11-13 May 2021
Mexico/General timezone
- jose.benitez@cern.ch
Support
Astroparticle physics and Cosmology
Date:
11 May 10:10 - 11:01
Conveners
-
- Dr. Carraminana, Alberto (INAOE)
Timetable | Contribution List
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The knowledge of the spectrum and the composition of cosmic rays with energies from $10$ TeV to $1$ PeV is very uncertain. Detail measurements on these quantities are needed if models on the origin, acceleration mechanism and propagation of galactic cosmic rays are to be tested. In this contribution we present a detail study on the most abundant component of cosmic rays around TeVs, i.e., protons
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Presented by Dr. Juan Carlos ARTEAGA VELAZQUEZ
on
11/5/2021
at
10:10
In the past, due to the technological limitations of direct and indirect cosmic ray detectors, the observations made on the energy interval from 10 TeV to 1 PeV of the all-particle cosmic-ray energy spectrum have poor statistics and are dominated by large systematics errors. The High Altitude Water Cherenkov (HAWC) observatory, is a new generation air shower detector built with the aim of monitori
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Presented by Mr. Jorge Antonio MORALES SOTO
on
11/5/2021
at
15:27
Today it is well known that cosmological models must describe an accelerated expansion of the Universe in the current era. To achieve this, sources of matter capable of generating this acceleration are considered, which are commonly called dark energy. A cosmological constant Λ is an important candidate for dark energy that provides a good explanation for the current acceleration. But the cosmolo
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Presented by Dr. Carlos RODRIGUEZ-BENITES
on
11/5/2021
at
15:44