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Gamma-ray burst investigation via polarimetry and spectroscopy (GRIPS)

Abstract : The primary scientific goal of the GRIPS mission is to revolutionize our understanding of the early universe using γ-ray bursts. We propose a new generation gamma-ray observatory capable of unprecedented spectroscopy over a wide range of γ-ray energies (200 keV-50 MeV) and of polarimetry (200-1000 keV). The γ-ray sensitivity to nuclear absorption features enables the measurement of column densities as high as 1028cm - 2. Secondary goals achievable by this mission include direct measurements of all types of supernova interiors through γ-rays from radioactive decays, nuclear astrophysics with massive stars and novae, and studies of particle acceleration near compact stars, interstellar shocks, and clusters of galaxies.
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Contributor : Christine Hadrossek Connect in order to contact the contributor
Submitted on : Thursday, February 16, 2012 - 5:32:06 PM
Last modification on : Wednesday, December 22, 2021 - 3:34:29 AM

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J. Greiner, A. Iyudin, G. Kanbach, A. Zoglauer, R. Diehl, et al.. Gamma-ray burst investigation via polarimetry and spectroscopy (GRIPS). Experimental Astronomy, springer Link, 2009, 23, pp.91-120. ⟨10.1007/S10686-008-9102-0⟩. ⟨in2p3-00671104⟩



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