Multi-messenger studies with the Pierre Auger Observatory
Povzetek
Over the past decade the multi-messenger astrophysics has emerged as a distinct discipline,
providing unique insights into the properties of high-energy phenomena in the Universe. The
Pierre Auger Observatory, located in Malargüe, Argentina, is the world’s largest cosmic ray
detector sensitive to photons, neutrinos, and hadrons at ultra-high energies. Using its data, stringent
limits on photon and neutrino fluxes at EeV energies have been obtained. The collaboration uses
the excellent angular resolution and the neutrino identification capabilities of the Observatory
for follow-up studies of events detected in gravitational waves or other messengers, through
cooperation with global multi-messenger networks. We present a science motivation together
with an overview of the multi-messenger capabilities and results of the Pierre Auger Observatory.
Ključne besede
high-energy cosmic phenomena;multi-messenger astrophysical studies;cosmic rays;gamma-rays;neutrinos;Pierre Auger Observatory;
Podatki
| Jezik: | Angleški jezik |
|---|---|
| Leto izida: | 2021 |
| Tipologija: | 1.08 - Objavljeni znanstveni prispevek na konferenci |
| Organizacija: | UNG - Univerza v Novi Gorici |
| UDK: | 539.1 |
| COBISS: |
106800131
|
| ISSN: | 1824-8039 |
| Št. ogledov: | 777 |
| Št. prenosov: | 0 |
| Ocena: | 0 (0 glasov) |
| Metapodatki: |
|
Ostali podatki
| URN: | URN:SI:UNG |
|---|---|
| Strani: | str. 1-6 |
| Čas izdaje: | 2021 |
| ID: | 15230076 |
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