PIC simulation methods for cosmic radiation and plasma instabilities

Particle acceleration in collisionless plasma systems is a central question in astroplasma and astroparticle physics. The structure of the acceleration regions, electron–ion energy equilibration, preacceleration of particles at shocks to permit further energization by diffusive shock acceleration, r...

Full description

Saved in:
Bibliographic Details
Published in:Progress in particle and nuclear physics 2020-03, Vol.111, p.103751, Article 103751
Main Authors: Pohl, M., Hoshino, M., Niemiec, J.
Format: Article
Language:English
Subjects:
Collisionless shocks
Cosmic rays
Particle acceleration
Particle-in-cell simulations
Plasma instabilities
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-c410t-9f2c81c246924a652bcd406c41f95bf0d0681676f3c381dcbe56ce3c6b9dddb3
cites cdi_FETCH-LOGICAL-c410t-9f2c81c246924a652bcd406c41f95bf0d0681676f3c381dcbe56ce3c6b9dddb3
container_end_page
container_issue
container_start_page 103751
container_title Progress in particle and nuclear physics
container_volume 111
creator Pohl, M.
Hoshino, M.
Niemiec, J.
description Particle acceleration in collisionless plasma systems is a central question in astroplasma and astroparticle physics. The structure of the acceleration regions, electron–ion energy equilibration, preacceleration of particles at shocks to permit further energization by diffusive shock acceleration, require knowledge of the distribution function of particles besides the structure and dynamic of electromagnetic fields, and hence a kinetic description is desirable. Particle-in-cell simulations offer an appropriate, if computationally expensive method of essentially conducting numerical experiments that explore kinetic phenomena in collisionless plasma. We review recent results of PIC simulations of astrophysical plasma systems, particle acceleration, and the instabilities that shape them.
doi_str_mv 10.1016/j.ppnp.2019.103751
format article
fullrecord <record><control><sourceid>elsevier_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1016_j_ppnp_2019_103751</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><els_id>S0146641019300869</els_id><sourcerecordid>S0146641019300869</sourcerecordid><originalsourceid>FETCH-LOGICAL-c410t-9f2c81c246924a652bcd406c41f95bf0d0681676f3c381dcbe56ce3c6b9dddb3</originalsourceid><addsrcrecordid>eNp9kE1LxDAQhoMouK7-AU_5A10zaZq24EXWr4UFPew9pJMEZ-kXSRX893ap5z0NzMvzzvAwdg9iAwL0w3Ezjv24kQLqeZGXBVywFVRlnkkp1SVbCVA60wrENbtJ6ShmSIFasefP3ZYn6r5bO9HQ885PX4NLPAyR45A6Qh6toyW0veNja1NnOfVpsg21NJFPt-wq2Db5u_-5ZofXl8P2Pdt_vO22T_sM58NTVgeJFaBUupbK6kI26JTQcxjqognCCV2BLnXIMa_AYeMLjT5H3dTOuSZfM7nUYhxSij6YMVJn468BYU4azNGcNJiTBrNomKHHBfLzYz_ko0lIvkfvKHqcjBvoHP4HR4dnNQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>PIC simulation methods for cosmic radiation and plasma instabilities</title><source>ScienceDirect Journals</source><creator>Pohl, M. ; Hoshino, M. ; Niemiec, J.</creator><creatorcontrib>Pohl, M. ; Hoshino, M. ; Niemiec, J.</creatorcontrib><description>Particle acceleration in collisionless plasma systems is a central question in astroplasma and astroparticle physics. The structure of the acceleration regions, electron–ion energy equilibration, preacceleration of particles at shocks to permit further energization by diffusive shock acceleration, require knowledge of the distribution function of particles besides the structure and dynamic of electromagnetic fields, and hence a kinetic description is desirable. Particle-in-cell simulations offer an appropriate, if computationally expensive method of essentially conducting numerical experiments that explore kinetic phenomena in collisionless plasma. We review recent results of PIC simulations of astrophysical plasma systems, particle acceleration, and the instabilities that shape them.</description><identifier>ISSN: 0146-6410</identifier><identifier>EISSN: 1873-2224</identifier><identifier>DOI: 10.1016/j.ppnp.2019.103751</identifier><language>eng</language><publisher>Elsevier B.V</publisher><subject>Collisionless shocks ; Cosmic rays ; Particle acceleration ; Particle-in-cell simulations ; Plasma instabilities</subject><ispartof>Progress in particle and nuclear physics, 2020-03, Vol.111, p.103751, Article 103751</ispartof><rights>2019 Elsevier B.V.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c410t-9f2c81c246924a652bcd406c41f95bf0d0681676f3c381dcbe56ce3c6b9dddb3</citedby><cites>FETCH-LOGICAL-c410t-9f2c81c246924a652bcd406c41f95bf0d0681676f3c381dcbe56ce3c6b9dddb3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27923,27924</link.rule.ids></links><search><creatorcontrib>Pohl, M.</creatorcontrib><creatorcontrib>Hoshino, M.</creatorcontrib><creatorcontrib>Niemiec, J.</creatorcontrib><title>PIC simulation methods for cosmic radiation and plasma instabilities</title><title>Progress in particle and nuclear physics</title><description>Particle acceleration in collisionless plasma systems is a central question in astroplasma and astroparticle physics. The structure of the acceleration regions, electron–ion energy equilibration, preacceleration of particles at shocks to permit further energization by diffusive shock acceleration, require knowledge of the distribution function of particles besides the structure and dynamic of electromagnetic fields, and hence a kinetic description is desirable. Particle-in-cell simulations offer an appropriate, if computationally expensive method of essentially conducting numerical experiments that explore kinetic phenomena in collisionless plasma. We review recent results of PIC simulations of astrophysical plasma systems, particle acceleration, and the instabilities that shape them.</description><subject>Collisionless shocks</subject><subject>Cosmic rays</subject><subject>Particle acceleration</subject><subject>Particle-in-cell simulations</subject><subject>Plasma instabilities</subject><issn>0146-6410</issn><issn>1873-2224</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LxDAQhoMouK7-AU_5A10zaZq24EXWr4UFPew9pJMEZ-kXSRX893ap5z0NzMvzzvAwdg9iAwL0w3Ezjv24kQLqeZGXBVywFVRlnkkp1SVbCVA60wrENbtJ6ShmSIFasefP3ZYn6r5bO9HQ885PX4NLPAyR45A6Qh6toyW0veNja1NnOfVpsg21NJFPt-wq2Db5u_-5ZofXl8P2Pdt_vO22T_sM58NTVgeJFaBUupbK6kI26JTQcxjqognCCV2BLnXIMa_AYeMLjT5H3dTOuSZfM7nUYhxSij6YMVJn468BYU4azNGcNJiTBrNomKHHBfLzYz_ko0lIvkfvKHqcjBvoHP4HR4dnNQ</recordid><startdate>202003</startdate><enddate>202003</enddate><creator>Pohl, M.</creator><creator>Hoshino, M.</creator><creator>Niemiec, J.</creator><general>Elsevier B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>202003</creationdate><title>PIC simulation methods for cosmic radiation and plasma instabilities</title><author>Pohl, M. ; Hoshino, M. ; Niemiec, J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c410t-9f2c81c246924a652bcd406c41f95bf0d0681676f3c381dcbe56ce3c6b9dddb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Collisionless shocks</topic><topic>Cosmic rays</topic><topic>Particle acceleration</topic><topic>Particle-in-cell simulations</topic><topic>Plasma instabilities</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pohl, M.</creatorcontrib><creatorcontrib>Hoshino, M.</creatorcontrib><creatorcontrib>Niemiec, J.</creatorcontrib><collection>CrossRef</collection><jtitle>Progress in particle and nuclear physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Pohl, M.</au><au>Hoshino, M.</au><au>Niemiec, J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>PIC simulation methods for cosmic radiation and plasma instabilities</atitle><jtitle>Progress in particle and nuclear physics</jtitle><date>2020-03</date><risdate>2020</risdate><volume>111</volume><spage>103751</spage><pages>103751-</pages><artnum>103751</artnum><issn>0146-6410</issn><eissn>1873-2224</eissn><abstract>Particle acceleration in collisionless plasma systems is a central question in astroplasma and astroparticle physics. The structure of the acceleration regions, electron–ion energy equilibration, preacceleration of particles at shocks to permit further energization by diffusive shock acceleration, require knowledge of the distribution function of particles besides the structure and dynamic of electromagnetic fields, and hence a kinetic description is desirable. Particle-in-cell simulations offer an appropriate, if computationally expensive method of essentially conducting numerical experiments that explore kinetic phenomena in collisionless plasma. We review recent results of PIC simulations of astrophysical plasma systems, particle acceleration, and the instabilities that shape them.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.ppnp.2019.103751</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0146-6410
ispartof Progress in particle and nuclear physics, 2020-03, Vol.111, p.103751, Article 103751
issn 0146-6410
1873-2224
language eng
recordid cdi_crossref_primary_10_1016_j_ppnp_2019_103751
source ScienceDirect Journals
subjects Collisionless shocks
Cosmic rays
Particle acceleration
Particle-in-cell simulations
Plasma instabilities
title PIC simulation methods for cosmic radiation and plasma instabilities
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-13T04%3A15%3A35IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-elsevier_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=PIC%20simulation%20methods%20for%20cosmic%20radiation%20and%20plasma%20instabilities&rft.jtitle=Progress%20in%20particle%20and%20nuclear%20physics&rft.au=Pohl,%20M.&rft.date=2020-03&rft.volume=111&rft.spage=103751&rft.pages=103751-&rft.artnum=103751&rft.issn=0146-6410&rft.eissn=1873-2224&rft_id=info:doi/10.1016/j.ppnp.2019.103751&rft_dat=%3Celsevier_cross%3ES0146641019300869%3C/elsevier_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c410t-9f2c81c246924a652bcd406c41f95bf0d0681676f3c381dcbe56ce3c6b9dddb3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true