| Title: | Science with the Global Cosmic-ray Observatory (GCOS) |
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| Authors: | ID Alves Batista, Rafael (Author)
ID Ahlers, M. (Author)
ID Assis, Pedro (Author)
ID Battisti, Markus Gottfried (Author)
ID Bellido, J. A. (Author)
ID Bhatnagar, S. (Author)
ID Bismark, K. (Author)
ID Bister, Teresa (Author)
ID Boháčová, Martina (Author)
ID Vorobiov, Serguei (Author), et al. |
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| Files: |  ICRC2023_281.pdf (692,24 KB)
MD5: F92A92B9CE1EC0246FE396B25C144609
 https://pos.sissa.it/444/
https://pos.sissa.it/444/281/pdf
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| Language: | English |
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| Work type: | Unknown |
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| Typology: | 1.08 - Published Scientific Conference Contribution |
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| Organization: | UNG - University of Nova Gorica
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| Abstract: | The Global Cosmic-ray Observatory (GCOS) is a proposed large-scale observatory for studying
ultra-high-energy cosmic particles, including ultra-high-energy cosmic rays (UHECRs), photons,
and neutrinos. Its primary goal is to characterise the properties of the highest-energy particles in
Nature with unprecedented accuracy, and to identify their elusive sources. With an aperture at least a ten-fold larger than existing observatories, this next-generation facility should start operating after 2030, when present-day detectors will gradually cease their activities. Here we briefly review the scientific case motivating GCOS. We present the status of the project, preliminary ideas for its design, and some estimates of its capabilities. |
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| Keywords: | ultra-high-energy cosmic rays, UHE photons, UHE neutrinos, the Global Cosmic-ray Observatory project |
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| Publication status: | Published |
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| Publication version: | Version of Record |
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| Publication date: | 01.01.2023 |
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| Year of publishing: | 2023 |
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| Number of pages: | str. 1-10 |
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| PID: | 20.500.12556/RUNG-8470-a3e1b396-49ea-8911-7501-b8bd04dd82e7  |
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| COBISS.SI-ID: | 165973507 |
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| UDC: | 52 |
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| ISSN on article: | 1824-8039 |
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| NUK URN: | URN:SI:UNG:REP:I9U6UW6R |
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| Publication date in RUNG: | 27.09.2023 |
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| Views: | 923 |
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| Downloads: | 5 |
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