Anomalous Longitudinal Shower Profiles and Hadronic Interactions
The bulk of air showers initiated by very high energy cosmic rays exhibits a longitudinal development in depth with a single well-defined shower maximum. However, a small fraction of showers has a profile that differs considerably from this average behaviour. In extreme cases, such anomalous longitu...
Gespeichert in:
Veröffentlicht in: | arXiv.org 2011-11 |
---|---|
Hauptverfasser: | , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | |
container_start_page | |
container_title | arXiv.org |
container_volume | |
creator | Baus, Colin Engel, Ralph Pierog, Tanguy Ulrich, Ralf Unger, Michael |
description | The bulk of air showers initiated by very high energy cosmic rays exhibits a longitudinal development in depth with a single well-defined shower maximum. However, a small fraction of showers has a profile that differs considerably from this average behaviour. In extreme cases, such anomalous longitudinal profiles can even have two distinct shower maxima. We discuss the properties of the primary interactions that lead to such profiles. Simulations are used to estimate the rate of anomalous profiles in dependence of primary energy, mass, and characteristic features of hadronic multiparticle production at very high energies. |
doi_str_mv | 10.48550/arxiv.1111.0504 |
format | Article |
fullrecord | <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_1111_0504</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2082312557</sourcerecordid><originalsourceid>FETCH-LOGICAL-a934-9fa180e51fb5517074b862a78b8a6599b5ed7fa75b69460f903006bfa3e443253</originalsourceid><addsrcrecordid>eNotz81LwzAYBvAgCI65uycpeO5889WkN8dQNygouHt5uyaa0SUzaf3479c5n8tzeXjgR8gNhbnQUsI9xh_3Nadj5iBBXJAJ45zmWjB2RWYp7QCAFYpJySfkYeHDHrswpKwK_t31Q-s8dtnbR_g2MXuNwbrOpAx9m62wjcG7bbb2vYm47V3w6ZpcWuySmf33lGyeHjfLVV69PK-XiyrHkou8tEg1GEltIyVVoESjC4ZKNxoLWZaNNK2yqGRTlKIAWwIHKBqL3AjBmeRTcnu-_dPVh-j2GH_rk7I-KcfB3XlwiOFzMKmvd2GIIyXVDDTjdPQqfgRXpVPQ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2082312557</pqid></control><display><type>article</type><title>Anomalous Longitudinal Shower Profiles and Hadronic Interactions</title><source>arXiv.org</source><source>Free E- Journals</source><creator>Baus, Colin ; Engel, Ralph ; Pierog, Tanguy ; Ulrich, Ralf ; Unger, Michael</creator><creatorcontrib>Baus, Colin ; Engel, Ralph ; Pierog, Tanguy ; Ulrich, Ralf ; Unger, Michael</creatorcontrib><description>The bulk of air showers initiated by very high energy cosmic rays exhibits a longitudinal development in depth with a single well-defined shower maximum. However, a small fraction of showers has a profile that differs considerably from this average behaviour. In extreme cases, such anomalous longitudinal profiles can even have two distinct shower maxima. We discuss the properties of the primary interactions that lead to such profiles. Simulations are used to estimate the rate of anomalous profiles in dependence of primary energy, mass, and characteristic features of hadronic multiparticle production at very high energies.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1111.0504</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Cosmic ray showers ; Cosmic rays ; Dependence ; Maxima ; Physics - High Energy Astrophysical Phenomena</subject><ispartof>arXiv.org, 2011-11</ispartof><rights>2011. 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><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>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,784,885,27925</link.rule.ids><backlink>$$Uhttps://doi.org/10.7529/ICRC2011/V02/1130$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.1111.0504$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Baus, Colin</creatorcontrib><creatorcontrib>Engel, Ralph</creatorcontrib><creatorcontrib>Pierog, Tanguy</creatorcontrib><creatorcontrib>Ulrich, Ralf</creatorcontrib><creatorcontrib>Unger, Michael</creatorcontrib><title>Anomalous Longitudinal Shower Profiles and Hadronic Interactions</title><title>arXiv.org</title><description>The bulk of air showers initiated by very high energy cosmic rays exhibits a longitudinal development in depth with a single well-defined shower maximum. However, a small fraction of showers has a profile that differs considerably from this average behaviour. In extreme cases, such anomalous longitudinal profiles can even have two distinct shower maxima. We discuss the properties of the primary interactions that lead to such profiles. Simulations are used to estimate the rate of anomalous profiles in dependence of primary energy, mass, and characteristic features of hadronic multiparticle production at very high energies.</description><subject>Cosmic ray showers</subject><subject>Cosmic rays</subject><subject>Dependence</subject><subject>Maxima</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotz81LwzAYBvAgCI65uycpeO5889WkN8dQNygouHt5uyaa0SUzaf3479c5n8tzeXjgR8gNhbnQUsI9xh_3Nadj5iBBXJAJ45zmWjB2RWYp7QCAFYpJySfkYeHDHrswpKwK_t31Q-s8dtnbR_g2MXuNwbrOpAx9m62wjcG7bbb2vYm47V3w6ZpcWuySmf33lGyeHjfLVV69PK-XiyrHkou8tEg1GEltIyVVoESjC4ZKNxoLWZaNNK2yqGRTlKIAWwIHKBqL3AjBmeRTcnu-_dPVh-j2GH_rk7I-KcfB3XlwiOFzMKmvd2GIIyXVDDTjdPQqfgRXpVPQ</recordid><startdate>20111102</startdate><enddate>20111102</enddate><creator>Baus, Colin</creator><creator>Engel, Ralph</creator><creator>Pierog, Tanguy</creator><creator>Ulrich, Ralf</creator><creator>Unger, Michael</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><scope>GOX</scope></search><sort><creationdate>20111102</creationdate><title>Anomalous Longitudinal Shower Profiles and Hadronic Interactions</title><author>Baus, Colin ; Engel, Ralph ; Pierog, Tanguy ; Ulrich, Ralf ; Unger, Michael</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a934-9fa180e51fb5517074b862a78b8a6599b5ed7fa75b69460f903006bfa3e443253</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Cosmic ray showers</topic><topic>Cosmic rays</topic><topic>Dependence</topic><topic>Maxima</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><toplevel>online_resources</toplevel><creatorcontrib>Baus, Colin</creatorcontrib><creatorcontrib>Engel, Ralph</creatorcontrib><creatorcontrib>Pierog, Tanguy</creatorcontrib><creatorcontrib>Ulrich, Ralf</creatorcontrib><creatorcontrib>Unger, Michael</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 UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</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><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Baus, Colin</au><au>Engel, Ralph</au><au>Pierog, Tanguy</au><au>Ulrich, Ralf</au><au>Unger, Michael</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Anomalous Longitudinal Shower Profiles and Hadronic Interactions</atitle><jtitle>arXiv.org</jtitle><date>2011-11-02</date><risdate>2011</risdate><eissn>2331-8422</eissn><abstract>The bulk of air showers initiated by very high energy cosmic rays exhibits a longitudinal development in depth with a single well-defined shower maximum. However, a small fraction of showers has a profile that differs considerably from this average behaviour. In extreme cases, such anomalous longitudinal profiles can even have two distinct shower maxima. We discuss the properties of the primary interactions that lead to such profiles. Simulations are used to estimate the rate of anomalous profiles in dependence of primary energy, mass, and characteristic features of hadronic multiparticle production at very high energies.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1111.0504</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2011-11 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_1111_0504 |
source | arXiv.org; Free E- Journals |
subjects | Cosmic ray showers Cosmic rays Dependence Maxima Physics - High Energy Astrophysical Phenomena |
title | Anomalous Longitudinal Shower Profiles and Hadronic Interactions |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-01T09%3A42%3A36IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Anomalous%20Longitudinal%20Shower%20Profiles%20and%20Hadronic%20Interactions&rft.jtitle=arXiv.org&rft.au=Baus,%20Colin&rft.date=2011-11-02&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1111.0504&rft_dat=%3Cproquest_arxiv%3E2082312557%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2082312557&rft_id=info:pmid/&rfr_iscdi=true |