Event calendar file
11-15 September 2017
Mexico/General timezone
- ismd2017@nucleares.unam.mx
Support
Cosmic ray and astroparticle physics (I)
Date:
14 Sep 16:45 - 18:50
Conveners
-
- Mario Rodriguez, Juan Carlos Arteaga
- Chairperson: Mario Rodríguez
Timetable | Contribution List
Displaying 5
contributions
out of
5
ALICE is one of the four big experiments of the LHC at CERN. Located 40 m underground with 30 m of overburden rock it can also operate to detect atmospheric muons produced by cosmic ray interactions with the atmosphere. The analysis of the data collected with cosmic triggers from 2010 until 2013, corresponding to around 30 days of live time, will be presented. Exploiting the specific capability o
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Presented by Dr. Arturo FERNANDEZ TELLEZ
on
14/9/2017
at
23:25
Beta disintegration is studied in the presence of a magnetic field, which imposes a preferential direction on the emission of neutrinos. We explore the possibility that this anisotropy in neutrino emission can account for observed Pulsar's velocities (kicks). The conditions under which the anisotropic emission of neutrinos (due to the magnetic field present in the system) causes a “kick” of th
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Presented by Dr. Daryel MANREZA
on
14/9/2017
at
22:35
In this talk I will review recent results about the cosmic ray spectrum
and chemical composition in the $10^{15}$-$10^{18}$ eV energy range. At lower
edge of this energy range we are quite confident that cosmic rays are
mainly of galactic origin, while at energies greater than those covered
in the same energy interval we have strong hints of an extra-galactic
origin of the radiation. Ind
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Presented by Andrea CHIAVASSA
on
14/9/2017
at
21:45
The Pierre Auger Observatory is the largest cosmic ray detector ever built. It was designed to detect the highest energy particles in the Universe, and it has been taking data since 2004. Our published results range from the measurement of the flux suppression at the highest energies to limits on 1000-PeV neutrinos, from limits on the flux of EeV neutrons from the Galaxy to the measurement of the
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Presented by Prof. Miguel MOSTAFA
on
14/9/2017
at
22:10
The KASCADE-Grande observatory was a ground-based air shower array devoted to the study of the energy and composition of cosmic rays with energies from 1 PeV to 1 EeV. The experiment consisted of different detector systems which allowed the simultaneous measurement of distinct components of the air showers (EAS), such as the muon content. In this contribution, we study the total muon number and th
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Presented by Dr. Juan Carlos ARTEAGA VELAZQUEZ
on
14/9/2017
at
23:00
