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Sample Text ÔÚGaussian 09 µÄ¼ÆËãÓ«¹â·¢É俼ÂÇÁËÈܼÁ»¯Ð§Ó¦µÄËãÀýÖУ¨ÈçÏÂËùʾ£©£¬ÔÚ7²½¼ÆËãÖУ¬¸÷×Ô¶ÁÈ¡µÄchkÎļþ·Ö±ðÊÇÄĸö°¡£¿»¹ÓоÍÊǾßÌåµÄ¡°Æ½ºâÈܽ⡱ºÍ¡°·ÇƽºâÈܽ⡱ÊÇʲôÒâ˼£¿ ллָµ¼£¬¿àÄÕÁ˺ü¸ÌìµÄÒ»¸öÎÊÌâÁË£¬ÄóöÀ´´ó¼ÒÌÖÂÛһϠFluoresence example: Emission (Fluorescence) from First Excited State (n¡ú¦Ð*) of Acetaldehyde Here we study the cycle: Acetaldehyde Excitation and Emission Cycle The primary process of interest is the emission, but this example shows how to study the complete cycle including the solvent effects. Step 1: Ground state geometry optimization and frequencies (equilibrium solvation). This is a standard Opt Freq calculation on the ground state including PCM equilibrium solvation. %chk=01-ac # B3LYP/6-31+G(d,p) Opt Freq SCRF=(Solvent=Ethanol) Acetaldehyde ground state 0 1 C C,1,RA X,2,1.,1,A O,2,RB,3,A,1,180.,0 X,1,1.,2,90.,3,0.,0 H,1,R1,2,A1,5,0.,0 H,1,R23,2,A23,5,B23,0 H,1,R23,2,A23,5,-B23,0 H,2,R4,1,A4,3,180.,0 RA=1.53643 RB=1.21718 R1=1.08516 R23=1.08688 R4=1.10433 A=62.1511 A1=110.51212 A23=109.88119 A4=114.26114 B23=120.56468 Step 2: Vertical excitation with linear response solvation. This is a TD-DFT calculation of the vertical excitation, therefore at the ground state equilibrium geometry, with the default solvation: linear response, non-equilibrium. We perform a single-point TD-DFT calculation, which defaults to non-equilibrium solvation. The results of this job will be used to identify which state or states are of interest and their ordering. These results give a reasonable description of the solvation of the excited state, but not quite as good as that from a state-specific solvation calculation. In this case, we see that the n->¦Ð* state is the first excited state. Next, we will use the state-specific method to produce a better description of the vertical excitation step. %chk=02-ac # B3LYP/6-31+G(d,p) TD=NStates=6 SCRF=(Solvent=Ethanol) Geom=Check Guess=Read Acetaldehyde: linear response vertical excited states 0 1 Step 3: State-specific solvation of the vertical excitation. This will require two job steps: first the ground state calculation is done, specifying NonEq=write in the PCM input section, in order to store the information about non-equilibrium solvation based on the ground state. Second, the actual state-specific calculation is done, reading in the necessary information for non-equilibrium solvation using NonEq=read. %chk=03-ac # B3LYP/6-31+G(d,p) SCRF=(Solvent=Ethanol,Read) Geom=Check Guess=Read Acetaldehyde: prepare for state-specific non-eq solvation by saving the solvent reaction field from the ground state 0 1 NonEq=write --link1-- %chk=03-ac # B3LYP/6-31+G(d,p) TD(NStates=6,Root=1) SCRF=(Solvent=Ethanol,StateSpecific,Read) Geom=Check Guess=Read Acetaldehyde: read non-eq solvation from ground state and compute energy of the first excited with the state-specific method 0 1 NonEq=read Step 4: Relaxation of the excited state geometry. Next, we perform a TD-DFT geometry optimization, with equilibrium, linear response solvation, in order to find the minimum energy point on the excited state potential energy surface. Since this is a TD-DFT optimization, the program defaults to equilibrium solvation. As is typical of such cases, the molecule has a plane of symmetry in the ground state but the symmetry is broken in the excited state, so the ground state geometry is perturbed slightly to break symmetry at the start of the optimization. %chk=04-ac # B3LYP/6-31+G(d,p) TD=(Read,NStates=6,Root=1) SCRF=(Solvent=Ethanol) Geom=Modify Guess=Read Opt=RCFC Acetaldehyde: excited state opt Modify geometry to break Cs symmetry since first excited state is A" 0 1 4 1 2 3 10.0 5 1 2 7 -50.0 Step 5: Vibrational frequencies of the excited state structure. Now we run a frequency calculation to verify that the geometry located in step 4 is a minimum. The results could also be used as part of a Franck-Condon calculation if desired (see below). This is a numerical frequency calculation. %chk=05-ac # B3LYP/6-31+G(d,p) TD=(Read,NStates=6,Root=1) Freq SCRF=(Solvent=Ethanol) Geom=Check Guess=Read Acetaldehyde excited state freq 0 1 Step 6: Emission state-specific solvation (part 1). This step does state-specific equilibrium solvation of the excited state at its equilibrium geometry, writing out the solvation data for the next step via the PCM NonEq=write input. %chk=06-ac # B3LYP/6-31+G(d,p) TD=(Read,NStates=6,Root=1) SCRF=(Solvent=Ethanol,StateSpecific,Read) Geom=Check Guess=Read Acetaldehyde emission state-specific solvation at first excited state optimized geometry 0 1 NonEq=write Step 7: Emission to final ground state (part 2). Finally, we compute the ground state energy with non-equibrium solvation, at the excited state geometry and with the static solvation from the excited state. %chk=07-ac # B3LYP/6-31+G(d,p) SCRF=(Solvent=Ethanol,Read) Geom=Check Guess=Read Acetaldehyde: ground state non-equilibrium at excited state geometry. 0 1 NonEq=read |
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youzhizhe(½ð±Ò+3, 1STÇ¿Ìû+1): лл½»Á÷¡£ 2011-08-25 23:38:45
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ÎÒ·ÖÎöÁËÒ»ÏÂÄǼ¸²½µÄ¼ÆË㣬µÄÈ·µÚ6²½ÐèÒªµÚ4²½µÄchk µÚ3²½Ê¹ÓõÚ1»òµÚ2²½µÄ¶¼ÐÐ µÚ6²½ºÍµÚ7²½¼ÆËãÊǺ͵Ú3²½µÄÁ½¸ö¼ÆËãÏà¶ÔÓ¦£¬Ö»²»¹ýµÚ6/7²½ÊÇ·¢É䣬µÚ3²½ÊǼ¤·¢£¬µÚ6/7Á½²½µÃµ½µÄÄÜÁ¿Ö®²î¾ÍÊǾ¹ýÖ¸¶¨Ì¬µÄÈܼÁ»¯Ð§Ó¦Ð£ÕýÖ®ºóµÄÓ«¹â·¢ÉäÄÜÁ¿£¬¾¹ýת»»¿ÉÒԵõ½Ó«¹âµÄ·¢É䲨³¤¡£ ¹ØÓÚÆ½ºâºÍ·ÇƽºâµÄÎÊÌâÊǺÍstatespecific¼ÆËãÓÐ×Ų»¿É·ÖµÄ¹ØÏµµÄ£¬Äã¿ÉÒÔ¿´Ò»ÏÂÏÂÃæµÄÓ¢ÎIJ¿·Ö£¬ÕâÊÇÎÒǰһ¶Îʱ¼ä´ÓGaussian¹Ù·½¼¼Êõ¹ËÎÊÄÇÀïµÃµ½µÄÏêϸ½âÊÍ£¬¼¸¾ä»°¾«Á·²»³öÀ´£¬·ÒëÒ²ÒªºÄ·ÑÒ»¶Îʱ¼ä£¬ÄãÄÍÐĶÁÒ»¶Á¡£ ÁíÍ⣬Èç¹ûÄãÊÇÓõÄÊÇGaussian 09 A.01»òÕßA.02£¬ÇëʹÓÃExternalIteration»òÕßSelfConsistent´úÌæStatespecificÑ¡ÏÒòΪºóÕßÓеãÎÊÌ⣬Èç¹ûÊÇG09 B.01£¬ÓÃÕâÈý¸öÑ¡ÏîÖ®Ò»¶¼ÐУ¬ÒâÒåÏàͬ¡£ =========================================== The "StateSpecific" approach in this context applies to the excited state, and yes it involves solving self-consistently the "fast" component of the solvent polarization for the target state and non-equilibrium solvation for the "slow" component of the solvent polarization (i.e. the "slow" component of the solvent polarization comes from the origin state). The total polarization is always partitioned into two components, "slow" and "fast". The "slow" part can be regarded as the reorganization of the solvent molecules as a response to a change in the electronic density of the solute. The "fast" part can be regarded as the response of the electrons in the solvent to a change in the electronic density of the solute. For a change in the electronic density of the solute such as a vertical electronic transition, the "slow" component of the polarization is much slower than the timescale of the electronic transition, so the solvent does not have time to respond in this way to the vertical electronic transition. The "fast" component of the polarization, on the other hand, is closer in timescale to the vertical electronic transition on the solute. In an equilibrium solvation calculation, both components are in equilibrium with the solute's density. By default, all ground state calculations assume equilibrium solvation, as well as geometry optimizations of excited states (and also any calculation that involves the computation of the relaxed density of the excited state). Again, in equilibrium solvation processes, both the "slow" and "fast" component of the solvent polarization are in equilibrium with the excited state density. In the case of a TD energy calculation (no excited state density or geometry optimization) for the computation of a vertical electronic excitation, the default is to do a non-equilibrium process. For this case then, the "fast" component of the polarization "responds" to the change in the solute density from ground to excited state, but the "slow" component did not have time to "respond" so it still comes from the one that was in equilibrium with the solute's ground state density. This is the case of both "Step 2" and "Step 3" in the example shown in the manual. In "Step 2", an energy calculation using TD is performed, thus it defaults to non-equilibrium solvation. The solvation effects on the excited states energies are computed by means of a linear response approach. The absorption energies via the linear response approach only are those reported directly in the output of this "Step 2" job. In "Step 3", a step further is taken and a correction of the linear response excitation energy is performed by solving the "fast" component of the solvent polarization self-consistently with the selected excited state density (the "State-Specific" approach). This is generally an improvement over the excitation energies obtained by linear response alone. Note that since this "State-Specific" approach involves the calculation of the excited state density, the program would default to doing an equilibrium solvation calculation on the excited state. However, the goal of "Step 3" is to compute the vertical excitation energy, so as mentioned above, we would like to use the "slow" component of the solvent polarization from the ground state calculation (in "Step 3", the first part does an equilibrium calculation on the ground state saving the solvent reaction field to the checkpoint file) and solving self-consistently the "fast" component with the excited state density (the second part of "Step 3" reads the reaction field from the checkpoint file, the one from the ground state calculation, keeps the "slow" component as is, and solves the "fast" component self-consistently with the excited state density). The absorption energy via the "State-Specific" approach is the energy difference between the excited state energy after all PCM corrections from the non-equilibrium calculation in "Step 3" and the ground state energy resulting from the equilibrium process (either first part of "Step 3" or final, optimized geometry, energy from "Step 1", the two ground state energies should be the same). In a TD geometry optimization of an excited state, since one is looking for the equilibrium geometry, the default is to do equilibrium solvation, so the two components, "slow" and "fast", of the polarization are in equilibrium with the solute's excited state density. All "Step 4", "Step 5" and "Step 6" use equilibrium solvation for the selected excited state. The emission energy (vertical energy of the excited to ground state transition) by means of a linear response approach can be found in the output of "Step 4". For the final (optimized) geometry in "Step 4", the "excitation energy" shown in this output would be equal to the emission energy since it is the result of an equilibrium calculation on the selected excited state. "Step 6" and "Step 7" are analogous to the two parts of "Step 3" but this time for the opposite transition (excited to ground states). Thus, "Step 6" is analogous to the first part of "Step 3", it is an equilibrium calculation on the origin state (now the excited state) in which both "slow" and "fast" components of solvent polarization are solved self-consistently with the excited state density (this calculation can be regarded as a correction of the excited state energy beyond the linear response approach, which was done in "Step 4" . Now, this "Step 6" saves the solvent reaction field to the checkpoint file. "Step 7" reads this information from the file (just like the second part of "Step 3" and performs a non-equilibrium calculation of the ground state energy, using the "slow" component of the solvent polarization from the excited state calculation ("Step 6" and only doing the "fast" component of the solvent polarization self-consistent with the ground state density. The emission energy via the "State-Specific" approach would be the energy difference between the excited state energy after all PCM corrections from "Step 6" and the ground state energy resulting from the non-equilibrium process in "Step 7". |

5Â¥2011-08-25 11:25:18
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4Â¥2011-08-24 10:18:13
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6Â¥2011-08-25 11:28:27
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7Â¥2011-08-26 09:30:24
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8Â¥2011-08-31 09:13:52
Illusionist
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9Â¥2011-11-28 23:55:37
Illusionist
Òø³æ (ÕýʽдÊÖ)
- Ó¦Öú: 20 (СѧÉú)
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- É¢½ð: 1001
- ºì»¨: 15
- Ìû×Ó: 431
- ÔÚÏß: 329.1Сʱ
- ³æºÅ: 1123329
- ×¢²á: 2010-10-15
- רҵ: °ëµ¼Ìå¾§ÌåÓ뱡Ĥ²ÄÁÏ
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10Â¥2011-11-29 12:42:52









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. Now, this "Step 6" saves the solvent reaction field to the checkpoint file. "Step 7" reads this information from the file (just like the second part of "Step 3"