30 August 2022 to 12 September 2022
Conference venue: OAC conference center, Kolymbari, Crete, Greece. The conference will take place in Crete in physical form, however participation is also possible via internet
Europe/Athens timezone
"Second MODE Workshop on Differentiable Programming for Experiment Design" following after ICNFP2022 (https://indico.cern.ch/event/1145124/)

Muon measurements at the Pierre Auger Observatory

6 Sept 2022, 16:30
20m
Room 3

Room 3

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

Speaker

Eva Santos

Description

Muons in extensive air showers have large decay lengths and small
radiative energy losses. Therefore, muons can reach surface and underground detector arrays while keeping relevant information about the hadronic cascade. Data from several air shower experiments reveal inconsistencies in our current high-energy hadronic interaction models.
In most experiments, a larger muon content is observed compared to the hadronic model predictions. In this contribution, we report on the measurements of the muon content of air showers performed with the surface detector array of the Pierre Auger Observatory. In particular, we will focus on the overall muon content and its fluctuations. We also report on the first direct measurements of the muon content using the Engineering Array of underground muon detectors.

Details

Dr. Eva Santos, FZU - Institute of Physics of the Czech Academy of Sciences, Czech Republic, https://www.fzu.cz/en/home

Is this abstract from experiment? Yes
Name of experiment and experimental site Pierre Auger Collaboration, Observatorio Pierre Auger, Av. San Martíın Norte 304, 5613 Malargüe, Argentina
Is the speaker for that presentation defined? Yes
Internet talk Maybe

Author

Eva Santos

Presentation materials