A Search for Point Sources of EeV Neutrons
@inproceedings{Collaboration2012ASF, title={A Search for Point Sources of EeV Neutrons}, author={The Pierre Auger Collaboration}, year={2012} }
A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicative of a flux of neutral particles from a discrete source. The search covers from −90◦ to +15◦ in declination using four different energy ranges above 1 EeV (10 eV). The method used in this search is more sensitive to neutrons than to photons. The upper limit on a neutron flux is derived for a dense grid of directions…
11 Citations
Constraints to UHE cosmic ray source scenarios with all the major observables of the Pierre Auger Observatory
- Physics
- 2018
Unveiling the mystery of the sources of ultra high energetic cosmic rays (UHECR) that possess energies above 1018 eV is one of the most urgent questions in contemporary astroparticle physics.
Up to…
Ultra-high-energy cosmic rays The intersection of the Cosmic and Energy Frontiers
- Physics, EducationAstroparticle Physics
- 2022
Highlights from the Pierre Auger Observatory
- PhysicsProceedings of Frontier Research in Astrophysics – III — PoS(FRAPWS2018)
- 2019
The existence of a cosmic ray flux of a still unknown origin with particles reaching energies millions of times higher than those attained at the LHC continues to intrigue the scientific community.…
Growth of Accreting Supermassive Black Hole Seeds and Neutrino Radiation
- Physics
- 2015
In the framework of microscopic theory of black hole (MTBH), which explores the most important processes of rearrangement of vacuum state and spontaneous breaking of gravitation gauge symmetry at…
Cosmic-ray astronomy at the highest energies with ten years of data of the Pierre Auger observatory
- Physics
- 2015
Identifying the sources of the ultra-high energy cosmic rays (UHECRs, above 10^{18} eV), the most energetic particles known in the universe, would be an important leap forward for both the…
Different approaches to determine the composition of the ultra-high energy cosmic rays in the Pierre Auger Observatory
- Physics
- 2014
The motivation of this PhD thesis is to improve the capabilities to determine the mass composition of the ultra-high energy cosmic rays in the Pierre Auger Observatory. The measure of their mass…
Reviewing the latest results from the Pierre Auger Observatory
- Chemistry
- 2014
The Pierre Auger Observatory was built to help unveil the properties of ultra-high energy cosmic rays with energies from 1017 to 1020 eV. In this paper we review the latest results obtained from data…
Constraining the sources of ultra-high energy cosmic rays with multi-messenger data
- Physics
- 2014
Ultra-high energy cosmic rays (UHECRs) are cosmic rays with energy exceeding 10¹⁸ electronvolts. The sources of these particles remain unknown despite decades of research. This thesis presents a…
Neutrino Lighthouse at Sagittarius A
- Physics
- 2014
We investigate whether a subset of high-energy events observed by IceCube may be due to neutrinos from Sagittarius A*. We check both spatial and temporal coincidences of IceCube events with other…
References
SHOWING 1-10 OF 10 REFERENCES
Consejo Nacional de Ciencia y Tecnología (CONACYT), Mexico; Ministerie van Onderwijs
- Cultuur en Wetenschap
Rouillé-d’Orfeuil for the Pierre Auger Collaboration, “Search for Galactic point-sources
- 2005
Rouillé-d'Orfeuil for the Pierre Auger Collaboration
- Proc. 32nd ICRC (Beijing)
- 2011
Czech Republic; Centre de Calcul IN2P3/CNRS
Xunta de Galicia, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy
- FEDER funds, Ministerio de Ciencia e Innovación and Consolider-Ingenio 2010 (CPAN)
We are very grateful to the following agencies and organizations for financial support
Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant Nos. N N202
MEIF-CT-2005-025057, European Union 7th Framework Program, Grant No. PIEF-GA-2008-220240, and UNESCO
C. Bonifazi for the Pierre Auger Collaboration, “The angular resolution of the Pierre
- J. 619,
- 2005