Abstract
We report evidence for the first generation of XUV spectra from relativistic surface high-harmonic generation (SHHG) on plasma mirrors at a kilohertz repetition rate, emitted simultaneously with energetic electrons. SHHG spectra and electron angular distributions are measured as a function of the experimentally controlled plasma density gradient scale length for three increasingly short and intense driving pulses: 24~fs and , 8~fs and , and finally 4~fs and , where is the peak vector potential normalized by with the elementary charge , the electron rest mass , and the vacuum light velocity . For all driver pulses, we observe correlated relativistic SHHG and electron emission in the range , with an optimum gradient scale length of .
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