Relativistic plasma expansion with Maxwell-Ju¨ttner distribution

A self-similar analytical solution is proposed to describe the relativistic ion acceleration with the local Maxwell-Ju¨ttner relativistic distribution electrons. It is an alternative to the existing static model [M. Passoni and M. Lontano, Phys. Rev. Lett. 101, 115001 (2008)], which exploits a limit...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physics of plasmas 2013-11, Vol.20 (11)
Hauptverfasser: Huang, Yongsheng, Wang, Naiyan, Tang, Xiuzhang, Shi, Yijin
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 11
container_start_page
container_title Physics of plasmas
container_volume 20
creator Huang, Yongsheng
Wang, Naiyan
Tang, Xiuzhang
Shi, Yijin
description A self-similar analytical solution is proposed to describe the relativistic ion acceleration with the local Maxwell-Ju¨ttner relativistic distribution electrons. It is an alternative to the existing static model [M. Passoni and M. Lontano, Phys. Rev. Lett. 101, 115001 (2008)], which exploits a limited solution for the acceleration potential. With our model, the potential is finite naturally and has an upper limitation proportional to the square root of the electron temperature. The divergent potential in the non-relativistic case is the linear items of the Taylor expansion of that obtained relativistic one here. The energy distribution of ions and the dependence of the ion momentum on the acceleration time are obtained analytically. Maximum ion energy has an upper limitation decided by the finite potential difference. In the ultra-relativistic region, the ion energy at the ion front is proportional to t4/5 and the energy of the ions behind the ion front is proportional to t2/3 since the field there is shielded by the ions beyond them and the field at the ion front is the most intense.
doi_str_mv 10.1063/1.4834496
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1567105573</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2129499683</sourcerecordid><originalsourceid>FETCH-LOGICAL-c1353-dd1a575800e8938b02a9af4aea001c80e7fdf2c7b5b413a2cd60f6d64629b3ee3</originalsourceid><addsrcrecordid>eNpd0MtKw0AUBuBBFKzVhW8QcKOL1DOZ-7IUr1QEUXA3TJIJTsnNmYmtb-Rz-GSmtCtX5yw-fn5-hM4xzDBwco1nVBJKFT9AEwxSpYILerj9BaSc0_djdBLCCgAoZ3KC5i-2NtF9uRBdkfS1CY1J7KY3bXBdm6xd_EiezGZt6zp9HH5_YmytT8qRe5cPcTSn6KgydbBn-ztFb7c3r4v7dPl897CYL9MCE0bSssSGCSYBrFRE5pAZZSpqrAHAhQQrqrLKCpGznGJisqLkUPGSU56pnFhLpuhyl9v77nOwIerGhWLsZVrbDUFjxgUGxgQZ6cU_uuoG347tdIYzRZXicquudqrwXQjeVrr3rjH-W2PQ2zE11vsxyR-iUGbz</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2129499683</pqid></control><display><type>article</type><title>Relativistic plasma expansion with Maxwell-Ju¨ttner distribution</title><source>AIP Journals Complete</source><source>AIP Digital Archive</source><source>Alma/SFX Local Collection</source><creator>Huang, Yongsheng ; Wang, Naiyan ; Tang, Xiuzhang ; Shi, Yijin</creator><creatorcontrib>Huang, Yongsheng ; Wang, Naiyan ; Tang, Xiuzhang ; Shi, Yijin</creatorcontrib><description>A self-similar analytical solution is proposed to describe the relativistic ion acceleration with the local Maxwell-Ju¨ttner relativistic distribution electrons. It is an alternative to the existing static model [M. Passoni and M. Lontano, Phys. Rev. Lett. 101, 115001 (2008)], which exploits a limited solution for the acceleration potential. With our model, the potential is finite naturally and has an upper limitation proportional to the square root of the electron temperature. The divergent potential in the non-relativistic case is the linear items of the Taylor expansion of that obtained relativistic one here. The energy distribution of ions and the dependence of the ion momentum on the acceleration time are obtained analytically. Maximum ion energy has an upper limitation decided by the finite potential difference. In the ultra-relativistic region, the ion energy at the ion front is proportional to t4/5 and the energy of the ions behind the ion front is proportional to t2/3 since the field there is shielded by the ions beyond them and the field at the ion front is the most intense.</description><identifier>ISSN: 1070-664X</identifier><identifier>EISSN: 1089-7674</identifier><identifier>DOI: 10.1063/1.4834496</identifier><language>eng</language><publisher>Melville: American Institute of Physics</publisher><subject>Acceleration ; Dependence ; Electron energy ; Electron temperature ; Energy distribution ; Mathematical analysis ; Mathematical models ; Plasma physics ; Plasmas ; Relativism ; Relativistic effects ; Relativistic plasmas ; Roots ; Self-similarity ; Static models ; Taylor series</subject><ispartof>Physics of plasmas, 2013-11, Vol.20 (11)</ispartof><rights>2013 AIP Publishing LLC.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c1353-dd1a575800e8938b02a9af4aea001c80e7fdf2c7b5b413a2cd60f6d64629b3ee3</citedby><cites>FETCH-LOGICAL-c1353-dd1a575800e8938b02a9af4aea001c80e7fdf2c7b5b413a2cd60f6d64629b3ee3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids></links><search><creatorcontrib>Huang, Yongsheng</creatorcontrib><creatorcontrib>Wang, Naiyan</creatorcontrib><creatorcontrib>Tang, Xiuzhang</creatorcontrib><creatorcontrib>Shi, Yijin</creatorcontrib><title>Relativistic plasma expansion with Maxwell-Ju¨ttner distribution</title><title>Physics of plasmas</title><description>A self-similar analytical solution is proposed to describe the relativistic ion acceleration with the local Maxwell-Ju¨ttner relativistic distribution electrons. It is an alternative to the existing static model [M. Passoni and M. Lontano, Phys. Rev. Lett. 101, 115001 (2008)], which exploits a limited solution for the acceleration potential. With our model, the potential is finite naturally and has an upper limitation proportional to the square root of the electron temperature. The divergent potential in the non-relativistic case is the linear items of the Taylor expansion of that obtained relativistic one here. The energy distribution of ions and the dependence of the ion momentum on the acceleration time are obtained analytically. Maximum ion energy has an upper limitation decided by the finite potential difference. In the ultra-relativistic region, the ion energy at the ion front is proportional to t4/5 and the energy of the ions behind the ion front is proportional to t2/3 since the field there is shielded by the ions beyond them and the field at the ion front is the most intense.</description><subject>Acceleration</subject><subject>Dependence</subject><subject>Electron energy</subject><subject>Electron temperature</subject><subject>Energy distribution</subject><subject>Mathematical analysis</subject><subject>Mathematical models</subject><subject>Plasma physics</subject><subject>Plasmas</subject><subject>Relativism</subject><subject>Relativistic effects</subject><subject>Relativistic plasmas</subject><subject>Roots</subject><subject>Self-similarity</subject><subject>Static models</subject><subject>Taylor series</subject><issn>1070-664X</issn><issn>1089-7674</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNpd0MtKw0AUBuBBFKzVhW8QcKOL1DOZ-7IUr1QEUXA3TJIJTsnNmYmtb-Rz-GSmtCtX5yw-fn5-hM4xzDBwco1nVBJKFT9AEwxSpYILerj9BaSc0_djdBLCCgAoZ3KC5i-2NtF9uRBdkfS1CY1J7KY3bXBdm6xd_EiezGZt6zp9HH5_YmytT8qRe5cPcTSn6KgydbBn-ztFb7c3r4v7dPl897CYL9MCE0bSssSGCSYBrFRE5pAZZSpqrAHAhQQrqrLKCpGznGJisqLkUPGSU56pnFhLpuhyl9v77nOwIerGhWLsZVrbDUFjxgUGxgQZ6cU_uuoG347tdIYzRZXicquudqrwXQjeVrr3rjH-W2PQ2zE11vsxyR-iUGbz</recordid><startdate>20131101</startdate><enddate>20131101</enddate><creator>Huang, Yongsheng</creator><creator>Wang, Naiyan</creator><creator>Tang, Xiuzhang</creator><creator>Shi, Yijin</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7U5</scope></search><sort><creationdate>20131101</creationdate><title>Relativistic plasma expansion with Maxwell-Ju¨ttner distribution</title><author>Huang, Yongsheng ; Wang, Naiyan ; Tang, Xiuzhang ; Shi, Yijin</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1353-dd1a575800e8938b02a9af4aea001c80e7fdf2c7b5b413a2cd60f6d64629b3ee3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Acceleration</topic><topic>Dependence</topic><topic>Electron energy</topic><topic>Electron temperature</topic><topic>Energy distribution</topic><topic>Mathematical analysis</topic><topic>Mathematical models</topic><topic>Plasma physics</topic><topic>Plasmas</topic><topic>Relativism</topic><topic>Relativistic effects</topic><topic>Relativistic plasmas</topic><topic>Roots</topic><topic>Self-similarity</topic><topic>Static models</topic><topic>Taylor series</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Huang, Yongsheng</creatorcontrib><creatorcontrib>Wang, Naiyan</creatorcontrib><creatorcontrib>Tang, Xiuzhang</creatorcontrib><creatorcontrib>Shi, Yijin</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Solid State and Superconductivity Abstracts</collection><jtitle>Physics of plasmas</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Huang, Yongsheng</au><au>Wang, Naiyan</au><au>Tang, Xiuzhang</au><au>Shi, Yijin</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Relativistic plasma expansion with Maxwell-Ju¨ttner distribution</atitle><jtitle>Physics of plasmas</jtitle><date>2013-11-01</date><risdate>2013</risdate><volume>20</volume><issue>11</issue><issn>1070-664X</issn><eissn>1089-7674</eissn><abstract>A self-similar analytical solution is proposed to describe the relativistic ion acceleration with the local Maxwell-Ju¨ttner relativistic distribution electrons. It is an alternative to the existing static model [M. Passoni and M. Lontano, Phys. Rev. Lett. 101, 115001 (2008)], which exploits a limited solution for the acceleration potential. With our model, the potential is finite naturally and has an upper limitation proportional to the square root of the electron temperature. The divergent potential in the non-relativistic case is the linear items of the Taylor expansion of that obtained relativistic one here. The energy distribution of ions and the dependence of the ion momentum on the acceleration time are obtained analytically. Maximum ion energy has an upper limitation decided by the finite potential difference. In the ultra-relativistic region, the ion energy at the ion front is proportional to t4/5 and the energy of the ions behind the ion front is proportional to t2/3 since the field there is shielded by the ions beyond them and the field at the ion front is the most intense.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/1.4834496</doi></addata></record>
fulltext fulltext
identifier ISSN: 1070-664X
ispartof Physics of plasmas, 2013-11, Vol.20 (11)
issn 1070-664X
1089-7674
language eng
recordid cdi_proquest_miscellaneous_1567105573
source AIP Journals Complete; AIP Digital Archive; Alma/SFX Local Collection
subjects Acceleration
Dependence
Electron energy
Electron temperature
Energy distribution
Mathematical analysis
Mathematical models
Plasma physics
Plasmas
Relativism
Relativistic effects
Relativistic plasmas
Roots
Self-similarity
Static models
Taylor series
title Relativistic plasma expansion with Maxwell-Ju¨ttner distribution
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-10T00%3A10%3A37IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Relativistic%20plasma%20expansion%20with%20Maxwell-Ju%C2%A8ttner%20distribution&rft.jtitle=Physics%20of%20plasmas&rft.au=Huang,%20Yongsheng&rft.date=2013-11-01&rft.volume=20&rft.issue=11&rft.issn=1070-664X&rft.eissn=1089-7674&rft_id=info:doi/10.1063/1.4834496&rft_dat=%3Cproquest_cross%3E2129499683%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2129499683&rft_id=info:pmid/&rfr_iscdi=true