High energy QCD scattering, the shape of gravity on an IR brane, and the Froissart bound

被引:49
作者
Giddings, SB [1 ]
机构
[1] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[2] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[3] Stanford Univ, SLAC, Stanford, CA 94305 USA
关键词
D O I
10.1103/PhysRevD.67.126001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
High-energy scattering in nonconformal gauge theories is investigated using the AdS/conformal field theory (CFT) dual string-gravity theory. It is argued that strong-gravity processes, such as black hole formation, play an important role in the dual dynamics. Further information about this dynamics is found by performing a linearized analysis of gravity for a mass near an infrared brane; this gives the far field approximation to black hole or other strong-gravity effects, and in particular allows us to estimate their shape. From this shape, one can infer a total scattering cross section that grows with center of mass energy as ln(2) E, saturating the Froissart bound.
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