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		<title><![CDATA[Multiwfn forum]]></title>
		<link>http://sobereva.com/wfnbbs/index.php</link>
		<description><![CDATA[The most recent topics at Multiwfn forum.]]></description>
		<lastBuildDate>Tue, 22 Sep 2026 03:48:37 +0000</lastBuildDate>
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		<item>
			<title><![CDATA[The G16 C.02 input files is not ran]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1877&amp;action=new</link>
			<description><![CDATA[<p>Dear Tian,<br />Thank you very much.</p><p>Sincerely,<br />Saeed</p>]]></description>
			<author><![CDATA[dummy@example.com (saeed_E)]]></author>
			<pubDate>Tue, 22 Sep 2026 03:48:37 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1877&amp;action=new</guid>
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		<item>
			<title><![CDATA[STEOM-DLPNO-CCSD for S1-T1 energy gap calculations input]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1876&amp;action=new</link>
			<description><![CDATA[<p>Dear Prof. Tian,<br />&#160; &#160; &#160;Thank you so much for your answer and new suggestions for e^T code. I shall try them. <br />Regards<br />Arivu</p>]]></description>
			<author><![CDATA[dummy@example.com (Arivu)]]></author>
			<pubDate>Sun, 20 Sep 2026 16:28:28 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1876&amp;action=new</guid>
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		<item>
			<title><![CDATA[NTOs Vs Hole-Electron Analysis in ORCA]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1875&amp;action=new</link>
			<description><![CDATA[<p>Dear Prof. Tian,<br />&#160; &#160; Got it. Thank you so much for your reply.&#160; <br />Regards<br />Arivu</p>]]></description>
			<author><![CDATA[dummy@example.com (Arivu)]]></author>
			<pubDate>Fri, 18 Sep 2026 17:08:24 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1875&amp;action=new</guid>
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		<item>
			<title><![CDATA[Atomic radii and solute cavity options for SMD]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1874&amp;action=new</link>
			<description><![CDATA[<p>1 You just need to use scrf=SMD, no additional keywords are needed.</p><p>2 For Br and I, I recommend to modify radii as mentioned in my blog article <a href="http://sobereva.com/613" rel="nofollow">http://sobereva.com/613</a>. For other elements, simply use the default radii in SMD should be OK.</p><p>For charged ions, uESE performs notably better than SMD, see <a href="http://sobereva.com/593" rel="nofollow">http://sobereva.com/593</a>. If you need better solvation energy of ions, using uESE instead is recommended.</p><p>3 I didn&#039;t take care of this parameter and thus cannot comment on it.</p>]]></description>
			<author><![CDATA[dummy@example.com (sobereva)]]></author>
			<pubDate>Sun, 13 Sep 2026 11:38:06 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1874&amp;action=new</guid>
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			<title><![CDATA[AdNDP on Orca output]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1873&amp;action=new</link>
			<description><![CDATA[<p>Hello,</p><p>Currently output file of ORCA+NBO is not officially supported by the AdNDP function in Multiwfn.</p>]]></description>
			<author><![CDATA[dummy@example.com (sobereva)]]></author>
			<pubDate>Sun, 30 Aug 2026 03:58:10 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1873&amp;action=new</guid>
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		<item>
			<title><![CDATA[Clarification regarding sobEDA.sh script and memory issues.]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1872&amp;action=new</link>
			<description><![CDATA[<p>Dear Professor,</p><p>Thank you for your efforts. I have executed the command for memory allocation, and it worked. </p><p>The calculation has completed successfully.</p><p>Best,<br />Gayathri</p>]]></description>
			<author><![CDATA[dummy@example.com (G_a_y_a_t_h_r_i7421)]]></author>
			<pubDate>Fri, 28 Aug 2026 06:10:32 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1872&amp;action=new</guid>
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		<item>
			<title><![CDATA[Permanent address of latest binary package and source code of Multiwfn]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1871&amp;action=new</link>
			<description><![CDATA[<p>For convenience, now the permanent address for accessing Multiwfn is available:</p><p>Latest Linux source code<br /><a href="http://sobereva.com/multiwfn/misc/Multiwfn_latest_src_Linux.zip" rel="nofollow">http://sobereva.com/multiwfn/misc/Multi … _Linux.zip</a></p><p>Latest Linux noGUI binary package<br /><a href="http://sobereva.com/multiwfn/misc/Multiwfn_latest_bin_Linux_noGUI.zip" rel="nofollow">http://sobereva.com/multiwfn/misc/Multi … _noGUI.zip</a></p><p>Latest Windows binary package<br /><a href="http://sobereva.com/multiwfn/misc/Multiwfn_latest_bin_Win64.7z" rel="nofollow">http://sobereva.com/multiwfn/misc/Multi … n_Win64.7z</a></p><br /><p>The addresses will not be changed, but the files will be automatically updated when new version of Multiwfn is released.</p>]]></description>
			<author><![CDATA[dummy@example.com (sobereva)]]></author>
			<pubDate>Sat, 22 Aug 2026 17:33:41 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1871&amp;action=new</guid>
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			<title><![CDATA[recent changes in CP2K]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1862&amp;action=new</link>
			<description><![CDATA[<div class="quotebox"><cite>Dirk wrote:</cite><blockquote><div><p>Sorry for the repeated request, but there is still a remaining issue with the input generated by multiwfn:</p><p> *******************************************************************************<br /> *&#160; &#160;___&#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160;*<br /> *&#160; /&#160; &#160;\&#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; *<br /> * [ABORT]&#160; The specified keyword &#039;TYPE&#039; is not available anymore: The keyword *<br /> *&#160; \___/&#160; &#160; MOTION/CELL_OPT/TYPE has been removed because cell optimizations&#160; *<br /> *&#160; &#160; |&#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160;now always use DIRECT_CELL_OPT.&#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; *<br /> *&#160; O/|&#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; *<br /> * /| |&#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; *<br /> * / \&#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160; &#160;input/input_parsing.F:262 *<br /> *******************************************************************************</p></div></blockquote></div><p>This issue has been solved in Multiwfn 2026.8.21</p>]]></description>
			<author><![CDATA[dummy@example.com (sobereva)]]></author>
			<pubDate>Fri, 21 Aug 2026 08:13:20 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1862&amp;action=new</guid>
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		<item>
			<title><![CDATA[File .47 options]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1859&amp;action=new</link>
			<description><![CDATA[<p>Thank you for your reply.</p>]]></description>
			<author><![CDATA[dummy@example.com (jimkress)]]></author>
			<pubDate>Fri, 21 Aug 2026 05:23:57 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1859&amp;action=new</guid>
		</item>
		<item>
			<title><![CDATA[NTOs for SF-TDA in ORCA]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1861&amp;action=new</link>
			<description><![CDATA[<p>Hello,</p><p>Unfortunately NTO is not supported for spin-flip case.</p>]]></description>
			<author><![CDATA[dummy@example.com (sobereva)]]></author>
			<pubDate>Thu, 06 Aug 2026 11:19:12 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1861&amp;action=new</guid>
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		<item>
			<title><![CDATA[Imaginary frequency with relativistic X2C Hamiltonian in ORCA6.1.1]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1856&amp;action=new</link>
			<description><![CDATA[<p>Dear Tian,<br />The attached file includes the final and seemingly reasonable and scientific justification for the observed low negative imaginary frequency for TlF3...CA complex. Such a justification is based on the PES scan exactly along the negative normal mode using Gview.<br />I would be highly grateful if you kindly have a look and let me know your opinion.</p><p>Sincerely,<br />Saeed</p><p><a href="http://sobereva.com/wfnbbs/uploads/71a0ce66099dfb0a1f63173f82bee60b.pdf" rel="nofollow">CRUCIAL_explanations2.pdf</a></p>]]></description>
			<author><![CDATA[dummy@example.com (saeed_E)]]></author>
			<pubDate>Wed, 05 Aug 2026 18:36:27 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1856&amp;action=new</guid>
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			<title><![CDATA[Multiwfn Failure to Read log file]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1860&amp;action=new</link>
			<description><![CDATA[<p>Please make sure that you are using the latest version of ORCA and Multiwfn. Old versions may have incompatible problem (ORCA frequently changes output format among different versions). If you are indeed using the latest versions, please send your ORCA output file to my E-mail, I will check.</p>]]></description>
			<author><![CDATA[dummy@example.com (sobereva)]]></author>
			<pubDate>Wed, 05 Aug 2026 07:03:28 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1860&amp;action=new</guid>
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			<title><![CDATA[IRI Interaction region indicator analysis for Excited States]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1857&amp;action=new</link>
			<description><![CDATA[<p>It is fully possible, the only requirement is that you should load wavefunction file corresponding to excited state into Multiwfn, please check <a href="http://sobereva.com/wfnbbs/viewtopic.php?id=306" rel="nofollow">http://sobereva.com/wfnbbs/viewtopic.php?id=306</a></p>]]></description>
			<author><![CDATA[dummy@example.com (sobereva)]]></author>
			<pubDate>Fri, 31 Jul 2026 01:47:25 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1857&amp;action=new</guid>
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			<title><![CDATA[RESP charges]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1855&amp;action=new</link>
			<description><![CDATA[<div class="quotebox"><cite>Ainosya wrote:</cite><blockquote><div><p>Hello,</p><p>I am not sure what you mean by G09 being unable to compute RESP charges. Both the ORCA and Gaussian09 manuals provide the necessary input to compute them.</p><p>For Gaussian09, the input is as follows:</p><p>```<br />#P HF/6-31G* Pop=MK IOp(6/33=2) IOp(6/41=15) IOp(6/42=15) IOp(6/50=1)<br /># Test Units(Ang,Deg)<br />```</p><p>I am also using the MK method with Multiwfn, yet there is still a large discrepancy compared to ORCA, which uses COSMO I believe</p></div></blockquote></div><br /><p>Please carefully look at Kollman&#039;s original paper of RESP charge (J. Phys. Chem., 97, 10269 (1993)), and relevant part of Multiwfn manual (Section 3.9.16). RESP charge is not a variant of ESP fitting charge just with additional constraints, but it defined specific fitting scheme. The so-called RESP charge in ORCA and Gaussian only enable users to manually set simple constraints, while it doesn&#039;t directly follow the full procedure of RESP charge fitting in Kollman&#039;s paper, so the results are not comparable.</p><p>Even for MK charges, which is one of the simplest ESP fitting charge, the results of Multiwfn and ORCA/Gaussian can also be detectably different even based one exactly the same wavefunction, because the spatial distribution of fitting points are not completely identical in these programs. ESP fitting charge is known to be sensitive to distribution and density of fitting points. In Multiwfn, the default density of fitting points is fine enough and can lead to basically converged result, and the point distribution strictly follows the original MK definition.</p>]]></description>
			<author><![CDATA[dummy@example.com (sobereva)]]></author>
			<pubDate>Fri, 17 Jul 2026 04:59:45 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1855&amp;action=new</guid>
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			<title><![CDATA[A very important question about http://sobereva.com/soft/adddiffuse]]></title>
			<link>http://sobereva.com/wfnbbs/viewtopic.php?id=1854&amp;action=new</link>
			<description><![CDATA[<p>Dear Tian,<br />Thank you very much.</p><p>Sincerely yours,<br />Saeed</p>]]></description>
			<author><![CDATA[dummy@example.com (saeed_E)]]></author>
			<pubDate>Thu, 16 Jul 2026 11:55:55 +0000</pubDate>
			<guid>http://sobereva.com/wfnbbs/viewtopic.php?id=1854&amp;action=new</guid>
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