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Dense Electron-Positron Plasmas and Ultraintense γ rays from Laser-Irradiated Solids

C. P. Ridgers, C. S. Brady, R. Duclous, J. G. Kirk, K. Bennett, T. D. Arber, A. P. L. Robinson, and A. R. Bell
Phys. Rev. Lett. 108, 165006 – Published 19 April 2012
Physics logo See Synopsis: A Blast of Gamma Rays and Positrons

Abstract

In simulations of a 10 PW laser striking a solid, we demonstrate the possibility of producing a pure electron-positron plasma by the same processes as those thought to operate in high-energy astrophysical environments. A maximum positron density of 1026m3 can be achieved, 7 orders of magnitude greater than achieved in previous experiments. Additionally, 35% of the laser energy is converted to a burst of γ rays of intensity 1022Wcm2, potentially the most intense γ-ray source available in the laboratory. This absorption results in a strong feedback between both pair and γ-ray production and classical plasma physics in the new “QED-plasma” regime.

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  • Received 30 September 2011

DOI:https://doi.org/10.1103/PhysRevLett.108.165006

© 2012 American Physical Society

Synopsis

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A Blast of Gamma Rays and Positrons

Published 19 April 2012

The next generation of ultrahigh energy lasers will be able to produce extremely dense electron-positron plasmas and intense bursts of gamma rays, according to simulations, and both will lead to new types of experiments.

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Authors & Affiliations

C. P. Ridgers1,2, C. S. Brady3, R. Duclous4, J. G. Kirk5, K. Bennett3, T. D. Arber3, A. P. L. Robinson2, and A. R. Bell1,2

  • 1Clarendon Laboratory, University of Oxford, Parks Road, Oxford, OX1 3PU, United Kingdom
  • 2Central Laser Facility, STFC Rutherford-Appleton Laboratory, Chilton, Didcot, Oxfordshire, OX11 0QX, United Kingdom
  • 3Centre for Fusion, Space and Astrophysics, University of Warwick, Coventry, CV4 7AL, United Kingdom
  • 4Commissariat à l’Energie Atomique, DAM DIF, F-91297 Arpajon, France
  • 5Max-Planck-Institut für Kernphysik, Postfach 10 39 80, 69029 Heidelberg, Germany

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Issue

Vol. 108, Iss. 16 — 20 April 2012

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