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In recent years, the rapid development of ultrashort pulse laser technology has made it possible to regulate the ionization and dissociation dynamics of atoms and molecules. Among them, the microscopic dynamics of molecular dissociation have always been a hot topic. The phenomenon of molecular dissociation, which is caused by the interaction between femtosecond intense laser fields and $\text{H}_2^+$ molecules, has attracted widespread attention. Previous theoretical studies on the dissociation of $\text{H}_2^+$ molecules mainly focused on studying its dissociation dynamics through numerical calculations, with relatively few theoretical models. This paper aims to establish a simple classical model to describe the dissociation dynamics. Firstly, this paper calculates the joint distribution of nuclear energy and electronic energy in the dissociation process of $\text{H}_2^+$ molecules under the action of pump lasers by numerically solving the Schrödinger equation. The results prove that $\text{H}_2^+$ molecules initially in the ground state are dissociated into ${\rm H}^+ + {\rm H}^*$ after absorbing a pump photon in the pump light field. Next, this paper studies the dissociation dynamics of $\text{H}_2^+$ molecules in time-delayed two-color femtosecond lasers. We find that it greatly depends on the specific forms of the pump light and the probe light. By utilizing the dependence of the dissociation kinetic energy release (KER) spectrum on the time delay of the two-color femtosecond lasers, we retrieve the sub-attosecond microscopic dynamic behaviors of electrons and atomic nuclei in the dissociation process. Furthermore, we establish a classical model based on the conservation of energy and momentum to describe the dissociation dynamics. This model can qualitatively predict the ion dissociation KER spectrum depending on the time delay of the two-color femtosecond lasers. The electronic resonant transition between the molecular ground state and the first excited state caused by the probe light will affect the ion kinetic energy spectrum in the dissociation process. Namely, the ion kinetic energy spectrum is dependent on the frequency of the probe laser. By taking advantage of this characteristic, we propose a scheme to reconstruct the evolution of the internuclear distance with time. Our reconstruction results can qualitatively predict the trend of the numerical simulation results, and this scheme may provide some theoretical guidance for experiments.
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Keywords:
- femtosecond laser /
- hydrogen molecular ion /
- dissociation dynamics
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Google Scholar
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Google Scholar
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Google Scholar
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Google Scholar
[11] Jolicard G, Atabek O 1992 Phys. Rev. A 46 5845
Google Scholar
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Google Scholar
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[15] Xu H, Li Zhi C, He F, Wang X, Atia T N A, Kielpinski D, Sang R T, Litvinyuk I V 2017 Nat. Commun. 8 15849
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Google Scholar
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Google Scholar
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Google Scholar
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Google Scholar
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Google Scholar
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图 1 不同电子本征态对应的核间距依赖的分子势能面
Fig. 1. Molecular potential energy surfaces as a function of the internuclear distance for different electronic eigenstates.
图 2 单色泵浦光作用下解离动力学稳定时的核动能与电子能量的联合分布
Fig. 2. Joint distribution of the nuclear and electron energy after the dissociation caused by the monochromatic pump laser.
图 3 序列双色激光中$\text{H}_2^+$的延迟时间依赖的离子解离动能谱 (a)经(10)式计算所得的$\text{H}_2^+$的离子解离动能谱, 其中探测光$\tau_{2}=2 T_{2}$, $\lambda_{2}=580$ nm; (b)—(d) 与(a)相同, 区别仅在于探测光脉冲时间为$\tau_{2}=4 T_{2},\;6 T_{2} 和8 T_{2}$. 图中实线是经典模型的计算结果
Fig. 3. Time-dependent dissociation kinetic energy spectra of $\text{H}_2^+$ in sequential two-color femtosecond lasers: (a) The dissociation kinetic energy spectra of $\text{H}_2^+$ calculated by Eq. (10), in which $\tau_{2}=2 T_{2}$ and $\lambda_{2}=580$ nm; (b)−(d) the same as panel (a), but $\tau_{2}=4 T_{2},\;6 T_{2}和8 T_{2}$, respectively. The solid lines are the results calculated by the classical model.
图 4 (10)式计算得到的不同探测光波长下$\text{H}_2^+$的延迟时间依赖的离子解离动能谱 (a)探测光脉冲时间为$\tau_{2}=6 T_{2}$, 波长为$\lambda_{2}=180$ nm; (b)—(d)与(a)相同, 区别仅在于探测光波长为$\lambda_{2}=288,\;410,\;580\;{\mathrm{nm}}$
Fig. 4. Dissociation KER spectra calculated by Eq. (10) as a function of $t_{\rm{d}}$: (a) $\tau_{2}=6 T_{2}$ and $\lambda_{2}=180$ nm; (b)−(d) the same as (a), but $\lambda_{2}=288,\;410,\;580\;{\mathrm{nm}}$, respectively.
图 5 利用动能谱重构的核间距的时间演化与数值结果对比
Fig. 5. Comparison between the reconstructed time evolution of the internuclear distance and the numerical simulation results.
表 1 利用波长依赖的动能谱重构出的$\text{H}_2^+$解离过程中核间距的时间演化
Table 1. Reconstructed time evolution of the internuclear distance in the dissociation process of $\text{H}_2^+$ utilizing the wavelength-dependence KER spectra.
$\lambda_{2}/{\rm{nm}}$ $\omega_{2}/{\rm{a.u.}}$ $R/{\rm{a.u.}}$ $t_{\rm{d}}/{\rm{a.u.}}$ $t=t_{\rm{d}}+T_{2}$ $ \langle t \rangle $ $\Delta t$ $ \langle R \rangle $ $\Delta R$ $180$ [0.21093, 0.2953] $[2.5, 3.05]$ $[0, 20]$ $[25, 45]$ $35$ $10$ $2.75$ $0.25$ $288$ [0.13183, 0.18456] $[3.3, 3.85]$ $[0, 47]$ $[40, 87]$ $63.5$ $23.5$ $3.6$ $0.3$ $410$ [0.0926, 0.12964] $[3.9, 4.45]$ $[0, 60]$ $[57, 117]$ $87$ $30$ $4.2$ $0.3$ $580$ [0.06546, 0.09164] $[4.45, 5.0]$ $[20, 70]$ $[100, 150]$ $125$ $25$ $4.7$ $0.3$ 
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[1] Alnaser A S, Tong X M, Osipov T, et al. 2004 Phys. Rev. A 93 183202
Google Scholar
[2] Manschwetus B, Nubbemeyer T, Gorling K, Steinmeyer G, Eichmann U, Rottke H, Sandner W 2009 Phys. Rev. Lett. 102 113002
Google Scholar
[3] Mi Y H, Peng P, Camus N, et al. 2020 Phys. Rev. Lett. 125 173201
Google Scholar
[4] Pan S Z, Zhang W B, Li H, et al. 2021 Phys. Rev. Lett. 126 063201
Google Scholar
[5] Guo Z N, Zhang Z H, Deng Y K, Wang J G, Ye D F, Liu J, Liu Y Q 2024 Phys. Rev. Lett. 132 143201
Google Scholar
[6] 张颖, 王兴, 徐忠锋, 任洁茹, 张艳宁, 周贤明, 梁昌慧, 张小安 2024 物理学报 73 023101
Google Scholar
Zhang Y, Wang X, Xu Z F, Ren J R, Zhang Y N, Zhou X M, Liang C H, Zhang X A 2024 Acta Phys. Sin. 73 023101
Google Scholar
[7] 骆炎, 余璇, 雷建廷, 陶琛玉, 张少锋, 朱小龙, 马新文, 闫顺成, 赵晓辉 2024 物理学报 73 044101
Google Scholar
Luo Y, Yu X, Lei J T, Tao C Y, Zhang S F, Zhu X L, Ma X W, Yan S C, Zhao X H 2024 Acta Phys. Sin. 73 044101
Google Scholar
[8] Jin W W, Wang C C, Zhao X G, et al. 2024 Chin. Phys. Lett. 41 053101
Google Scholar
[9] Bucksbaum P H, Zavriyev A, Muller H G, Schumacher D W 2019 Phys. Rev. Lett. 64 1883
Google Scholar
[10] Frasinski L J, Posthumus J H, Plumridge J, Codling K, Taday P F, Langley A J 1999 Phys. Rev. Lett. 83 3625
Google Scholar
[11] Jolicard G, Atabek O 1992 Phys. Rev. A 46 5845
Google Scholar
[12] Posthumus J H, Plumridge J, Frasinski L J, et al. 2000 J. Phys. B: At. Mol. Opt. Phys. 33 L563
Google Scholar
[13] Niikura H, Légaré F, Hasbani R, Ivanov M Y, Villeneuve D M, Corkum P B 2003 Nature 421 826
Google Scholar
[14] Staudte A, Pavičić D, Chelkowski S, et al. 2007 Phys. Rev. Lett. 98 073003
Google Scholar
[15] Xu H, Li Zhi C, He F, Wang X, Atia T N A, Kielpinski D, Sang R T, Litvinyuk I V 2017 Nat. Commun. 8 15849
Google Scholar
[16] Hanus V, Kangaparambil S, Larimian S, et al. 2019 Phys. Rev. Lett. 123 263201
Google Scholar
[17] Li X K, Yu X T, Ma P, Zhao X N, Wang C C, Luo S Z, Ding D J 2022 Chin. Phys. B 31 103304
Google Scholar
[18] Leth H A, Madsen L B, Mølmer K 2010 Phys. Rev. A 81 053409
Google Scholar
[19] Leth H A, Madsen L B, Mølmer K 2010 Phys. Rev. A 81 053410
Google Scholar
[20] Liu K L, Barth I 2021 Phys. Rev. A 103 013103
Google Scholar
[21] Sami F, Vafaee M, Shokri B 2016 J. Phys. B: At. Mol. Opt. Phys. 44 165601
Google Scholar
[22] Zhao M M, Li L H, Si B W, Wang B B, Fu B N, Han Y C 2022 Chin. Phys. Lett. 39 083401
Google Scholar
[23] Hu T C, Zhu S K, Zhao Y N, et al. 2022 Chin. Phys. B 31 047901
Google Scholar
[24] Pavicic D, Kiess A, Hansch T W, Figger H 2005 Phys. Rev. Lett. 94 163002
Google Scholar
[25] Magrakvelidze M, He F, Niederhausen T, Litvinyuk I V, Thumm U 2009 Phys. Rev. A 79 033410
Google Scholar
[26] Kling M F, Siedschlag C, Verhoef A J, et al. 2006 Science 312 246
Google Scholar
[27] Esry B D, Sayler A M, Wang P Q, Carnes K D, BenItzhak I 2006 Phys. Rev. Lett. 97 013003
Google Scholar
[28] Guo W, Lu X Q, Zhao D, Wang X L 2014 Phys. Scr. 89 025401
Google Scholar
[29] Krausz F, Ivanov M 2009 Rev. Mod. Phys. 81 163
Google Scholar
[30] Feng L Q 2015 Phys. Rev. A 92 053832
Google Scholar
[31] Roudnev V, Esry B D, Itzhak I B 2004 Phys. Rev. Lett. 93 163601
Google Scholar
[32] Gibson G N, Li M, Guo C, Neira J 1997 Phys. Rev. Lett. 79 2022
Google Scholar
[33] Alnaser A S, Ulrich B, Tong X M, et al. 2005 Phys. Rev. A 72 030702
Google Scholar
[34] Hua J J, Esry B D 2009 Phys. Rev. A 80 013413
Google Scholar
[35] Benis E P, Bakarezos M, Papadogiannis N A, et al. 2012 Phys. Rev. A 86 043428
Google Scholar
[36] Hu H T, Xu H, Bai Y, Sang R T, Litvinyuk I V, Liu P, Li R X 2016 Phys. Rev. A 94 053415
Google Scholar
[37] Fischer B, Kremer M, Pfeifer T, et al. 2010 Phys. Rev. Lett. 105 223001
Google Scholar
[38] Jia Z M, Zeng Z N, Li R X, Xu Z Z, Deng Y P 2014 Phys. Rev. A 89 023419
Google Scholar
[39] Zhang J, Pan X F, Du H, Xu T T, Guo J, Liu X S 2017 Opt. Commun. 382 495
Google Scholar
[40] Liu K L, Zhang Q B, Lu P X 2012 Phys. Rev. A 86 033410
Google Scholar
[41] Wanie V 2016 J. Phys. B: At. Mol. Opt. Phys. 49 025601
Google Scholar
[42] Balint K G G 2015 Theory of Molecular Collisions (Cambridge: Royal Society of Chemistry
[43] Lu R F, Zhang P Y, Han K L 2008 Phys. Rev. E 77 066701
Google Scholar
[44] Lehtovaara L, Toivanen J, Eloranta J 2007 J. Comput. Phys. 221 148
Google Scholar
[45] Feit M D, Fleck Jr J A, Steiger A 1982 J. Comput. Phys. 47 412
Google Scholar
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