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Journal of Physics B Atomic Molecular and Optical Physics

Reply to comment on ‘Time-resolved resonant photoionization of He using a time-dependent Feshbach method with ultrashort laser pulses’

Carlos Mario Granados–Castro, José Luis Sanz‐Vicario

Published Jun 26, 2014• 0 citations
Publisher

Abstract

In this reply we amend the effect of misusing an analytical formula derived in 2007 Phys. Rev. A 75 013407, but containing a misprint subsequently corrected in a recently published erratum, 2013 Phys. Rev. A 87 069905(E). Two new corrected figures are included in this reply with the gradual formation of the resonance Fano profile for the lowest and third-lowest He 1P o resonant states. The comparison between our ab initio time-dependent Feshbach method and the analytical perturbative formula is rather good in the temporal domain for the time sequence shown during and after the laser pulse up to 50 fs, although still far from reaching the final asymptotic form. Other comments are also replied to. Finally, we emphasize that in the LabTalk published on 4 June 2013, we do not mention the inadequacy of any analytical formula whatsoever and the figure caption clearly refers to the asymptotic form of the Fano profile.

DOI
10.1088/0953-4075/47/13/138002

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The paper presents a theory that solves analytically the time-dependent three-level problem of the scheme $\mathrm{discrete}\phantom{\rule{0.28em}{0ex}}|0\ensuremath{\rangle}\phantom{\rule{0.28em}{0ex}}\underset{\mathrm{as}\phantom{\rule{0.16em}{0ex}}\mathrm{pulse}\phantom{\rule{0.16em}{0ex}}{\ensuremath{\omega}}_{1}}{\overset{\mathrm{weak}\phantom{\rule{0.16em}{0ex}}}{\ensuremath{\rightarrow}}}\phantom{\rule{0.28em}{0ex}}\mathrm{resonance}\phantom{\rule{0.28em}{0ex}}|1\ensuremath{\rangle}\phantom{\rule{0.28em}{0ex}}\underset{\mathrm{fs}\phantom{\rule{0.16em}{0ex}}\mathrm{pulse}\phantom{\rule{0.16em}{0ex}}{\ensuremath{\omega}}_{2}}{\overset{\mathrm{moderately}\phantom{\rule{0.16em}{0ex}}\mathrm{strong}\phantom{\rule{0.16em}{0ex}}}{\ensuremath{\rightarrow}}}\phantom{\rule{0.28em}{0ex}}\mathrm{resonance}\phantom{\rule{0.28em}{0ex}}|2\ensuremath{\rangle}$, where $|0\ensuremath{\rangle}$ is a discrete state, and $|1\ensuremath{\rangle}$ and $|2\ensuremath{\rangle}$ are energy-normalized resonance states. The attosecond and femtosecond pulses with central frequencies ${\ensuremath{\omega}}_{1}$ and ${\ensuremath{\omega}}_{2}$ (${\ensuremath{\omega}}_{1}\ensuremath{\gg}{\ensuremath{\omega}}_{2}$) act with ultrashort time delay, ${t}_{D}$. The formalism leads to analytic expressions for photoelectron emission probabilities, ${P}_{i}(E,t)$, $i=1,2$, in the energy region of the two resonance states, whose calculation in terms of N-electron matrix elements and external control parameters can be carried out economically for any such three-level system. The problem is first solved analytically, within the rotating wave approximation, for the case where the femtosecond pulse is rectangular. The weak attosecond pulse can have any temporal shape. The final solution for two pulses with arbitrary shape (Gaussian in our case) is then achieved by fitting numerically the shape of the femtosecond pulse to a sum of rectangular pulses. The formulas for ${P}_{i}(E,t)$ involve, among other things, the Fano discrete-resonance asymmetry parameter $q$, and the resonance-resonance asymmetry parameter Q, defined by us in previous work. They also involve the complex energy poles of the two resonances, a result which accounts for the whole contribution of the open channels of energy-normalized scattering states into which they decay. The theory is applied to the calculation from first principles, using compact state-specific discrete and resonance wave functions, of observable aspects of the time-resolved dynamics associated with the processes $\mathrm{He}$ $1{s}^{2}$ $^{1}S$ $\ensuremath{\rightarrow}$ $(2s2p)$ $^{1}P^{o}$ $\ensuremath{\leftrightarrow}$ $(2{p}^{2})$ $^{1}D$. Calculations show that the $(2{p}^{2})$ $^{1}D$ resonance is 0.295 eV (4200 nm) below the energy of $(2s2p)$ $^{1}P^{o}$, (60.15 eV), and its width is 0.067 eV. For the transition $1{s}^{2}$ $^{1}S$ $\ensuremath{\rightarrow}$ $(2s2p)$ $^{1}P^{o}$, the full width at half maximum (FWHM) of the Gaussian pulse is 160 as. The few-cycle midinfrared pulse coupling the resonance states is also Gaussian, whose duration is varied in the range of a few decades of femtoseconds. Its intensity is in the range $5\ifmmode\times\else\texttimes\fi{}{10}^{10}--5\ifmmode\times\else\texttimes\fi{}{10}^{11}$ $\mathrm{W}/\mathrm{c}{\mathrm{m}}^{2}$. The external control parameters are the intensity and the FWHM of the femtosecond pulse, as well as the ${t}_{D}$. For a given value of ${t}_{D}$, the FWHM of the second pulse is a crucial control parameter. The results include the time-resolved formation of either the $(2s2p)$ $^{1}P^{o}$ or the $(2{p}^{2})$ $^{1}D$ resonance, while they are coupled with each other. For the $(2s2p)$ $^{1}P^{o}$ state, comparison is made with the case where the time-dependent buildup of its asymmetric profile, excited from $1{s}^{2}$ $^{1}S$ by the same attosecond pulse, is calculated in the absence of coupling to another resonance. The result is in harmony with that of our earlier work on this problem. For the $(2{p}^{2})$ $^{1}D$ resonance excited from $(2s2p)$ $^{1}P^{o}$, the time-resolved buildup of its profile does not develop into an asymmetric peak due to the fact that $Q$ has the very large value of $\ensuremath{\approx}\ensuremath{-}1300$. Instead, it finishes as an Autler-Townes doublet.

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Reply to “Comment on ‘Solution of the Schrödinger equation for the time-dependent linear potential’ ”

I. Guedes

In this reply I discuss further the misconception in my paper [Phys. Rev. A 63, 034102 (2001)] related to the solution of the Schr\"odinger equation for a particle in a time-dependent linear potential.

Physical Review A•Jul 8, 2003•18 citations
In this reply we amend the effect of misusing an analytical formula derived in 2007 Phys. Rev. A 75 013407, but containing a misprint subsequently corrected in a recently published erratum, 2013 Phys. Rev. A 87 069905(E). Two new corrected figures are included in this reply with the gradual formation of the resonance Fano profile for the lowest and third-lowest He 1P o resonant states. The comparison between our ab initio time-dependent Feshbach method and the analytical perturbative formula is rather good in the temporal domain for the time sequence shown during and after the laser pulse up to 50 fs, although still far from reaching the final asymptotic form. Other comments are also replied to. Finally, we emphasize that in the LabTalk published on 4 June 2013, we do not mention the inadequacy of any analytical formula whatsoever and the figure caption clearly refers to the asymptotic form of the Fano profile.
Recently, we introduced [C. Ufrecht and E. Giese, Phys. Rev. A 101, 053615 (2020)] a technique to calculate the phase of light-pulse atom interferometers caused by the presence of perturbation potentials and underlined its power by an illustrative example. In the preceding Comment [B. Dubetsky, Phys. Rev. A 102, 027301 (2020)], it was pointed out that other, less idealized situations could have been calculated as well. Our Reply emphasizes that our method is correct, the results from our example can be trivially generalized to other perturbations, and intricate effects of local environments can be even more prominent but also treated by our technique.
The paper presents a theory that solves analytically the time-dependent three-level problem of the scheme $\mathrm{discrete}\phantom{\rule{0.28em}{0ex}}|0\ensuremath{\rangle}\phantom{\rule{0.28em}{0ex}}\underset{\mathrm{as}\phantom{\rule{0.16em}{0ex}}\mathrm{pulse}\phantom{\rule{0.16em}{0ex}}{\ensuremath{\omega}}_{1}}{\overset{\mathrm{weak}\phantom{\rule{0.16em}{0ex}}}{\ensuremath{\rightarrow}}}\phantom{\rule{0.28em}{0ex}}\mathrm{resonance}\phantom{\rule{0.28em}{0ex}}|1\ensuremath{\rangle}\phantom{\rule{0.28em}{0ex}}\underset{\mathrm{fs}\phantom{\rule{0.16em}{0ex}}\mathrm{pulse}\phantom{\rule{0.16em}{0ex}}{\ensuremath{\omega}}_{2}}{\overset{\mathrm{moderately}\phantom{\rule{0.16em}{0ex}}\mathrm{strong}\phantom{\rule{0.16em}{0ex}}}{\ensuremath{\rightarrow}}}\phantom{\rule{0.28em}{0ex}}\mathrm{resonance}\phantom{\rule{0.28em}{0ex}}|2\ensuremath{\rangle}$, where $|0\ensuremath{\rangle}$ is a discrete state, and $|1\ensuremath{\rangle}$ and $|2\ensuremath{\rangle}$ are energy-normalized resonance states. The attosecond and femtosecond pulses with central frequencies ${\ensuremath{\omega}}_{1}$ and ${\ensuremath{\omega}}_{2}$ (${\ensuremath{\omega}}_{1}\ensuremath{\gg}{\ensuremath{\omega}}_{2}$) act with ultrashort time delay, tD{t}_{D}tD​. The formalism leads to analytic expressions for photoelectron emission probabilities, Pi(E,t){P}_{i}(E,t)Pi​(E,t), i=1,2i=1,2i=1,2, in the energy region of the two resonance states, whose calculation in terms of N-electron matrix elements and external control parameters can be carried out economically for any such three-level system. The problem is first solved analytically, within the rotating wave approximation, for the case where the femtosecond pulse is rectangular. The weak attosecond pulse can have any temporal shape. The final solution for two pulses with arbitrary shape (Gaussian in our case) is then achieved by fitting numerically the shape of the femtosecond pulse to a sum of rectangular pulses. The formulas for Pi(E,t){P}_{i}(E,t)Pi​(E,t) involve, among other things, the Fano discrete-resonance asymmetry parameter qqq, and the resonance-resonance asymmetry parameter Q, defined by us in previous work. They also involve the complex energy poles of the two resonances, a result which accounts for the whole contribution of the open channels of energy-normalized scattering states into which they decay. The theory is applied to the calculation from first principles, using compact state-specific discrete and resonance wave functions, of observable aspects of the time-resolved dynamics associated with the processes He\mathrm{He}He 1s21{s}^{2}1s2 1S^{1}S1S $\ensuremath{\rightarrow}$ (2s2p)(2s2p)(2s2p) 1Po^{1}P^{o}1Po $\ensuremath{\leftrightarrow}$ (2p2)(2{p}^{2})(2p2) 1D^{1}D1D. Calculations show that the (2p2)(2{p}^{2})(2p2) 1D^{1}D1D resonance is 0.295 eV (4200 nm) below the energy of (2s2p)(2s2p)(2s2p) 1Po^{1}P^{o}1Po, (60.15 eV), and its width is 0.067 eV. For the transition 1s21{s}^{2}1s2 1S^{1}S1S $\ensuremath{\rightarrow}$ (2s2p)(2s2p)(2s2p) 1Po^{1}P^{o}1Po, the full width at half maximum (FWHM) of the Gaussian pulse is 160 as. The few-cycle midinfrared pulse coupling the resonance states is also Gaussian, whose duration is varied in the range of a few decades of femtoseconds. Its intensity is in the range $5\ifmmode\times\else\texttimes\fi{}{10}^{10}--5\ifmmode\times\else\texttimes\fi{}{10}^{11}$ W/cm2\mathrm{W}/\mathrm{c}{\mathrm{m}}^{2}W/cm2. The external control parameters are the intensity and the FWHM of the femtosecond pulse, as well as the tD{t}_{D}tD​. For a given value of tD{t}_{D}tD​, the FWHM of the second pulse is a crucial control parameter. The results include the time-resolved formation of either the (2s2p)(2s2p)(2s2p) 1Po^{1}P^{o}1Po or the (2p2)(2{p}^{2})(2p2) 1D^{1}D1D resonance, while they are coupled with each other. For the (2s2p)(2s2p)(2s2p) 1Po^{1}P^{o}1Po state, comparison is made with the case where the time-dependent buildup of its asymmetric profile, excited from 1s21{s}^{2}1s2 1S^{1}S1S by the same attosecond pulse, is calculated in the absence of coupling to another resonance. The result is in harmony with that of our earlier work on this problem. For the (2p2)(2{p}^{2})(2p2) 1D^{1}D1D resonance excited from (2s2p)(2s2p)(2s2p) 1Po^{1}P^{o}1Po, the time-resolved buildup of its profile does not develop into an asymmetric peak due to the fact that QQQ has the very large value of $\ensuremath{\approx}\ensuremath{-}1300$. Instead, it finishes as an Autler-Townes doublet.