Event calendar file
27-29 March 2023
Mexico/General timezone
D1-Talks
Date:
27 Mar 09:15 - 10:00
Conveners
-
Cosmic Rays
- Dr. Martínez-Huerta, Humberto (Departamento de Física y Matemáticas, UDEM)
Timetable | Contribution List
Displaying 3
contributions
out of
3
The number of muons in extensive air showers (EAS) is a useful quantity to investigate the composition of high-energy cosmic rays by indirect detection techniques. It is also a sensitive probe for tests of high-energy hadronic interaction models at laboratory energies that are several orders of magnitude larger than those achieved at current particle physics facilities. For these reasons, it is i
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Presented by Dr. Juan Carlos ARTEAGA VELAZQUEZ
on
27/3/2023
at
15:45
Simulations with CORSIKA and EXPACS Software were performed to complete calculations based on Dorman’s general theory of atmospheric electric field effects on secondary cosmic rays. The calculations were done for the particles detected at the Sierra Negra Cosmic Ray Observatory, located at a height of 4580 m a.s.l. Variations of 1.15-3.47% on the intensity of the charged component were estimated
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Presented by Mrs. Jania NEWTON
on
27/3/2023
at
15:30
In the quest for particle dark matter and physics beyond the Standard Model, the possibility of the existence of neutral long-lived particles (LLPs) has been proposed. The MATHUSLA project is designed as a surface experiment to detect possible LLPs produced in collisions at the CERN High-Luminosity Large Hadron Collider (HL-LHC). The MATHUSLA detector will cover a 10^4 m^2 surface and will have 9
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Presented by Prof. Paolo CAMARRI
on
27/3/2023
at
15:15
