2014
DOI: 10.7287/peerj.preprints.353v1
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A third-generation dispersion and third-generation hydrogen bonding corrected PM6 method: PM6-D3H+

Abstract: We present new dispersion and hydrogen bond corrections to the PM6 method, PM6-D3H+, and its implementation in the GAMESS program. The method combines the DFT-D3 dispersion correction by Grimme et al with a modified version of the H+ hydrogen bond correction by Korth. Overall, the interaction energy of PM6-D3H+ is very similar to PM6-DH2 and PM6-DH+, with RMSD and MAD values within 0.02 kcal/mol of one another. The main difference is that the geometry optimizations of 88 complexes result in 82, 6, 0, and 0 geo… Show more

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Cited by 18 publications
(22 citation statements)
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“…In this paper we benchmark the NMR chemical shift predictions on Ubiquitin and GB3. The structures are geometry optimized using PM6-D3H+ ( Kromann et al, 2014 ) using the PCM solvation model ( Tomasi, Mennucci & Cammi, 2005 ; Steinmann et al, 2013 ) and the CHARMM22/CMAP force field ( Mackerell, 2004 ) using the GB/SA solvation model ( Qiu et al, 1997 ) with the 1UBQ ( Vijay-Kumar, Bugg & Cook, 1987 ) and 2OED ( Ulmer et al, 2003 ) structures as starting points. The PM6-D3H+ optimizations are done using the GAMESS program ( Schmidt et al, 1993 ) with a convergence criterion of 5 × 10 −4 atomic units, while the CHARMM22/CMAP optimizations are done using TINKER ( Ponder & Richards, 1987 ) with the default convergence criterion of 0.01 kcal/mole/Å.…”
Section: Methodsmentioning
confidence: 99%
“…In this paper we benchmark the NMR chemical shift predictions on Ubiquitin and GB3. The structures are geometry optimized using PM6-D3H+ ( Kromann et al, 2014 ) using the PCM solvation model ( Tomasi, Mennucci & Cammi, 2005 ; Steinmann et al, 2013 ) and the CHARMM22/CMAP force field ( Mackerell, 2004 ) using the GB/SA solvation model ( Qiu et al, 1997 ) with the 1UBQ ( Vijay-Kumar, Bugg & Cook, 1987 ) and 2OED ( Ulmer et al, 2003 ) structures as starting points. The PM6-D3H+ optimizations are done using the GAMESS program ( Schmidt et al, 1993 ) with a convergence criterion of 5 × 10 −4 atomic units, while the CHARMM22/CMAP optimizations are done using TINKER ( Ponder & Richards, 1987 ) with the default convergence criterion of 0.01 kcal/mole/Å.…”
Section: Methodsmentioning
confidence: 99%
“…All energy terms are computed using gas phase geometries. ∆H f (X) is computed using either PM6 (Stewart, 2007) or PM6-D3H+ (Kromann et al, 2014) while ∆G • solv (X) is computed using either the SMD (Marenich et al, 2009) or COSMO (Klamt and Schüürmann, 1993) solvation method. The PM6-D3H+ and SMD calculations are performed with the GAMESS program (Schmidt et al, 1993), the latter using the semiempirical PCM interface developed by Steinmann et al (2013), while the COSMO calculations are performed using MOPAC2012.…”
Section: Computational Methodologymentioning
confidence: 99%
“…All energy terms are computed using gas phase geometries. ∆H f (X) is computed using either PM6 (Stewart, 2007) or PM6-D3H+ (Kromann et al, 2014) while ∆G • solv (X) is computed using either the SMD (Marenich et al, 2009) or COSMO (Klamt and Schüürmann, 1993) solvation method. The PM6-D3H+…”
Section: Computational Methodologymentioning
confidence: 99%