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See, for example, M. Gyulassy and L. McLerran, nucl-th/0405013
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See, for example, M. Gyulassy and L. McLerran, nucl-th/0405013; R. Rapp, J. Phys. G 30, S951 (2004).
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See, for example, M. Gyulassy and L. McLerran, nucl-th/0405013; R. Rapp, J. Phys. G 30, S951 (2004).
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J. Phys. G
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Phys. Rev. D
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R. V. Gavai and S. Gupta, Phys. Rev. D 68, 034506 (2003); Nucl. Phys. B; Proc. Suppl. 129, 524 (2004).
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Nucl. Phys. B; Proc. Suppl.
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S. Choe et al., Phys. Rev. D 65, 054501 (2002).
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Phys. Rev. D
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J. Berges and K. Rajagopal, Nucl. Phys. B538, 215 (1999); M. A. Halasz et al., Phys. Rev. D 58, 096007 (1998).
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Halasz, M.A.1
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0344511720
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Preliminary results for the bare Taylor coefficients of the condensate at lattice spacing a = 1/47 in QCD with two flavors of quarks were presented in S. Choe et al., Nucl. Phys. B, Proc. Suppl. 106, 462 (2002). The bare series for the condensate has been also been studied earlier in the NJL model in O. Miyamura et al., Phys. Rev. D 66, 077502 (2002).
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Nucl. Phys. B, Proc. Suppl.
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Choe, S.1
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10944241581
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Preliminary results for the bare Taylor coefficients of the condensate at lattice spacing a = 1/47 in QCD with two flavors of quarks were presented in S. Choe et al., Nucl. Phys. B, Proc. Suppl. 106, 462 (2002). The bare series for the condensate has been also been studied earlier in the NJL model in O. Miyamura et al., Phys. Rev. D 66, 077502 (2002).
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Phys. Rev. D
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Miyamura, O.1
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19
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13544253556
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note
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s, care must be taken to absorb the sign into the multiplicative renormalization constant, so that the renormalizations of mass and chiral condensate differ by a sign. Equation (12) shows that this sign will not appear in the expansion of the condensate, but will then appear in the chiral Ward identities and the Maxwell relations.
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20
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13544253557
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private communication
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J.-P. Blaizot (private communication).
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Blaizot, J.-P.1
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13544270073
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S. Gupta, hep-lat/0202005
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S. Gupta, hep-lat/0202005.
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S. Hands and D. N. Walters, Phys. Rev. D 69, 076011 (2004); S. Hands and C. G. Strouthos, Phys. Rev. D 70, 056006 (2004).
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Phys. Rev. D
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C. Bernard, et al., Phys. Rev. D 45, 3854 (1992); S. Gottlieb, et al., Phys. Rev. D 47, 3619 (1993).
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Phys. Rev. D
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C. Bernard, et al., Phys. Rev. D 45, 3854 (1992); S. Gottlieb, et al., Phys. Rev. D 47, 3619 (1993).
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Phys. Rev. D
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13544267605
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M. D'Elia, A. Di Giacomo, and C Pica, hep-lat/0408008
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M. D'Elia, A. Di Giacomo, and C Pica, hep-lat/0408008.
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43
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84863933714
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hep-lat/0407041
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Preliminary exploration of this part of the QCD. phase diagram may-be found in J. B. Kogut and D. K. Sinclair. Phys. Rev. D 70, 074509 (2004); hep-lat/0407041; S. Gupta, hep-lat/0202005.
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Phys. Rev. D
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Sinclair, D.K.2
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13544252649
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S. Gupta, hep-lat/0202005
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Preliminary exploration of this part of the QCD. phase diagram may-be found in J. B. Kogut and D. K. Sinclair. Phys. Rev. D 70, 074509 (2004); hep-lat/0407041; S. Gupta, hep-lat/0202005.
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45
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13544276982
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note
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3 plane is due to a lattice artifact called saturation, which occurs when each lattice site contains the maximum number of allowed fermions. This is why the downward curve has been shown dotted in Fig. 8.
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