Pade estimate of QCD's infrared boundary

被引:6
作者
Chishtie, FA [1 ]
Elias, V
Steele, TG
机构
[1] Univ Western Ontario, Dept Appl Math, London, ON N6A 3K7, Canada
[2] Univ Saskatchewan, Dept Phys & Engn Phys, Saskatoon, SK S7N 5E2, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
D O I
10.1016/S0370-2693(01)00788-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A mass scale mu (c) representing the boundary between effective theories of strong interactions and perturbative QCD (infrared and ultraviolet regimes) exists when the beta -function is characterized by a simple pole. This behaviour. which is known to occur in N = 1 supersymmetric Yang-Mills theories, leads to an infrared attractor in the evolution of the coupling constant, with the mass scale mu (c) of the attractor providing a natural boundary between the infrared and ultraviolet regimes. It is demonstrated that [2 \2], [3 \1] and [1 \3] Pade-approximant versions of the three-flavour (n(f) = 3) QCD beta -function each contain a simple pole corresponding to such an infrared attractor. All three approximants, separately considered, are seen to lead to nearly equivalent estimates for the mass scale mu (c). (C) 2001 Published by Elsevier Science B.V.
引用
收藏
页码:279 / 283
页数:5
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