BibTex format
@article{Sarri:2014:10.1103/PhysRevLett.113.224801,
author = {Sarri, G and Corvan, DJ and Schumaker, W and Cole, JM and Di, Piazza A and Ahmed, H and Harvey, C and Keitel, CH and Krushelnick, K and Mangles, SPD and Najmudin, Z and Symes, D and Thomas, AGR and Yeung, M and Zhao, Z and Zepf, M},
doi = {10.1103/PhysRevLett.113.224801},
journal = {Physical Review Letters},
pages = {1--5},
title = {Ultrahigh brilliance multi-MeV gamma-Ray beams from nonlinear relativistic Thomson scattering},
url = {http://dx.doi.org/10.1103/PhysRevLett.113.224801},
volume = {113},
year = {2014}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - We report on the generation of a narrow divergence (θγ<2.5 mrad), multi-MeV (Emax≈18 MeV) and ultrahigh peak brilliance (>1.8×1020 photons s−1 mm−2 mrad−2 0.1% BW) γ-ray beam from the scattering of an ultrarelativistic laser-wakefield accelerated electron beam in the field of a relativistically intense laser (dimensionless amplitude a0≈2). The spectrum of the generated γ-ray beam is measured, with MeV resolution, seamlessly from 6 to 18 MeV, giving clear evidence of the onset of nonlinear relativistic Thomson scattering. To the best of our knowledge, this photon source has the highest peak brilliance in the multi-MeV regime ever reported in the literature.
AU - Sarri,G
AU - Corvan,DJ
AU - Schumaker,W
AU - Cole,JM
AU - Di,Piazza A
AU - Ahmed,H
AU - Harvey,C
AU - Keitel,CH
AU - Krushelnick,K
AU - Mangles,SPD
AU - Najmudin,Z
AU - Symes,D
AU - Thomas,AGR
AU - Yeung,M
AU - Zhao,Z
AU - Zepf,M
DO - 10.1103/PhysRevLett.113.224801
EP - 5
PY - 2014///
SN - 0031-9007
SP - 1
TI - Ultrahigh brilliance multi-MeV gamma-Ray beams from nonlinear relativistic Thomson scattering
T2 - Physical Review Letters
UR - http://dx.doi.org/10.1103/PhysRevLett.113.224801
UR - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000348132200005&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR - https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.113.224801
UR - http://hdl.handle.net/10044/1/21918
VL - 113
ER -