摘要The potential of pp →p γγp →pGp process in scenarios of the Arkani-Hamed, Dimopoulos, Dvali (ADD) and Randall-Sundrum (RS) model at the LHC is examined, and 95% C.L. bounds on the model parameters are obtained. It is found that the sensitivity of the model parameters can be improved in the present colliders by using this reaction.
Abstract：The potential of pp →p γγp →pGp process in scenarios of the Arkani-Hamed, Dimopoulos, Dvali (ADD) and Randall-Sundrum (RS) model at the LHC is examined, and 95% C.L. bounds on the model parameters are obtained. It is found that the sensitivity of the model parameters can be improved in the present colliders by using this reaction.
S. C. İnan. Direct Graviton Production via Photon-Photon Fusion at the CERN-LHC[J]. 中国物理快报, 2012, 29(3): 31301-031301.
S. C. İ, nan. Direct Graviton Production via Photon-Photon Fusion at the CERN-LHC. Chin. Phys. Lett., 2012, 29(3): 31301-031301.
[1] Arkani-Hamed N, Dimopoulos S and Dvali G 1998 Phys. Lett. B 429 263
[2] Antoniadis I, Arkani-Hamed N, Dimopoulos S and G Dvali 1998 Phys. Lett. B 436 257
[3] Arkani-Hamed N, Dimopoulos S and Dvali G 1999 Phys. Rev. D 59 086004
[4] Randall L and Sundrum R 1999 Phys. Rev. Lett. 83 3370
[5] Goldberger W D and Wise M B 1999 Phys. Rev. Lett. 83 4922
[6] Abulencia A et al (CDF Collaboration) 2007 Phys. Rev. Lett. 98 112001
[7] Aaltonen T et al (CDF Collaboration) 2007 Phys. Rev. Lett. 99 242002
[8] Aaltonen T et al (CDF Collaboration) 2008 Phys. Rev. D 77 052004
[9] Aaltonen T et al (CDF Collaboration) 2009 Phys. Rev. Lett. 102 242001
[10] Aaltonen T et al (CDF Collaboration) 2009 Phys. Rev. Lett. 102 222002
[11] Kepka O and Royon C 2007 Phys. Rev. D 76 034012
[12] Rangel M et al 2007 Nucl. Phys. B 774 53
[13] Lietti S M et al 2001 Phys. Lett. B 497 243
[14] Piotrzkowski K 2001 Phys. Rev. D 63 071502
[15] Khoze V A, Martin A D, Orava R and Ryskin M G 2001 Eur. Phys. J. C 19 313
[16] Goncalves V P and Machado M V T 2007 Phys. Rev. D 75 031502
[17] Machado M V T 2008 Phys. Rev. D 78 034016
[18] İ. Şahin İ and İnan S C 2009 J. High Energy Phys. 09 069
[19] Atağ S, İnan S C and Şahin İ 2009 Phys. Rev. D 80 075009
[20] İnan S C 2010 Phys. Rev. D 81 115002
[21] Chapon E, Royon C and Kepka O 2010 Phys. Rev. D 81 074003
[22] Şahin İ and Billur A A 2011 Phys. Rev. D 83 035011
[23] Şahin İ and Köksal M 2011 J. High Energy Phys. 03 100
[24] İnan S C, Billur A A 2011 Phys. Rev. D 84 095002
[25] Albrow M G et al (FP420 R and D Collaboration) 2008 arXiv:0806.0302[hep-ex]
[26] Kepka O and Royon C 2008 Phys. Rev. D 78 073005
[27] Albrow M et al 2006 Report No. CERN-TOTEM-NOTE-2006-005
[28] Budnev V M et al 1975 Phys. Rep. 15 181
[29] Baur G et al 2002 Phys. Rep. 364 359
[30] Guidice G F, Ratazzi R and Wells J D 1999 Nucl. Phys. B 544 3
[31] Han T, Lykken J D and Zhank R J 1999 Phys. Rev. D 59 105006
[32] Davoudiasl H, Hewett J L and Rizzo T 2000 Phys. Rev. Lett. 84 2080
[33] Hewett J and Spiropulu M 2002 Annu. Rev. Nucl. Part. Sci. 52 397
[34] Mathews P and Ravindran V 2005 Nucl. Phys. B 713 333
[35] Mathews P and Ravindran V 2006 Nucl. Phys. B 753 1
[36] Kumar M C, Mathews P and Ravindran V 2007 Eur. Phys. J. C 49 599
[37] Chatrchyan S et al (CMS Collaboration) 2011 J. High Energy Phys. 05 085
[38] Aaltonen T et al (CDF Collaboration) 2011 Phys. Rev. D 83 011102
2012, Vol. 29 
