  Hard X-/soft Gamma-ray astronomy (> 100 keV) is a crucial field for the study
of important astrophysical phenomena such as the 511 keV positron annihilation
line in the Galactic center region and its origin, gamma-ray bursts, soft
gamma-ray repeaters, nuclear lines from SN explosions and more. However,
several key questions in this field require sensitivity and angular resolution
that are hardly achievable with present technology. A new generation of
instruments suitable to focus hard X-/soft Gamma-rays is necessary to overcome
the technological limitations of current direct-viewing telescopes. One
solution is using Laue lenses based on Bragg's diffraction in a transmission
configuration. To date, this technology is in an advanced stage of development
and further efforts are being made in order to significantly increase its
technology readiness level (TRL). To this end, massive production of suitable
crystals is required, as well as an improvement of the capability of their
alignment. Such a technological improvement could be exploited in stratospheric
balloon experiments and, ultimately, in space missions with a telescope of
about 20 m focal length, capable of focusing over a broad energy pass-band. We
present the latest technological developments of the TRILL (Technological
Readiness Increase for Laue Lenses) project, supported by ASI, devoted to the
advancement of the technological readiness of Laue lenses. We show the method
we developed for preparing suitable bent Germanium and Silicon crystals and the
latest advancements in crystals alignment technology.
