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High harmonics from relativistically oscillating plasma surfaces—a high brightness attosecond source at keV photon energies

2007/11/15 by M Zepf, M. Zepf, B. Dromey +31
Physics and Astronomy · #Atomic and Molecular Physics #Atomic physics #Attosecond #Brightness #Computational physics #Harmonics #Laser #Laser-Matter Interactions and Applications #Laser-Plasma Interactions and Diagnostics #Nuclear physics #Optics #Photon #Physics #Plasma #Quantum mechanics #Ultrashort pulse

paper · doi:10.1088/0741-3335/49/12b/s14

openalex publication_date 2007/11/15 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

An intense laser pulse interacting with a near discontinuous plasma vacuum interface causes the plasma surface to perform relativistic oscillations. The reflected laser radiation then contains very high order harmonics of fundamental frequency and-according to current theory-must be bunched in radiation bursts of a few attoseconds duration. Recent experimental results have demonstrated x-ray harmonic radiation extending to 3.3 angstrom (3.8 keV, order n > 3200) with the harmonic conversion efficiency scaling as eta(n) n(-2.5) over the entire observed spectrum ranging from 17 nm to 3.3 angstrom. This scaling holds up to a maximum order, n(RO) 81 8(1/2)gamma(3), where gamma is the peak value of the Lorentz factor, above which the harmonic efficiency decreases more rapidly. The coherent nature of the generated harmonics is demonstrated by the highly directional beamed emission, which for photon energy h nu > 1 keV is found to be into a cone angle similar to 4 degrees, significantly less than that of the incident laser cone (20 degrees).

Citations