Loading…
Simultaneous acceleration of protons and electrons at nonrelativistic quasiparallel collisionless shocks
We study diffusive shock acceleration (DSA) of protons and electrons at nonrelativistic, high Mach number, quasiparallel, collisionless shocks by means of self-consistent 1D particle-in-cell simulations. For the first time, both species are found to develop power-law distributions with the universal...
Saved in:
Published in: | Physical review letters 2015-02, Vol.114 (8), p.085003-085003, Article 085003 |
---|---|
Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-c485t-8d8b8dfc172c807ddf9137e1c2c172a62c39a14510fe5e6021d3a54aac45ff323 |
---|---|
cites | cdi_FETCH-LOGICAL-c485t-8d8b8dfc172c807ddf9137e1c2c172a62c39a14510fe5e6021d3a54aac45ff323 |
container_end_page | 085003 |
container_issue | 8 |
container_start_page | 085003 |
container_title | Physical review letters |
container_volume | 114 |
creator | Park, Jaehong Caprioli, Damiano Spitkovsky, Anatoly |
description | We study diffusive shock acceleration (DSA) of protons and electrons at nonrelativistic, high Mach number, quasiparallel, collisionless shocks by means of self-consistent 1D particle-in-cell simulations. For the first time, both species are found to develop power-law distributions with the universal spectral index -4 in momentum space, in agreement with the prediction of DSA. We find that scattering of both protons and electrons is mediated by right-handed circularly polarized waves excited by the current of energetic protons via nonresonant hybrid (Bell) instability. Protons are injected into DSA after a few gyrocycles of shock drift acceleration (SDA), while electrons are first preheated via SDA, then energized via a hybrid acceleration process that involves both SDA and Fermi-like acceleration mediated by Bell waves, before eventual injection into DSA. Using the simulations we can measure the electron-proton ratio in accelerated particles, which is of paramount importance for explaining the cosmic ray fluxes measured on Earth and the multiwavelength emission of astrophysical objects such as supernova remnants, radio supernovae, and galaxy clusters. We find the normalization of the electron power law is ≲10^{-2} of the protons for strong nonrelativistic shocks. |
doi_str_mv | 10.1103/physrevlett.114.085003 |
format | article |
fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_1181630</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1663897238</sourcerecordid><originalsourceid>FETCH-LOGICAL-c485t-8d8b8dfc172c807ddf9137e1c2c172a62c39a14510fe5e6021d3a54aac45ff323</originalsourceid><addsrcrecordid>eNqFkU1P3DAQhi3UCpaPv4AiTr2EzsSJ7RwrVGillYpoe7aM42hNvfFiOyvx7xkIcK1kaeTX74xn5mHsHOESEfjX3eYpJ7cPrhQS2ktQHQA_YCsE2deSpE9sRQrWPYA8Ysc5PwAANkIdsqOmk0LRWbHNb7-dQzGTi3OujLUuuGSKj1MVx2qXYokT6dNQ0YMt6fVWqilOyQXy7X0u3laPs8l-Z5IJwYXKxhB8phrB5VzlTbT_8in7PJqQ3dlbPGF_r7__ufpRr3_d_Lz6tq5tq7pSq0Hdq2G0KBurQA7D2COXDm3zIhnRWN4bbDuE0XVOQIMDN11rjG27ceQNP2EXS91IjelsfXF2Y-M0UfcaUaHgQKYvi4kGfJxdLnrrM40elj1olEqggpbj_61CcNXLhiuyisVqU8xEZ9S75LcmPWkE_UJN3xK1O7dfEzUSWr1Qo8Tztz_m-60bPtLeMfFnLxKY1w</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1663897238</pqid></control><display><type>article</type><title>Simultaneous acceleration of protons and electrons at nonrelativistic quasiparallel collisionless shocks</title><source>American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)</source><creator>Park, Jaehong ; Caprioli, Damiano ; Spitkovsky, Anatoly</creator><creatorcontrib>Park, Jaehong ; Caprioli, Damiano ; Spitkovsky, Anatoly</creatorcontrib><description>We study diffusive shock acceleration (DSA) of protons and electrons at nonrelativistic, high Mach number, quasiparallel, collisionless shocks by means of self-consistent 1D particle-in-cell simulations. For the first time, both species are found to develop power-law distributions with the universal spectral index -4 in momentum space, in agreement with the prediction of DSA. We find that scattering of both protons and electrons is mediated by right-handed circularly polarized waves excited by the current of energetic protons via nonresonant hybrid (Bell) instability. Protons are injected into DSA after a few gyrocycles of shock drift acceleration (SDA), while electrons are first preheated via SDA, then energized via a hybrid acceleration process that involves both SDA and Fermi-like acceleration mediated by Bell waves, before eventual injection into DSA. Using the simulations we can measure the electron-proton ratio in accelerated particles, which is of paramount importance for explaining the cosmic ray fluxes measured on Earth and the multiwavelength emission of astrophysical objects such as supernova remnants, radio supernovae, and galaxy clusters. We find the normalization of the electron power law is ≲10^{-2} of the protons for strong nonrelativistic shocks.</description><identifier>ISSN: 0031-9007</identifier><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/physrevlett.114.085003</identifier><identifier>PMID: 25768768</identifier><language>eng</language><publisher>United States: American Physical Society</publisher><subject>Acceleration ; Activation ; Bells ; High Mach number ; Instability ; Simulation ; Supernova remnants ; Supernovae</subject><ispartof>Physical review letters, 2015-02, Vol.114 (8), p.085003-085003, Article 085003</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c485t-8d8b8dfc172c807ddf9137e1c2c172a62c39a14510fe5e6021d3a54aac45ff323</citedby><cites>FETCH-LOGICAL-c485t-8d8b8dfc172c807ddf9137e1c2c172a62c39a14510fe5e6021d3a54aac45ff323</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/25768768$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/1181630$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Park, Jaehong</creatorcontrib><creatorcontrib>Caprioli, Damiano</creatorcontrib><creatorcontrib>Spitkovsky, Anatoly</creatorcontrib><title>Simultaneous acceleration of protons and electrons at nonrelativistic quasiparallel collisionless shocks</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>We study diffusive shock acceleration (DSA) of protons and electrons at nonrelativistic, high Mach number, quasiparallel, collisionless shocks by means of self-consistent 1D particle-in-cell simulations. For the first time, both species are found to develop power-law distributions with the universal spectral index -4 in momentum space, in agreement with the prediction of DSA. We find that scattering of both protons and electrons is mediated by right-handed circularly polarized waves excited by the current of energetic protons via nonresonant hybrid (Bell) instability. Protons are injected into DSA after a few gyrocycles of shock drift acceleration (SDA), while electrons are first preheated via SDA, then energized via a hybrid acceleration process that involves both SDA and Fermi-like acceleration mediated by Bell waves, before eventual injection into DSA. Using the simulations we can measure the electron-proton ratio in accelerated particles, which is of paramount importance for explaining the cosmic ray fluxes measured on Earth and the multiwavelength emission of astrophysical objects such as supernova remnants, radio supernovae, and galaxy clusters. We find the normalization of the electron power law is ≲10^{-2} of the protons for strong nonrelativistic shocks.</description><subject>Acceleration</subject><subject>Activation</subject><subject>Bells</subject><subject>High Mach number</subject><subject>Instability</subject><subject>Simulation</subject><subject>Supernova remnants</subject><subject>Supernovae</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqFkU1P3DAQhi3UCpaPv4AiTr2EzsSJ7RwrVGillYpoe7aM42hNvfFiOyvx7xkIcK1kaeTX74xn5mHsHOESEfjX3eYpJ7cPrhQS2ktQHQA_YCsE2deSpE9sRQrWPYA8Ysc5PwAANkIdsqOmk0LRWbHNb7-dQzGTi3OujLUuuGSKj1MVx2qXYokT6dNQ0YMt6fVWqilOyQXy7X0u3laPs8l-Z5IJwYXKxhB8phrB5VzlTbT_8in7PJqQ3dlbPGF_r7__ufpRr3_d_Lz6tq5tq7pSq0Hdq2G0KBurQA7D2COXDm3zIhnRWN4bbDuE0XVOQIMDN11rjG27ceQNP2EXS91IjelsfXF2Y-M0UfcaUaHgQKYvi4kGfJxdLnrrM40elj1olEqggpbj_61CcNXLhiuyisVqU8xEZ9S75LcmPWkE_UJN3xK1O7dfEzUSWr1Qo8Tztz_m-60bPtLeMfFnLxKY1w</recordid><startdate>20150227</startdate><enddate>20150227</enddate><creator>Park, Jaehong</creator><creator>Caprioli, Damiano</creator><creator>Spitkovsky, Anatoly</creator><general>American Physical Society</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20150227</creationdate><title>Simultaneous acceleration of protons and electrons at nonrelativistic quasiparallel collisionless shocks</title><author>Park, Jaehong ; Caprioli, Damiano ; Spitkovsky, Anatoly</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c485t-8d8b8dfc172c807ddf9137e1c2c172a62c39a14510fe5e6021d3a54aac45ff323</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Acceleration</topic><topic>Activation</topic><topic>Bells</topic><topic>High Mach number</topic><topic>Instability</topic><topic>Simulation</topic><topic>Supernova remnants</topic><topic>Supernovae</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Park, Jaehong</creatorcontrib><creatorcontrib>Caprioli, Damiano</creatorcontrib><creatorcontrib>Spitkovsky, Anatoly</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Park, Jaehong</au><au>Caprioli, Damiano</au><au>Spitkovsky, Anatoly</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Simultaneous acceleration of protons and electrons at nonrelativistic quasiparallel collisionless shocks</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2015-02-27</date><risdate>2015</risdate><volume>114</volume><issue>8</issue><spage>085003</spage><epage>085003</epage><pages>085003-085003</pages><artnum>085003</artnum><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>We study diffusive shock acceleration (DSA) of protons and electrons at nonrelativistic, high Mach number, quasiparallel, collisionless shocks by means of self-consistent 1D particle-in-cell simulations. For the first time, both species are found to develop power-law distributions with the universal spectral index -4 in momentum space, in agreement with the prediction of DSA. We find that scattering of both protons and electrons is mediated by right-handed circularly polarized waves excited by the current of energetic protons via nonresonant hybrid (Bell) instability. Protons are injected into DSA after a few gyrocycles of shock drift acceleration (SDA), while electrons are first preheated via SDA, then energized via a hybrid acceleration process that involves both SDA and Fermi-like acceleration mediated by Bell waves, before eventual injection into DSA. Using the simulations we can measure the electron-proton ratio in accelerated particles, which is of paramount importance for explaining the cosmic ray fluxes measured on Earth and the multiwavelength emission of astrophysical objects such as supernova remnants, radio supernovae, and galaxy clusters. We find the normalization of the electron power law is ≲10^{-2} of the protons for strong nonrelativistic shocks.</abstract><cop>United States</cop><pub>American Physical Society</pub><pmid>25768768</pmid><doi>10.1103/physrevlett.114.085003</doi><tpages>1</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0031-9007 |
ispartof | Physical review letters, 2015-02, Vol.114 (8), p.085003-085003, Article 085003 |
issn | 0031-9007 1079-7114 |
language | eng |
recordid | cdi_osti_scitechconnect_1181630 |
source | American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list) |
subjects | Acceleration Activation Bells High Mach number Instability Simulation Supernova remnants Supernovae |
title | Simultaneous acceleration of protons and electrons at nonrelativistic quasiparallel collisionless shocks |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-27T20%3A49%3A38IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Simultaneous%20acceleration%20of%20protons%20and%20electrons%20at%20nonrelativistic%20quasiparallel%20collisionless%20shocks&rft.jtitle=Physical%20review%20letters&rft.au=Park,%20Jaehong&rft.date=2015-02-27&rft.volume=114&rft.issue=8&rft.spage=085003&rft.epage=085003&rft.pages=085003-085003&rft.artnum=085003&rft.issn=0031-9007&rft.eissn=1079-7114&rft_id=info:doi/10.1103/physrevlett.114.085003&rft_dat=%3Cproquest_osti_%3E1663897238%3C/proquest_osti_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c485t-8d8b8dfc172c807ddf9137e1c2c172a62c39a14510fe5e6021d3a54aac45ff323%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1663897238&rft_id=info:pmid/25768768&rfr_iscdi=true |