Single Shot Characterization of High Transformer Ratio Wakefields in Nonlinear Plasma Acceleration.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
31 Jan 2020
Historique:
revised: 12 11 2019
received: 24 09 2019
entrez: 15 2 2020
pubmed: 15 2 2020
medline: 15 2 2020
Statut: ppublish

Résumé

Plasma wakefields can enable very high accelerating gradients for frontier high energy particle accelerators, in excess of 10  GeV/m. To overcome limits on single stage acceleration, specially shaped drive beams can be used in both linear and nonlinear plasma wakefield accelerators (PWFA), to increase the transformer ratio, implying that the drive beam deceleration is minimized relative to acceleration obtained in the wake. In this Letter, we report the results of a nonlinear PWFA, high transformer ratio experiment using high-charge, longitudinally asymmetric drive beams in a plasma cell. An emittance exchange process is used to generate variable drive current profiles, in conjunction with a long (multiple plasma wavelength) witness beam. The witness beam is energy modulated by the wakefield, yielding a response that contains detailed spectral information in a single-shot measurement. Using these methods, we generate a variety of beam profiles and characterize the wakefields, directly observing transformer ratios up to R=7.8. Furthermore, a spectrally based reconstruction technique, validated by 3D particle-in-cell simulations, is introduced to obtain the drive beam current profile from the decelerating wake data.

Identifiants

pubmed: 32058730
doi: 10.1103/PhysRevLett.124.044802
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

044802

Auteurs

R Roussel (R)

Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.

G Andonian (G)

Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.

W Lynn (W)

Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.

K Sanwalka (K)

Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.

R Robles (R)

Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.

C Hansel (C)

Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.

A Deng (A)

Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.

G Lawler (G)

Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.

J B Rosenzweig (JB)

Department of Physics and Astronomy, University of California, Los Angeles, California 90095, USA.

G Ha (G)

Argonne National Laboratory, Argonne, Illinois 60439, USA.

J Seok (J)

Argonne National Laboratory, Argonne, Illinois 60439, USA.

J G Power (JG)

Argonne National Laboratory, Argonne, Illinois 60439, USA.

M Conde (M)

Argonne National Laboratory, Argonne, Illinois 60439, USA.

E Wisniewski (E)

Argonne National Laboratory, Argonne, Illinois 60439, USA.

D S Doran (DS)

Argonne National Laboratory, Argonne, Illinois 60439, USA.

C E Whiteford (CE)

Argonne National Laboratory, Argonne, Illinois 60439, USA.

Classifications MeSH