Curvature induced phase transition is thoroughly investigated in a four-
fermion theory with N components of fermions for arbitrary space-time
dimensions (2β€D<4). We adopt the 1/N expansion method and calculate
the effective potential for a composite operator ΟΛβΟ. The
resulting effective potential is expanded asymptotically in terms of the
space-time curvature R by using the Riemann normal coordinate. We assume that
the space-time curves slowly and keep only terms independent of R and terms
linear in R. Evaluating the effective potential it is found that the
first-order phase transition is caused and the broken chiral symmetry is
restored for a large positive curvature. In the space-time with a negative
curvature the chiral symmetry is broken down even if the coupling constant of
the four-fermion interaction is sufficiently small. We present the behavior of
the dynamically generated fermion mass. The critical curvature, Rcrβ, which
divides the symmetric and asymmetric phases is obtained analytically as a
function of the space-time dimension D. At the four-dimensional limit our
result Rcrβ agrees with the exact results known in de Sitter space and
Einstein universe.Comment: 19 pages, uses LaTeX, eepic.st