Jul 10 – 22, 2023
Orthodox Academy of Crete, Kolymbari, Crete, Greece (Hybrid mode)
Europe/Athens timezone

Measurement of the energy spectra of proton, Helium and Boron cosmic-rays with CALET on the International Space Station

Jul 18, 2023, 4:00 PM
20m
Room 1

Room 1

Talk Cosmology, Astrophysics, Gravity, Mathematical Physics Cosmology, Astrophysics, Gravity, Mathematical Physics

Speakers

Dr Sandro Gonzi (Università degli Studi di Firenze e INFN)Dr Sandro Gonzi (University of Florence (Department of Physics and Astronomy), National Institute for Nuclear Physics INFN (Division of Florence), National Research Council CNR (Institute of Applied Physics IFAC))

Description

The Calorimetric Electron Telescope (CALET) is a cosmic-ray observatory operating since October 2015 aboard the International Space Station (ISS). The primary scientific goal of the CALET mission is to perform a high-precision measurement of the inclusive spectrum of cosmic electrons and positrons up to about 20 TeV, where the shape of the spectrum might indicate the presence of nearby cosmic-ray sources or dark matter signatures. The CALET mission is also able to investigate the mechanism of cosmic-ray acceleration and propagation in the Galaxy, by performing direct measurements of the energy spectra and elemental composition of cosmic-ray nuclei from H to Fe and the abundance of trans-iron elements, up to Zr (Z = 40), in the energy range reaching the PeV scale. Finally, CALET can monitor the gamma-ray sky up to about 10 TeV, search for signals from gravitational-wave event candidates, and observe gamma-ray burst events. The CALET detector, consisting of a charge detector, an imaging calorimeter and a total absorption calorimeter has a total thickness of about 30 radiation lengths at normal incidence. The instrument can achieve a clear separation between hadrons and electrons and between charged particles and gamma-rays. In this contribution we summarize the most recent results obtained from data processed since the beginning of the mission, by focusing on the measured spectra of cosmic-ray proton, Helium and Boron, the latter flux compared with that of Carbon to investigate the secondary-to-primary abundance ratio B/C.

Details

Name: Sandro Gonzi
Title: Dr
Institution name: University of Florence (Department of Physics and Astronomy), National Institute for Nuclear Physics INFN (Division of Florence), National Research Council CNR (Institute of Applied Physics IFAC)
Country: Italy
Webpage of institution: https://www.fisica.unifi.it/index.html?newlang=eng

Is this abstract from experiment? Yes
Name of experiment and experimental site CALET Collaboration
Is the speaker for that presentation defined? Yes
Internet talk Maybe

Author

Dr Sandro Gonzi (University of Florence (Department of Physics and Astronomy), National Institute for Nuclear Physics INFN (Division of Florence), National Research Council CNR (Institute of Applied Physics IFAC))

Presentation materials