CALET on the ISS: a high energy astroparticle physics experiment

14th International Conference on Topics in Astroparticle and Underground Physics

物理学;天文学

Marrocchesi, Pier Simone^1,2

Dept. of Physical Sciences, Earth and Environment, Via Roma 56, Siena

1-53100, Italy^1

INFN Sezione di Pisa, Largo Bruno Pontecorvo 3, Pisa

1-56127, Italy^2

关键词: Astroparticle physics;    Cosmic ray propagation;    High-energy resolution;    High-precision measurement;    International Space stations;    Italian Space Agency;    Japanese experiment modules;    Science objectives;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/718/5/052023/pdf
DOI  :  10.1088/1742-6596/718/5/052023

学科分类：天文学(综合)

来源: IOP

【 摘 要 】

CALET is a space mission of the Japanese Aerospace Agency (JAXA) in collaboration with the Italian Space Agency (ASI) and NASA. The CALET instrument (CALorimetric Electron Telescope) is planned for a long exposure on the JEM-EF, an external platform of the Japanese Experiment Module KIBO, aboard the International Space Station (ISS). The main science objectives include high precision measurements of the inclusive electron (+positron) spectrum below 1 TeV and the exploration of the energy region above 1 TeV, where the shape of the high end of the spectrum might reveal the presence of nearby sources of acceleration. With an excellent energy resolution and low background contamination CALET will search for possible spectral signatures of dark matter with both electrons and gamma rays. It will also measure the high energy spectra and relative abundance of cosmic nuclei from proton to iron and detect trans-iron elements up to Z ∼ 40. With a large exposure and high energy resolution, CALET will be able to verify and complement the observations of CREAM, PAMELA and AMS-02 on a possible deviation from a pure power-law of proton and He spectra in the region of a few hundred GeV and to extend the study to the multi-TeV region. CALET will also contribute to clarify the present experimental picture on the energy dependence of the boron/carbon ratio, below and above 1 TeV/n, thereby providing valuable information on cosmic-ray propagation in the galaxy. Gamma-ray transients will be studied with a dedicated Gamma-ray Burst Monitor (GBM).