Search for ultra high energy cosmic ray sources
Earlier we suggested a new method to search for sources and anisotropy of the arrival directions of ultra high energy particles. Here using this method we analyzed the data of the Yakutsk EAS array and found that particle fluxes with energies E < 4.1019 eV come to the Earth from our Galaxy and th...
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ftdoajarticles:oai:doaj.org/article:b89f44e87bc441c8853777a5e84d38d3 2023-05-15T18:45:27+02:00 Search for ultra high energy cosmic ray sources Mikhailov A.A. Kolosov V.A. 2017-01-01T00:00:00Z https://doi.org/10.1051/epjconf/201714507004 https://doaj.org/article/b89f44e87bc441c8853777a5e84d38d3 EN eng EDP Sciences https://doi.org/10.1051/epjconf/201714507004 https://doaj.org/toc/2100-014X 2100-014X doi:10.1051/epjconf/201714507004 https://doaj.org/article/b89f44e87bc441c8853777a5e84d38d3 EPJ Web of Conferences, Vol 145, p 07004 (2017) Physics QC1-999 article 2017 ftdoajarticles https://doi.org/10.1051/epjconf/201714507004 2022-12-31T04:42:11Z Earlier we suggested a new method to search for sources and anisotropy of the arrival directions of ultra high energy particles. Here using this method we analyzed the data of the Yakutsk EAS array and found that particle fluxes with energies E < 4.1019 eV come to the Earth from our Galaxy and the arrival directions of particles correlate with known pulsars. The chance probability of correlating particles with pulsars and the anisotropy of the distribution of particles is 10−4–10−5. We also analyzed the Telescope Array (TA) data with energies E < 4.1019 eV by our method and found that the maximum of the distribution of particles points to extragalactic sources but the direction of the maximum does not coincide with the maximum direction of the distribution of particles found by the authors of the Telescope Array data (the maximums of the arrival directions received by two different methods of analyses differ by about 10%). Article in Journal/Newspaper Yakutsk Directory of Open Access Journals: DOAJ Articles Yakutsk EPJ Web of Conferences 145 07004 |
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Directory of Open Access Journals: DOAJ Articles |
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English |
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Physics QC1-999 |
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Physics QC1-999 Mikhailov A.A. Kolosov V.A. Search for ultra high energy cosmic ray sources |
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Physics QC1-999 |
description |
Earlier we suggested a new method to search for sources and anisotropy of the arrival directions of ultra high energy particles. Here using this method we analyzed the data of the Yakutsk EAS array and found that particle fluxes with energies E < 4.1019 eV come to the Earth from our Galaxy and the arrival directions of particles correlate with known pulsars. The chance probability of correlating particles with pulsars and the anisotropy of the distribution of particles is 10−4–10−5. We also analyzed the Telescope Array (TA) data with energies E < 4.1019 eV by our method and found that the maximum of the distribution of particles points to extragalactic sources but the direction of the maximum does not coincide with the maximum direction of the distribution of particles found by the authors of the Telescope Array data (the maximums of the arrival directions received by two different methods of analyses differ by about 10%). |
format |
Article in Journal/Newspaper |
author |
Mikhailov A.A. Kolosov V.A. |
author_facet |
Mikhailov A.A. Kolosov V.A. |
author_sort |
Mikhailov A.A. |
title |
Search for ultra high energy cosmic ray sources |
title_short |
Search for ultra high energy cosmic ray sources |
title_full |
Search for ultra high energy cosmic ray sources |
title_fullStr |
Search for ultra high energy cosmic ray sources |
title_full_unstemmed |
Search for ultra high energy cosmic ray sources |
title_sort |
search for ultra high energy cosmic ray sources |
publisher |
EDP Sciences |
publishDate |
2017 |
url |
https://doi.org/10.1051/epjconf/201714507004 https://doaj.org/article/b89f44e87bc441c8853777a5e84d38d3 |
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Yakutsk |
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Yakutsk |
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Yakutsk |
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Yakutsk |
op_source |
EPJ Web of Conferences, Vol 145, p 07004 (2017) |
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https://doi.org/10.1051/epjconf/201714507004 https://doaj.org/toc/2100-014X 2100-014X doi:10.1051/epjconf/201714507004 https://doaj.org/article/b89f44e87bc441c8853777a5e84d38d3 |
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https://doi.org/10.1051/epjconf/201714507004 |
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EPJ Web of Conferences |
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145 |
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07004 |
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