Manifestation of Ricci scalar like a matter field as well as a geometr
ical field, at high energy, has been noted earlier [9]. Here, its inte
raction, with another scalar field is considered in four-dimensional c
urved space-time. This interaction leads to the production of a large
number of pairs of spinless particle-antiparticle due to expansion of
the early universe in the vacuum state (provided by temperature depend
ent Coleman-Weinberg like potential for Ricci field), where spontaneou
s symmetry breaking takes place.