scholarly journals Erratum:QQ¯potential in the Schwinger model on curved space-time [Phys. Rev. D63, 065009 (2001)]

2001 ◽  
Vol 64 (4) ◽  
Author(s):  
H. Mohseni Sadjadi ◽  
Kh. Saaidi
Keyword(s):  
Space Time ◽  
Curved Space ◽  
Schwinger Model

Path integrals and the solution of the Schwinger model in curved space-time

1986 ◽  
Vol 33 (8) ◽  
pp. 2262-2266 ◽  
Author(s):  
J. Barcelos-Neto ◽  
Ashok Das
Keyword(s):  
Path Integrals ◽  
Space Time ◽  
Curved Space ◽  
Schwinger Model

Schwinger model in curved space-time

1983 ◽  
Vol 27 (12) ◽  
pp. 2893-2905 ◽  
Author(s):  
Richard Gass
Keyword(s):  
Space Time ◽  
Curved Space ◽  
Schwinger Model

Chiral Schwinger model in curved space-time

1986 ◽  
Vol 32 (4) ◽  
pp. 527-530 ◽  
Author(s):  
J. Barcelos-Neto ◽  
Ashok Das
Keyword(s):  
Space Time ◽  
Curved Space ◽  
Schwinger Model

scholarly journals QQ¯potential in the Schwinger model on curved space-time

2001 ◽  
Vol 63 (6) ◽  
Author(s):  
H. Mohseni Sadjadi ◽  
Kh. Saaidi
Keyword(s):  
Space Time ◽  
Curved Space ◽  
Schwinger Model

scholarly journals ε-EXPANSION IN QUANTUM FIELD THEORY IN CURVED SPACE–TIME

1998 ◽  
Vol 13 (16) ◽  
pp. 2857-2874
Author(s):  
IVER H. BREVIK ◽  
HERNÁN OCAMPO ◽  
SERGEI ODINTSOV
Keyword(s):  
Field Theory ◽  
Quantum Field Theory ◽  
Space Time ◽  
Quantum Field ◽  
Curved Space ◽  
Njl Model ◽  
Effective Lagrangian ◽  
Special Solutions ◽  
Curvature Approximation ◽  
Symmetric Phase

We discuss ε-expansion in curved space–time for asymptotically free and asymptotically nonfree theories. The existence of stable and unstable fixed points is investigated for fϕ4 theory and SU(2) gauge theory. It is shown that ε-expansion maybe compatible with aysmptotic freedom on special solutions of the RG equations in a special ase (supersymmetric theory). Using ε-expansion RG technique, the effective Lagrangian for covariantly constant gauge SU(2) field and effective potential for gauged NJL model are found in (4-ε)-dimensional curved space (in linear curvature approximation). The curvature-induced phase transitions from symmetric phase to asymmetric phase (chromomagnetic vacuum and chiral symmetry broken phase, respectively) are discussed for the above two models.

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