GRI: focusing on the evolving violent Universe
J\"urgen Kn\"odlseder (CESR), Peter Von Ballmoos (CESR), Filippo, Frontera (UNIFE), Angela Bazzano, Finn E. Christensen (DNSC), Margarida, Hernanz (CSIC-IEEC), Cornelia Wunderer (SSL)

TL;DR
The GRI mission concept aims to revolutionize gamma-ray astronomy by providing unprecedented sensitivity and resolution in the soft gamma-ray to hard X-ray range through innovative focusing optics and formation flying spacecraft.
Contribution
This paper introduces the GRI mission concept, featuring a novel Laue lens and multilayer mirror for high-sensitivity gamma-ray observations, with a unique formation flying design.
Findings
Unprecedented sensitivity in 200-1300 keV range
Angular resolution better than 30 arcsec
Potential to study violent cosmic phenomena in detail
Abstract
The Gamma-Ray Imager (GRI) is a novel mission concept that will provide an unprecedented sensitivity leap in the soft gamma-ray domain by using for the first time a focusing lens built of Laue diffracting crystals. The lens will cover an energy band from 200 - 1300 keV with an effective area reaching 600 cm2. It will be complemented by a single reflection multilayer coated mirror, extending the GRI energy band into the hard X-ray regime, down to ~10 keV. The concentrated photons will be collected by a position sensitive pixelised CZT stack detector. We estimate continuum sensitivities of better than 10^-7 ph/cm2/s/keV for a 100 ks exposure; the narrow line sensitivity will be better than 3 x 10^-6 ph/cm2/s for the same integration time. As focusing instrument, GRI will have an angular resolution of better than 30 arcsec within a field of view of roughly 5 arcmin - an unprecedented…
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Taxonomy
TopicsComputational Physics and Python Applications
