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

Greiner, J. (author)
Iyudin, A. (author)
Kanbach, G. (author)
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Zoglauer, A. (author)
Diehl, R. (author)
Ryde, Felix (author)
KTH,Partikel- och astropartikelfysik
Hartmann, D. (author)
Kienlin, A. V. (author)
McBreen, S. (author)
Ajello, M. (author)
Bagoly, Z. (author)
Balasz, L. G. (author)
Barbiellini, G. (author)
Bellazini, R. (author)
Bezrukov, L. (author)
Bisikalo, D. V. (author)
Bisnovaty-Kogan, G. (author)
Boggs, S. (author)
Bykov, A. (author)
Cherepashuk, A. M. (author)
Chernenko, A. (author)
Collmar, W. (author)
DiCocco, G. (author)
Dröge, W. (author)
Gierlik, M. (author)
Hanlon, L. (author)
Horvath, I. (author)
Hudec, R. (author)
Kiener, J. (author)
Labanti, C. (author)
Langer, N. (author)
Larsson, S. (author)
Lichti, G. (author)
Lipunov, V. M. (author)
Lubsandorgiev, B. K. (author)
Majczyna, A. (author)
Mannheim, K. (author)
Marcinkowski, R. (author)
Marisaldi, M. (author)
McBreen, B. (author)
Meszaros, A. (author)
Orlando, E. (author)
Panasyuk, M. I. (author)
Pearce, Mark, 1970- (author)
KTH,Partikel- och astropartikelfysik
Pian, E. (author)
Poleschuk, R. V. (author)
Pollo, A. (author)
Pozanenko, A. (author)
Savaglio, S. (author)
Shustov, B. (author)
Strong, A. (author)
Svertilov, S. (author)
Tatischeff, V. (author)
Uvarov, J. (author)
Varshalovich, D. A. (author)
Wunderer, C. B. (author)
Wrochna, G. (author)
Zabrodskij, A. G. (author)
Zeleny, L. M. (author)
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 (creator_code:org_t)
2008-07-29
2009
English.
In: Experimental astronomy. - : Springer Science and Business Media LLC. - 0922-6435 .- 1572-9508. ; 23:1, s. 91-120
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The primary scientific goal of the GRIPS mission is to revolutionize our understanding of the early universe using gamma-ray bursts. We propose a new generation gamma-ray observatory capable of unprecedented spectroscopy over a wide range of gamma-ray energies (200 keV-50 MeV) and of polarimetry (200-1000 keV). The gamma-ray sensitivity to nuclear absorption features enables the measurement of column densities as high as 10(28)cm (-aEuro parts per thousand 2). Secondary goals achievable by this mission include direct measurements of all types of supernova interiors through gamma-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.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

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