Published May 21, 2010
| Version v1
Journal article
Pulse-Length Dependence of the Anisotropy of Laser-Driven Cluster Explosions: Transition to the Impulsive Regime for Pulses Approaching the Few-Cycle Limit
Creators
- 1. Department of Physics, Imperial College London, London, SW7 2AZ (United Kingdom)
- 2. Central Laser Facility, STFC Rutherford Appleton Laboratory, Didcot OX11 0QX (United Kingdom)
Description
We have experimentally observed anisotropic ion emission from Xe and Ar clusters under intense ultrashort (∼30 fs) laser irradiation, with up to 1.8 times more energetic ions emitted in the direction perpendicular to the laser polarization than in the parallel direction. As the pulse length was varied in the range of 8-160 fs, we found this anisotropy to first grow and then diminish. Treating electrons inside the unexpanded cluster as a harmonic oscillator qualitatively demonstrates how intracluster electric field can result in an ion emission anisotropy of this kind. Our observations give direct access to the initial charging dynamics present in the first few cycles of an intense laser field interacting with any nanoscale dielectric.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 104
- Journal Issue
- 20
- Journal Page Range
- p. 203401-203401.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42003846
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- ANISOTROPY; ARGON; ATOMIC CLUSTERS; DIELECTRIC MATERIALS; ELECTRIC FIELDS; ELECTRONS; HARMONIC OSCILLATORS; ION EMISSION; LASER RADIATION; NANOSTRUCTURES; POLARIZATION; PULSES; TAIL IONS; XENON
- Descriptors DEC
- CHARGED PARTICLES; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; ELEMENTS; EMISSION; FERMIONS; FLUIDS; GASES; IONS; LEPTONS; MATERIALS; NONMETALS; RADIATIONS; RARE GASES
Optional Information
- Notes
- (c) 2010 The American Physical Society