-
3
-
-
16844381370
-
-
16, 1147 (1977); 16, 1169 (1977); 7, 1109 (1978).
-
B.A. Freedman and L.D. McLerran, Phys. Rev. D 16, 1130 (1977); 16, 1147 (1977); 16, 1169 (1977); 7, 1109 (1978).
-
(1977)
Phys. Rev. D
, vol.16
, pp. 1130
-
-
Freedman, B.A.1
McLerran, L.D.2
-
12
-
-
0000358984
-
-
B. Datta, P.K. Sahu, J.D. Anand, and A. Goyal, ibid. 283, 313 (1992).
-
(1992)
Ibid.
, vol.283
, pp. 313
-
-
Datta, B.1
Sahu, P.K.2
Anand, J.D.3
Goyal, A.4
-
13
-
-
0000723965
-
-
M. Dey, I. Bombaci, J. Dey, S. Ray, and B.C. Samanta, Phys. Lett. B 438, 123 (1998).
-
(1998)
Phys. Lett. B
, vol.438
, pp. 123
-
-
Dey, M.1
Bombaci, I.2
Dey, J.3
Ray, S.4
Samanta, B.C.5
-
14
-
-
0000306274
-
-
D. Blaschke, H. Grigorian, G. Poghosyan, C.D. Roberts, and S.M. Schmidt, Phys. Lett. B 450, 207 (1999).
-
(1999)
Phys. Lett. B
, vol.450
, pp. 207
-
-
Blaschke, D.1
Grigorian, H.2
Poghosyan, G.3
Roberts, C.D.4
Schmidt, S.M.5
-
17
-
-
33744643361
-
-
J. Phys. G 9, 1487 (1983);
-
(1983)
J. Phys. G
, vol.9
, pp. 1487
-
-
-
18
-
-
0000719914
-
-
K. Schertier, C. Greiner, J. Schaffner-Bielich, and M.H. Thoma, Nucl. Phys. A677, 463 (2000).
-
(2000)
Nucl. Phys. A
, vol.677
, pp. 463
-
-
Schertier, K.1
Greiner, C.2
Schaffner-Bielich, J.3
Thoma, M.H.4
-
22
-
-
4243268578
-
-
In thé fj.-T plane, if the chiral critical endpoint exists at relatively high temperatures, as suggested by: M. Stephanov, K. Rajagopal, and E. Shuryak, Phys. Rev. Lett. 81, 4816 (1998);
-
(1998)
Phys. Rev. Lett.
, vol.81
, pp. 4816
-
-
Stephanov, M.1
Rajagopal, K.2
Shuryak, E.3
-
23
-
-
18044366808
-
-
Phys. Rev. D 60, 114028 (1999), then, implicitly, it is natural that the chiral transition at fi-4O, T=0, is strongly first order.
-
(1999)
Phys. Rev. D
, vol.60
, pp. 114028
-
-
-
24
-
-
0038543806
-
-
Chiral symmetry is not a rigorous order parameter if any quark mass is nonzero, or when color superconductivity occurs for Nf=3: T. Schäfer and F. Wilczek, Phys. Rev. Lett. 82, 3956 (1999);
-
(1999)
Phys. Rev. Lett.
, vol.82
, pp. 3956
-
-
Schäfer, T.1
Wilczek, F.2
-
25
-
-
18044376488
-
-
Phys. Rev. D 60, 074014 (1999);
-
(1999)
Phys. Rev. D
, vol.60
, pp. 074014
-
-
-
26
-
-
18544391423
-
-
17J. This does not affect our qualitative conclusions about a strongly first order chiral transition at /-4O, T=0.
-
R.D. Pisarski, Phys. Rev. C 62,035202 (2000);[17J. This does not affect our qualitative conclusions about a strongly first order chiral transition at /-4O, T=0.
-
(2000)
Phys. Rev. C
, vol.62
, pp. 035202
-
-
Pisarski, R.D.1
-
27
-
-
33750656148
-
-
K. Rajagopal and F. Wilczek, hep-ph/0011333.
-
K. Rajagopal and F. Wilczek, hep-ph/0011333.
-
-
-
-
30
-
-
33750653983
-
-
note
-
See Eq. (4.52) of Ref. [3J. This transformation differs from that of [21], but agrees with the final version of [22J.
-
-
-
-
33
-
-
33750651885
-
-
note
-
The uncertainty in G0= 10.374 ±.13 is due to errors in numerical integration. We take the central value of [2]; within errors, it agrees with [3J.
-
-
-
-
34
-
-
33750634617
-
-
note
-
in Eq. (3) we take or/A) to three loop order. If instead one uses j(A) to two loop order, then for the same value of A//I (= 1,2,3), fic changes by ~ +10%. However, the same /xc can be obtained by shifting Kip, by ~ + 10%; with this shift, the pressure changes by <1.5% in all three cases.
-
-
-
-
36
-
-
4244118354
-
-
Phys. Rev. Lett. 76, 1417 (1996); Phys. Rev. D 53, 3421 (1996)
-
E. Braaten and A. Nieto, ibid. 51, 6990 (1995); Phys. Rev. Lett. 76, 1417 (1996); Phys. Rev. D 53, 3421 (1996);
-
(1995)
Ibid.
, vol.51
, pp. 6990
-
-
Braaten, E.1
Nieto, A.2
-
39
-
-
16644382014
-
-
61, 074016 (2000); 62, 045004 (2000); 63, 105008 (2001)
-
Phys. Rev. D 61, 014017 (2000); 61, 074016 (2000); 62, 045004 (2000); 63, 105008 (2001);
-
(2000)
Phys. Rev. D
, vol.61
, pp. 014017
-
-
-
40
-
-
0001651218
-
-
Phys. Lett. B 470, 181 (1999)
-
J.-P. Blaizot, E. lancu, and A. Rebhan, Phys. Rev. Lett. 83, 2906 (1999); Phys. Lett. B 470, 181 (1999);
-
(1999)
Phys. Rev. Lett.
, vol.83
, pp. 2906
-
-
Blaizot, J.-P.1
Lancu, E.2
Rebhan, A.3
-
41
-
-
33750640581
-
-
A. Peshier, hep-ph/9910451; hep-ph/0011250.
-
A. Peshier, hep-ph/9910451; hep-ph/0011250.
-
-
-
-
43
-
-
0000950374
-
-
B. Kastening, ibid. 56, 8107 (1997);
-
(1997)
Ibid.
, vol.56
, pp. 8107
-
-
Kastening, B.1
-
44
-
-
0034907057
-
-
hep-th/0010197; ibid, (to be published), hep-ph/0010294.
-
R. Parwani, hep-th/0010197; Phys. Rev. D 1 63, 054014 (2001); ibid, (to be published), hep-ph/0010294.
-
(2001)
Phys. Rev. D 1
, vol.63
, pp. 054014
-
-
Parwani, R.1
-
48
-
-
17044364764
-
-
62, 054013 (2000); 62, 054016 (2000)
-
W.E. Brown, J.T. Liu, and H. Ren, Phys. Rev. D 61, 114012 (2000); 62, 054013 (2000); 62, 054016 (2000);
-
(2000)
Phys. Rev. D
, vol.61
, pp. 114012
-
-
Brown, W.E.1
Liu, J.T.2
Ren, H.3
-
50
-
-
0000891137
-
-
T. DeGrand, R.L. Jaffe, K. Johnson, and J. Kiskis, Phys. Rev. D 12, 2060 (1975)
-
(1975)
Phys. Rev. D
, vol.12
, pp. 2060
-
-
Degrand, T.1
Jaffe, R.L.2
Johnson, K.3
Kiskis, J.4
-
51
-
-
33750644319
-
-
hep-ph/9802419, and references therein.
-
A.V. Manohar, hep-ph/9802419, and references therein.
-
-
-
Manohar, A.V.1
-
57
-
-
0034178695
-
-
2D /Nc, and chiral density waves form [E. Shuster and D.T. Son, Nucl. Phys. B573, 434 (2000)J.
-
(2000)
Nucl. Phys.
, vol.B573
, pp. 434
-
-
Shuster, E.1
Son, D.T.2
-
59
-
-
16644379018
-
-
When fi<.px, the pressure is small if it is dominated by the thermal Polyakov loop [R.D. Pisarski, Phys. Rev. D 62, 111501R (2000)]; and if its expectation value is also small. Why this should be true, especially ifNj-4Nc, is unclear [35]. Perhaps ms£Q has a greater effect when p-/j.x.
-
(2000)
Phys. Rev. D
, vol.62
-
-
Pisarski, R.D.1
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