Ultra-high energy nuclei source in the direction to Virgo cluster

The significant anisotropy in the arrival directions of the 69 events with energy E> 55 EeV detected by Pierre Auger collaboration is located in the 20-degree region centered near Cen A. Not only the 2-point, but also the 3-point and 4-point autocorrelation functions are completely saturated by t...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
1. Verfasser: Semikoz, Dmitri V
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title
container_volume
creator Semikoz, Dmitri V
description The significant anisotropy in the arrival directions of the 69 events with energy E> 55 EeV detected by Pierre Auger collaboration is located in the 20-degree region centered near Cen A. Not only the 2-point, but also the 3-point and 4-point autocorrelation functions are completely saturated by this region. Besides there is an deficit of events in the direction of Virgo cluster. If one assumes that the excess around Cen A is due to heavy nuclei shifted from Virgo, one can explain 20-degree scale of this anomaly. Also location of the highest energy event between the Cen A region and the Virgo cluster supports this idea. Magnitude and direction of the magnetic field is similar in this case to those expected for Galactic models. The existence of nuclei sources in the sky opens the road for a self-consistent description of Auger data.
doi_str_mv 10.48550/arxiv.1009.3879
format Article
fullrecord <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_1009_3879</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1009_3879</sourcerecordid><originalsourceid>FETCH-LOGICAL-a659-55c1e26b6bde28ace3700d0f4cf85934633b54d5f797315cce55d5e80822402b3</originalsourceid><addsrcrecordid>eNotzz1PwzAUhWEvHVDLzoT8BxJubN_EHquKL6kSS2GNnOubxFJIkJMg-u-hwHT0Lkd6hLgpIDcWEe58-oqfeQHgcm0rdyX2r8OSfNbHrpc8curOclxp4CjnaU3EMo5y6VmGmJiWOP3UJN9i6iZJwzovnHZi0_ph5uv_3YrTw_3p8JQdXx6fD_tj5kt0GSIVrMqmbAIr64l1BRCgNdRadNqUWjdoAraVq3SBRIwYkC1YpQyoRm_F7d_tL6H-SPHdp3N9odQXiv4G7g5Dag</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Ultra-high energy nuclei source in the direction to Virgo cluster</title><source>arXiv.org</source><creator>Semikoz, Dmitri V</creator><creatorcontrib>Semikoz, Dmitri V</creatorcontrib><description>The significant anisotropy in the arrival directions of the 69 events with energy E&gt; 55 EeV detected by Pierre Auger collaboration is located in the 20-degree region centered near Cen A. Not only the 2-point, but also the 3-point and 4-point autocorrelation functions are completely saturated by this region. Besides there is an deficit of events in the direction of Virgo cluster. If one assumes that the excess around Cen A is due to heavy nuclei shifted from Virgo, one can explain 20-degree scale of this anomaly. Also location of the highest energy event between the Cen A region and the Virgo cluster supports this idea. Magnitude and direction of the magnetic field is similar in this case to those expected for Galactic models. The existence of nuclei sources in the sky opens the road for a self-consistent description of Auger data.</description><identifier>DOI: 10.48550/arxiv.1009.3879</identifier><language>eng</language><subject>Physics - High Energy Astrophysical Phenomena ; Physics - High Energy Physics - Phenomenology</subject><creationdate>2010-09</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/1009.3879$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.1009.3879$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Semikoz, Dmitri V</creatorcontrib><title>Ultra-high energy nuclei source in the direction to Virgo cluster</title><description>The significant anisotropy in the arrival directions of the 69 events with energy E&gt; 55 EeV detected by Pierre Auger collaboration is located in the 20-degree region centered near Cen A. Not only the 2-point, but also the 3-point and 4-point autocorrelation functions are completely saturated by this region. Besides there is an deficit of events in the direction of Virgo cluster. If one assumes that the excess around Cen A is due to heavy nuclei shifted from Virgo, one can explain 20-degree scale of this anomaly. Also location of the highest energy event between the Cen A region and the Virgo cluster supports this idea. Magnitude and direction of the magnetic field is similar in this case to those expected for Galactic models. The existence of nuclei sources in the sky opens the road for a self-consistent description of Auger data.</description><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - High Energy Physics - Phenomenology</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzz1PwzAUhWEvHVDLzoT8BxJubN_EHquKL6kSS2GNnOubxFJIkJMg-u-hwHT0Lkd6hLgpIDcWEe58-oqfeQHgcm0rdyX2r8OSfNbHrpc8curOclxp4CjnaU3EMo5y6VmGmJiWOP3UJN9i6iZJwzovnHZi0_ph5uv_3YrTw_3p8JQdXx6fD_tj5kt0GSIVrMqmbAIr64l1BRCgNdRadNqUWjdoAraVq3SBRIwYkC1YpQyoRm_F7d_tL6H-SPHdp3N9odQXiv4G7g5Dag</recordid><startdate>20100920</startdate><enddate>20100920</enddate><creator>Semikoz, Dmitri V</creator><scope>GOX</scope></search><sort><creationdate>20100920</creationdate><title>Ultra-high energy nuclei source in the direction to Virgo cluster</title><author>Semikoz, Dmitri V</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a659-55c1e26b6bde28ace3700d0f4cf85934633b54d5f797315cce55d5e80822402b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - High Energy Physics - Phenomenology</topic><toplevel>online_resources</toplevel><creatorcontrib>Semikoz, Dmitri V</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Semikoz, Dmitri V</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Ultra-high energy nuclei source in the direction to Virgo cluster</atitle><date>2010-09-20</date><risdate>2010</risdate><abstract>The significant anisotropy in the arrival directions of the 69 events with energy E&gt; 55 EeV detected by Pierre Auger collaboration is located in the 20-degree region centered near Cen A. Not only the 2-point, but also the 3-point and 4-point autocorrelation functions are completely saturated by this region. Besides there is an deficit of events in the direction of Virgo cluster. If one assumes that the excess around Cen A is due to heavy nuclei shifted from Virgo, one can explain 20-degree scale of this anomaly. Also location of the highest energy event between the Cen A region and the Virgo cluster supports this idea. Magnitude and direction of the magnetic field is similar in this case to those expected for Galactic models. The existence of nuclei sources in the sky opens the road for a self-consistent description of Auger data.</abstract><doi>10.48550/arxiv.1009.3879</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier DOI: 10.48550/arxiv.1009.3879
ispartof
issn
language eng
recordid cdi_arxiv_primary_1009_3879
source arXiv.org
subjects Physics - High Energy Astrophysical Phenomena
Physics - High Energy Physics - Phenomenology
title Ultra-high energy nuclei source in the direction to Virgo cluster
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-07T06%3A51%3A58IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Ultra-high%20energy%20nuclei%20source%20in%20the%20direction%20to%20Virgo%20cluster&rft.au=Semikoz,%20Dmitri%20V&rft.date=2010-09-20&rft_id=info:doi/10.48550/arxiv.1009.3879&rft_dat=%3Carxiv_GOX%3E1009_3879%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true