From BETTENS |-at-| MPS.OHIO-STATE.EDU Fri Dec 9 16:18:39 1994 Received: from ohstpw.mps.ohio-state.edu for BETTENS%!at!%MPS.OHIO-STATE.EDU by www.ccl.net (8.6.9/930601.1506) id PAA05980; Fri, 9 Dec 1994 15:32:23 -0500 From: Received: from MPS.OHIO-STATE.EDU by MPS.OHIO-STATE.EDU (PMDF V4.3-10 #5888) id <01HKG0JKZHI88Y55SS;at;MPS.OHIO-STATE.EDU>; Fri, 09 Dec 1994 15:32:15 -0500 (EST) Date: Fri, 09 Dec 1994 15:32:15 -0500 (EST) Subject: Open shell hydrocarbons, AM1 ROHF versus UHF To: chemistry _-at-_)ccl.net Message-id: <01HKG0JL2P8Y8Y55SS -8 at 8- MPS.OHIO-STATE.EDU> X-VMS-To: IN%"chemistry /at\ccl.net" MIME-version: 1.0 Content-type: TEXT/PLAIN; CHARSET=US-ASCII Content-transfer-encoding: 7BIT Dear Netters, Thanks to those of you who responded to my last posting on the 14th of November regarding spin contamination. Before summarizing these responses I would like to ask one further question which is related to my last question in the previous posting. I will then compile all responses and post a summary. My question concerns ROHF versus UHF calculations using the AM1 semiempirical model. Is anybody aware of any published work which recommends the use of either in calculating heats of formation, specifically for hydrocarbon open shell species? I have examined the original paper of Dewar, M.J.S.; Zoebisch, E.G.; Healy, E.F. and Stewart, J.J.P., J. Am. Chem. Soc., 107 (1985) 3902 where AM1 was introduced. In this work the heats of formation of 6 hydrocarbon radicals (all doublets) where compared with the experimental values. I could find no indication as to whether the reported calculations used the UHF or ROHF approaches. This is important because the calculated heats for each approach produces significantly different results. I consequently repeated the calculations on the 6 hydrocarbon radicals given in the above paper and found the following heats of formation (kcal mol^{-1}). I also give the values of S^2 and the reported heats as well as the current experimental values (from J. Phys. Chem. Ref. Data, 17 (1988) Sup. 1) for comparison below. AM1 AM1 Reported UHF S^2 ROHF AM1 Exp. Exp. - Calc.(ROHF) CH3 29.95 0.7613 31.25 31.25 34.8(3) 3.6 C2H3 60.46 0.8589 64.78 64.78 63.4(10) -1.4 C2H5 15.49 0.7619 18.14 15.48 28 10 CH2CHCH2 30.20 0.9300 38.58 38.58 39 0 (CH3)2CH 3.61 0.7622 6.80 10.07 22.3(6) 15.5 (CH3)3C -6.14 0.7623 -2.66 -2.66 11.0(6) 13.7 For C2H5 the authors seem to have reported the UHF value. I was not able to reproduce the reported result for (CH3)2CH with either the ROHF or the UHF result. I was able to reproduce the calculated heat of formation for this species given by Dewar, M.J.S. and Thiel, W., J. Am. Chem. Soc., 99 (1977) 4907, using the MNDO Hamiltonian. In this earlier work the authors explicitly stated that they used ROHF heats of formation calculated with MNDO. It is noted that for the remaining species the reported AM1 heats of formation also appear to be the ROHF values. While agreement with the experimental values are not terrific and appear particularly bad for the larger saturated hydrocarbon species, they are adequate for my purposes given that these errors can be taken as typical for calculated heats of formation of analogous but larger open shell hydrocarbon radicals. Does anybody know of any further studies, using the AM1 Hamiltonian, on radicals where the calculated heats of formation have been compared with experiment? It seems to me, from the above table, that the UHF results are not useful in comparison with the ROHF results, and that the extent of spin contamination tends to increase with molecular size and unsaturation, being close to 0.75 for the most saturated species. For instance, I repeated the calculation on triplet linear C19 given by Novoa et al., Inorganica Chemica Acta 198-200 (1992) 133, using UHF and ROHF. I obtained the same heat of formation as these authors with no assumed symmetry in the linear chain and using the UHF AM1 Hamiltonian. However, I obtained an S^2 of 4.356 (should be 2) and a ROHF heat of formation of 678.72 kcal mol^{-1}, which is greater than the UHF value by 24.17 kcal mol^{-1}! I would very much appreciate any helpful comments or literature references which deals with any of the above issues I've raised here about AM1 and its applicability of open shell systems. Regards, Ryan Bettens, OSU Physics Department, BETTENS.,at,.MPS.OHIO-STATE.edu