shu
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