4.8 Article

Ultrahigh Brilliance Multi-MeV γ-Ray Beams from Nonlinear Relativistic Thomson Scattering

期刊

PHYSICAL REVIEW LETTERS
卷 113, 期 22, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.113.224801

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资金

  1. EPSRC [EP/L013975/1, EP/I029206/1]
  2. STFC [ST/J002062/1]
  3. NSF CAREER [1054164]
  4. EPSRC [EP/L013975/1, EP/H00601X/1, EP/I029206/1] Funding Source: UKRI
  5. STFC [ST/J002062/1] Funding Source: UKRI
  6. Direct For Mathematical & Physical Scien
  7. Division Of Physics [1054164] Funding Source: National Science Foundation

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We report on the generation of a narrow divergence (theta(gamma) < 2.5 mrad), multi-MeV (E-max approximate to 18 MeV) and ultrahigh peak brilliance (> 1.8 x 10(20) photons s(-1) mm(-2) mrad(-2) 0.1% BW) gamma-ray beam from the scattering of an ultrarelativistic laser-wakefield accelerated electron beam in the field of a relativistically intense laser (dimensionless amplitude a(0) approximate to 2). The spectrum of the generated gamma- 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.

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