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		<title><![CDATA[Multiwfn forum / UV/Vis absorption simulation of diradicals]]></title>
		<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1530</link>
		<description><![CDATA[The most recent posts in UV/Vis absorption simulation of diradicals.]]></description>
		<lastBuildDate>Thu, 12 Sep 2024 07:29:44 +0000</lastBuildDate>
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			<title><![CDATA[Re: UV/Vis absorption simulation of diradicals]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?pid=4602#p4602</link>
			<description><![CDATA[<p>Hi, my suggestion is to use the MRSF-TDDFT method in the free software package <a href="https://www.msg.chem.iastate.edu/gamess/download.html" rel="nofollow">GAMESS</a>. The SF-TDDFT method in ORCA/GAMESS suffers from the spin-contamination problem during practical calculations, while MRSF-TDDFT is almost exact spin-pure (whose spin-contamination can hardly be seen). It is very easy to perform an MRSF-TDDFT calculation. Here is an example:</p><p><strong>Step 1.</strong> perform an ROKS (i.e. RODFT) calculation<br />Open-shell ROKS calculations are usually not easy. It is recommended to use PySCF/Gaussian to perform this calculation. The <a href="https://github.com/pyscf/pyscf/" rel="nofollow">PySCF</a> input file is show below</p><div class="codebox"><pre class="vscroll"><code>from pyscf import gto, dft, lib
from mokit.lib.py2fch_direct import fchk

lib.num_threads(64)
mol = gto.M()
mol.atom = &#039;&#039;&#039;
C   -0.12264859        0.00599759       -0.75931820
C   -0.13393227        0.05086047        0.75572332
O    1.29017598        0.03740604       -0.91156021
O    1.12879647       -0.57344495        0.94545004
H   -0.54539878       -0.92543383       -1.16182063
H   -0.91791476       -0.55372886        1.23567184
H   -0.13429527        1.07605238        1.15229831
H   -0.56478278        0.88229116       -1.25644448
&#039;&#039;&#039;

mol.basis = &#039;aug-cc-pVDZ&#039;
mol.charge = 0
mol.spin = 2
mol.verbose = 4
mol.build(parse_arg=False)

mf = dft.ROKS(mol)
mf.xc = &#039;bhandhlyp&#039;
mf.grids.atom_grid = (99,590)
mf.max_cycle = 128
mf.max_memory = 128000 #MB
old_e = mf.kernel()

mo = mf.stability()[0]
dm = mf.make_rdm1(mo, mf.mo_occ)
mf.kernel(dm0=dm)

mf.stability()
fchk(mf, &#039;high_spin.fch&#039;, density=True)</code></pre></div><p>Submit the PySCF job</p><div class="codebox"><pre><code>python test.py &gt;test.out 2&gt;&amp;1</code></pre></div><p>Here <strong>fchk()</strong> is a module in the open-source package <a href="https://gitlab.com/jxzou/mokit" rel="nofollow">MOKIT</a>. To run this example, you need to install PySCF and MOKIT (which can both be installed via `conda install`).</p><p><strong>Step 2.</strong> transfer molecular orbitals (MO) and generate input files<br />After the PySCF job is accomplished, one obtains the wave function file high_spin.fch. Now run the following command</p><div class="codebox"><pre><code>fch2inp high_spin.fch -mrsf</code></pre></div><p>One obtains the file high_spin.inp, which contains MRSF-TDDFT keywords, Cartesian coordinates, basis set data and converged ROKS MOs.</p><p><strong>Step 3.</strong> perform the MRSF-TDDFT calculation<br />Run the following command</p><div class="codebox"><pre><code>/path_to_gamsss/rungms high_spin.inp 00 48 &gt;high_spin.gms 2&gt;&amp;1</code></pre></div><p>Here 48 CPU cores are used for parallel computations.</p>]]></description>
			<author><![CDATA[dummy@example.com (jxzou)]]></author>
			<pubDate>Thu, 12 Sep 2024 07:29:44 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?pid=4602#p4602</guid>
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		<item>
			<title><![CDATA[Re: UV/Vis absorption simulation of diradicals]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?pid=4601#p4601</link>
			<description><![CDATA[<p>The provided information is not enough to figure out the reason. BTW, using NEVPT2 would be more reliable. There is a CASSCF tutorial of ORCA on its website, you can consult it, which described in detail how to perform CASSCF and multireference calculations on transition metal complexes.</p>]]></description>
			<author><![CDATA[dummy@example.com (sobereva)]]></author>
			<pubDate>Thu, 12 Sep 2024 07:05:13 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?pid=4601#p4601</guid>
		</item>
		<item>
			<title><![CDATA[UV/Vis absorption simulation of diradicals]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?pid=4600#p4600</link>
			<description><![CDATA[<p>Hello, I am studying for the organometallic cobalt complex having diradical characteristics (experimentally observed).</p><p>The thing I want to do is simulation of UV-Vis absorption spectra simulation about singlet diradical organometallic compound.</p><p>Could I simulate that by using Orca and Multiwfn?</p><p>If possible, how can I set the keyword for the Orca? I tried spin-flip TDDFT calculation for the compounds but, it fails with a error message (Error: CSI/TDDFT) ... aborted.)</p><p>Here, my last trial of input files.</p><p>!B3LYP DEF2-SVP CPCM(acetonitrile) PAL8<br />%maxcore 8000<br />%TDDFT<br />SF TRUE<br />NROOTS 30<br />END<br />* xyz 3 1 Co.xyz *</p>]]></description>
			<author><![CDATA[dummy@example.com (zmfhtm2045)]]></author>
			<pubDate>Wed, 11 Sep 2024 18:27:08 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?pid=4600#p4600</guid>
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