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R. D. Pisarski and M. H. G. Tytgat, in Hirschegg ’97: QCD Phase Transitions, edited by H. Feldmeier et al. (GSI Publishing, Darmstadt, 1997)
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R. D. Pisarski and M. H. G. Tytgat, in Hirschegg ’97: QCD Phase Transitions, edited by H. Feldmeier et al. (GSI Publishing, Darmstadt, 1997).
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E. Shuryak, Zh. Éksp. Teor. Fiz 74, 408 (1978) [Sov. Phys. JETP 47, 212 (1978)];
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Shuryak, E.1
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85037203029
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L can be diagonalized by a global gauge rotation. For a (Formula presented) matrix, (Formula presented) is maximized when L is a constant phase times the unit matrix; for a (Formula presented) matrix, then, L must be an element of the center
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L can be diagonalized by a global gauge rotation. For a (Formula presented) matrix, (Formula presented) is maximized when L is a constant phase times the unit matrix; for a (Formula presented) matrix, then, L must be an element of the center.
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46
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85037210782
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For discussion, consider what happens if the Debye mass is negative, so that the signs of (Formula presented) and (Formula presented) are switched, with (Formula presented) and (Formula presented). In this case, the favored vacuum maximizes (Formula presented), with (Formula presented) an element of the center; then the vacuum might break (Formula presented) to (Formula presented)
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For discussion, consider what happens if the Debye mass is negative, so that the signs of (Formula presented) and (Formula presented) are switched, with (Formula presented) and (Formula presented). In this case, the favored vacuum maximizes (Formula presented), with (Formula presented) an element of the center; then the vacuum might break (Formula presented) to (Formula presented).
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47
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0000929312
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T. Bhattacharya, A. Gocksch, C. Korthals Altes, and R. D. Pisarski, Nucl. Phys. B383, 497 (1992);
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Bhattacharya, T.1
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Pisarski, R.D.4
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49
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85037178737
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To ensure that the average (Formula presented) Wilson line transforms gauge covariantly, as in Eq. (3), the average is over “U” shaped Wilson paths: averaging over (Formula presented), the path is spatial from (Formula presented) to (Formula presented), temporal up to (Formula presented), and finally, spatial back to (Formula presented)
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To ensure that the average (Formula presented) Wilson line transforms gauge covariantly, as in Eq. (3), the average is over “U” shaped Wilson paths: averaging over (Formula presented), the path is spatial from (Formula presented) to (Formula presented), temporal up to (Formula presented), and finally, spatial back to (Formula presented).
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50
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18544391423
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R. D. Pisarski, Phys. Rev. C 62, 035202 (2000) and references therein.
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Pisarski, R.D.1
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0007437698
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M. Billo, M. Caselle, A. D’Adda, and S. Panzeri, Int. J. Mod. Phys. A 12, 1783 (1997).
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Int. J. Mod. Phys. A
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Billo, M.1
Caselle, M.2
D’Adda, A.3
Panzeri, S.4
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54
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0042492825
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As a function of N, the order of the deconfining transition in (Formula presented) gauge theories appears to be similar to that for the N-state Potts models [F. Y. Wu, Rev. Mod. Phys. 54, 235 (1982)]. While (Formula presented) (Formula presented)-spins (trivially) interact like Potts spins for (Formula presented) and (Formula presented), they are not the same when (Formula presented) 29.
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Rev. Mod. Phys.
, vol.54
, pp. 235
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Wu, F.Y.1
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55
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0001071646
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In mean field theory, though, Potts models are a special case of (Formula presented) models [R. G. Priest and T. C. Lubensky, Phys. Rev. B 13, 4159 (1976)]; thus I suggest that the proper view is that both deconfining and Potts transitions are driven by those of (Formula presented) spins.
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(1976)
Phys. Rev. B
, vol.13
, pp. 4159
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Priest, R.G.1
Lubensky, T.C.2
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58
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85037222886
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(Formula presented) is measurable from the two point function of the Wilson line near (Formula presented) From Eq. (11), the mass squared for the real part of (Formula presented) is (Formula presented), while that for the imaginary part is (Formula presented), with (Formula presented) from Eq. (4). Given (Formula presented) (Formula presented) can be measured by comparing these two masses. This should be done not at high temperature, but close to (Formula presented) At high temperature, (Formula presented) is nearly an (Formula presented) matrix and (Formula presented). The real and imaginary parts of (Formula presented) satisfy a geometric constraint, and cannot be varied independently. The constraint is invalid near (Formula presented) where the average (Formula presented) is not an (Formula presented) matrix. (Formula presented) is applicable for real (Formula presented) [or (Formula presented) transforms thereof] at all T
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(Formula presented) is measurable from the two point function of the Wilson line near (Formula presented) From Eq. (11), the mass squared for the real part of (Formula presented) is (Formula presented), while that for the imaginary part is (Formula presented), with (Formula presented) from Eq. (4). Given (Formula presented) (Formula presented) can be measured by comparing these two masses. This should be done not at high temperature, but close to (Formula presented) At high temperature, (Formula presented) is nearly an (Formula presented) matrix and (Formula presented). The real and imaginary parts of (Formula presented) satisfy a geometric constraint, and cannot be varied independently. The constraint is invalid near (Formula presented) where the average (Formula presented) is not an (Formula presented) matrix. (Formula presented) is applicable for real (Formula presented) [or (Formula presented) transforms thereof] at all T.
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59
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85037203806
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Mean field theory fails close to a second order transition, but the effect of nontrivial critical exponents can be included, as in Eq. (12) of
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Mean field theory fails close to a second order transition, but the effect of nontrivial critical exponents can be included, as in Eq. (12) of 4. The critical point for two colors is (Formula presented), while three colors is near an (Formula presented) fixed point.
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60
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0010819268
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The renormalized (Formula presented) Wilson line is given after extracting an overall renormalization constant. This constant is fixed by setting (Formula presented) at some temperature, such as (Formula presented) as (Formula presented) [E. Gava and R. Jengo, Phys. Lett. 105B, 285 (1981), 629, and
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Gava, E.1
Jengo, R.2
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61
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0031521444
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A. V. Smilga, Phys. Rep. 291, 1 (1997)]. In lattice perturbation theory, the ultraviolet divergence in the Wilson line is (Formula presented) after exponentiation, for some constant d and lattice spacing a. To isolate this divergence, it might be useful to measure the distribution of eigenvalues for the (Formula presented) Wilson line, and then compute the trace from that distribution.
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(1997)
Phys. Rep.
, vol.291
, pp. 1
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Smilga, A.V.1
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62
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4744354575
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K. Enqvist, K. Kajantie, L. Kärkkäinen, and K. Rummukainen, Phys. Lett. B 249, 107 (1990).
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Enqvist, K.1
Kajantie, K.2
Kärkkäinen, L.3
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69
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0003984846
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Cambridge University Press, Cambridge, England
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M. Le Bellac, Thermal Field Theory (Cambridge University Press, Cambridge, England, 1996).
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(1996)
Thermal Field Theory
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Le Bellac, M.1
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70
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85037223801
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Define null vectors (Formula presented) and (Formula presented) (Formula presented), and (Formula presented)With (Formula presented) the Debye mass squared, and (Formula presented) the normalized integral over (Formula presented), the usual Lagrangian for hard thermal loops is (Formula presented)
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Define null vectors (Formula presented) and (Formula presented) (Formula presented), and (Formula presented)With (Formula presented) the Debye mass squared, and (Formula presented) the normalized integral over (Formula presented), the usual Lagrangian for hard thermal loops is (Formula presented) 39. This does not look like the expansion of a Wilson line, though. However, an equivalent form is (Formula presented)which does look like an expansion of exponentials of (Formula presented) and (Formula presented).
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