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Naslov:Search for photons above ▫$10^19$▫ eV with the surface detector of the Pierre Auger Observatory
Avtorji:ID Abreu, P. (Avtor)
ID Filipčič, Andrej (Avtor)
ID Lundquist, Jon Paul (Avtor)
ID Shivashankara, Shima Ujjani (Avtor)
ID Stanič, Samo (Avtor)
ID Vorobiov, Serguei (Avtor)
ID Zavrtanik, Danilo (Avtor)
ID Zavrtanik, Marko (Avtor)
ID Zehrer, Lukas (Avtor), et al.
Datoteke:URL https://iopscience.iop.org/article/10.1088/1475-7516/2023/05/021
 
.pdf Abreu_2023_J._Cosmol._Astropart._Phys._2023_021.pdf (2,46 MB)
MD5: 0663DE568AD1B7183CF4596E7200D50A
 
URL https://doi.org/10.1088/1475-7516/2023/05/021
 
Jezik:Angleški jezik
Vrsta gradiva:Neznano
Tipologija:1.01 - Izvirni znanstveni članek
Organizacija:UNG - Univerza v Novi Gorici
Opis:We use the surface detector of the Pierre Auger Observatory to search for air showers initiated by photons with an energy above 10[sup]19 eV. Photons in the zenith angle range from 30 deg. to 60 deg. can be identified in the overwhelming background of showers initiated by charged cosmic rays through the broader time structure of the signals induced in the water-Cherenkov detectors of the array and the steeper lateral distribution of shower particles reaching ground. Applying the search method to data collected between January 2004 and June 2020, upper limits at 95% CL are set to an E[sup]-2 diffuse flux of ultra-high energy photons above 10[sup]19 eV, 2 × 10[sup]19 eV and 4 × 10[sup]19 eV amounting to 2.11 × 10[sup]-3, 3.12 × 10[sup]-4 and 1.72 × 10[sup]-4 km-2 sr-1 yr-1, respectively. While the sensitivity of the present search around 2 × 10[sup]19 eV approaches expectations of cosmogenic photon fluxes in the case of a pure-proton composition, it is one order of magnitude above those from more realistic mixed-composition models. The inferred limits have also implications for the search of super-heavy dark matter that are discussed and illustrated.
Ključne besede:ultra-high-energy cosmic rays, UHE photons, Pierre Auger Observatory, extensive air showers, water Cherenkov detectors
Status publikacije:Objavljeno
Verzija publikacije:Objavljena publikacija
Datum objave:01.05.2023
Leto izida:2023
Št. strani:str. 1-24
Številčenje:Vol. 2023, no. 5, [article no.] 021
PID:20.500.12556/RUNG-8344-9752b62b-ce75-126b-3644-be3ad0e385b4 Novo okno
COBISS.SI-ID:161596675 Novo okno
UDK:52
ISSN pri članku:1475-7516
DOI:10.1088/1475-7516/2023/05/021 Novo okno
NUK URN:URN:SI:UNG:REP:OF9VYJWQ
Datum objave v RUNG:18.08.2023
Število ogledov:697
Število prenosov:8
Metapodatki:XML RDF-CHPDL DC-XML DC-RDF
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Gradivo je del revije

Naslov:Journal of cosmology and astroparticle physics
Založnik:Institute of Physics Pub.
ISSN:1475-7516
COBISS.SI-ID:389627 Novo okno

Gradivo je financirano iz projekta

Financer:ARRS - Agencija za raziskovalno dejavnost Republike Slovenije
Številka projekta:P1-0031
Naslov:Večglasniška astrofizika

Licence

Licenca:CC BY 4.0, Creative Commons Priznanje avtorstva 4.0 Mednarodna
Povezava:http://creativecommons.org/licenses/by/4.0/deed.sl
Opis:To je standardna licenca Creative Commons, ki daje uporabnikom največ možnosti za nadaljnjo uporabo dela, pri čemer morajo navesti avtorja.

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