Dynamics of laser-induced molecular alignment in the impulsive and adiabatic regimes: A direct comparison
Quantum-mechanical calculations are performed of the dynamic alignment of linear molecules induced by a strong nonresonant laser field. Within this framework we have treated in a unified fashion the alignment with laser pulses of varying duration from the short pulse impulsive limit ({tau}{sub pulse...
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Published in: | Physical review. A, Atomic, molecular, and optical physics Vol. 72; no. 2 |
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Main Authors: | , , |
Format: | Journal Article |
Language: | English |
Published: |
United States
01-08-2005
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Subjects: | |
Online Access: | Get full text |
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Summary: | Quantum-mechanical calculations are performed of the dynamic alignment of linear molecules induced by a strong nonresonant laser field. Within this framework we have treated in a unified fashion the alignment with laser pulses of varying duration from the short pulse impulsive limit ({tau}{sub pulse}<<T{sub rot}) to the long pulse adiabatic limit ({tau}{sub pulse}>T{sub rot}). The temporal behavior of the alignment in both these limits, and in the intermediate pulse duration regime, have been analyzed. For the impulsive limit the dependence of the degree of maximum alignment upon the laser pulse duration was examined and the intensity-dependent optimum pulse duration explained. A comparison between the degree of alignment under the same conditions of pulse intensity and rotational temperature was performed between the impulsive and adiabatic cases. The adiabatic case was found to always provide a better degree of alignment for a given intensity which we show is due to the zero relative phasing between the component states of the superposition that form the pendular states. We have explicitly calculated the angular distribution of an ensemble of linear molecules as it evolves through a rotational revival; a rich structure is found that may be useful in guiding future experiments that utilize the field free alignment in a revival. |
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ISSN: | 1050-2947 1094-1622 |
DOI: | 10.1103/PhysRevA.72.023420 |