Modeling radiative-shocks created by laser–cluster interactions-Reference-Cited by-同舟云学术

Modeling radiative-shocks created by laser–cluster interactions

Published:2020-03 Issue:3 Volume:27 Page:033301
ISSN:1070-664X
Container-title:Physics of Plasmas
language:en
Short-container-title:Physics of Plasmas

Author:

Scott R. H. H.¹^ORCID,Booth N.¹,Hawkes S. J.¹,Symes D. R.¹,Hooker C.¹,Doyle H. W.²,Olsson-Robbie S. I.³,Lowe H. F.³^ORCID,Price C. J.³,Bigourd D.⁴,Patankar S.⁵,Mecseki K.⁶,Gumbrell E. T.⁷,Smith R. A.³

Affiliation:

1. Central Laser Facility, STFC Rutherford Appleton Laboratory, Harwell Oxford, Didcot OX11 0QX, United Kingdom

2. First Light Fusion, Mead Rd., Yarnton, Kidlington OX5 1QU, United Kingdom

3. Department of Physics, The Blackett Laboratory, Imperial College London, London SW7 2AZ, United Kingdom

4. IMS Bordeaux University, UMR CNRS 5218, Bat. A31, 351 Cours de la Liberation, 33400 Talence, France

5. Lawrence Livermore National Laboratory, P.O. Box 808, Livermore, California 94550, USA

6. SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, California 94025, USA

7. Plasma Physics Division, AWE Aldermaston, Reading RG7 4PR, United Kingdom

Funder

Atomic Weapons Establishment

Engineering and Physical Sciences Research Council

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Link

http://aip.scitation.org/doi/pdf/10.1063/1.5136070

Reference25 articles.

1. From lasers to the universe: Scaling laws in laboratory astrophysics

2. Analysis of microscopic magnitudes of radiative blast waves launched in xenon clusters with collisional-radiative steady-state simulations

3. The acceleration of cosmic rays in shock fronts - I

4. Turbulent amplification of magnetic field and diffusive shock acceleration of cosmic rays

5. Instability of Taylor-Sedov blast waves propagating through a uniform gas

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