Time-resolved x-ray diffraction from laser excited crystals
Optica Publishing Group (1997) thd2
Abstract:
We have constructed an ultra-fast time-dependant x-ray diffraction experiment in order to probe laser-induced phase transitions in solids. Such studies have previously been performed using laser probes in the infra-red, visible or ultraviolet spectral range. However, in order to directly probe structures in solids, it is necessary to use x-ray radiation. A laser system producing pulses with a duration of 100 fs has been set-up adjacent to a bending magnet at the Advanced Light Source (ALS). In addition an averaging streak camera with a temporal jitter smaller than 1.5 ps has been incorporated [1]. This diagnostic will permit us to study lattice disordering in materials such as Si. Single-shot measurements were also made using a Kentech streak camera.Ultrafast x-ray diffraction using a streak-camera detector in averaging mode
OPTICS LETTERS 22:13 (1997) 1012-1014
X-ray spectroscopic studies of hot, dense iron plasma formed by subpicosecond high intensity KrF laser irradiation
Applied Physics Letters 69:24 (1996) 3686-3688
Abstract:
The time-integrated x-ray emission from a hot, dense iron plasma has been recorded. The iron plasma was created when a target with a 1000-脜-thick iron layer buried beneath 1000 脜 of plastic was irradiated by a 300 fs pulse of 249 nm laser light at an intensity of approximately 1017 W cm-2. Two models have been used to construct a synthetic x-ray spectrum. The first employs detailed, spectroscopically accurate atomic data and the second uses a local thermodynamic equilibrium opacity model. The detailed model shows fairly good agreement with experiment whereas the opacity model only shows agreement in the gross features. 漏 1996 American Institute of Physics.Multicenter wavefunctions in opacity calculations for dense plasmas
Laser and Particle Beams Cambridge University Press (CUP) 14:4 (1996) 555-560
Corrections to Bremsstrahlung and Thomson Scattering at the Solar Center
The Astrophysical Journal American Astronomical Society 466:2 (1996) l115-l118