Event calendar file
4-12 November 2010
Morelia, Michoacan
Mexico/General timezone
- arteaga@ifm.umich.mx
Support
Session II NU.CR
Place
Location: Morelia, Michoacan
Room: Hall B, Hotel Fiesta Inn
Date:
9 Nov 16:00 - 21:00
Conveners
-
- Dr. Sahu, Sarira (UNAM)
-
- Dr. Pérez-Lorenzana, Abdel (CINVESTAV)
Timetable | Contribution List
Displaying 9
contributions
out of
9
In this contribution, the all-particle energy spectrum from 10^16 to 10^18 eV, as reconstructed from the KASCADE-Grande data, is presented. As it will be shown, in this interval the cosmic ray spectrum does not follow a simple power-law behavior due to the presence of two unexpected and significative features in the flux. Along with these results, a brief description of the experiment and the ana
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Presented by Dr. Juan Carlos ARTEAGA VELAZQUEZ
on
10/11/2010
at
0:00
Gamma-Ray Bursts (GRBs) are the most powerful explosion in the universe. They are possible candidates of the sources of Ultra-high energy cosmic rays (UHECRs) and very high-energy neutrinos/gamma-rays. I would like to review the explosion mechanism of GRBs and how UHECRs can be produced in GRBs. I would like to present our recent study on the central engine of GRBs with some movies of numerical si
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Presented by Prof. Shigehiro NAGATAKI
on
9/11/2010
at
23:00
The flux of cosmic rays above 10^18 eV has been measured with unprecedented precision using the Pierre Auger Observatory. We describe the present status of the Auger Observatory and discuss the latest results obtained by the Auger Observatory with emphasis on the update of the correlation of the arrival directions of the most energetic cosmic rays with nearby active galactic nuclei, the measurem
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Presented by Dr. Luis VILLASENOR
on
10/11/2010
at
1:00
on
9/11/2010
at
22:30
Oscillations between active and sterile neutrinos remain as an open possibility to explain some anomalous experimental observations. In a four-neutrino (three active plus one sterile) mixing scheme, we use the Magnus expansion of the evolution operator to study the evolution of neutrino flavor amplitudes within the Earth. We apply this formalism to calculate the transition probabilities from activ
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Presented by Dr. Mario Andres ACERO ORTEGA
on
9/11/2010
at
22:00
