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The SU(3) Beta Function from Numerical Stochastic Perturbation Theory · Around

2013

The SU(3) Beta Function from Numerical Stochastic Perturbation Theory

Horsley, R., Perlt, H., Rakow, P. E. L. et al.

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Understand

The SU(3) beta function is computed from Wilson loops to 20th order numerical stochastic perturbation theory.

An attempt is made to include massless fermions, whose contribution is known analytically to 4th order.
The question whether the theory admits an infrared stable fixed point is addressed.

Built on

M. A. Shifman, Nucl. Phys. B 173
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M. Lüscher, Nucl. Phys. B 180
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G. Parisi and Y. -S. Wu, Sci. Sin. 24
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I. I. Kogan and M. A. Shifman, Phys. Rev. Lett. 75
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Earlier work this paper cites.

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Then

M. Göckeler, R. Horsley, A. C. Irving, D. Pleiter, P. E. L. Rakow, G. Schierholz and H. Stüben, Phys. Rev. D 73
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Later among the works it cites.
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Original
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Later among the works it cites.
R. Horsley, G. Hotzel, E.-M. Ilgenfritz, R. Millo, H. Perlt, P. E. L. Rakow, Y. Nakamura, G. Schierholz and A. Schiller, Phys. Rev. D 86
Original
2012
Later among the works it cites.

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