Cosmic Ray Production in Supernovae
We give a brief review of the origin and acceleration of cosmic rays (CRs), emphasizing the production of CRs at different stages of supernova evolution by the first-order Fermi shock acceleration mechanism. We suggest that supernovae with trans-relativistic outflows, despite being rather rare, may...
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| Veröffentlicht in: | Space Sci.Rev 2018-02, Vol.214 (1), p.1-34, Article 41 |
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| creator | Bykov, A. M. Ellison, D. C. Marcowith, A. Osipov, S. M. |
| description | We give a brief review of the origin and acceleration of cosmic rays (CRs), emphasizing the production of CRs at different stages of supernova evolution by the first-order Fermi shock acceleration mechanism. We suggest that supernovae with trans-relativistic outflows, despite being rather rare, may accelerate CRs to energies above
10
18
eV
over the first year of their evolution. Supernovae in young compact clusters of massive stars, and interaction powered superluminous supernovae, may accelerate CRs well above the PeV regime. We discuss the acceleration of the bulk of the galactic CRs in isolated supernova remnants and re-acceleration of escaped CRs by the multiple shocks present in superbubbles produced by associations of OB stars. The effects of magnetic field amplification by CR driven instabilities, as well as superdiffusive CR transport, are discussed for nonthermal radiation produced by nonlinear shocks of all speeds including trans-relativistic ones. |
| doi_str_mv | 10.1007/s11214-018-0479-4 |
| format | Article |
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10
18
eV
over the first year of their evolution. Supernovae in young compact clusters of massive stars, and interaction powered superluminous supernovae, may accelerate CRs well above the PeV regime. We discuss the acceleration of the bulk of the galactic CRs in isolated supernova remnants and re-acceleration of escaped CRs by the multiple shocks present in superbubbles produced by associations of OB stars. The effects of magnetic field amplification by CR driven instabilities, as well as superdiffusive CR transport, are discussed for nonthermal radiation produced by nonlinear shocks of all speeds including trans-relativistic ones.</description><identifier>ISSN: 0038-6308</identifier><identifier>EISSN: 1572-9672</identifier><identifier>DOI: 10.1007/s11214-018-0479-4</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Acceleration ; Aerospace Technology and Astronautics ; Astrophysics ; Astrophysics and Astroparticles ; Cosmic rays ; Evolution ; Magnetic fields ; Massive stars ; Nonthermal radiation ; Physics ; Physics and Astronomy ; Planetology ; Radiation ; Relativism ; Relativistic effects ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Stellar evolution ; Stellar magnetic fields ; Supernova ; Supernova remnants ; Supernovae ; X-rays</subject><ispartof>Space Sci.Rev, 2018-02, Vol.214 (1), p.1-34, Article 41</ispartof><rights>Springer Science+Business Media B.V., part of Springer Nature 2018</rights><rights>Space Science Reviews is a copyright of Springer, (2018). All Rights Reserved.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c350t-eb2e6fdd80e92d808b9f9305c63e5a8166d82b8412fe55edf015ba557a3ccdbe3</citedby><cites>FETCH-LOGICAL-c350t-eb2e6fdd80e92d808b9f9305c63e5a8166d82b8412fe55edf015ba557a3ccdbe3</cites><orcidid>0000-0002-3971-0910</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11214-018-0479-4$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11214-018-0479-4$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,881,27901,27902,41464,42533,51294</link.rule.ids><backlink>$$Uhttps://hal.science/hal-01707539$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Bykov, A. M.</creatorcontrib><creatorcontrib>Ellison, D. C.</creatorcontrib><creatorcontrib>Marcowith, A.</creatorcontrib><creatorcontrib>Osipov, S. M.</creatorcontrib><title>Cosmic Ray Production in Supernovae</title><title>Space Sci.Rev</title><addtitle>Space Sci Rev</addtitle><description>We give a brief review of the origin and acceleration of cosmic rays (CRs), emphasizing the production of CRs at different stages of supernova evolution by the first-order Fermi shock acceleration mechanism. We suggest that supernovae with trans-relativistic outflows, despite being rather rare, may accelerate CRs to energies above
10
18
eV
over the first year of their evolution. Supernovae in young compact clusters of massive stars, and interaction powered superluminous supernovae, may accelerate CRs well above the PeV regime. We discuss the acceleration of the bulk of the galactic CRs in isolated supernova remnants and re-acceleration of escaped CRs by the multiple shocks present in superbubbles produced by associations of OB stars. The effects of magnetic field amplification by CR driven instabilities, as well as superdiffusive CR transport, are discussed for nonthermal radiation produced by nonlinear shocks of all speeds including trans-relativistic ones.</description><subject>Acceleration</subject><subject>Aerospace Technology and Astronautics</subject><subject>Astrophysics</subject><subject>Astrophysics and Astroparticles</subject><subject>Cosmic rays</subject><subject>Evolution</subject><subject>Magnetic fields</subject><subject>Massive stars</subject><subject>Nonthermal radiation</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetology</subject><subject>Radiation</subject><subject>Relativism</subject><subject>Relativistic effects</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Stellar evolution</subject><subject>Stellar magnetic fields</subject><subject>Supernova</subject><subject>Supernova remnants</subject><subject>Supernovae</subject><subject>X-rays</subject><issn>0038-6308</issn><issn>1572-9672</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNp1kE1LAzEQhoMoWD9-gLeFnjxEZ5LNJjmWolYoKH6cQ3Y3q1vaTU26hf57s6yIFy8ZCM_zMvMScoVwgwDyNiIyzCmgopBLTfMjMkEhGdWFZMdkAsAVLTioU3IW4wpgsOSETOc-btoqe7GH7Dn4uq92re-ytste-60Lnd9bd0FOGruO7vJnnpP3-7u3-YIunx4e57MlrbiAHXUlc0VT1wqcZulVpW40B1EV3AmrsChqxUqVI2ucEK5uAEVphZCWV1VdOn5OrsfcT7s229BubDgYb1uzmC3N8AcoQQqu95jY6chug__qXdyZle9Dl9YzqDVPlxeCJQpHqgo-xuCa31gEMzRgxt5SsjJDbyZPDhudmNjuw4U_yf9K3wsqbb0</recordid><startdate>20180201</startdate><enddate>20180201</enddate><creator>Bykov, A. 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M.</creatorcontrib><creatorcontrib>Ellison, D. C.</creatorcontrib><creatorcontrib>Marcowith, A.</creatorcontrib><creatorcontrib>Osipov, S. 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M.</au><au>Ellison, D. C.</au><au>Marcowith, A.</au><au>Osipov, S. M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Cosmic Ray Production in Supernovae</atitle><jtitle>Space Sci.Rev</jtitle><stitle>Space Sci Rev</stitle><date>2018-02-01</date><risdate>2018</risdate><volume>214</volume><issue>1</issue><spage>1</spage><epage>34</epage><pages>1-34</pages><artnum>41</artnum><issn>0038-6308</issn><eissn>1572-9672</eissn><abstract>We give a brief review of the origin and acceleration of cosmic rays (CRs), emphasizing the production of CRs at different stages of supernova evolution by the first-order Fermi shock acceleration mechanism. We suggest that supernovae with trans-relativistic outflows, despite being rather rare, may accelerate CRs to energies above
10
18
eV
over the first year of their evolution. Supernovae in young compact clusters of massive stars, and interaction powered superluminous supernovae, may accelerate CRs well above the PeV regime. We discuss the acceleration of the bulk of the galactic CRs in isolated supernova remnants and re-acceleration of escaped CRs by the multiple shocks present in superbubbles produced by associations of OB stars. The effects of magnetic field amplification by CR driven instabilities, as well as superdiffusive CR transport, are discussed for nonthermal radiation produced by nonlinear shocks of all speeds including trans-relativistic ones.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11214-018-0479-4</doi><tpages>34</tpages><orcidid>https://orcid.org/0000-0002-3971-0910</orcidid></addata></record> |
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| subjects | Acceleration Aerospace Technology and Astronautics Astrophysics Astrophysics and Astroparticles Cosmic rays Evolution Magnetic fields Massive stars Nonthermal radiation Physics Physics and Astronomy Planetology Radiation Relativism Relativistic effects Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Stellar evolution Stellar magnetic fields Supernova Supernova remnants Supernovae X-rays |
| title | Cosmic Ray Production in Supernovae |
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