The TRILL project: increasing the technological readiness of Laue lenses
Lisa Ferro, Enrico Virgilli, Miguel Moita, Filippo Frontera, Piero, Rosati, Cristiano Guidorzi, Claudio Ferrari, Riccardo Lolli, Ezio Caroli,, Natalia Auricchio, John B. Stephen, Stefano Del Sordo, Carmelo Gargano,, Stefano Squerzanti, Mauro Pucci, Olivier Limousin, Aline Meuris

TL;DR
The TRILL project advances Laue lens technology for hard X-/soft Gamma-ray astronomy by developing bent crystal preparation and alignment methods to improve focus and sensitivity for future space missions.
Contribution
This work introduces new methods for preparing and aligning bent Germanium and Silicon crystals, enhancing the technological readiness of Laue lenses.
Findings
Successful development of bent crystal preparation techniques
Improved crystal alignment technology
Enhanced potential for space-based gamma-ray telescopes
Abstract
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…
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