Photoemission from the gas phase using soft x-ray fs pulses: an investigation of the space-charge effects
Creators
- 1. Dipartimento di Scienze, Università degli Studi Roma Tre, Via della Vasca Navale 84, 00146 Roma (Italy)
- 2. Graduate School of Materials Science, University of Hyogo, Kamigori-cho, Ako-gun, Hyogo 678-1297 (Japan)
- 3. Department of Physics, Kyoto University, Kyoto 606-8502 (Japan)
- 4. Department of Chemistry, Graduate School of Science, Hiroshima University, Higashi-hiroshima, Hiroshima 739-8526 (Japan)
- 5. The Graduate University for Advanced Studies, Institute for Molecular Science, Okazaki, Aichi 444-8585 (Japan)
- 6. JASRI/XFEL, 1-1-1 Kouto, Sayo-cho, Sayo-gun, Hyogo 679-5198 (Japan)
- 7. Physical and Chemical Research Infrastructure Group, Advanced Photon Technology Division, RIKEN SPring-8 Center, 1-1-1 Kouto, Sayo-cho, Sayo-gun, Hyogo 679-5148 (Japan)
Description
An experimental and computational investigation of the space-charge effects occurring in ultrafast photoelectron spectroscopy from the gas phase is presented. The target sample CF3I is excited by ultrashort (100 fs) far-ultraviolet radiation pulses produced by a free-electron laser. The modification of the energy distribution of the photoelectrons, i.e. the shift and broadening of the spectral structures, is monitored as a function of the pulse intensity. The experimental results are compared with computational simulations which employ a Barnes–Hut algorithm to calculate the effect of individual Coulomb forces acting among the particles. In the presented model, a survey spectrum acquired at low radiation fluence is used to determine the initial energy distribution of the electrons after the photoemission event. The spectrum modified by the space-charge effects is then reproduced by N-body calculations that simulate the dynamics of the photoelectrons subject to the individual mutual Coulomb repulsion and to the attractive force of the positive ions. The employed numerical method accounts for the space-charge effects on the energy distribution and allows to reproduce the complete photoelectron spectrum and not just a specific photoemission structure. The simulations also provide information on the time evolution of the space-charge effects on the picosecond scale. Differences with the case of photoemission from solid samples are highlighted and discussed. The presented simulation procedure, although it omits the analysis of angular distribution, constitutes an effective simplified model that allows to predict and account for space-charge effects on the photoelectron energy spectrum in time-resolved photoemission experiments with high-intensity pulsed sources. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1367-2630/abcbc6Additional details
Identifiers
Publishing Information
- Journal Title
- New Journal of Physics
- Journal Volume
- 22
- Journal Issue
- 12
- Journal Page Range
- [13 p.]
- ISSN
- 1367-2630
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 52052366
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- ANGULAR DISTRIBUTION; CATIONS; COMPUTERIZED SIMULATION; COULOMB FIELD; ELECTRONS; ENERGY SPECTRA; FAR ULTRAVIOLET RADIATION; FREE ELECTRON LASERS; PHOTOELECTRON SPECTROSCOPY; PHOTOEMISSION; SOFT X RADIATION; TIME RESOLUTION
- Descriptors DEC
- CHARGED PARTICLES; DISTRIBUTION; ELECTRIC FIELDS; ELECTROMAGNETIC RADIATION; ELECTRON SPECTROSCOPY; ELEMENTARY PARTICLES; EMISSION; FERMIONS; IONIZING RADIATIONS; IONS; LASERS; LEPTONS; RADIATIONS; RESOLUTION; SECONDARY EMISSION; SIMULATION; SPECTRA; SPECTROSCOPY; TIMING PROPERTIES; ULTRAVIOLET RADIATION; X RADIATION