  The Cherenkov Telescope Array (CTA) is a future ground-based gamma-ray
astronomy detector that will consist of more than 100 Imaging Atmospheric
Cherenkov Telescopes of different sizes. The total reflective surface of
roughly 10 000 m$^2$ requires unprecedented technological efforts towards a
cost-efficient production of light-weight and reliable mirror substrates at
high production rate. We report on a new mirror concept proposed for CTA
developed by INFN, which is based on the replication from a spherical convex
mold under low pressure. The mirror substrate is an open structure design made
by thin glass layers at the mirror's front and rear interspaced by steel
cylinders. A first series of nominal size mirrors has been produced, for which
we discuss the optical properties in terms of radius of curvature and focusing
power.
