TY - JOUR
T1 - Development of hard X-ray polarimeter for γ-ray bursts
AU - Gunji, S.
AU - Suzuki, T.
AU - Sato, F.
AU - Sakurai, H.
AU - Tokanai, F.
AU - Saito, Y.
AU - Kubota, A.
N1 - Funding Information:
This work has been carried out with the support of a Grant-in-Aid for Scientific Research by the Japan Ministry of Education.
PY - 2004
Y1 - 2004
N2 - The radiation mechanism of gamma-ray bursts (GRBs) is one of the most interesting topics in the field of astrophysics. According to the fireball model, the γ-rays from GRBs should be much polarized. So we have been developing a Compton scattering type hard X-ray polarimeter for GRBs using segmented scintillators and multianode photomultipliers. We carried out basic experiments and computer simulations to investigate the basic performance. As the results, it was recognized that the designed polarimeter can detect the polarization of hard X-rays from GRBs with both the flux 10 times more than that of Crab nebula and the duration of 10 s if the hard X-rays are 8.6% polarized.
AB - The radiation mechanism of gamma-ray bursts (GRBs) is one of the most interesting topics in the field of astrophysics. According to the fireball model, the γ-rays from GRBs should be much polarized. So we have been developing a Compton scattering type hard X-ray polarimeter for GRBs using segmented scintillators and multianode photomultipliers. We carried out basic experiments and computer simulations to investigate the basic performance. As the results, it was recognized that the designed polarimeter can detect the polarization of hard X-rays from GRBs with both the flux 10 times more than that of Crab nebula and the duration of 10 s if the hard X-rays are 8.6% polarized.
KW - Hard X-ray polarimeter
KW - Scientific ballooning
KW - γ-ray bursts
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U2 - 10.1016/j.asr.2003.09.049
DO - 10.1016/j.asr.2003.09.049
M3 - Article
AN - SCOPUS:2442463206
VL - 33
SP - 1771
EP - 1776
JO - Life sciences and space research
JF - Life sciences and space research
SN - 0273-1177
IS - 10
ER -