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Table-Top Laser-Based Source of Femtosecond, Collimated, Ultrarelativistic Positron Beams

G. Sarri, W. Schumaker, A. Di Piazza, M. Vargas, B. Dromey, M. E. Dieckmann, V. Chvykov, A. Maksimchuk, V. Yanovsky, Z. H. He, B. X. Hou, J. A. Nees, A. G. R. Thomas, C. H. Keitel, M. Zepf, and K. Krushelnick
Phys. Rev. Lett. 110, 255002 – Published 20 June 2013
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Abstract

The generation of ultrarelativistic positron beams with short duration (τe+30fs), small divergence (θe+3mrad), and high density (ne+10141015cm3) from a fully optical setup is reported. The detected positron beam propagates with a high-density electron beam and γ rays of similar spectral shape and peak energy, thus closely resembling the structure of an astrophysical leptonic jet. It is envisaged that this experimental evidence, besides the intrinsic relevance to laser-driven particle acceleration, may open the pathway for the small-scale study of astrophysical leptonic jets in the laboratory.

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  • Received 20 December 2012

DOI:https://doi.org/10.1103/PhysRevLett.110.255002

© 2013 American Physical Society

Synopsis

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Tabletop Particle Accelerator

Published 20 June 2013

Dense electron-positron streams, similar to those found in astrophysical jets, can be made using a relatively simple tabletop laser setup.

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Authors & Affiliations

G. Sarri1, W. Schumaker2, A. Di Piazza3, M. Vargas2, B. Dromey1, M. E. Dieckmann1, V. Chvykov2, A. Maksimchuk2, V. Yanovsky2, Z. H. He2, B. X. Hou2, J. A. Nees2, A. G. R. Thomas2, C. H. Keitel3, M. Zepf1,4, and K. Krushelnick2

  • 1School of Mathematics and Physics, The Queen’s University of Belfast, BT7 1NN Belfast, United Kingdom
  • 2Center for Ultrafast Optical Science, University of Michigan, Ann Arbor, Michigan 48109-2099, USA
  • 3Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany
  • 4Helmholtz Institute Jena, Fröbelstieg 3, 07743 Jena, Germany

Comments & Replies

Comment on “Table-Top Laser-Based Source of Femtosecond, Collimated, Ultrarelativistic Positron Beams”

G. J. Williams, Hui Chen, J. Kim, S. Kerr, and H. Y. Khater
Phys. Rev. Lett. 124, 179501 (2020)

Sarri et al. Reply:

G. Sarri, W. Schumaker, A. Di Piazza, M. Vargas, B. Dromey, M. E. Dieckmann, V. Chvykov, A. Maksimchuk, V. Yanovsky, Z. H. He, B. X. Hou, J. A. Nees, A. G. R. Thomas, C. H. Keitel, M. Zepf, and K. Krushelnick
Phys. Rev. Lett. 124, 179502 (2020)

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Vol. 110, Iss. 25 — 21 June 2013

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