×
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

Uncertainty of parton distribution functions due to physical observables in a global analysis

  • The recent measurement of the differential γ+c-jet cross section, performed at the Tevatron collider in Run II by the D0 collaboration, is studied in a next-to-leading order (NLO) global QCD analysis to assess its impact on the proton parton distribution functions (PDFs). We show that these data lead to a significant change in the gluon and charm quark distributions. We demonstrate also that there is an inconsistency between the new high precision HERA I+II combined data and Tevatron measurement. Moreover, in this study we investigate the impact of older EMC measurements of charm structure function Fc2 on the PDFs and compare the results with those from the analysis of Tevatron data. We show that both of them have the same impact on the PDFs, and thus can be recognized as the same evidence for the inefficiency of perturbative QCD in dealing with charm production in some kinematic regions.
      PCAS:
  • 加载中
  • [1] R. D. Ball et al. (NNPDF Collaboration), arXiv:1605.06515[hep-ph]
    [2] L. A. Harland-Lang, A. D. Martin, P. Motylinski, and R. S. Thorne, arXiv:1412.3989
    [3] J. Gao, M. Guzzi, J. Huston, H. L. Lai, Z. Li, P. Nadolsky, J. Pumplin, and D. Stump et al., Phys. Rev. D, 89(3):033009(2014)
    [4] A. D. Martin, W. J. Stirling, R. S. Thorne, and G. Watt, Eur. Phys. J. C, 63:189(2009)
    [5] R. D. Ball, V. Bertone, S. Carrazza, C. S. Deans, L. Del Debbio, S. Forte, A. Guffanti, and N. P. Hartland et al, Nucl. Phys. B, 867:244(2013)
    [6] L. Del Debbio et al. (NNPDF Collaboration), JHEP, 0703:039(2007) doi:10.1088/1126-6708/2007/03/039[hep-ph/0701127]
    [7] C. Bourrely and J. Soffer, arXiv:1502.02517
    [8] S. Alekhin, J. Bluemlein, and S. Moch, Phys. Rev. D, 89(5):054028(2014)
    [9] P. Jimenez-Delgado, and E. Reya, Phys. Rev. D, 89(7):074049(2014)
    [10] P. Aurenche, R. Baier, and M. Fontannaz, Phys. Rev. D, 42:1440(1990)
    [11] P. Aurenche, M. Fontannaz, J. P. Guillet, B. A. Kniehl, E. Pilon, and M. Werlen, Eur. Phys. J. C, 9:107(1999)
    [12] S. Catani, M. Fontannaz, J. P. Guillet, and E. Pilon, JHEP, 0205:028(2002)
    [13] V. M. Abazov et al (D0 Collaboration), Phys. Lett. B, 714:32(2012) doi:10.1016/j.physletb.2012.06.056[arXiv:1203.5865[hep-ex]]
    [14] T. Aaltonen et al (CDF Collaboration), Phys. Rev. Lett., 111(4):042003(2013) doi:10.1103/PhysRevLett.111.042003[arXiv:1303.6136[hep-ex]]
    [15] P. H. Beauchemin, V. A. Bednyakov, G. I. Lykasov, and Y. Y. Stepanenko, Phys. Rev. D, 92(3):034014(2015) doi:10.1103/PhysRevD.92.034014[arXiv:1410.2616[hep-ph]]
    [16] G. Bailas and V. P. Goncalves, Eur. Phys. J. C, 76(3):105(2016) doi:10.1140/epjc/s10052-016-3941-z[arXiv:1512.06007[hep-ph]]
    [17] V. A. Bednyakov, M. A. Demichev, G. I. Lykasov, T. Stavreva, and M. Stockton, Phys. Lett. B, 728:602(2014) doi:10.1016/j.physletb.2013.12.031[arXiv:1305.3548[hep-ph]]
    [18] V. M. Abazov et al (D0 Collaboration), Phys. Lett. B, 719:354(2013)[arXiv:1210.5033[hep-ex]]
    [19] S. Rostami, A. Khorramian, A. Aleedaneshvar, and M. Goharipour, arXiv:1510.08421
    [20] H. Abramowicz et al, Eur. Phys. J. C, 73(2):2311(2013)
    [21] J. J. Aubert et al, Nucl. Phys. B, 213:31(1983)
    [22] J. J. Aubert et al (European Muon Collaboration), Phys. Lett. B, 110:73(1982)
    [23] P. Jimenez-Delgado, T. J. Hobbs, J. T. Londergan, and W. Melnitchouk, Phys. Rev. Lett., 114(8):082002(2015)
    [24] H. Abramowicz et al (H1 and ZEUS Collaborations), Eur. Phys. J. C, 75(12):580(2015)
    [25] V. M. Abazov et al (D0 Collaboration), Phys. Rev. Lett., 102:192002(2009) doi:10.1103/PhysRevLett.102.192002[arXiv:0901.0739[hep-ex]]
    [26] T. Aaltonen et al (CDF Collaboration), Phys. Rev. D, 81:052006(2010) doi:10.1103/PhysRevD.81.052006[arXiv:0912.3453[hep-ex]]
    [27] T. P. Stavreva and J. F. Owens, Phys. Rev. D, 79:054017(2009) doi:10.1103/PhysRevD.79.054017[arXiv:0901.3791[hep-ph]]
    [28] T. Stavreva, I. Schienbein, F. Arleo, K. Kovarik, F. Olness, J. Y. Yu, and J. F. Owens, JHEP, 1101:152(2011)
    [29] S. Alekhin, J. Blumlein, and S. Moch, Phys. Rev. D, 89(5):054028(2014) doi:10.1103/PhysRevD.89.054028[arXiv:1310.3059[hep-ph]]
    [30] S. Dulat et al, Phys. Rev. D, 93(3):033006(2016) doi:10.1103/PhysRevD.93.033006[arXiv:1506.07443[hep-ph]]
    [31] R. D. Ball et al (NNPDF Collaboration), JHEP, 1504, 040(2015) doi:10.1007/JHEP04(2015)040[arXiv:1410.8849[hep-ph]]
    [32] A. Accardi, L. T. Brady, W. Melnitchouk, J. F. Owens, and N. Sato, Phys. Rev. D, 93(11):114017(2016) doi:10.1103/PhysRevD.93.114017[arXiv:1602.03154[hep-ph]]
    [33] H. Khanpour, A. N. Khorramian, and S. A. Tehrani, J. Phys. G, 40:045002(2013)
    [34] S. Alekhin et al, Eur. Phys. J. C, 75(7):304(2015)
    [35] M. Botje, Comput. Phys. Commun., 182:490(2011) doi:10.1016/j.cpc.2010.10.020[arXiv:1005.1481[hep-ph]]
    [36] F. James and M. Roos, Comput. Phys. Commun., 10:343(1975) doi:10.1016/0010-4655(75)90039-9
    [37] A. C. Benvenuti et al (BCDMS Collaboration), Phys. Lett. B, 223:485(1989)
    [38] W. G. Seligman, C. G. Arroyo, L. de Barbaro, P. de Barbaro, A. O. Bazarko, R. H. Bernstein, A. Bodek, and T. Bolton et al, Phys. Rev. Lett., 79:1213(1997)
    [39] L. W. Whitlow, E. M. Riordan, S. Dasu, S. Rock, and A. Bodek, Phys. Lett. B, 282:475(1992)
    [40] M. Arneodo et al (New Muon Collaboration), Nucl. Phys. B, 487:3(1997)
    [41] A. Aktas et al (H1 Collaboration), Phys. Lett. B, 653:134(2007) doi:10.1016/j.physletb.2007.07.050[arXiv:0706.3722[hep-ex]]
    [42] S. Chekanov et al (ZEUS Collaboration), Nucl. Phys. B, 765:1(2007) doi:10.1016/j.nuclphysb.2006.09.018[hep-ex/0608048]
    [43] S. Chekanov et al (ZEUS Collaboration), Phys. Lett. B, 547:164(2002) doi:10.1016/S0370-2693(02)02763-6[hep-ex/0208037]
    [44] V. M. Abazov et al (D0 Collaboration), Phys. Rev. D, 88:091102(2013)
    [45] V. M. Abazov et al (D0 Collaboration), Phys. Rev. D, 76, 012003(2007)
    [46] V. M. Abazov et al (D0 Collaboration), Phys. Rev. Lett., 112(15):151803(2014); Phys. Rev. Lett., 114(4):049901(2015)
    [47] T. A. Aaltonen et al (CDF Collaboration), Phys. Lett. B, 692:232(2010)
    [48] T. Aaltonen et al (CDF Collaboration), Phys. Rev. Lett., 102:181801(2009)
    [49] G. Aad et al (ATLAS Collaboration), Eur. Phys. J. C, 73(8):2509(2013)
    [50] G. Aad et al (ATLAS Collaboration), Phys. Rev. D, 86:014022(2012)
    [51] G. Aad et al (ATLAS Collaboration), Phys. Rev. D, 85:072004(2012)
    [52] S. Chatrchyan et al (CMS Collaboration), Phys. Rev. Lett., 109:111806(2012)
    [53] S. Chatrchyan et al (CMS Collaboration), Phys. Rev. D, 85:032002(2012)
    [54] S. Chatrchyan et al (CMS Collaboration), Phys. Rev. D, 90(3):032004(2014)
    [55] S. Chekanov et al (ZEUS Collaboration), Eur. Phys. J. C, 42:1(2005) doi:10.1140/epjc/s2005-02293-x[hep-ph/0503274]
    [56] F. D. Aaron et al (H1 and ZEUS Collaborations), JHEP, 1001:109(2010) doi:10.1007/JHEP01(2010)109[arXiv:0911.0884[hep-ex]]
    [57] D. Mason et al (NuTeV Collaboration), Phys. Rev. Lett., 99:192001(2007)
    [58] D. de Florian, R. Sassot, P. Zurita, and M. Stratmann, Phys. Rev. D, 85:074028(2012)
    [59] R. S. Thorne and R. G. Roberts, Phys. Rev. D, 57:6871(1998)
    [60] V. Bertone, R. Frederix, S. Frixione, J. Rojo, and M. Sutton, JHEP, 1408:166(2014)
    [61] T. Carli, D. Clements, A. Cooper-Sarkar, C. Gwenlan, G. P. Salam, F. Siegert, P. Starovoitov, and M. Sutton, Eur. Phys. J. C, 66:503(2010)
    [62] J. Alwall et al, JHEP, 1407:079(2014)
    [63] J. M. Campbell and R. K. Ellis, Nucl. Phys. Proc. Suppl., 205-206:10(2010)
    [64] J. Pumplin, D. Stump, R. Brock, D. Casey, J. Huston, J. Kalk, H. L. Lai and W. K. Tung, Phys. Rev. D, 65:014013(2001)[hep-ph/0101032]
    [65] E. Hoffmann and R. Moore, Z. Phys. C, 20:71(1983)
    [66] B. A. Kniehl, G. Kramer, I. Schienbein, and H. Spiesberger, Eur. Phys. J. C, 72:2082(2012)[arXiv:1202.0439[hep-ph]]
    [67] A. Kusina, K. KovaŹik, T. Je o, D. B. Clark, F. I. Olness, I. Schienbein and J. Y. Yu, PoS DIS, 2014:047(2014)[arXiv:1408.1114[hep-ph]]
    [68] F. Arbabifar, A. N. Khorramian, and M. Soleymaninia, Phys. Rev. D, 89(3):034006(2014)[arXiv:1311.1830[hep-ph]]
    [69] G. Altarelli and G. Parisi, Nucl. Phys. B, 126:298(1977)
    [70] V. N. Gribov and L. N. Lipatov, Sov. J. Nucl. Phys., 15:438(1972)[Yad. Fiz. 15, 781(1972)]
    [71] Y. L. Dokshitzer, Sov. Phys. JETP 46:641(1977); Zh. Eksp. Teor. Fiz., 73:1216(1977)
    [72] S. J. Brodsky, P. Hoyer, C. Peterson, and N. Sakai, Phys. Lett. B, 93:451(1980)
    [73] S. J. Brodsky, C. Peterson, and N. Sakai, Phys. Rev. D, 23:2745(1981)
    [74] F. S. Navarra, M. Nielsen, C. A. A. Nunes, and M. Teixeira, Phys. Rev. D, 54:842(1996)[hep-ph/9504388]
    [75] S. Paiva, M. Nielsen, F. S. Navarra, F. O. Duraes, and L. L. Barz, Mod. Phys. Lett. A, 13:2715(1998)[hep-ph/9610310]
    [76] W. Melnitchouk and A. W. Thomas, Phys. Lett. B, 414:134(1997)[hep-ph/9707387]
    [77] J. Pumplin, Phys. Rev. D, 73:114015(2006)[hep-ph/0508184]
    [78] P. M. Nadolsky, H. L. Lai, Q. H. Cao, J. Huston, J. Pumplin, D. Stump, W. K. Tung, and C.-P. Yuan, Phys. Rev. D, 78:013004(2008)
    [79] S. Dulat, T. J. Hou, J. Gao, J. Huston, J. Pumplin, C. Schmidt, D. Stump, and C.-P. Yuan, Phys. Rev. D, 89(7):073004(2014)
    [80] B. W. Harris, J. Smith, and R. Vogt, Nucl. Phys. B, 461:181(1996)
    [81] S. J. Brodsky and S. Gardner, Phys. Rev. Lett., 116(1):019101(2016)[arXiv:1504.00969[hep-ph]]
    [82] J. Blumlein, arXiv:1511.00229
    [83] K. Kovarik and T. Stavreva, arXiv:1206.2175[hep-ph]
    [84] T. Boettcher, P. Ilten, and M. Williams, arXiv:1512.06666
    [85] R. Aaij et al (LHCb Collaboration), Nucl. Phys. B, 871:1(2013)[arXiv:1302.2864[hep-ex]]
    [86] N. Y. Ivanov, Nucl. Phys. B, 814:142(2009)[arXiv:0812.0722[hep-ph]]
    [87] L. N. Ananikyan and N. Y. Ivanov, Nucl. Phys. B, 762:256(2007)[hep-ph/0701076]
    [88] L. N. Ananikyan and N. Y. Ivanov, Phys. Rev. D, 75:014010(2007)[hep-ph/0609074]
    [89] D. Boer et al, arXiv:1108.1713[nucl-th]
    [90] E. Laenen, S. Riemersma, J. Smith, and W. L. van Neerven, Nucl. Phys. B, 392:162(1993); S. Riemersma, J. Smith, and W. L. van Neerven, Phys. Lett. B, 347:143(1995)[hep-ph/9411431]
  • 加载中

Get Citation
Alireza Aleedaneshvar, Muhammad Goharipour and Saeedeh Rostami. Uncertainty of parton distribution functions due to physical observables in a global analysis[J]. Chinese Physics C, 2017, 41(2): 023101. doi: 10.1088/1674-1137/41/2/023101
Alireza Aleedaneshvar, Muhammad Goharipour and Saeedeh Rostami. Uncertainty of parton distribution functions due to physical observables in a global analysis[J]. Chinese Physics C, 2017, 41(2): 023101.  doi: 10.1088/1674-1137/41/2/023101 shu
Milestone
Received: 2016-09-05
Article Metric

Article Views(1523)
PDF Downloads(62)
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:

Uncertainty of parton distribution functions due to physical observables in a global analysis

Abstract: The recent measurement of the differential γ+c-jet cross section, performed at the Tevatron collider in Run II by the D0 collaboration, is studied in a next-to-leading order (NLO) global QCD analysis to assess its impact on the proton parton distribution functions (PDFs). We show that these data lead to a significant change in the gluon and charm quark distributions. We demonstrate also that there is an inconsistency between the new high precision HERA I+II combined data and Tevatron measurement. Moreover, in this study we investigate the impact of older EMC measurements of charm structure function Fc2 on the PDFs and compare the results with those from the analysis of Tevatron data. We show that both of them have the same impact on the PDFs, and thus can be recognized as the same evidence for the inefficiency of perturbative QCD in dealing with charm production in some kinematic regions.

    HTML

Reference (90)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return