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Conferences > CLEO_SI > 2012 > JW4A > JW4A.18

Recombination Amplitude Calculation for Noble Gases beyond Strong Field Approximation in Length and Acceleration Gauge

Siddharth Bhardwaj, Sang-Kil Son, Robin Santra, and Franz X Kärtner

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Abstract

Recombination is a critical step in tomographic orbital imaging and quantitative modeling of HHG. We calculate and compare recombination amplitudes in length and acceleration gauge, beyond Strong Field Approximation, for noble gases used in HHG.

© 2012 Optical Society of America

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