SearcharxivSearch

arXiv subjects

C. Cirelli

Publications and source records attributed to C. Cirelli.

3 recordsLinked to original sources

Resonance effects in photoemission time delays

We present measurements of single-photon ionization time delays between valence electrons of argon and neon using a coincidence detection technique that allows for the simultaneous measurement of both species under identical conditions. Taking into account the chirp of the ionizing single attosecond pulse (attochirp) ensures that the clock of our measurement technique is started at the same time for both types of electrons, revealing with high accuracy and resolution energy-dependent time delays of a few tens of attoseconds. By comparing our results with theoretical predictions, we confirm that the so-called Wigner delay correctly describes single-photon ionization delays as long as atomic resonances can be neglected. Our data, however, also reveal that such resonances can greatly affect the measured delays beyond the simple Wigner picture.

physics.atom-ph

Sequential Tunneling vs. Electron Correlation in Multiple Photo-ionization

We take advantage of the information provided by use of elliptical polarization in a recent two-electron release time experiment [A.N. Pfeiffer et al., Nature Physics 7, 428 (2011)]. This allows a comparative test of the currently dominant conjectures regarding independent-electron tunneling theory vs. fully electron-correlated classical release theory to describe electron release in strong-field double ionization.

physics.atom-ph

Direct observation of Space Charge Dynamics by picosecond Low Energy Electron Scattering

The electric field governing the dynamics of space charge produced by high intensity femtosecond laser pulses focused on a copper surface is investigated by time-resolved low-energy-electron-scattering. The pump-probe experiment has a measured temporal resolution of better than 35 ps at 55 eV probe electron energy. The probe electron acceleration due to space charge is reproduced within a 3-dimensional non-relativistic model, which determines an effective number of electrons in the space charge electron cloud and its initial diameter. Comparison of the simulations with the experiments indicates a Coulomb explosion, which is consistent with transients in the order of 1 ns, the terminal kinetic energy of the cloud and the thermoemission currents predicted by the Richardson-Dushman formula.

cond-mat.mtrl-sci