From slee@ccl.net  Thu Dec  9 10:54:31 1993
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From: slee@ccl.net (Thomas Slee)
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Subject: Hypercube announces ChemPlus.
To: chemistry@ccl.net
Date: 	Thu, 9 Dec 1993 10:40:02 -0500
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aterloo, December 8, 1993

Hypercube is pleased to announce the release of ChemPlus, a set of
extensions for HyperChem.  ChemPlus requires HyperChem Release 3
for Windows, and has an introductory price of $395 US.

ChemPlus brings many new capabilities to HyperChem users.  Some of the 
major features include high-quality ball-and-stick images, 3D renderings 
of molecular orbitals, conformational searching, evaluation of Log P, 
of surface areas and of other indicators, automated building of 
sugars and crystals, amino acid sequence editing, and RMS overlay.

ChemPlus is closely integrated with HyperChem: it adds the individual
modules into the HyperChem menus for easy access and all programs use
Dynamic Data Exchange for smooth communication with HyperChem.

For more information, including a detailed description of ChemPlus's
features, contact us on Internet at info@hyper.com.

Hypercube, Inc.         419 Phillip Street, Waterloo, Ontario, N2L 3X2.
Phone:	(519) 725-4040                             FAX:  (519) 725-5193

From AZHARI@FRCU.EUN.EG  Thu Dec  9 11:54:36 1993
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Date: Thu, 09 Dec 1993 18:04:12 +0000 (O)
Subject: on-line CADPAC manual
To: chemistry@ccl.net
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Dear Netters:

Would you please if someone have an online manual for CADPAC VERSION 5.0 
to send it to me by e-mail. Thanks a lot. 

Adel

From mercie@med.cornell.edu  Thu Dec  9 13:42:41 1993
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Date: Thu, 9 Dec 1993 13:26:08 -0500 (EST)
From: Gustavo Mercier <mercie@med.cornell.edu>
Subject: ADF/DFT and 1st row d-d transitions
To: chemistry@ccl.net
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Hi, Netters!

May be somebody could shed some light in a simple test of DFT and 
transition metal complexes with rather poor results.

I am puzzled by the results obtained using ADF v. 1.0.2 (Aug. 1993):

I am attempting to reproduce calculations on the spectroscopy of
M(H2O)6 (+n), where M is a first row transition metal, and n varies
>from 2 to 3.

The geometry is Th (although, the highest compatible symmetry
available in ADF is D2h). This leaves the M-O, O-H, and M-O-H
as the only internal coordinates necessary to specify the whole system.
Th symmetry is forced through proper construction of the Z-mat. The
density is symmetry constrained up to D2h symmetry.The excited states are computed at the optimized ground state geometry.

I am using the II basis set (double zeta Slater functions with triple 
zeta for 3d orbitals in the metal), and the default xc functional
(implementaion of VWN parameterization of CA MC simulations of an 
electron gas). All computations are unrestricted, including those 
with singlet states for the purpose of proper comparison with the 
excited states. The frozen core approximation is used with the core
of the Metal corresponding to [Ne], so the 3s,3p electrons are also
part of the valence shell.

To speeds things: integration = 2.5 (lowest adequate accuracy for integrals),
scfconvergence 0.001, gconv = 0.01 with M-O and H2O geometries as initial
input corresponding to standard H2O geometry and M-O 1.95 - 2.15 Angstroms.

This is what I get:

	M	Configuration (&) 	   State	Energy (x 1000 cm-1)
 ----------------------------------------------------------------------------

	Cr+3      d3 t2g(3)                 4A1.g              0
                     t2g(2) eg              4Tx.g(?)     16.9  (17.4, 17.6)*

	Mn+2      d5 t2g(3) eg(2)           6A1.g              0
		  d5 t2g(4) eg              4Tx.g(?)     12.1  (18.9)

	Fe+3      d5 t2g(3) eg(2)           6A1.g              0
                     t2g(4) eg              4Tx.g(?)      9.7  (12.6)

        Co+3      d6 t2g(6)                 1A1.g              0
                     t2g(5) eg              1Tx.g(?)      9.7  (16.6, 18.9)

(&) In Th symmetry the nomenclature Eg/u Tg/u is retained, but in D2h
symmetry is reduced and Eg -> A1.g, with T2g -> B1.g + B2.g + B3.g. The
ground state orbital energies do show BX.g to have proper degeneracies.
Similarly, the two HOMO's in A1.g symmetry are degenerate.

(?) x=1 or 2 the exact definition of the state is unclear to me. See below
for the orbital occupation numbers.

(*) values in parenthesis are from Anderson et.al. Inorg. Chem. 1986, 25,
2728-2732. These are experimental results that a new version of INDO/S
is able to reproduce.

I am surprised that not even a qualitative trend is reproduced. Extensions
to include Stoll's correction or increase the basis set to add polarization
functions in the light atoms (Basis Set III) do not appear to improve the
situation.

Could you comment on these results? Are DFT methods inadequate to address
spectroscopy questions such as the levels of d-d transitions?
Do any HF based methods be adequate (e.g. HF/MP2, MCSCF etc)? We are
doing this work as a test of the reliability of computations we intend
to do on the spin density of metalloporphyrins and some Lanthanide complexes
that have not been parameterized within the INDO/S formalism.

Below I have reproduced the occupation numbers used in my calculations as
specified in ADF.  spin 1 // spin 2

     			Cr

A1.G	7 // 7 			A1.G	8 // 7 
B1.G	3 // 2			B1.G	3 // 2
B2.G	3 // 2			B2.G	2 // 2
B3.G	3 // 2			B3.G	3 // 2
A1.U	0 // 0			A1.U	0 // 0
B1.U	5 // 5			B1.U	5 // 5
B2.U	5 // 5			B2.U	5 // 5
B3.U	5 // 5			B3.U	5 // 5

			Mn

A1.G	9 // 7 			A1.G	8 // 7 
B1.G	3 // 2			B1.G	3 // 2
B2.G	3 // 2			B2.G	3 // 3
B3.G	3 // 2			B3.G	3 // 2
A1.U	0 // 0			A1.U	0 // 0
B1.U	5 // 5			B1.U	5 // 5
B2.U	5 // 5			B2.U	5 // 5
B3.U	5 // 5			B3.U	5 // 5

			Fe

A1.G	9 // 7 			A1.G	8 // 7 
B1.G	3 // 2			B1.G	3 // 2
B2.G	3 // 2			B2.G	3 // 3
B3.G	3 // 2			B3.G	3 // 2
A1.U	0 // 0			A1.U	0 // 0
B1.U	5 // 5			B1.U	5 // 5
B2.U	5 // 5			B2.U	5 // 5
B3.U	5 // 5			B3.U	5 // 5

			Co

A1.G	7 // 7 			A1.G	8 // 7 
B1.G	3 // 3			B1.G	3 // 3
B2.G	3 // 3			B2.G	2 // 3
B3.G	3 // 3			B3.G	3 // 3
A1.U	0 // 0			A1.U	0 // 0
B1.U	5 // 5			B1.U	5 // 5
B2.U	5 // 5			B2.U	5 // 5
B3.U	5 // 5			B3.U	5 // 5


Gus Mercier
mercie@cumc.cornell.edu

From PEARLMAN@VAX.PHR.UTEXAS.EDU  Thu Dec  9 14:54:26 1993
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Date:    Thu, 9 Dec 1993 13:34:13 -0600 (CST)
From: PEARLMAN@VAX.PHR.UTEXAS.EDU
Message-Id: <931209133413.508@VAX.PHR.UTEXAS.EDU>
Subject: how-to book on writing code for parallel platforms
To: CHEMISTRY@ccl.net
X-Vmsmail-To: SMTP%"CHEMISTRY@ccl.net"


In response to a recent inquiry:

A *very* good book discussing coding for parallel platforms is:
   B. Bauer, "Practical Parallel Programming," Academic Press, 1992.

It includes clear discussions of both introductory and advanced concepts.
It provides numerous examples of both FORTRAN and C code (not pseudo-code
but actual code which the user could compile and execute).  The book will
be useful regardless of hardware platform but will be particularly useful
to programmers working on Silicon Graphics hardware.

  --- Bob Pearlman



From ross@cgl.ucsf.EDU  Thu Dec  9 15:01:47 1993
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From: ross@cgl.ucsf.edu (Bill Ross )
To: chemistry@ccl.net
Subject: Re: van der Waals parameters


	Date: Thu, 09 Dec 1993 08:12:32 -0500
	From: nauss@ucmodl.che.uc.EDU (Jeffrey L. Nauss)
	Subject: Re:  van der Waals parameters
	To: ross@cgl.ucsf.EDU (Bill Ross )
	Message-id: <9312091312.AA19486@ucmodl.che.uc.edu>
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	Bill - 

	I disagree with your explanation of R and sigma.  Acoording to Moore
	in his book "Physical Chemistry" (4th edition) page 128, sigma for the
	Lennard- Jones potential is the value of r (distance) where the
	potential energy equals zero, i.e. where the curve crosses the x-axis
	other than where r approaches infinity.

	On the other hand, according to Hill in "Introduction to Statistical
	Thermodynamics", Appendix IV, pg 484, r* is the distance at the
	potential minimum.  Thus r* = sigma * 2^(1/6).


							Jeff Nauss

	************************************************************************
	*  Dr. Jeffrey L. Nauss             * Telephone: 513-556-0148          *
	*  Department of Chemistry          * Fax: 513-556-9239                *
	*  University of Cincinnati         * e-mail: nauss@ucmodl.che.uc.edu  *
	*  Cincinnati, OH 45221-0172        *                                  *
	************************************************************************

Since the combining rule for sigma is the same as it would be
for 2 * R*, and the sigmas in Allen & Tildesly p 21 look like
2 * R*'s, I apparently made a wrong assumption. Thanks to Jeff
Nauss for the correction.

Bill Ross

