×
近期发现有不法分子冒充我刊与作者联系,借此进行欺诈等不法行为,请广大作者加以鉴别,如遇诈骗行为,请第一时间与我刊编辑部联系确认(《中国物理C》(英文)编辑部电话:010-88235947,010-88236950),并作报警处理。
本刊再次郑重声明:
(1)本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
(2)本刊采编系统作者中心是投稿的唯一路径,该系统为ScholarOne远程稿件采编系统,仅在本刊投稿网网址(https://mc03.manuscriptcentral.com/cpc)设有登录入口。本刊不接受其他方式的投稿,如打印稿投稿、E-mail信箱投稿等,若以此种方式接收投稿均为假冒。
(3)所有投稿均需经过严格的同行评议、编辑加工后方可发表,本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿,并收取发表费用,均为假冒。
                  
《中国物理C》(英文)编辑部
2024年10月30日

Implications of the RK and RK* anomalies

  • We discuss the implications of the recently reported RK and RK* anomalies, the lepton flavor non-universality in the B→ Kl+l- and B→ K*l+l- decay channels. Using two sets of hadronic inputs of form factors, we perform a fit of new physics to the RK and RK* data, and significant new physics contributions are found. We suggest the study of lepton flavor universality in a number of related rare B, Bs,Bc and Λb decay channels, and in particular we give predictions for the μ-to-e ratios of decay widths with different polarizations of the final state particles, and of the b→ dl+l- processes, which are presumably more sensitive to the structure of the underlying new physics. With the new physics contributions embedded in the Wilson coefficients, we present theoretical predictions for lepton flavor non-universality in these processes.
      PCAS:
  • 加载中
  • [1] G. Hiller and F. Kruger, Phys. Rev. D, 69:074020 (2004) doi:10.1103/PhysRevD.69.074020[hep-ph/0310219]
    [2] W. Altmannshofer, P. Ball, A. Bharucha, A. J. Buras, D. M. Straub, and M. Wick, JHEP, 0901:019 (2009) doi:10.1088/1126-6708/2009/01/019[arXiv:0811.1214[hepph]]
    [3] A. K. Alok, A. Datta, A. Dighe, M. Duraisamy, D. Ghosh, and D. London, JHEP, 1111:121 (2011) doi:10.1007/JHEP11(2011)121[arXiv:1008.2367[hep-ph]]
    [4] S. Descotes-Genon, D. Ghosh, J. Matias, and M. Ramon, JHEP, 1106:099 (2011) doi:10.1007/JHEP06(2011)099[arXiv:1104.3342[hep-ph]]
    [5] W. Altmannshofer, P. Paradisi, and D. M. Straub, JHEP, 1204:008 (2012) doi:10.1007/JHEP04(2012)008[arXiv:1111.1257[hep-ph]]
    [6] C. Hambrock and G. Hiller, Phys. Rev. Lett., 109:091802 (2012) doi:10.1103/PhysRevLett.109.091802[arXiv:1204.4444[hep-ph]]
    [7] S. Descotes-Genon, J. Matias, M. Ramon, and J. Virto, JHEP, 1301:048 (2013) doi:10.1007/JHEP01(2013)048[arXiv:1207.2753[hep-ph]]
    [8] S. Descotes-Genon, J. Matias, and J. Virto, Phys. Rev. D, 88:074002 (2013) doi:10.1103/PhysRevD.88.074002[arXiv:1307.5683[hep-ph]]
    [9] W. Altmannshofer and D. M. Straub, Eur. Phys. J. C, 73:2646 (2013) doi:10.1140/epjc/s10052-013-2646-9[arXiv:1308.1501[hep-ph]]
    [10] A. J. Buras and J. Girrbach, JHEP, 1312:009 (2013) doi:10.1007/JHEP12(2013)009[arXiv:1309.2466[hep-ph]]
    [11] A. Datta, M. Duraisamy, and D. Ghosh, Phys. Rev. D, 89(7):071501 (2014) doi:10.1103/PhysRevD.89.071501[arXiv:1310.1937[hep-ph]]
    [12] D. Ghosh, M. Nardecchia, and S. A. Renner, JHEP, 1412:131 (2014) doi:10.1007/JHEP12(2014)131[arXiv:1408.4097[hepph]]
    [13] B. Gripaios, M. Nardecchia, and S. A. Renner, JHEP, 1606:083 (2016) doi:10.1007/JHEP06(2016)083[arXiv:1509.05020[hep-ph]]
    [14] R. Barbieri, G. Isidori, A. Pattori, and F. Senia, Eur. Phys. J. C, 76(2):67 (2016) doi:10.1140/epjc/s10052-016-3905-3[arXiv:1512.01560[hep-ph]]
    [15] F. Feruglio, P. Paradisi, and A. Pattori, Phys. Rev. Lett., 118(1):011801 (2017) doi:10.1103/PhysRevLett.118.011801[arXiv:1606.00524[hep-ph]]
    [16] G. Hiller and M. Schmaltz, JHEP, 1502:055 (2015) doi:10.1007/JHEP02(2015)055[arXiv:1411.4773[hep-ph]]
    [17] D. Das, G. Hiller, M. Jung, and A. Shires, JHEP, 1409:109 (2014) doi:10.1007/JHEP09(2014)109[arXiv:1406.6681[hepph]]
    [18] S. W. Wang and Y. D. Yang, Adv. High Energy Phys., 2016:5796131 (2016) doi:10.1155/2016/5796131[arXiv:1608.03662[hep-ph]]
    [19] Q. Y. Hu, X. Q. Li, and Y. D. Yang, Eur. Phys. J. C, 77(3):190 (2017) doi:10.1140/epjc/s10052-017-4748-2[arXiv:1612.08867[hep-ph]]
    [20] J. Lyon and R. Zwicky, Phys. Rev. D, 88(9):094004 (2013) doi:10.1103/PhysRevD.88.094004[arXiv:1305.4797[hep-ph]]
    [21] J. Lyon and R. Zwicky, arXiv:1406.0566[hep-ph]
    [22] R. Aaij et al (LHCb Collaboration), Phys. Rev. Lett., 111:191801 (2013) doi:10.1103/PhysRevLett.111.191801[arXiv:1308.1707[hep-ex]]
    [23] R. Aaij et al (LHCb Collaboration), JHEP, 1602:104 (2016) doi:10.1007/JHEP02(2016)104[arXiv:1512.04442[hep-ex]]
    [24] D. Becirevic and A. Tayduganov, Nucl. Phys. B, 868:368 (2013) doi:10.1016/j.nuclphysb.2012.11.016[arXiv:1207.4004[hep-ph]]
    [25] C. H. Chen, T. Nomura, and H. Okada, Phys. Rev. D, 94(11):115005 (2016) doi:10.1103/PhysRevD.94.115005[arXiv:1607.04857[hep-ph]]
    [26] H. Gong, Y. D. Yang, and X. B. Yuan, JHEP, 1305:062 (2013) doi:10.1007/JHEP05(2013)062[arXiv:1301.7535[hepph]]
    [27] S. Jger and J. Martin Camalich, JHEP, 1305:043 (2013) doi:10.1007/JHEP05(2013)043[arXiv:1212.2263[hep-ph]]
    [28] E. Kou, C. D. L, and F. S. Yu, JHEP, 1312:102 (2013) doi:10.1007/JHEP12(2013)102[arXiv:1305.3173[hep-ph]]
    [29] S. Sahoo and R. Mohanta, Phys. Rev. D, 91(9):094019 (2015) doi:10.1103/PhysRevD.91.094019[arXiv:1501.05193[hep-ph]]
    [30] F. Mahmoudi, S. Neshatpour, and J. Virto, Eur. Phys. J. C, 74(6):2927 (2014) doi:10.1140/epjc/s10052-014-2927-y[arXiv:1401.2145[hep-ph]]
    [31] I. Ahmed and A. Rehman, arXiv:1703.09627[hep-ph]
    [32] V. G. Chobanova, T. Hurth, F. Mahmoudi, D. Martinez Santos, and S. Neshatpour, JHEP, 1707:025 (2017) doi:10.1007/JHEP07(2017)025[arXiv:1702.02234[hep-ph]]
    [33] B. Capdevila, S. Descotes-Genon, L. Hofer, and J. Matias, JHEP, 1704:016 (2017) doi:10.1007/JHEP04(2017)016[arXiv:1701.08672[hep-ph]]
    [34] R. Aaij et al (LHCb Collaboration), Phys. Rev. Lett., 113:151601 (2014) doi:10.1103/PhysRevLett.113.151601[arXiv:1406.6482[hep-ex]]
    [35] R. Aaij et al (LHCb Collaboration), JHEP, 1708:055 (2017) doi:10.1007/JHEP08(2017)055[arXiv:1705.05802[hep-ex]]
    [36] M. Ciuchini, A. M. Coutinho, M. Fedele, E. Franco, A. Paul, L. Silvestrini, and M. Valli, arXiv:1704.05447[hep-ph]
    [37] B. Capdevila, A. Crivellin, S. Descotes-Genon, J. Matias, and J. Virto, arXiv:1704.05340[hep-ph]
    [38] W. Altmannshofer, P. Stangl, and D. M. Straub, Phys. Rev. D, 96(5):055008 (2017) doi:10.1103/PhysRevD.96.055008[arXiv:1704.05435[hep-ph]]
    [39] L. S. Geng, B. Grinstein, S. Jger, J. Martin Camalich, X. L. Ren, and R. X. Shi, arXiv:1704.05446[hep-ph]
    [40] G. D'Amico, M. Nardecchia, P. Panci, F. Sannino, A. Strumia, R. Torre, and A. Urbano, JHEP, 1709:010 (2017) doi:10.1007/JHEP09(2017)010[arXiv:1704.05438[hep-ph]]
    [41] G. Hiller and I. Nisandzic, Phys. Rev. D, 96(3):035003 (2017) doi:10.1103/PhysRevD.96.035003[arXiv:1704.05444[hep-ph]]
    [42] A. Celis, J. Fuentes-Martin, A. Vicente, and J. Virto, Phys. Rev. D, 96(3):035026 (2017) doi:10.1103/PhysRevD.96.035026[arXiv:1704.05672[hep-ph]]
    [43] D. Bečirević and O. Sumensari, JHEP, 1708:104 (2017)doi:10.1007/JHEP08(2017)104[arXiv:1704.05835[hep-ph]]
    [44] D. Ghosh, arXiv:1704.06240[hep-ph]
    [45] Y. Cai, J. Gargalionis, M. A. Schmidt, and R. R. Volkas, JHEP, 1710:047 (2017) doi:10.1007/JHEP10(2017)047[arXiv:1704.05849[hep-ph]]
    [46] J. F. Kamenik, Y. Soreq, and J. Zupan, arXiv:1704.06005[hep-ph]
    [47] F. Sala and D. M. Straub, Phys. Lett. B, 774:205 (2017) doi:10.1016/j.physletb.2017.09.072[arXiv:1704.06188[hep-ph]]
    [48] S. Di Chiara, A. Fowlie, S. Fraser, C. Marzo, L. Marzola, M. Raidal, and C. Spethmann, Nucl. Phys. B, 923:245 (2017) doi:10.1016/j.nuclphysb.2017.08.003[arXiv:1704.06200[hep-ph]]
    [49] A. K. Alok, D. Kumar, J. Kumar, and R. Sharma, arXiv:1704.07347[hep-ph]
    [50] A. K. Alok, B. Bhattacharya, A. Datta, D. Kumar, J. Kumar, and D. London, arXiv:1704.07397[hep-ph]
    [51] J. Ellis, M. Fairbairn, and P. Tunney, arXiv:1705.03447[hepph]
    [52] F. Bishara, U. Haisch, and P. F. Monni, Phys. Rev. D, 96(5):055002 (2017) doi:10.1103/PhysRevD.96.055002[arXiv:1705.03465[hep-ph]]
    [53] Y. Tang and Y. L. Wu, arXiv:1705.05643[hep-ph]
    [54] A. Datta, J. Kumar, J. Liao, and D. Marfatia, arXiv:1705.08423[hep-ph]
    [55] D. Das, C. Hati, G. Kumar, and N. Mahajan, arXiv:1705.09188[hep-ph]
    [56] D. Bardhan, P. Byakti, and D. Ghosh, Phys. Lett. B, 773:505 (2017) doi:10.1016/j.physletb.2017.08.062[arXiv:1705.09305[hep-ph]]
    [57] S. Matsuzaki, K. Nishiwaki, and R. Watanabe, JHEP, 1708:145 (2017) doi:10.1007/JHEP08(2017)145[arXiv:1706.01463[hep-ph]]
    [58] C. W. Chiang, X. G. He, J. Tandean, and X. B. Yuan, arXiv:1706.02696[hep-ph]
    [59] S. Khalil, arXiv:1706.07337[hep-ph]
    [60] S. Descotes-Genon, L. Hofer, J. Matias, and J. Virto, JHEP, 1606:092 (2016) doi:10.1007/JHEP06(2016)092[arXiv:1510.04239[hep-ph]]
    [61] R. H. Li, C. D. Lu, W. Wang, and X. X. Wang, Phys. Rev. D, 79:014013 (2009) doi:10.1103/PhysRevD.79.014013[arXiv:0811.2648[hep-ph]]
    [62] W. Wang, Y. L. Shen, and C. D. Lu, Phys. Rev. D, 79:054012 (2009) doi:10.1103/PhysRevD.79.054012[arXiv:0811.3748[hep-ph]]
    [63] R. H. Li, C. D. Lu, and W. Wang, Phys. Rev. D, 79:034014 (2009) doi:10.1103/PhysRevD.79.034014[arXiv:0901.0307[hep-ph]]
    [64] W. Wang, Phys. Rev. D, 83:014008 (2011) doi:10.1103/PhysRevD.83.014008[arXiv:1008.5326[hep-ph]]
    [65] R. R. Horgan, Z. Liu, S. Meinel, and M. Wingate, Phys. Rev. D, 89(9):094501 (2014) doi:10.1103/PhysRevD.89.094501[arXiv:1310.3722[hep-lat]]
    [66] W. Detmold, C.-J. D. Lin, S. Meinel, and M. Wingate, Phys. Rev. D, 87(7):074502 (2013) doi:10.1103/PhysRevD.87.074502[arXiv:1212.4827[hep-lat]]
    [67] C. D. Lu and W. Wang, Phys. Rev. D, 85:034014 (2012) doi:10.1103/PhysRevD.85.034014[arXiv:1111.1513[hep-ph]]
    [68] M. Dring, U. G. Meiner, and W. Wang, JHEP, 1310:011 (2013) doi:10.1007/JHEP10(2013)011[arXiv:1307.0947[hepph]]
    [69] B. Dey, Phys. Rev. D, 92:033013 (2015) doi:10.1103/PhysRevD.92.033013[arXiv:1505.02873[hep-ex]]
    [70] J. Gratrex, M. Hopfer, and R. Zwicky, Phys. Rev. D, 93(5):054008 (2016) doi:10.1103/PhysRevD.93.054008[arXiv:1506.03970[hep-ph]]
    [71] B. Dey, Phys. Rev. D, 95(3):033004 (2017) doi:10.1103/PhysRevD.95.033004[arXiv:1609.06115[hep-ph]]
    [72] P. Ball and R. Zwicky, Phys. Rev. D, 71:014015 (2005) doi:10.1103/PhysRevD.71.014015[hep-ph/0406232]
    [73] P. Ball and R. Zwicky, Phys. Rev. D, 71:014029 (2005) doi:10.1103/PhysRevD.71.014029[hep-ph/0412079]
    [74] A. Bharucha, D. M. Straub, and R. Zwicky, JHEP, 1608:098 (2016) doi:10.1007/JHEP08(2016)098[arXiv:1503.05534[hep-ph]]
    [75] C. Bouchard et al (HPQCD Collaboration), Phys. Rev. D, 88(5):054509 (2013) Erratum:[Phys. Rev. D, 88(7):079901 (2013)] doi:10.1103/PhysRevD.88.079901, 10.1103/PhysRevD.88.054509[arXiv:1306.2384[hep-lat]]
    [76] C. Bobeth, G. Hiller, and G. Piranishvili, JHEP, 0712:040 (2007) doi:10.1088/1126-6708/2007/12/040[arXiv:0709.4174[hep-ph]]
    [77] M. Bordone, G. Isidori, and A. Pattori, Eur. Phys. J. C, 76(8):440 (2016) doi:10.1140/epjc/s10052-016-4274-7[arXiv:1605.07633[hep-ph]]
    [78] M. Beneke, T. Feldmann, and D. Seidel, Nucl. Phys. B, 612:25 (2001) doi:10.1016/S0550-3213(01)00366-2[hepph/0106067]
    [79] Q. Chang and Y. H. Gao, Nucl. Phys. B, 845:179 (2011) doi:10.1016/j.nuclphysb.2010.12.003[arXiv:1101.1272[hep-ph]]
    [80] R. Gauld, F. Goertz, and U. Haisch, Phys. Rev. D, 89:015005 (2014) doi:10.1103/PhysRevD.89.015005[arXiv:1308.1959[hep-ph]]
    [81] Q. Chang, X. Q. Li, and Y. D. Yang, J. Phys. G, 41:105002 (2014) doi:10.1088/0954-3899/41/10/105002[arXiv:1312.1302[hep-ph]]
    [82] G. Hiller and M. Schmaltz, Phys. Rev. D, 90:054014 (2014) doi:10.1103/PhysRevD.90.054014[arXiv:1408.1627[hep-ph]]
    [83] B. Gripaios, M. Nardecchia, and S. A. Renner, JHEP, 1505:006 (2015) doi:10.1007/JHEP05(2015)006[arXiv:1412.1791[hep-ph]]
    [84] L. Calibbi, A. Crivellin, and T. Ota, Phys. Rev. Lett., 115:181801 (2015) doi:10.1103/PhysRevLett.115.181801[arXiv:1506.02661[hep-ph]]
    [85] R. Alonso, B. Grinstein, and J. Martin Camalich, JHEP, 1510:184 (2015) doi:10.1007/JHEP10(2015)184[arXiv:1505.05164[hep-ph]]
    [86] D. Bečirević, S. Fajfer, and N. Konik, Phys. Rev. D, 92(1):014016 (2015) doi:10.1103/PhysRevD.92.014016[arXiv:1503.09024[hep-ph]]
    [87] P. Cox, A. Kusenko, O. Sumensari, and T. T. Yanagida, JHEP, 1703:035 (2017) doi:10.1007/JHEP03(2017)035[arXiv:1612.03923[hep-ph]]
    [88] D. Bečirević, S. Fajfer, N. Konik, and O. Sumensari, Phys. Rev. D, 94(11):115021 (2016) doi:10.1103/PhysRevD.94.115021[arXiv:1608.08501[hep-ph]]
    [89] A. Greljo, G. Isidori, and D. Marzocca, JHEP, 1507:142 (2015) doi:10.1007/JHEP07(2015)142[arXiv:1506.01705[hepph]]
    [90] X. Q. Li, Y. D. Yang, and X. Zhang, JHEP, 1608:054 (2016) doi:10.1007/JHEP08(2016)054[arXiv:1605.09308[hep-ph]]
    [91] Q. Y. Hu, X. Q. Li and Y. D. Yang, Eur. Phys. J. C, 77(4):228 (2017) doi:10.1140/epjc/s10052-017-4794-9[arXiv:1701.04029[hep-ph]]
    [92] C. H. Chen, T. Nomura, and H. Okada, Phys. Lett. B, 774:456 (2017) doi:10.1016/j.physletb.2017.10.005[arXiv:1703.03251[hep-ph]]
    [93] A. Crivellin, G. D'Ambrosio, and J. Heeck, Phys. Rev. Lett., 114:151801 (2015) doi:10.1103/PhysRevLett.114.151801[arXiv:1501.00993[hep-ph]]
    [94] A. Crivellin, G. D'Ambrosio, and J. Heeck, Phys. Rev. D, 91(7):075006 (2015) doi:10.1103/PhysRevD.91.075006[arXiv:1503.03477[hep-ph]]
    [95] D. Aristizabal Sierra, F. Staub, and A. Vicente, Phys. Rev.D, 92(1):015001 (2015) doi:10.1103/PhysRevD.92.015001[arXiv:1503.06077[hep-ph]]
    [96] A. Crivellin, L. Hofer, J. Matias, U. Nierste, S. Pokorski, and J. Rosiek, Phys. Rev. D, 92(5):054013 (2015) doi:10.1103/PhysRevD.92.054013[arXiv:1504.07928[hep-ph]]
    [97] D. Bečirević, O. Sumensari, and R. Zukanovich Funchal, Eur. Phys. J. C, 76(3):134 (2016) doi:10.1140/epjc/s10052-016-3985-0[arXiv:1602.00881[hep-ph]]
    [98] A. Celis, J. Fuentes-Martin, M. Jung, and H. Serodio, Phys. Rev. D, 92(1):015007 (2015) doi:10.1103/PhysRevD.92.015007[arXiv:1505.03079[hep-ph]]
    [99] A. Falkowski, M. Nardecchia, and R. Ziegler, JHEP, 1511:173 (2015) doi:10.1007/JHEP11(2015)173[arXiv:1509.01249[hep-ph]]
    [100] B. Allanach, F. S. Queiroz, A. Strumia, and S. Sun, Phys. Rev. D, 93(5):055045 (2016) Erratum:[Phys. Rev. D, 95(11):119902 (2017)] doi:10.1103/PhysRevD.93.055045, 10.1103/PhysRevD.95.119902[arXiv:1511.07447[hep-ph]]
    [101] K. Fuyuto, W. S. Hou, and M. Kohda, Phys. Rev. D, 93(5):054021 (2016) doi:10.1103/PhysRevD.93.054021[arXiv:1512.09026[hep-ph]]
    [102] C. W. Chiang, X. G. He, and G. Valencia, Phys. Rev. D, 93(7):074003 (2016) doi:10.1103/PhysRevD.93.074003[arXiv:1601.07328[hep-ph]]
    [103] A. Crivellin, J. Fuentes-Martin, A. Greljo, and G. Isidori, Phys. Lett. B, 766:77 (2017) doi:10.1016/j.physletb.2016.12.057[arXiv:1611.02703[hepph]]
    [104] A. Datta, J. Liao, and D. Marfatia, Phys. Lett. B, 768:265 (2017) doi:10.1016/j.physletb.2017.02.058[arXiv:1702.01099[hep-ph]]
    [105] E. Megias, G. Panico, O. Pujolas, and M. Quiros, JHEP, 1609:118 (2016) doi:10.1007/JHEP09(2016)118[arXiv:1608.02362[hep-ph]]
    [106] E. Megias, M. Quiros, and L. Salas, JHEP, 1707:102 (2017) doi:10.1007/JHEP07(2017)102[arXiv:1703.06019[hep-ph]]
    [107] G. Blanger, C. Delaunay, and S. Westhoff, Phys. Rev. D, 92:055021 (2015) doi:10.1103/PhysRevD.92.055021[arXiv:1507.06660[hep-ph]]
    [108] A. Carmona and F. Goertz, Phys. Rev. Lett., 116(25):251801 (2016) doi:10.1103/PhysRevLett.116.251801[arXiv:1510.07658[hep-ph]]
    [109] P. Ber, T. Feldmann, and D. van Dyk, JHEP, 1501:155 (2015) doi:10.1007/JHEP01(2015)155[arXiv:1410.2115[hepph]]
    [110] W. Detmold and S. Meinel, Phys. Rev. D, 93(7):074501 (2016) doi:10.1103/PhysRevD.93.074501[arXiv:1602.01399[hep-lat]]
    [111] P. Colangelo, F. De Fazio, and W. Wang, Phys. Rev. D, 81:074001 (2010) doi:10.1103/PhysRevD.81.074001[arXiv:1002.2880[hep-ph]]
    [112] R. H. Li, C. D. Lu, and W. Wang, Phys. Rev. D, 79:094024 (2009) doi:10.1103/PhysRevD.79.094024[arXiv:0902.3291[hep-ph]]
    [113] R. Aaij et al (LHCb Collaboration), JHEP, 1307:084 (2013) doi:10.1007/JHEP07(2013)084[arXiv:1305.2168[hep-ex]]
    [114] R. Aaij et al (LHCb Collaboration), JHEP, 1509:179 (2015) doi:10.1007/JHEP09(2015)179[arXiv:1506.08777[hep-ex]]
    [115] R. Aaij et al (LHCb Collaboration), JHEP, 1506:115 (2015) doi:10.1007/JHEP06(2015)115[arXiv:1503.07138[hep-ex]]
    [116] R. Aaij et al (LHCb Collaboration), Phys. Lett. B, 743:46 (2015) doi:10.1016/j.physletb.2015.02.010[arXiv:1412.6433[hep-ex]]
    [117] B. Bhattacharya, A. Datta, D. London, and S. Shivashankara, Phys. Lett. B, 742:370 (2015) doi:10.1016/j.physletb.2015.02.011[arXiv:1412.7164[hep-ph]]
    [118] R. Aaij et al (LHCb Collaboration), JHEP, 1510:034 (2015) doi:10.1007/JHEP10(2015)034[arXiv:1509.00414[hep-ex]]
    [119] A. Ali, A. Y. Parkhomenko, and A. V. Rusov, Phys. Rev. D, 89(9):094021 (2014) doi:10.1103/PhysRevD.89.094021[arXiv:1312.2523[hep-ph]]
    [120] Z. H. Li, Z. G. Si, Y. Wang, and N. Zhu, Nucl. Phys. B, 900:198 (2015) doi:10.1016/j.nuclphysb.2015.09.008
  • 加载中

Get Citation
Wei Wang and Shuai Zhao. Implications of the RK and RK* anomalies[J]. Chinese Physics C, 2018, 42(1): 013105. doi: 10.1088/1674-1137/42/1/013105
Wei Wang and Shuai Zhao. Implications of the RK and RK* anomalies[J]. Chinese Physics C, 2018, 42(1): 013105.  doi: 10.1088/1674-1137/42/1/013105 shu
Milestone
Received: 2017-08-29
Fund

    Supported by National Natural Science Foundation of China (11575110, 11655002, 11735010), Natural Science Foundation of Shanghai (15DZ2272100, 15ZR1423100), Young Thousand Talents Plan and Key Laboratory for Particle Physics, Astrophysics and Cosmology, Ministry of Education

Article Metric

Article Views(1718)
PDF Downloads(17)
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

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Implications of the RK and RK* anomalies

    Corresponding author: Shuai Zhao,
  • 1. INPAC, Shanghai Key Laboratory for Particle Physics and Cosmology, School of Physics and Astronomy, Shanghai Jiao-Tong University, Shanghai 200240, China
Fund Project:  Supported by National Natural Science Foundation of China (11575110, 11655002, 11735010), Natural Science Foundation of Shanghai (15DZ2272100, 15ZR1423100), Young Thousand Talents Plan and Key Laboratory for Particle Physics, Astrophysics and Cosmology, Ministry of Education

Abstract: We discuss the implications of the recently reported RK and RK* anomalies, the lepton flavor non-universality in the B→ Kl+l- and B→ K*l+l- decay channels. Using two sets of hadronic inputs of form factors, we perform a fit of new physics to the RK and RK* data, and significant new physics contributions are found. We suggest the study of lepton flavor universality in a number of related rare B, Bs,Bc and Λb decay channels, and in particular we give predictions for the μ-to-e ratios of decay widths with different polarizations of the final state particles, and of the b→ dl+l- processes, which are presumably more sensitive to the structure of the underlying new physics. With the new physics contributions embedded in the Wilson coefficients, we present theoretical predictions for lepton flavor non-universality in these processes.

    HTML

Reference (120)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return