Precision Measurement of Boron-to-Carbon ratio in Cosmic Rays from 2 GV to 2 TV with the Alpha Magnetic Spectrometer on the International Space Station
AMS-02 is a wide acceptance high-energy physics experiment installed on the International Space Station in May 2011 and it has been operating continuously since then. AMS-02 is able to separate cosmic rays light nuclei (\(1\leq Z \leq 8\)) with contaminations less than \(10^{-3}\). The ratio between...
Gespeichert in:
Veröffentlicht in: | arXiv.org 2017-01 |
---|---|
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 | mato, Valerio the AMS-02 Collaboration |
description | AMS-02 is a wide acceptance high-energy physics experiment installed on the International Space Station in May 2011 and it has been operating continuously since then. AMS-02 is able to separate cosmic rays light nuclei (\(1\leq Z \leq 8\)) with contaminations less than \(10^{-3}\). The ratio between the cosmic rays Boron and Carbon fluxes is known to be very sensitive to the properties of the propagation of cosmic rays in the Galaxy, being Boron a secondary product of spallation on the interstellar medium of heavier primary elements such as Carbon and Oxygen. A precise measurement reaching the TeV region can significantly help understanding cosmic rays propagation in the Galaxy and the amount of matter traversed before reaching Earth. The status of the measurement of the boron-to-carbon ratio based on 10 millions Boron and Carbon events is presented. |
format | Article |
fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2075235078</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2075235078</sourcerecordid><originalsourceid>FETCH-proquest_journals_20752350783</originalsourceid><addsrcrecordid>eNqNzN1Kw0AQBeClIFi07zDQ68C6a0xvbag_FwWxpbdlDBOzJdmJOxPEJ_F13YoP4NXhMN-cmZk772-K1a1zl2YhcrLWurvKlaWfm--XRE2QwBG2hDIlGigqcAtrThwL5aLG9JbPCTUwhAg1yxAaeMUvgTbxAA4eD6Ccc3-Az6AdaEdw348dwhbfI2nmu5EazZqUEuS5M3mOucTzbsQ-C2wIdvrbr81Fi73Q4i-vzPJhs6-fijHxx0SixxNP-beXo7NV6Xxpq5X_n_oBHv9XZA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2075235078</pqid></control><display><type>article</type><title>Precision Measurement of Boron-to-Carbon ratio in Cosmic Rays from 2 GV to 2 TV with the Alpha Magnetic Spectrometer on the International Space Station</title><source>Free E- Journals</source><creator>mato, Valerio ; the AMS-02 Collaboration</creator><creatorcontrib>mato, Valerio ; the AMS-02 Collaboration</creatorcontrib><description>AMS-02 is a wide acceptance high-energy physics experiment installed on the International Space Station in May 2011 and it has been operating continuously since then. AMS-02 is able to separate cosmic rays light nuclei (\(1\leq Z \leq 8\)) with contaminations less than \(10^{-3}\). The ratio between the cosmic rays Boron and Carbon fluxes is known to be very sensitive to the properties of the propagation of cosmic rays in the Galaxy, being Boron a secondary product of spallation on the interstellar medium of heavier primary elements such as Carbon and Oxygen. A precise measurement reaching the TeV region can significantly help understanding cosmic rays propagation in the Galaxy and the amount of matter traversed before reaching Earth. The status of the measurement of the boron-to-carbon ratio based on 10 millions Boron and Carbon events is presented.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Alpha rays ; Boron ; Carbon ; Cosmic ray propagation ; Cosmic rays ; Fluxes ; Galactic cosmic rays ; Galaxies ; High energy astronomy ; International Space Station ; Interstellar matter ; Multinational space ventures ; Propagation ; Space stations ; Spallation</subject><ispartof>arXiv.org, 2017-01</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><link.rule.ids>776,780</link.rule.ids></links><search><creatorcontrib>mato, Valerio</creatorcontrib><creatorcontrib>the AMS-02 Collaboration</creatorcontrib><title>Precision Measurement of Boron-to-Carbon ratio in Cosmic Rays from 2 GV to 2 TV with the Alpha Magnetic Spectrometer on the International Space Station</title><title>arXiv.org</title><description>AMS-02 is a wide acceptance high-energy physics experiment installed on the International Space Station in May 2011 and it has been operating continuously since then. AMS-02 is able to separate cosmic rays light nuclei (\(1\leq Z \leq 8\)) with contaminations less than \(10^{-3}\). The ratio between the cosmic rays Boron and Carbon fluxes is known to be very sensitive to the properties of the propagation of cosmic rays in the Galaxy, being Boron a secondary product of spallation on the interstellar medium of heavier primary elements such as Carbon and Oxygen. A precise measurement reaching the TeV region can significantly help understanding cosmic rays propagation in the Galaxy and the amount of matter traversed before reaching Earth. The status of the measurement of the boron-to-carbon ratio based on 10 millions Boron and Carbon events is presented.</description><subject>Alpha rays</subject><subject>Boron</subject><subject>Carbon</subject><subject>Cosmic ray propagation</subject><subject>Cosmic rays</subject><subject>Fluxes</subject><subject>Galactic cosmic rays</subject><subject>Galaxies</subject><subject>High energy astronomy</subject><subject>International Space Station</subject><subject>Interstellar matter</subject><subject>Multinational space ventures</subject><subject>Propagation</subject><subject>Space stations</subject><subject>Spallation</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqNzN1Kw0AQBeClIFi07zDQ68C6a0xvbag_FwWxpbdlDBOzJdmJOxPEJ_F13YoP4NXhMN-cmZk772-K1a1zl2YhcrLWurvKlaWfm--XRE2QwBG2hDIlGigqcAtrThwL5aLG9JbPCTUwhAg1yxAaeMUvgTbxAA4eD6Ccc3-Az6AdaEdw348dwhbfI2nmu5EazZqUEuS5M3mOucTzbsQ-C2wIdvrbr81Fi73Q4i-vzPJhs6-fijHxx0SixxNP-beXo7NV6Xxpq5X_n_oBHv9XZA</recordid><startdate>20170112</startdate><enddate>20170112</enddate><creator>mato, Valerio</creator><creator>the AMS-02 Collaboration</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>20170112</creationdate><title>Precision Measurement of Boron-to-Carbon ratio in Cosmic Rays from 2 GV to 2 TV with the Alpha Magnetic Spectrometer on the International Space Station</title><author>mato, Valerio ; the AMS-02 Collaboration</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20752350783</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Alpha rays</topic><topic>Boron</topic><topic>Carbon</topic><topic>Cosmic ray propagation</topic><topic>Cosmic rays</topic><topic>Fluxes</topic><topic>Galactic cosmic rays</topic><topic>Galaxies</topic><topic>High energy astronomy</topic><topic>International Space Station</topic><topic>Interstellar matter</topic><topic>Multinational space ventures</topic><topic>Propagation</topic><topic>Space stations</topic><topic>Spallation</topic><toplevel>online_resources</toplevel><creatorcontrib>mato, Valerio</creatorcontrib><creatorcontrib>the AMS-02 Collaboration</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</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></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>mato, Valerio</au><au>the AMS-02 Collaboration</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Precision Measurement of Boron-to-Carbon ratio in Cosmic Rays from 2 GV to 2 TV with the Alpha Magnetic Spectrometer on the International Space Station</atitle><jtitle>arXiv.org</jtitle><date>2017-01-12</date><risdate>2017</risdate><eissn>2331-8422</eissn><abstract>AMS-02 is a wide acceptance high-energy physics experiment installed on the International Space Station in May 2011 and it has been operating continuously since then. AMS-02 is able to separate cosmic rays light nuclei (\(1\leq Z \leq 8\)) with contaminations less than \(10^{-3}\). The ratio between the cosmic rays Boron and Carbon fluxes is known to be very sensitive to the properties of the propagation of cosmic rays in the Galaxy, being Boron a secondary product of spallation on the interstellar medium of heavier primary elements such as Carbon and Oxygen. A precise measurement reaching the TeV region can significantly help understanding cosmic rays propagation in the Galaxy and the amount of matter traversed before reaching Earth. The status of the measurement of the boron-to-carbon ratio based on 10 millions Boron and Carbon events is presented.</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, 2017-01 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2075235078 |
source | Free E- Journals |
subjects | Alpha rays Boron Carbon Cosmic ray propagation Cosmic rays Fluxes Galactic cosmic rays Galaxies High energy astronomy International Space Station Interstellar matter Multinational space ventures Propagation Space stations Spallation |
title | Precision Measurement of Boron-to-Carbon ratio in Cosmic Rays from 2 GV to 2 TV with the Alpha Magnetic Spectrometer on the International Space Station |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-25T17%3A30%3A01IST&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=Precision%20Measurement%20of%20Boron-to-Carbon%20ratio%20in%20Cosmic%20Rays%20from%202%20GV%20to%202%20TV%20with%20the%20Alpha%20Magnetic%20Spectrometer%20on%20the%20International%20Space%20Station&rft.jtitle=arXiv.org&rft.au=mato,%20Valerio&rft.date=2017-01-12&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2075235078%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2075235078&rft_id=info:pmid/&rfr_iscdi=true |