Humphrey W, Lu H, Logunov I, Werner H J, Schulten K
Beckman Institute for Advanced Science and Technology, University of Illinois at Urbana-Champaign, Urbana, Illinois 61801, USA.
Biophys J. 1998 Oct;75(4):1689-99. doi: 10.1016/S0006-3495(98)77611-8.
The primary all-trans --> 13-cis photoisomerization of retinal in bacteriorhodopsin has been investigated by means of quantum chemical and combined classical/quantum mechanical simulations employing the density matrix evolution method. Ab initio calculations on an analog of a protonated Schiff base of retinal in vacuo reveal two excited states S1 and S2, the potential surfaces of which intersect along the reaction coordinate through an avoided crossing, and then exhibit a second, weakly avoided, crossing or a conical intersection with the ground state surface. The dynamics governed by the three potential surfaces, scaled to match the in situ level spacings and represented through analytical functions, are described by a combined classical/quantum mechanical simulation. For a choice of nonadiabatic coupling constants close to the quantum chemistry calculation results, the simulations reproduce the observed photoisomerization quantum yield and predict the time needed to pass the avoided crossing region between S1 and S2 states at tau1 = 330 fs and the S1 --> ground state crossing at tau2 = 460 fs after light absorption. The first crossing follows after a 30 degrees torsion on a flat S1 surface, and the second crossing follows after a rapid torsion by a further 60 degrees. tau1 matches the observed fluorescence lifetime of S1. Adjusting the three energy levels to the spectral shift of D85N and D212N mutants of bacteriorhodospin changes the crossing region of S1 and S2 and leads to an increase in tau1 by factors 17 and 10, respectively, in qualitative agreement with the observed increase in fluorescent lifetimes.
利用密度矩阵演化方法,通过量子化学以及经典/量子力学相结合的模拟,对细菌视紫红质中视黄醛的初级全反式→13 - 顺式光异构化进行了研究。对真空中视黄醛质子化席夫碱类似物的从头算计算揭示了两个激发态S1和S2,其势能面沿着反应坐标通过一个避免交叉相交,然后与基态表面呈现第二个弱避免交叉或锥形交叉。由三个势能面控制的动力学,经缩放以匹配原位能级间距并通过解析函数表示,由经典/量子力学相结合的模拟描述。对于选择接近量子化学计算结果的非绝热耦合常数,模拟重现了观察到的光异构化量子产率,并预测了在光吸收后,通过S1和S2态之间的避免交叉区域所需的时间为τ1 = 330飞秒,以及S1→基态交叉所需的时间为τ2 = 460飞秒。第一次交叉发生在平坦的S1表面上扭转30度之后,第二次交叉发生在进一步快速扭转60度之后。τ1与观察到的S1荧光寿命相匹配。将三个能级调整到细菌视紫红质D85N和D212N突变体的光谱位移,会改变S1和S2的交叉区域,并导致τ1分别增加17倍和10倍,这与观察到的荧光寿命增加在定性上一致。