Loading…
Universal cosmic rays energy spectrum and the mass composition at the 'ankle' and above
We have used recently published data from the Pierre Auger Observatory and the Telescope Array Project to conclude some inferences concerning the origin and composition of ultra high-energy cosmic rays (UHECR). We advocate for model the UHECR flux as a combination of the Galactic and Extragalactic c...
Saved in:
Published in: | arXiv.org 2017-06 |
---|---|
Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | |
---|---|
cites | |
container_end_page | |
container_issue | |
container_start_page | |
container_title | arXiv.org |
container_volume | |
creator | Wibig, Tadeusz Wolfendale, Arnold W |
description | We have used recently published data from the Pierre Auger Observatory and the Telescope Array Project to conclude some inferences concerning the origin and composition of ultra high-energy cosmic rays (UHECR). We advocate for model the UHECR flux as a combination of the Galactic and Extragalactic components exchanging the dominant role at the famous feature of the energy spectrum called 'the ankle'. We put a special emphasis on the individual experiment energy resolution and possible biases it introduces. We have eventually combined the data from both big experiments to the one 'world average' UHECR spectrum and we used it, supported by the analysis of the distribution of the Extensive Air Shower (EAS) development maximum depth to find the UHECR mass composition of both: Galactic and Extragalactic components. We studied the dependence of the on mass composition on the cosmic ray source distribution in space. We present results for some models existing in the literature. We found the evidence of the deficit of Extragalactic sources in the vicinity of the Galaxy of the the UHECR, what is in concordance with the small scale anisotropy analysis results. |
format | article |
fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2075607576</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2075607576</sourcerecordid><originalsourceid>FETCH-proquest_journals_20756075763</originalsourceid><addsrcrecordid>eNqNykEKwjAUBNAgCBbtHT646KoQE9u6F8UDKC5LrF9NbZKanxZ6e0vxAC6GgZk3Y5GQcpPutkIsWExUc85FXogskxG7Xqzu0ZNqoHJkdAVeDQRo0T8HoBar4DsDyt4hvBCMIhqhaR3poJ0FFaY9UfbdYDI5dXM9rtj8oRrC-NdLtj4ezvtT2nr36ZBCWbvO2_EqBS-yfEyRy__UF1NgQVQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2075607576</pqid></control><display><type>article</type><title>Universal cosmic rays energy spectrum and the mass composition at the 'ankle' and above</title><source>Publicly Available Content Database</source><creator>Wibig, Tadeusz ; Wolfendale, Arnold W</creator><creatorcontrib>Wibig, Tadeusz ; Wolfendale, Arnold W</creatorcontrib><description>We have used recently published data from the Pierre Auger Observatory and the Telescope Array Project to conclude some inferences concerning the origin and composition of ultra high-energy cosmic rays (UHECR). We advocate for model the UHECR flux as a combination of the Galactic and Extragalactic components exchanging the dominant role at the famous feature of the energy spectrum called 'the ankle'. We put a special emphasis on the individual experiment energy resolution and possible biases it introduces. We have eventually combined the data from both big experiments to the one 'world average' UHECR spectrum and we used it, supported by the analysis of the distribution of the Extensive Air Shower (EAS) development maximum depth to find the UHECR mass composition of both: Galactic and Extragalactic components. We studied the dependence of the on mass composition on the cosmic ray source distribution in space. We present results for some models existing in the literature. We found the evidence of the deficit of Extragalactic sources in the vicinity of the Galaxy of the the UHECR, what is in concordance with the small scale anisotropy analysis results.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Anisotropy ; Augers ; Composition ; Cosmic ray showers ; Cosmic rays ; Dependence ; Energy resolution ; Energy spectra ; Galaxies ; High energy astronomy</subject><ispartof>arXiv.org, 2017-06</ispartof><rights>2017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2075607576?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>776,780,25732,36991,44569</link.rule.ids></links><search><creatorcontrib>Wibig, Tadeusz</creatorcontrib><creatorcontrib>Wolfendale, Arnold W</creatorcontrib><title>Universal cosmic rays energy spectrum and the mass composition at the 'ankle' and above</title><title>arXiv.org</title><description>We have used recently published data from the Pierre Auger Observatory and the Telescope Array Project to conclude some inferences concerning the origin and composition of ultra high-energy cosmic rays (UHECR). We advocate for model the UHECR flux as a combination of the Galactic and Extragalactic components exchanging the dominant role at the famous feature of the energy spectrum called 'the ankle'. We put a special emphasis on the individual experiment energy resolution and possible biases it introduces. We have eventually combined the data from both big experiments to the one 'world average' UHECR spectrum and we used it, supported by the analysis of the distribution of the Extensive Air Shower (EAS) development maximum depth to find the UHECR mass composition of both: Galactic and Extragalactic components. We studied the dependence of the on mass composition on the cosmic ray source distribution in space. We present results for some models existing in the literature. We found the evidence of the deficit of Extragalactic sources in the vicinity of the Galaxy of the the UHECR, what is in concordance with the small scale anisotropy analysis results.</description><subject>Anisotropy</subject><subject>Augers</subject><subject>Composition</subject><subject>Cosmic ray showers</subject><subject>Cosmic rays</subject><subject>Dependence</subject><subject>Energy resolution</subject><subject>Energy spectra</subject><subject>Galaxies</subject><subject>High energy astronomy</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNqNykEKwjAUBNAgCBbtHT646KoQE9u6F8UDKC5LrF9NbZKanxZ6e0vxAC6GgZk3Y5GQcpPutkIsWExUc85FXogskxG7Xqzu0ZNqoHJkdAVeDQRo0T8HoBar4DsDyt4hvBCMIhqhaR3poJ0FFaY9UfbdYDI5dXM9rtj8oRrC-NdLtj4ezvtT2nr36ZBCWbvO2_EqBS-yfEyRy__UF1NgQVQ</recordid><startdate>20170619</startdate><enddate>20170619</enddate><creator>Wibig, Tadeusz</creator><creator>Wolfendale, Arnold W</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20170619</creationdate><title>Universal cosmic rays energy spectrum and the mass composition at the 'ankle' and above</title><author>Wibig, Tadeusz ; Wolfendale, Arnold W</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20756075763</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Anisotropy</topic><topic>Augers</topic><topic>Composition</topic><topic>Cosmic ray showers</topic><topic>Cosmic rays</topic><topic>Dependence</topic><topic>Energy resolution</topic><topic>Energy spectra</topic><topic>Galaxies</topic><topic>High energy astronomy</topic><toplevel>online_resources</toplevel><creatorcontrib>Wibig, Tadeusz</creatorcontrib><creatorcontrib>Wolfendale, Arnold W</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wibig, Tadeusz</au><au>Wolfendale, Arnold W</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Universal cosmic rays energy spectrum and the mass composition at the 'ankle' and above</atitle><jtitle>arXiv.org</jtitle><date>2017-06-19</date><risdate>2017</risdate><eissn>2331-8422</eissn><abstract>We have used recently published data from the Pierre Auger Observatory and the Telescope Array Project to conclude some inferences concerning the origin and composition of ultra high-energy cosmic rays (UHECR). We advocate for model the UHECR flux as a combination of the Galactic and Extragalactic components exchanging the dominant role at the famous feature of the energy spectrum called 'the ankle'. We put a special emphasis on the individual experiment energy resolution and possible biases it introduces. We have eventually combined the data from both big experiments to the one 'world average' UHECR spectrum and we used it, supported by the analysis of the distribution of the Extensive Air Shower (EAS) development maximum depth to find the UHECR mass composition of both: Galactic and Extragalactic components. We studied the dependence of the on mass composition on the cosmic ray source distribution in space. We present results for some models existing in the literature. We found the evidence of the deficit of Extragalactic sources in the vicinity of the Galaxy of the the UHECR, what is in concordance with the small scale anisotropy analysis results.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2017-06 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2075607576 |
source | Publicly Available Content Database |
subjects | Anisotropy Augers Composition Cosmic ray showers Cosmic rays Dependence Energy resolution Energy spectra Galaxies High energy astronomy |
title | Universal cosmic rays energy spectrum and the mass composition at the 'ankle' and above |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-22T18%3A39%3A14IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=Universal%20cosmic%20rays%20energy%20spectrum%20and%20the%20mass%20composition%20at%20the%20'ankle'%20and%20above&rft.jtitle=arXiv.org&rft.au=Wibig,%20Tadeusz&rft.date=2017-06-19&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2075607576%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-proquest_journals_20756075763%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2075607576&rft_id=info:pmid/&rfr_iscdi=true |