Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger
- Autores
- García, Beatríz
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión aceptada
- Descripción
- A search for time-directional coincidences of ultra-high-energy (UHE) photons above 10 EeV with gravitational wave (GW) events from the LIGO/Virgo runs O1 to O3 is conducted with the Pierre Auger Observatory. Due to the distinctive properties of photon interactions and to the background expected from hadronic showers, a subset of the most interesting GW events is selected based on their localization quality and distance. Time periods of 1000 s around and 1 day after the GW events are analyzed. No coincidences are observed. Upper limits on the UHE photon fluence from a GW event are derived that are typically at ∼7 MeV cm−2 (time period 1000 s) and ∼35 MeV cm−2 (time period 1 day). Due to the proximity of the binary neutron star merger GW170817, the energy of the source transferred into UHE photons above 40 EeV is constrained to be less than 20% of its total GW energy. These are the first limits on UHE photons from GW sources.
Fil: Universidad Tecnológica Nacional. Facultad Regional Mendoza, Argentina
Peer Reviewed - Materia
- Ultra high energy cosmic rays, Pierre Auger Observatory, Cosmic Rays
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- 2024-05-02T13:47:56Z
- Repositorio
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- Institución
- Universidad Tecnológica Nacional
- OAI Identificador
- oai:ria.utn.edu.ar:20.500.12272/10704
Ver los metadatos del registro completo
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Search for ultra-high-energy photons from gravitational wave sources with the Pierre AugerGarcía, BeatrízUltra high energy cosmic rays, Pierre Auger Observatory, Cosmic RaysA search for time-directional coincidences of ultra-high-energy (UHE) photons above 10 EeV with gravitational wave (GW) events from the LIGO/Virgo runs O1 to O3 is conducted with the Pierre Auger Observatory. Due to the distinctive properties of photon interactions and to the background expected from hadronic showers, a subset of the most interesting GW events is selected based on their localization quality and distance. Time periods of 1000 s around and 1 day after the GW events are analyzed. No coincidences are observed. Upper limits on the UHE photon fluence from a GW event are derived that are typically at ∼7 MeV cm−2 (time period 1000 s) and ∼35 MeV cm−2 (time period 1 day). Due to the proximity of the binary neutron star merger GW170817, the energy of the source transferred into UHE photons above 40 EeV is constrained to be less than 20% of its total GW energy. These are the first limits on UHE photons from GW sources.Fil: Universidad Tecnológica Nacional. Facultad Regional Mendoza, ArgentinaPeer Reviewed2024-05-02T13:47:56Z2024-05-02T13:47:56Z2023-01-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/acceptedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articulopdfapplication/pdfThe Astrophysical Journalhttp://hdl.handle.net/20.500.12272/10704http://dx.doi.org/10.3847/1538-4357/acc862enginfo:eu-repo/semantics/openAccess2024-05-02T13:47:56Zhttp://creativecommons.org/publicdomain/zero/1.0/CC0 1.0 UniversalUniversidad Tecnológica Nacional. Facultad Regional MendozaCompartir igualreponame:Repositorio Institucional Abierto (UTN)instname:Universidad Tecnológica Nacional2026-09-24T12:48:37Zoai:ria.utn.edu.ar:20.500.12272/10704instacron:UTNInstitucionalhttp://ria.utn.edu.ar/Universidad públicaNo correspondehttp://ria.utn.edu.ar/oaigestionria@rec.utn.edu.ar; fsuarez@rec.utn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:a2026-09-24 12:48:39.162Repositorio Institucional Abierto (UTN) - Universidad Tecnológica Nacionalfalse |
| dc.title.none.fl_str_mv |
Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger |
| title |
Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger |
| spellingShingle |
Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger García, Beatríz Ultra high energy cosmic rays, Pierre Auger Observatory, Cosmic Rays |
| title_short |
Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger |
| title_full |
Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger |
| title_fullStr |
Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger |
| title_full_unstemmed |
Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger |
| title_sort |
Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger |
| dc.creator.none.fl_str_mv |
García, Beatríz |
| author |
García, Beatríz |
| author_facet |
García, Beatríz |
| author_role |
author |
| dc.subject.none.fl_str_mv |
Ultra high energy cosmic rays, Pierre Auger Observatory, Cosmic Rays |
| topic |
Ultra high energy cosmic rays, Pierre Auger Observatory, Cosmic Rays |
| dc.description.none.fl_txt_mv |
A search for time-directional coincidences of ultra-high-energy (UHE) photons above 10 EeV with gravitational wave (GW) events from the LIGO/Virgo runs O1 to O3 is conducted with the Pierre Auger Observatory. Due to the distinctive properties of photon interactions and to the background expected from hadronic showers, a subset of the most interesting GW events is selected based on their localization quality and distance. Time periods of 1000 s around and 1 day after the GW events are analyzed. No coincidences are observed. Upper limits on the UHE photon fluence from a GW event are derived that are typically at ∼7 MeV cm−2 (time period 1000 s) and ∼35 MeV cm−2 (time period 1 day). Due to the proximity of the binary neutron star merger GW170817, the energy of the source transferred into UHE photons above 40 EeV is constrained to be less than 20% of its total GW energy. These are the first limits on UHE photons from GW sources. Fil: Universidad Tecnológica Nacional. Facultad Regional Mendoza, Argentina Peer Reviewed |
| description |
A search for time-directional coincidences of ultra-high-energy (UHE) photons above 10 EeV with gravitational wave (GW) events from the LIGO/Virgo runs O1 to O3 is conducted with the Pierre Auger Observatory. Due to the distinctive properties of photon interactions and to the background expected from hadronic showers, a subset of the most interesting GW events is selected based on their localization quality and distance. Time periods of 1000 s around and 1 day after the GW events are analyzed. No coincidences are observed. Upper limits on the UHE photon fluence from a GW event are derived that are typically at ∼7 MeV cm−2 (time period 1000 s) and ∼35 MeV cm−2 (time period 1 day). Due to the proximity of the binary neutron star merger GW170817, the energy of the source transferred into UHE photons above 40 EeV is constrained to be less than 20% of its total GW energy. These are the first limits on UHE photons from GW sources. |
| publishDate |
2023 |
| dc.date.none.fl_str_mv |
2023-01-01 2024-05-02T13:47:56Z 2024-05-02T13:47:56Z |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/acceptedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
| format |
article |
| status_str |
acceptedVersion |
| dc.identifier.none.fl_str_mv |
The Astrophysical Journal http://hdl.handle.net/20.500.12272/10704 http://dx.doi.org/10.3847/1538-4357/acc862 |
| identifier_str_mv |
The Astrophysical Journal |
| url |
http://hdl.handle.net/20.500.12272/10704 http://dx.doi.org/10.3847/1538-4357/acc862 |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess 2024-05-02T13:47:56Z http://creativecommons.org/publicdomain/zero/1.0/ CC0 1.0 Universal Universidad Tecnológica Nacional. Facultad Regional Mendoza Compartir igual |
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openAccess |
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2024-05-02T13:47:56Z http://creativecommons.org/publicdomain/zero/1.0/ CC0 1.0 Universal Universidad Tecnológica Nacional. Facultad Regional Mendoza Compartir igual |
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pdf application/pdf |
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Universidad Tecnológica Nacional |
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Repositorio Institucional Abierto (UTN) - Universidad Tecnológica Nacional |
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gestionria@rec.utn.edu.ar; fsuarez@rec.utn.edu.ar |
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