Diffusive shock acceleration at laser-driven shocks: studying cosmic-ray accelerators in the laboratory

The non-thermal particle spectra responsible for the emission from many astrophysical systems are thought to originate from shocks via a first order Fermi process otherwise known as diffusive shock acceleration. The same mechanism is also widely believed to be responsible for the production of high...

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Main Authors: Reville, B, Bell, A, Gregori, G
Format: Journal article
Language:English
Published: 2013
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author Reville, B
Bell, A
Gregori, G
author_facet Reville, B
Bell, A
Gregori, G
author_sort Reville, B
collection OXFORD
description The non-thermal particle spectra responsible for the emission from many astrophysical systems are thought to originate from shocks via a first order Fermi process otherwise known as diffusive shock acceleration. The same mechanism is also widely believed to be responsible for the production of high energy cosmic rays. With the growing interest in collisionless shock physics in laser produced plasmas, the possibility of reproducing and detecting shock acceleration in controlled laboratory experiments should be considered. The various experimental constraints that must be satisfied are reviewed. It is demonstrated that several currently operating laser facilities may fulfil the necessary criteria to confirm the occurrence of diffusive shock acceleration of electrons at laser produced shocks. Successful reproduction of Fermi acceleration in the laboratory could open a range of possibilities, providing insight into the complex plasma processes that occur near astrophysical sources of cosmic rays. © IOP Publishing and Deutsche Physikalische Gesellschaft.
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spelling oxford-uuid:b59af0e5-86c4-49d4-85c2-d103d4d09ac72022-03-27T04:34:42ZDiffusive shock acceleration at laser-driven shocks: studying cosmic-ray accelerators in the laboratoryJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:b59af0e5-86c4-49d4-85c2-d103d4d09ac7EnglishSymplectic Elements at Oxford2013Reville, BBell, AGregori, GThe non-thermal particle spectra responsible for the emission from many astrophysical systems are thought to originate from shocks via a first order Fermi process otherwise known as diffusive shock acceleration. The same mechanism is also widely believed to be responsible for the production of high energy cosmic rays. With the growing interest in collisionless shock physics in laser produced plasmas, the possibility of reproducing and detecting shock acceleration in controlled laboratory experiments should be considered. The various experimental constraints that must be satisfied are reviewed. It is demonstrated that several currently operating laser facilities may fulfil the necessary criteria to confirm the occurrence of diffusive shock acceleration of electrons at laser produced shocks. Successful reproduction of Fermi acceleration in the laboratory could open a range of possibilities, providing insight into the complex plasma processes that occur near astrophysical sources of cosmic rays. © IOP Publishing and Deutsche Physikalische Gesellschaft.
spellingShingle Reville, B
Bell, A
Gregori, G
Diffusive shock acceleration at laser-driven shocks: studying cosmic-ray accelerators in the laboratory
title Diffusive shock acceleration at laser-driven shocks: studying cosmic-ray accelerators in the laboratory
title_full Diffusive shock acceleration at laser-driven shocks: studying cosmic-ray accelerators in the laboratory
title_fullStr Diffusive shock acceleration at laser-driven shocks: studying cosmic-ray accelerators in the laboratory
title_full_unstemmed Diffusive shock acceleration at laser-driven shocks: studying cosmic-ray accelerators in the laboratory
title_short Diffusive shock acceleration at laser-driven shocks: studying cosmic-ray accelerators in the laboratory
title_sort diffusive shock acceleration at laser driven shocks studying cosmic ray accelerators in the laboratory
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AT gregorig diffusiveshockaccelerationatlaserdrivenshocksstudyingcosmicrayacceleratorsinthelaboratory