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Title:Astroparticle studies at the Pierre Auger Observatory
Authors:ID Yang, Lili, University of Nova Gorica (Author)
Files: This document has no files that are freely available to the public. This document may have a physical copy in the library of the organization, check the status via COBISS. Link is opened in a new window
Language:English
Work type:Not categorized
Typology:3.14 - Invited Lecture at Foreign University
Organization:UNG - University of Nova Gorica
Abstract:The Pierre Auger Observatory (PAO), the world’s largest cosmic ray detector combines a large surface detector (SD) with an air fluorescence detector (FD). It is designed to observe extensive air showers (EAS) of billions of secondary particles induced by the UHECRs in the earths’ atmosphere. The “hybrid” design (i.e., detected simultaneously by SD and FD) provides wealth of information about shower development and excellent event reconstruction. Together with observations of UHECRs, the Surface Detector (SD) of the PAO is sensitive to UHE neutrinos through the observation of deeply initiated inclined down-going showers produced by neutrino interactions in the atmosphere, which method has been well established. On the other hand, high-energy photons can also be discriminated from background of charged cosmic rays based on their characters of the shower front. In this talk, I will give a review on recent results from PAO and introduce the ultra-high energy multi-messenger studies from PAO.
Keywords:Pierre Auger Observatory, cosmic rays, ultra-high energy
Place of performance:University of Johannesburg, South Africa
Year of performance:2017
PID:20.500.12556/RUNG-3541-e5b178a4-8af2-bcda-a08d-f88e68faaedd New window
COBISS.SI-ID:4989947 New window
NUK URN:URN:SI:UNG:REP:IDHHSS3Y
Publication date in RUNG:17.01.2018
Views:3669
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