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Date: Mon, 31 Oct 1994 15:08:00 +0900
From: Jerzy Rudzinski  <jerzy@fqs.fujitsu.co.jp>
Message-Id: <199410310608.PAA27456@fqs.fujitsu.co.jp>
To: chemistry@ccl.net
Subject: Summary - quadrapole moments



ORIGINAL MESSAGE:
>
> Dear Friends,
>
> I would very much appreciate receiving pointers to the public domain or
> commerial software that can calculate (after optization of the structure)
> quadropole moments of sizable molecules (about 100 atoms).
> Thank you!  With the best wish, Jerzy Rudzinski
>
===========================================================================

>>From: peon@medchem.dfh.dk (Per-Ola Norrby)
>>Subject: Re: CCL:quadrapole moments

        Jerzy,
        This can be done by Gaussian92, using a semi-empirical Hamiltonian
(eg, AM1).  It's far from public domain, academic price is approx. $2000.
It runs on any number of workstations and supercomputers.  More information
can be obtained by mailing info@gaussian.com

        Per-Ola Norrby

 *  Per-Ola Norrby
 *  The Royal Danish School of Pharmacy, Dept. of Med. Chem.
 *  Universitetsparken 2, DK 2100 Copenhagen, Denmark
 *  tel. +45-35376777-506, +45-35370850    fax +45-35372209
 *  Internet: peon@medchem.dfh.dk
===========================================================================
>>From: salahub@ERE.UMontreal.CA (Salahub Dennis)
>>Subject: CCL:quadrapole moments (fwd)
 
Density Functional Methods should be able to handle this problem, although
it would be demanding.  Since I see you are at Fujitsu, I might assume that
you can find substantial computer power...
The optimization step would be the most costly.  IF it were possible to
optimize with molecular mechanics or a semiempirical scheme, then fixed
geometry DFT would be far less costly.
You could try any one of several programs.  DGAUSS (from Cray...),
deMon (our program), DEFT (Alain St-Amant at the University of Ottawa)
for the Gaussian family. (Also GAUSSIAN, CADPAC etc. but I don't think
they can do 100 atoms, because the coulomb part is done exactly, with
all the integrals, whereas DGAUSS etc. use fits to auxiliary basis
functions), DMOL (from Biosym) uses numerical atomic orbitals; the folks
at Biosym MIGHT(?) like the challenge??..., ADF from Evert-Jan Baerends'
group in Amsterdam can use Slater orbitals and also numerical or gaussian
functions.
It might be worth checking some of these out on smaller molecules related
to those that interest you, before tackling the 100-atom cases.
Good luck!
-Dennis Salahub
--
************************************************************
*   Dennis Salahub               SALAHUB@ERE.UMONTREAL.CA  *
*   Departement de chimie        Tel. (514) 343-6755       *
*   Universite de Montreal       Fax  (514) 343-2468       *
*   C.P. 6128, Succ. Centre-ville                          *
*   Montreal, Quebec  H3C 3J7                              *
*   Canada                                                 *
************************************************************
 

===========================================================================
>>From: monge@anny.psgvb.com (Alessandro Monge)
>>Subject: Re: CCL:quadrapole moments

Dear Jerzy,
 
Schrodinger's ab initio quantum chemistry code, PS-GVB, allows the
calculation of multipole moments, from dipole through hexadecapole.
Geometry optimization can be carried out at the HF and HF/GVB level
with substantial CPU time savings as compared to any existing
commercial quantum chemistry program.  Timing advantages are in the
order of 5-10 with respect to Gaussian92 for large molecules,
depending upon basis set and machine.
 
PS-GVB uses novel numerical technology (based on Pseudo-Spectral
methods, originally developed for hydrodynamic simulations of
turbolence) involving both basis sets and numerical grids to solve the
equations of electronic structure theory.  PS-GVB is capable of
performing calculations involving up to 200 atoms, 5000 basis
functions, 50 GVB pairs for GVB calculations and is available on a
variety of platforms.
 
  
Alessandro Monge
 
------------------------------------------------------------------------
Alessandro Monge                      Schrodinger, Inc.
monge@psgvb.com                       (800) 20-PSGVB
 
=========================================================================
>>From: Wolfgang Sauer <sauer@organik.uni-erlangen.de>
>>Subject: Re: CCL:quadrapole moments

Dear Jerzy Rudzinski,
 
our semiempirical program package VAMP will give you electrical multipoles
up to currently octupoles. They are usually used e.g. to fit NAO point charges
to give the best representation of a molecule's ESP, or as property descriptors
in QSAR studies with our program Tsar through a transparent interface.
 
The only limit for the size of your molecular system lies in your hardware;
I myself use Vamp routinely on small peptides of about 100 heavy atoms (plus
ca. 100 hydrogens) on modern workstations without problem.
 

If you would like to get more information on Vamp or have some other questions,
please do not hesitate to contact either me or our distributor in Japan.
 
All the best,
                Wolfgang Sauer.
--
 
        Wolfgang Sauer                        ------------
                                             | ##  ##  ## |
        Oxford Molecular - CCC               |  ## ## ##  |
        Naegelsbachstr. 25                   |   ######   |
        D-91052 ERLANGEN, FRG                |     ##     |
                                             |     ##     |
        Tel : +49 9131 8796  0               |    ####    |
        Fax : +49 9131 8796 11                ------------
===========================================================================
 
 



From CHUCK@psipsy.uct.ac.za  Mon Oct 31 04:10:19 1994
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To: sling@euclid.chem.washington.edu (Song Ling), chemistry@ccl.net
From: "Marais, Charles F. "  <CHUCK@psipsy.uct.ac.za>
Date:         Mon, 31 Oct 1994 10:20:22 SAST-2
Subject:      Re: CCL:100% parallel MD
Priority: normal
X-mailer:     WinPMail v1.0 (R1)


> Will the
> -dt, dt approach generate the "same" trajectory as the 2dt one if the
> system is sensitive to initial conditions? 

This is very interesting.  Has much work been done on chaos in MD ? 
 Any pointers would be much appreciated.

C

Dr Charles Marais


Department of Chemistry
University of Cape Town
Private Bag
Rondebosch                                  chuck@uctvax.uct.ac.za
South Africa 7700                           chuck@psipsy.uct.ac.za
------------------------------------------------------------------

















From Bernd.Hartke@RUS.Uni-Stuttgart.DE  Mon Oct 31 04:22:26 1994
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Subject: looking for graphics software
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Date: Mon, 31 Oct 1994 10:12:21 +0100 (MEZ)
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Dear CCL readers,

our group of ab initio quantum chemists is looking for a suitable
graphics software that fits our particular needs: We want
- good 2D contour plots (including a really working labeling mechanism
  for contour lines),
- 3D renderings of potential energy surfaces (perspective, hidden line, etc.,
  but no fancy stuff),
- perhaps also 3D isosurfaces, but this is not a must,
- simple ball-and-stick plots of molecules and clusters (or the possibility
  to create these by a few simple steps),
- of course simple x,y-graphs etc.,
- publication-quality laser printer output (postscript)
All this should be realized as a subroutine library directly callable from
our own Fortran programs. And it need not be public domain; we are actually
willing to pay for it.
We do NOT need/want (and hence do not want to pay for):
- a black-box system,
- an elaborate graphical user interface,
- complicated, high-power graphics tools like photographic or video image
  processing, etc.
For example, to name a few real-life products, a full-blown AVS or IDL
package simply contains too many beautiful features we will never use;
something like CA-DISSPLA would be more in our line; while GNUPLOT has
a few shortcomings.
We would like the graphics to run on HP735, Sun SPARC, and possibly Silicon
Graphics machines.

Any recommendations, hints, and your own positive or negative experiences
are highly welcome!

Bernd Hartke

-- 
Dr. Bernd Hartke                  e-mail: bernd.hartke@rus.uni-stuttgart.de
Dep. of Theoretical Chemistry     e-mail: bxh@wiffin.chem.ucla.edu
University of Stuttgart           
Pfaffenwaldring 55                Phone: +49-711-685-4409
70569 Stuttgart                   FAX:   +49-711-685-4442
GERMANY

From winn@tph12.tuwien.ac.at  Mon Oct 31 05:22:27 1994
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	(1.37.109.4/16.2) id AA17053; Mon, 31 Oct 94 10:52:27 +0100
From: Martyn Winn <winn@tph12.tuwien.ac.at>
Subject: CCL:100% parallel MD 
To: chemistry@ccl.net
Date: Mon, 31 Oct 94 10:52:27 MEZ
Mailer: Elm [revision: 70.85]


Two points:
1) My impression is that there is much work devoted to
chaotic trajectories for small molecules (i.e. with a
small no. of degrees of freedom) but that the issue is
ignored for MD simulations of bulk systems. This is, of
course, purely for reasons of convenience.
2) If one is in a chaotic regime, then I'm sure that
the -dt, dt trajectory will differ from the 2dt trajectory,
but taken individually each would be a perfectly valid
trajectory. There would be no reason to prefer one over
the other. In fact, a chaotic trajectory is surely ideal
to satisfy the ergodic requirements of most MD simulations.

I wonder if anyone is answering the original question
about efficiency?!

Martyn Winn

--
***************** Dr. Martyn Winn **************************************
 \                                                                    /
  \ Institut fuer Theoretische Physik, Technische Universitaet Wien, /
   \  Wiedner Hauptstrasse 8-10, A-1040 Wien, Austria.              /
    \____                                                          /
         \      Tel: +43 1 58801 5678                             /  
          \     Fax: +43 1 5867760                               /
           \    E-mail: winn@tph12.tuwien.ac.at                 /
            \   URL: http://tph.tuwien.ac.at/~winn/me.html     /
             --------------------------------------------------

From CHMIGORN@NUSVM.NUS.SG  Mon Oct 31 06:22:28 1994
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From: "I.Novak" <CHMIGORN%NUSVM.BITNET@phem3.acs.ohio-state.edu>
Subject: VIEWERS FOR GAUSSIAN
To: CHEMISTRY@ccl.net
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Dear Netters,
here is the summary of responses received so far:
a) XMol available from anonymous ftp.msc.edu   pub/xmol
   Runs on Sun. Contact D.C.Doherty   doherty@msc.edu
 
b) Sybyl 6.1 supports G92 and runs on Sun
 
c) AMPAC GUI will manipulate G92 files and runs on Sun
   contact: Semichem Inc.  Dr A.Holder   aholder@CCTR.UMKC.EDU
 
Thanks to all who answered!
I.Novak    chmigorn@nusvm

From dimitris@3dp.com  Mon Oct 31 10:23:55 1994
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Does anyone know Peter Willett's e-mail address at the University of Sheffield
in the UK? Thanks for your help.



-- 
Dimitris K. Agrafiotis, PhD             | e-mail: dimitris@3dp.com
3-Dimensional Pharmaceuticals, Inc.     | tel:    (215) 222-8950
3700 Market Street                      | fax:    (215) 222-8960
Philadelphia, PA 19104



From dimitris@3dp.com  Mon Oct 31 10:28:15 1994
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Does anyone know Peter Willett's e-mail address at the University of Sheffield
in the UK? Thanks for your help.



-- 
Dimitris K. Agrafiotis, PhD             | e-mail: dimitris@3dp.com
3-Dimensional Pharmaceuticals, Inc.     | tel:    (215) 222-8950
3700 Market Street                      | fax:    (215) 222-8960
Philadelphia, PA 19104



From dimitris@3dp.com  Mon Oct 31 10:29:54 1994
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Does anyone know Peter Willett's e-mail address at the University of Sheffield
in the UK? Thanks for your help.



-- 
Dimitris K. Agrafiotis, PhD             | e-mail: dimitris@3dp.com
3-Dimensional Pharmaceuticals, Inc.     | tel:    (215) 222-8950
3700 Market Street                      | fax:    (215) 222-8960
Philadelphia, PA 19104



From dimitris@3dp.com  Mon Oct 31 10:31:34 1994
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Date: Fri, 28 Oct 1994 17:14:23 -0400
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Subject: Need C/C++ libraries for clustering
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I am looking for public/commercial C/C++ libraries for clustering large
amounts of multidimensional data. Your help would be greatly appreciated.
I will summarize and submit the responses to the list. Thanks for your
help.



-- 
Dimitris K. Agrafiotis, PhD             | e-mail: dimitris@3dp.com
3-Dimensional Pharmaceuticals, Inc.     | tel:    (215) 222-8950
3700 Market Street                      | fax:    (215) 222-8960
Philadelphia, PA 19104



From KEWISE@aardvark.ucs.uoknor.edu  Mon Oct 31 10:33:19 1994
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From: <KEWISE@aardvark.ucs.uoknor.edu>
Message-Id: <199410311423.JAA28673@www.ccl.net>
Date: Mon, 31 Oct 94 08:24 CST
Subject: Convergence in MOPAC C.I. calculations
To: CHEMISTRY@ccl.net
X-VMS-To: IN%"CHEMISTRY@ccl.net"


Hello,

I am using MOPAC 6.0 to do calculations on fairly large polycyclic
molecules related to porphyrins.  Part of this work involves optimizing
geometries and calculating energies for the cations and anions of these
molecules.  To make these calculations more accurate (hopefully) we are
using the configuration interaction options in MOPAC 6, but have encountered
some problems with convergence.  After reducing the gradient to below 1.0,
the optimization begins to oscillate, and shows no sign of convergence
after running for several hours.  A typical command line is as follows:

AM1 PRECISE CHARGE=-1 C.I.=(4,2) VECTORS NODIIS

We have also tried the eigenvector following converger with similar results.
If anyone has had experience with a similar problem, I would appreciate any
advice that you could provide on this subject.  The manual is a bit brief
on both configuration interaction calculations and convergence problems, so
I thought I might try here.  You can mail me directly and I will summarize
the responses to the list if there is interest.  Thanks in advance....

Kristopher Wise
University of Oklahoma
Department of Chemistry and Biochemistry
KEWISE@aardvark.ucs.uoknor.edu

From noy@tci005.uibk.ac.at  Mon Oct 31 10:34:53 1994
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From: noy@tci005.uibk.ac.at (Noy)
Message-Id: <9410311437.AA23668@tci005.uibk.ac.at>
Subject: 100% parallel MD (1st Summary)
To: chemistry@ccl.net
Date: Mon, 31 Oct 1994 15:37:53 +0100 (NFT)
Cc: supot@atc.atccu.chula.ac.th (Dr. Supot Hannongbua),
        nan@atc.atccu.chula.ac.th (Anan Tongra-ar), ypp@tci002.uibk.ac.at
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Dear fellows,
	Thanks a lot for your kind suggestions and comments.
I have summarized the response. All of the responses
will be posted on the next mail.
	Many responses  state that the connection of two MD trajectories
are in doubt, due to numerical error in integrating schemes. Some of
them believe that the reversibility of velocity is disturbed by the
coupling with Thermo-bath and the cut-off of the potential. However, a
few people agree on this idea. 
	My point of view is that the structural properties obtained
from connecting two MD trajectories are the same as running one MD
double time.
                                t0------------->t1
             t2 <---------------t0

             and
                                t0--------------------------------->t1

	If we look at the phase space (p,q)

      p
         |
         |          ta \
         |              \
         |                 \
         |                    \                  ....... t1
         |                      \ t0  ......./
         |                     ....+ 
         |                   /
         |            ...../
         |          *'
         |         t2
         |
         |___________________________________________  q          

        Well, I start equilibrating the system from the time ta up to
the time t0, which I am sure it is an equilibrium state. Then at this
point, I traditionally perform a simulation from time t0 to the time t1.
At the time t0, I revert the sign of all velocities and simulate in
parallel up to the time t2. I believe that both of the trajectories
from the time t0--->t1 and t0--->t2 are in equilibrium state. So, the
phase space should be expored correctly, isn't it ? The statistical
average shoud be, hence, conserved.
        If I revert all momentum back again from the time t2--->t0, then
two trajectories are connected to produce one longer run. My purpose
is to have longer time-correlation rather than having more statistical
samples. So, I must be sure that this is correct or not. Many people
are in doubt that the reconnection of two MD is invalid. I would like
to ask some comments if it is possible or not that ......

        Since the prediction of the next coordinates and velocities are
respective to the current (t) and the former (t-1) one. If I have this
in hand       t, t-1 and t+1        t = t0
        I integrate forwardly from  t0 ----> t1 using  t-1 as the previous
step and I integrate backwardly from t0----> t2 using  t+1 as the previous
step. Do you think the connectiong is smooth and neat ?
        As stated by many people that the past of the trajectory is lost
due to the numerical error in integration scheme, I would believe so.
Anyway, if both trajectories are still in the equilibrium state, they
should represent the phase space correctly. 
        Some ideas ?
                                                      my best regards,
                                                        Teerakiat
----------------------------------------------------------------------------
Teerakiat Kerdcharoen (NOY)

Institute of General and Inorganic and Theoretical Chemistry
Innrain 52a, A-6020 Innsbruck AUSTRIA
e-mail:  noy@tci2.uibk.ac.at, noy@tci.uibk.ac.at, c72454@cx.uibk.ac.at 
      :  noy@atc.atccu.chula.ac.th, noy@atc2.atccu.chula.ac.th ( Bangkok )
Research :  Molecular Dynamics simulations
         :  Computer Aided Molecular/Material Designs
-----------------------------------------------------------------------------
***  I have no past and no future. I just have today.


From rsefeck@watson.ibm.com  Mon Oct 31 12:22:32 1994
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Date: Mon, 31 Oct 94 11:43:36 EST
To: chemistry@ccl.net
Subject: J.P.Stewart number


 Does anyone know how to get in touch with Dr. J. P. Stewart?(MOPAC)
 I understand he is no longer at the Airforce Labs and that he may be at
 Fujitsu.
 But with 4 separate phone calls to Fujitsu no one has heard of him.
 Any help would be appreciated.
 Rich Sefecka
 IBM Watson Labs
 email me direct at RSEFECK@watson.ibm.com
 thanks


From kottalam@rhea.cray.com  Mon Oct 31 12:27:12 1994
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From: kottalam@rhea.cray.com (Jeyapandian Kottalam)
Message-Id: <9410311652.AA04798@wake.cray.com>
To: chemistry@ccl.net
Subject: Re:  CCL:100% parallel MD


> From: Martyn Winn <winn@tph12.tuwien.ac.at>
> 
> I wonder if anyone is answering the original question
> about efficiency?!

  I think the efficiency question did not evoke much discussion
because everyone would agree with the theoretical 100% parallelism.
However, the time-parallelism is not very interesting because it
is strictly limited to a factor of 2.  From the Massively Parallel
point of view, we would like to have scalability to 500 to 1000
processors even with slightly less than 100% parallelism.
  This factor of 2 limitation is in addition to (or in spite of)
the chaotic nature of MD trajectories.

Kottalam                           Phone: (USA) 612 683 3622
Cray Research, Inc.

From sunger@crl.com  Mon Oct 31 12:30:17 1994
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Date: Mon, 31 Oct 1994 08:23:22 -0800 (PST)
From: Stefan Unger <sunger@crl.com>
To: Dimitris Agrafiotis <dimitris@3dp.com>
Cc: chemistry@ccl.net
Subject: Re: CCL:Need C/C++ libraries for clustering
In-Reply-To: <9410281714.ZM10482@europa.3dp.com>
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You might try contacting Daylight Chemical (Irvine, CA).  They have worked
on just this problem.  Call Yossi Taitz 714-476-0451.  
Good luck.
Stefan

On Fri, 28 Oct 1994, Dimitris Agrafiotis wrote:

> I am looking for public/commercial C/C++ libraries for clustering large
> amounts of multidimensional data. Your help would be greatly appreciated.
> I will summarize and submit the responses to the list. Thanks for your
> help.
> 
> 
> 
> -- 
> Dimitris K. Agrafiotis, PhD             | e-mail: dimitris@3dp.com
> 3-Dimensional Pharmaceuticals, Inc.     | tel:    (215) 222-8950
> 3700 Market Street                      | fax:    (215) 222-8960
> Philadelphia, PA 19104
> 
> 
> 
> ---Administrivia: This message is automatically appended by the mail exploder:
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> 
> 

From jshaffer@anemone.usc.edu  Mon Oct 31 13:22:35 1994
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From: J Scott Shaffer <jshaffer@anemone.usc.edu>
Message-Id: <199410311803.KAA22945@anemone.usc.edu>
To: chemistry@ccl.net
Subject: Re: 100% parallel MD
Reply-To: jshaffer@che1.usc.edu



In my previous post, I botched the graph.  The phase point would be
reflected through Q=0 upon reversing the velocities, giving something
like: 


             P
              |          
              |          
              |     ta \
              |         \
              |           \
              |             \                t1
              |               \ t0  ......./
              |              ....+ 
              |              /
              |       ...../
              |     *'
              |    t2
              |
______________|___________________________________ Q
              |
              |
              |
              |
              |
              |
              |                 t0'
              |                .
              |               .
              |       t2'      .
              |        .      .
              |          .....
              |
              |
              |



Sorry for the wasted space.

Scott




From jshaffer@anemone.usc.edu  Mon Oct 31 13:24:08 1994
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From: J Scott Shaffer <jshaffer@anemone.usc.edu>
Message-Id: <199410311750.JAA22939@anemone.usc.edu>
To: chemistry@ccl.net
Subject: Re: 100% parallel MD (1st summary)
Reply-To: jshaffer@che1.usc.edu



Dear Dr. Kerdcharoen:

I have entered this discussion a little late, but here goes.  Song
Ling has presented these arguments earlier; here they are again in a
slightly different form.

Let's talk only about integrating Newton's equations, yielding MD
simulations in the NVE ensemble.  There are two points to be made:

(1) Disregarding numerical error in the time integration, to generate
    continuous trajectories, one must reverse the sign of the time
    step, dt ----> -dt, keeping the same values of the positions *and*
    velocities.

    Correct time correlation functions cannot be obtained by reversing
    the signs of velocities and connecting the two resulting
    trajectories.  By reversing the velocities, you change the
    location of the system in phase space, as illustrated below, by
    reflecting the momenta through the P=0 axis.  Thus, any time
    correlation functions that are calculated by joining the two
    trajectories would be incorrect, since the trajectories are not
    continuous in phase space.


The phase space (Q,P): The points ta, t0, t1, and t2 are those plotted
by Dr. Kerdcharoen in his first summary.  The point t0' is the phase
point obtained by reversing the velocities of the system at point t0;
the point t2' is the final location of the system in phase space after
integrating Newton's equations from point t0'.

                             P
                              |          
                              |          
                              |     ta \
                              |         \
                              |           \
                              |             \                t1
             t0'              |               \ t0  ......./
  t2'         .               |              ....+ 
    . .       .               |              /
       . .     .              |       ...../
         . . . .              |     *'
                              |    t2
                              |
______________________________|___________________________________ Q



(2) With numerical error in the integration of the equations of
    motion, no trajectory is reversible in practice.  This is
    illustrated nicely in Figure 3.1 of Allen and Tildesley, "Computer
    Simulation of Liquids", where they show that trajectories that
    should in principle be identical actually diverge from each other
    rapidly because of numerical error in the time integration.  

    This is not necessarily a problem in terms of calculating ensemble
    averages from MD.  In fact, if one were to use the dt ----> -dt
    reversal described in (1), this numerical error would be
    *essential*, otherwise you would end up back in the unequilibrated
    starting configuration!

Scott

=====================================================================
 J. Scott Shaffer                       jshaffer@che1.usc.edu
 Department of Chemical Engineering     
 University of Southern California      (213) 740-2067
 Los Angeles, CA  90089-1211  USA       (213) 740-8053 (FAX)
=====================================================================




From topper@cooper.edu  Mon Oct 31 13:25:17 1994
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From: Robert_Topper <topper@cooper.edu>
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To: CHEMISTRY@ccl.net, noy@tci005.uibk.ac.at
Subject: Re: CCL:100% parallel MD
Content-Length: 6112


BANDWIDTH ALERT:
A LONG discussion on chaos in molecular systems follows.
I hope that some find it interesting. - robert
>
> Two points:
> 1) My impression is that there is much work devoted to
> chaotic trajectories for small molecules (i.e. with a
> small no. of degrees of freedom) but that the issue is
> ignored for MD simulations of bulk systems. This is, of
> course, purely for reasons of convenience.

Yes and no...certainly most work in nonlinear dynamics and chaos
of MD trajectories has concentrated on small molecular models at fixed E,
but not simply for "reasons of convenience."  The fact of the
matter is that there remains a lot to learn about nonlinear
dynamics in conservative Hamiltonian systems, esp. in high-dimensional
spaces. There are nonlinear phenonema that only occur in systems
with dimension >/= 3 (ex: Arnold diffusion)...plus the beautiful
visualization tools suggested by Poincare (Poincare maps, or
"surfaces of section") are not unique phase-space maps in
>/= 3 dimensions.  Progress into understanding chaos in "big"
systems has been slow (but see recent papers in Physica D and JCP
for counterexamples). I personally believe that the problems
are less numerical than fundamental, and more basic theory needs
to emerge to make some progress.  Song Ling has just authored a series
of interesting papers on HCN isomerization and chaos (although he's
too modest to tell you so). I did my thesis research in this area.
I'd be glad to steer those who are interested towards a few key papers.

> 2) If one is in a chaotic regime, then I'm sure that
> the -dt, dt trajectory will differ from the 2dt trajectory,
> but taken individually each would be a perfectly valid
> trajectory. There would be no reason to prefer one over
> the other. In fact, a chaotic trajectory is surely ideal
> to satisfy the ergodic requirements of most MD simulations.
>
> I wonder if anyone is answering the original question
> about efficiency?!

Martyn has an excellent point. The "practical" consideration for those
interested in getting at the NVT or NpT ensembles (either directly
or otherwise) is: am I sampling "properly" and "completely" (i.e.,
does my sample accurately represent the statistical properties of
the distribution function I'm trying to mimic, and do I have enough
configurations)?  This doesn't necessarily mean that the trajectory
needs to be DYNAMICALLY correct...if you want only THERMODYNAMIC
properties. However, if you also want dynamic properties (autocorrelation
functions?), the distinction between a (-dt,dt) trajectory and a
(0,2t) trajectory could be relevant. I think this should be ironed
out before sweating out how to make the calculation efficient.  

That said, I personally don't believe that whether the trajectory 
is chaotic or not is relevant here. The Lyapunov exponent for the 
starting point in phase space will give the same "divergence rate" 
whether one integrates asymmetrically (0,2t) or symmetrically (-t, t)...
either numerically generated trajectory is just as "wrong" 
(or just as "right" depending on your point of view).  Chaos theory
tells us that it's fundamentally impossible to exactly GENERATE a
chaotic trajectory...unless you computer carries an infinite number
of significant figures.  Fundamentally, your ability to back-integrate 
on the interval (2t,0) is going to be just as poor (or good) as your 
ability to back-integrate (t,-t). If the trajectory is chaotic, it's 
chaotic. 

Chaos / nonlinear dynamics has some important things to say about
the calculation of thermodynamic properties using MD in terms
of satisfaction / nonsatisfaction of the Ergodic Hypothesis.
Constant-(NVE) computer experiments on many-oscillator systems carried out
by Fermi/Pasta/Ulam at the dawn of "computational experimentation"
showed that quasiperiodic volumes of phase space can be sizeable
no matter how many particles you have in the system. There are
volumes of phase space which may have non-zero "measure" and which are
(at least on the time scales of simulations) toroidal in shape.

Chaotic trajectories are what one hopes for in MD...they
come closest to satisfying the ergodic hypothesis, because they sample
a lot of phase space (in principle, they will sample all of
phase space given infinite time). However, even a chaotic
trajectory cannot sample the ENTIRE phase space on an MD time
scale IF there are "regular" regions of phase space...because such
regions are not accessible to a chaotic trajectory, they are excluded
from it (until Arnold diffusion, a very very slow process, sets in).
So one needs ways to "skip" between regular and chaotic regions of
phase space in one's sampling...sometimes. This is really probably
only an issue IF the regular regions have big volumes, and EITHER
(1) These "excluded phase-space volumes" lock out significant portions
of CONFIGURATION space, and/or
(2) one is averaging something which depends on configurations AND/OR
MOMENTA (i.e., your averaged quantity is defined in the full phase space).
Usually in thermodynamics one looks at properties which are solely
configuration-space averages, so (2) is not often the case.

Of course the "masters of MD" (you know who you are) have devised
various sampling tricks over the years to ensure that (1) and (2)
are not a problem. But when calculating phase-space averages in
the microcanonical ensemble, one must be aware of the potential
for trouble if there are sizeable and/or numerous "islands" of
quasiperiodicity in the "chaotic sea."

I hope that this is helpful or interesting -
awaiting inevitable flames
robert

************************************************************************
 Prof. Robert Q. Topper               internet:   topper@cooper.edu
 Department of Chemistry              phone:      (212) 353-4378
 The Cooper Union                     FAX:        (212) 353-4341 
 Cooper Square                        subway:     take the 6 to Astor Place 
 New York, NY 10003 USA                           or the N/R to 8th St/NYU
************************************************************************
Thermodynamics forever...

From bennett@ubaclu.unibas.ch  Mon Oct 31 13:26:24 1994
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Date: Mon, 31 Oct 1994 19:11:53 +0100
From: Frederick Bennett <bennett@ubaclu.unibas.ch>
Subject: C60 Z matrices summary
To: chemistry@ccl.net
Message-id: <bennett.1134014753B@ubaclu.unibas.ch>
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 Dear to whom it may concern,
                              some time ago I posted a request for Z
matrices for C60 that observed the molecular point group of the species. I
am posting a summary for those who are interested and for the sake of
providing a compilation for the CCL archives the replies a listed below.

Regards

Frederick Bennett

===============================================================================


David Heisterberg (djh@ccl.net)

    X70
    X71   X70   3.50
    X72   X70   3.50    X71    180.00
    X73   X70   3.50    X71     63.4349488229221   X72   0.00
    X77   X70   3.50    X71     63.4349488229221   X73  72.00
    X76   X70   3.50    X71     63.4349488229221   X73  144.00
    X75   X70   3.50    X71     63.4349488229221   X73 -144.00
    X74   X70   3.50    X71     63.4349488229221   X73  -72.00
    X78   X70   3.50    X71    116.565051177078    X73   36.00
    X79   X70   3.50    X71    116.565051177078    X73  108.00
    X80   X70   3.50    X71    116.565051177078    X73  180.00
    X82   X70   3.50    X71    116.565051177078    X73 -108.00
    X81   X70   3.50    X71    116.565051177078    X73  -36.00
    C2    X71   1.236   X70     80.00            X74    0.00
    C9    X71   1.236   X70     80.00            X74   72.00
    C18   X71   1.236   X70     80.00            X74  144.00
    C13   X71   1.236   X70     80.00            X74  -72.00
    C55   X71   1.236   X70     80.00            X74 -144.00
    C10   X72   1.236   X70     80.00            X79    0.00
    C34   X72   1.236   X70     80.00            X79   72.00
    C44   X72   1.236   X70     80.00            X79  144.00
    C6    X72   1.236   X70     80.00            X79  -72.00
    C29   X72   1.236   X70     80.00            X79 -144.00
    C3    X75   1.236   X70     80.00            X71    0.00
    C7    X75   1.236   X70     80.00            X71   72.00
    C22   X75   1.236   X70     80.00            X71  144.00
    C17   X75   1.236   X70     80.00            X71  -72.00
    C37   X75   1.236   X70     80.00            X71 -144.00
    C20   X76   1.236   X70     80.00            X71    0.00
    C19   X76   1.236   X70     80.00            X71   72.00
    C38   X76   1.236   X70     80.00            X71  144.00
    C57   X76   1.236   X70     80.00            X71  -72.00
    C59   X76   1.236   X70     80.00            X71 -144.00
    C56   X77   1.236   X70     80.00            X71    0.00
    C58   X77   1.236   X70     80.00            X71   72.00
    C28   X77   1.236   X70     80.00            X71  144.00
    C54   X77   1.236   X70     80.00            X71  -72.00
    C27   X77   1.236   X70     80.00            X71 -144.00
    C15   X73   1.236   X70     80.00            X71    0.00
    C53   X73   1.236   X70     80.00            X71   72.00
    C51   X73   1.236   X70     80.00            X71  144.00
    C16   X73   1.236   X70     80.00            X71  -72.00
    C49   X73   1.236   X70     80.00            X71 -144.00
    C8    X74   1.236   X70     80.00            X71    0.00
    C14   X74   1.236   X70     80.00            X71   72.00
    C47   X74   1.236   X70     80.00            X71  144.00
    C1    X74   1.236   X70     80.00            X71  -72.00
    C21   X74   1.236   X70     80.00            X71 -144.00
    C12   X78   1.236   X70     80.00            X72    0.00
    C30   X78   1.236   X70     80.00            X72   72.00
    C52   X78   1.236   X70     80.00            X72  144.00
    C5    X78   1.236   X70     80.00            X72  -72.00
    C25   X78   1.236   X70     80.00            X72 -144.00
    C4    X79   1.236   X70     80.00            X72    0.00
    C11   X79   1.236   X70     80.00            X72   72.00
    C26   X79   1.236   X70     80.00            X72  144.00
    C33   X79   1.236   X70     80.00            X72  -72.00
    C60   X79   1.236   X70     80.00            X72 -144.00
    C36   X80   1.236   X70     80.00            X72    0.00
    C35   X80   1.236   X70     80.00            X72   72.00
    C40   X80   1.236   X70     80.00            X72  144.00
    C42   X80   1.236   X70     80.00            X72  -72.00
    C39   X80   1.236   X70     80.00            X72 -144.00
    C43   X82   1.236   X70     80.00            X72    0.00
    C41   X82   1.236   X70     80.00            X72   72.00
    C24   X82   1.236   X70     80.00            X72  144.00
    C45   X82   1.236   X70     80.00            X72  -72.00
    C23   X82   1.236   X70     80.00            X72 -144.00
    C31   X81   1.236   X70     80.00            X72    0.00
    C46   X81   1.236   X70     80.00            X72   72.00
    C48   X81   1.236   X70     80.00            X72  144.00
    C32   X81   1.236   X70     80.00            X72  -72.00
    C50   X81   1.236   X70     80.00            X72 -144.00

========================================================================

E. Lewars (elewars@alchemy.chem.utoronto.ca)

1994 Sept 18

Frederick Bennett asked for a Z-matrix or some other info for the geometry
of C60.  Here are the Cartesians; they seem to have the exact correct symmetry.
It should be possible to use them to generate a Z-matrix, e.g. using MOPAC's
"0scf aigout noxyz" keywords. although I haven't tried this with C60.

60
Buckyball
C    3.451266498   0.685000000   0.000000000
C    3.451266498  -0.685000000   0.000000000
C   -3.451266498   0.685000000   0.000000000
C   -3.451266498  -0.685000000   0.000000000
C    0.685000000   0.000000000   3.451266498
C   -0.685000000   0.000000000   3.451266498
C    0.685000000   0.000000000  -3.451266498
C   -0.685000000   0.000000000  -3.451266498
C    0.000000000   3.451266498   0.685000000
C    0.000000000   3.451266498  -0.685000000
C    0.000000000  -3.451266498   0.685000000
C    0.000000000  -3.451266498  -0.685000000
C    3.003809890   1.409000000   1.171456608
C    3.003809890   1.409000000  -1.171456608
C    3.003809890  -1.409000000   1.171456608
C    3.003809890  -1.409000000  -1.171456608
C   -3.003809890   1.409000000   1.171456608
C   -3.003809890   1.409000000  -1.171456608
C   -3.003809890  -1.409000000   1.171456608
C   -3.003809890  -1.409000000  -1.171456608
C    1.409000000   1.171456608   3.003809890
C    1.409000000  -1.171456608   3.003809890
C   -1.409000000   1.171456608   3.003809890
C   -1.409000000  -1.171456608   3.003809890
C    1.409000000   1.171456608  -3.003809890
C    1.409000000  -1.171456608  -3.003809890
C   -1.409000000   1.171456608  -3.003809890
C   -1.409000000  -1.171456608  -3.003809890
C    1.171456608   3.003809890   1.409000000
C   -1.171456608   3.003809890   1.409000000
C    1.171456608   3.003809890  -1.409000000
C   -1.171456608   3.003809890  -1.409000000
C    1.171456608  -3.003809890   1.409000000
C   -1.171456608  -3.003809890   1.409000000
C    1.171456608  -3.003809890  -1.409000000
C   -1.171456608  -3.003809890  -1.409000000
C    2.580456608   0.724000000   2.279809890
C    2.580456608   0.724000000  -2.279809890
C    2.580456608  -0.724000000   2.279809890
C    2.580456608  -0.724000000  -2.279809890
C   -2.580456608   0.724000000   2.279809890
C   -2.580456608   0.724000000  -2.279809890
C   -2.580456608  -0.724000000   2.279809890
C   -2.580456608  -0.724000000  -2.279809890
C    0.724000000   2.279809890   2.580456608
C    0.724000000  -2.279809890   2.580456608
C   -0.724000000   2.279809890   2.580456608
C   -0.724000000  -2.279809890   2.580456608
C    0.724000000   2.279809890  -2.580456608
C    0.724000000  -2.279809890  -2.580456608
C   -0.724000000   2.279809890  -2.580456608
C   -0.724000000  -2.279809890  -2.580456608
C    2.279809890   2.580456608   0.724000000
C   -2.279809890   2.580456608   0.724000000
C    2.279809890   2.580456608  -0.724000000
C   -2.279809890   2.580456608  -0.724000000
C    2.279809890  -2.580456608   0.724000000
C   -2.279809890  -2.580456608   0.724000000
C    2.279809890  -2.580456608  -0.724000000
C   -2.279809890  -2.580456608  -0.724000000

===========================================================================
Jorge (JSMCM@jazz.ucc.uno.edu


Here is a Z-matrix for C60 that I made some time
ago for G92. The problem that my copy of G92 can 
not handle the Ih symmetry and default to C1 (no 
symmetry). The exact value of the angle a is 
63.43494886  By truncating the value of the angle 
a to 63.43 you can force  G92 to use D5D symmetry
 
Note: you must fix the two angles a and w.
      you can optimized distances f and d only
      f is the distance from the center of the C60 to the
        center of any pentagon
      d is the distance fron the center of pentagon to any
        of its Carbons.

x1
x2 1 f
x3 1 f 2 a
x4 1 f 2 a 3 w
x5 1 f 2 a 4 w
x6 1 f 2 a 5 w
x7 1 f 2 a 6 w
x8 1 1.0 2 90.0 3 0.0
x9 1 f 8 90.0 2 180.0
x10 1 f 9 a 8 180.0
x11 1 f 9 a 10 w
x12 1 f 9 a 11 w
x13 1 f 9 a 12 w
x14 1 f 9 a 13 w
c1a x2 d x1 90.0 x8  0.0
c2a x2 d x1 90.0 c1a 72.0
c3a x2 d x1 90.0 c2a 72.0
c4a x2 d x1 90.0 c3a 72.0
c5a x2 d x1 90.0 c4a 72.0
c1b x3 d x1 90.0 x2  0.0
c2b x3 d x1 90.0 c1b 72.0
c3b x3 d x1 90.0 c2b 72.0
c4b x3 d x1 90.0 c3b 72.0
c5b x3 d x1 90.0 c4b 72.0
c1c x4 d x1 90.0 x2  0.0
c2c x4 d x1 90.0 c1c 72.0
c3c x4 d x1 90.0 c2c 72.0
c4c x4 d x1 90.0 c3c 72.0
c5c x4 d x1 90.0 c4c 72.0
c1d x5 d x1 90.0 x2  0.0
c2d x5 d x1 90.0 c1d 72.0
c3d x5 d x1 90.0 c2d 72.0
c4d x5 d x1 90.0 c3d 72.0
c5d x5 d x1 90.0 c4d 72.0
c1e x6 d x1 90.0 x2  0.0
c2e x6 d x1 90.0 c1e 72.0
c3e x6 d x1 90.0 c2e 72.0
c4e x6 d x1 90.0 c3e 72.0
c5e x6 d x1 90.0 c4e 72.0
c1f x7 d x1 90.0 x2  0.0
c2f x7 d x1 90.0 c1f 72.0
c3f x7 d x1 90.0 c2f 72.0
c4f x7 d x1 90.0 c3f 72.0
c5f x7 d x1 90.0 c4f 72.0
c1g x9 d x1 90.0 x8  180.0
c2g x9 d x1 90.0 c1g 72.0
c3g x9 d x1 90.0 c2g 72.0
c4g x9 d x1 90.0 c3g 72.0
c5g x9 d x1 90.0 c4g 72.0
c1h x10 d x1 90.0 x9  0.0
c2h x10 d x1 90.0 c1h 72.0
c3h x10 d x1 90.0 c2h 72.0
c4h x10 d x1 90.0 c3h 72.0
c5h x10 d x1 90.0 c4h 72.0
c1i x11 d x1 90.0 x9  0.0
c2i x11 d x1 90.0 c1i 72.0
c3i x11 d x1 90.0 c2i 72.0
c4i x11 d x1 90.0 c3i 72.0
c5i x11 d x1 90.0 c4i 72.0
c1j x12 d x1 90.0 x9  0.0
c2j x12 d x1 90.0 c1j 72.0
c3j x12 d x1 90.0 c2j 72.0
c4j x12 d x1 90.0 c3j 72.0
c5j x12 d x1 90.0 c4j 72.0
c1k x13 d x1 90.0 x9  0.0
c2k x13 d x1 90.0 c1k 72.0
c3k x13 d x1 90.0 c2k 72.0
c4k x13 d x1 90.0 c3k 72.0
c5k x13 d x1 90.0 c4k 72.0
c1l x14 d x1 90.0 x9  0.0
c2l x14 d x1 90.0 c1l 72.0
c3l x14 d x1 90.0 c2l 72.0
c4l x14 d x1 90.0 c3l 72.0
c5l x14 d x1 90.0 c4l 72.0

f=3.32182409
d=1.24427177

a=63.43[494886]   [truncation will force D5D symm] 
w=72.0

enjoy

Jorge

============================================================================

Dr. James Stewart  (jstewart@fujitsu.com

Here is a MOPAC Z-matrix for C60.  There are two unknowns, as
required by symmetry.

James J. P. Stewart

 XX    0.0000000  0      0.000000  0      0.000000  0    0    0    0
 XX    3.4932251  1      0.000000  0      0.000000  0    1    0    0
 XX    3.4932243  0    108.000000  0      0.000000  0    1    2    0
 XX    3.4932243  0    108.000000  0      0.000000  0    2    1    3
 XX    3.4932243  0    108.000000  0     63.434949  0    2    1    3
 XX    3.4932243  0    108.000000  0    -63.434949  0    1    2    3
 XX    3.4932243  0    108.000000  0    -63.434949  0    1    6    2
 XX    3.4932243  0    108.000000  0     63.434949  0    1    3    2
 XX    3.4932243  0    108.000000  0      0.000000  0    5    2    1
 XX    3.4932243  0    108.000000  0      0.000000  0    3    1    2
 XX    3.4932243  0    108.000000  0    -63.434949  0    3    1    2
 XX    3.4932243  0    108.000000  0     63.434949  0    4    2    1
  C    1.2398064  1     90.000000  0      0.000000  0    1   12    6      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0    1   12   13      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0    1   12   13      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0    1   12   13      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0    1   12   13      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0    2   11    5      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0    2   11   18      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0    2   11   18      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0    2   11   18      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0    2   11   18      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0    3    5    6      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0    3    5   23      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0    3    5   23      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0    3    5   23      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0    3    5   23      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0    4    6    5      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0    4    6   28      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0    4    6   28      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0    4    6   28      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0    4    6   28      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0    5    3    4      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0    5    3   33      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0    5    3   33      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0    5    3   33      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0    5    3   33      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0    6    4    1      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0    6    4   38      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0    6    4   38      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0    6    4   38      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0    6    4   38      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0    7    9    1      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0    7    9   43      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0    7    9   43      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0    7    9   43      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0    7    9   43      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0    8   10    1      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0    8   10   48      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0    8   10   48      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0    8   10   48      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0    8   10   48      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0    9    7    5      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0    9    7   53      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0    9    7   53      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0    9    7   53      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0    9    7   53      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0   10    8   11      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0   10    8   58      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0   10    8   58      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0   10    8   58      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0   10    8   58      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0   11    2    9      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0   11    2   63      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0   11    2   63      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0   11    2   63      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0   11    2   63      0.0000
  C    1.2398104  0     90.000000  0      0.000000  0   12    1    4      0.0000
  C    1.2398104  0     90.000000  0     72.000000  0   12    1   68      0.0000
  C    1.2398104  0     90.000000  0    144.000000  0   12    1   68      0.0000
  C    1.2398104  0     90.000000  0   -144.000000  0   12    1   68      0.0000
  C    1.2398104  0     90.000000  0    -72.000000  0   12    1   68      0.0000



======================================================
Papernet Address :  Frederick R. Bennett
                    Institute for Physical Chemistry
                    Klingelbergstrasse 80
                    CH-4056 Basel
                    Switzerland

Mouthnet Address :  [41]-(61)-267-3821

Internet Address :  bennett@ubaclu.unibas.ch

======================================================

From rsefeck@watson.ibm.com  Mon Oct 31 14:22:38 1994
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To: chemistry@ccl.net
Subject: J.P. Stewart


 Thanks to all the members of this forum for the 32 responses I received
 on how to contact Dr. Stewart.
 Rich




From szeinfel@snfma1.if.usp.br  Mon Oct 31 15:22:41 1994
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Date: Mon, 31 Oct 1994 18:09:46 -0200 (EDT)
From: Rafael Iosef Najmanovich Szeinfeld {S <szeinfel@snfma1.if.usp.br>
To: computational chemistry <CHEMISTRY@ccl.net>
Subject: postscript papers.
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	Hi Netter's,
	Does someone knows if there are any available internet addresses
where we can find preprint papers or already published papers in 
postscript form, something like the high-energy-physics preprint service ?
	Thank's in advance,
					Rafael.
*-----------------------------------------------------------------------------*
* Rafael Iosef Najmanovich Szeinfeld   |SMAIL: Depto. de Bioquimica - B10 INF.*
* Dept. Biochemistry  -Chemistry Inst. |       Universidade de Sao Paulo      *
* Dept. Math. Physics -Physics Inst.   |       Av. Prof. Lineu Prestes 748    *
* University of Sao Paulo              |       CEP 05508-900                  *
* E-MAIL : szeinfel@snfma1.if.usp.br   |       Sao Paulo - SP - Brazil        *
*-----------------------------------------------------------------------------*

From d3g359@rahman.pnl.gov  Mon Oct 31 17:22:36 1994
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 @carbon.pnl.gov:CHEMISTRY@ccl.net id AA17639; Mon, 31 Oct 94 13:56:23 -0800
Date: Mon, 31 Oct 1994 13:56:23 -0800
Subject: Simulated IR spectra
To: CHEMISTRY@ccl.net
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All, I have seen a few papers in which an IR spectra is simulated
by a sum of gaussian (or triangular) functions based on IR frequencies 
and intensities from a QM program such as G92. Obviously, this is 
a crude approximation, since the width of the gaussians can only
be guessed. Still, it seems to be "useful" to compare to experiment.

Does anyone have opinions about this? Does anyone have a "rule
of thumb" about the width of the gaussians? Does anyone have
a program that already does this?

Thanks in advance.

John


------------------------------------------------------------------------------
  John Nicholas                             Office: (509) 375-6559
  Senior Research Scientist                    FAX: (509) 375-6631
  Molecular Science Research Center
  Pacific Northwest Laboratory
  Mailstop K1-90
  Richland, WA 99352
------------------------------------------------------------------------------


From SCHUBERT%cmda@randb.abbott.com  Mon Oct 31 17:30:03 1994
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Date: Mon, 31 Oct 1994 15:40:22 -0500 (CDT)
Subject: G92-DFT/AlphaVMS
To: chemistry@ccl.net
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I am hoping someone can help with a couple of problems I am having during the
testing of G92 on our Alpha running OpenVMS 6.1.

One problem was solved by DEC.  It required placing the following statement in
MDUTIL.C before the "#include <errno.h>" statement:

            #define cma$tis_errno_get_addr CMA$TIS_ERRNO_GET_ADDR

This cleared up a problem with symbol definition.

Another problem remains in MDUTIL.C.  The routine "isexe" does not correctly
determine the "uid" and "gid" so G92 is not able to execute the required links.
I got around this by setting the status (t = 1) in "getexen".

The third problem is a bigger nuisance.  When the archive values are printed at
the end of a run by link L9999, the values for real numbers have been shifted
by 2 bits, i.e., divided by 4.  For example, if the output should read
"HF = -72.4000", it will instead read "HF = -18.1000".

Has anybody else run into these problems?  Any help will be greatly
appreciated.

Jeff Schubert

Abbott Laboratories

schubert@cmda.abbott.com

From criscuol@genny.gensia.com  Mon Oct 31 17:42:46 1994
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Date: Mon, 31 Oct 1994 13:52:56 +48000
From: Fred Criscuolo <criscuol@gensia.com>
To: chemistry@ccl.net
Subject: Need source code for PDB library routines
Message-Id: <Pine.SGI.3.90.941031134553.17896A-100000@genny.gensia.com>
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Hi,
I'm porting a raytracing application to the IBM RS/6000.  Part of
the code we received has an IRIX binary library of PDB routines.
The routines are:
rw-r--r--2401/3000   1164 Jun 30 11:16 1992 PDBLookup.o
rw-r--r--2401/3000   1400 Jun 30 11:16 1992 PDBOffsets.o
rw-r--r--2401/3000   2472 Jun 30 11:16 1992 PDBReadATab.o
rw-r--r--2401/3000   6492 Jun 30 11:17 1992 PDBReadRec.o
rw-r--r--2401/3000   1108 Jun 30 11:17 1992 PDBReadRes.o
rw-r--r--2401/3000   1484 Jun 30 11:17 1992 PDBVersion.o
rw-r--r--2401/3000   3356 Jun 30 11:17 1992 PDBWriteRec.o
While this library, and the functions it supports, can be excluded from the
make process, I'd like to incorporate them.  I've scanned the public 
domain software available from Brookhaven but couldn't locate this library.
If anyone recognizes these routines and can tell me where they're from I'd
appreciate it.  In the application I'm porting this library is called 
libpdb.a.  Thanks in advance.
Fred


Fred Criscuolo
Chemistry and Biochemistry                        (619) 622-4113
Gensia, Inc.                                 
criscuol@gensia.com
                                      
                                  O       "There's more to life than rowing.. 
                                  /--/       But not much."          
        _________________________//|/_______________________
        \__________________________/_______________________/         
~~~~~~~~~ San Diego Rowing Club   /  est. 1888              ~~~~~~~~~~~~~~~~~
                                 /
                                /  





From C1790@SLVAXA.UMSL.EDU  Mon Oct 31 18:22:36 1994
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Date: Mon, 31 Oct 1994 16:24:47 -0500 (CDT)
From: BILL WELSH <C1790@SLVAXA.UMSL.EDU>
Subject: molecular modeling software for Sun SparcStations
To: chemistry@ccl.net
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Dear Netters,

From someone more familiar with SGI software, I'm looking for molecular 
modeling software that will run on a Sun SparcStation5 with a SparcII 
processor running the Solaris 1.1.1 O/S.  Price is an issue (of course).

I'm primarily interested in widely-distributed programs, commercial or 
otherwise (e.g., Insight, Cerius_2, Sybyl, Hyperchem, Macromodel, Semichem, 
Spartan, Gaussian [or other ab initio package]).  

Thanks ... Bill Welsh
Dept. of Chemistry
Univ. of Missouri-St. Louis
St. Louis, MO 63121



From mmcallis@alchemy.chem.utoronto.ca  Mon Oct 31 21:22:45 1994
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Date: Mon, 31 Oct 1994 20:30:21 -0500
From: Mike McAllister <mmcallis@alchemy.chem.utoronto.ca>
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To: chemistry@ccl.net
Subject: PMP3 ??



Does anyone know how (simply) to get the Gaussian programs to calculate
the PMP3 or PMP4 single point energies of ground state triplet wavefunctions?

Thank you,
Mike McAllister

From o-cha@cnj.digex.net  Mon Oct 31 21:28:27 1994
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From: "Matthew E. Harbowy" <o-cha@cnj.digex.net>
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Subject: Re: CCL:Convergence in MOPAC C.I. calculations
To: KEWISE@aardvark.ucs.uoknor.edu, chemistry@ccl.net
Date: Mon, 31 Oct 1994 20:47:14 +1900 (EST)
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>I am using MOPAC 6.0 to do calculations on fairly large polycyclic
>molecules related to porphyrins.  Part of this work involves optimizing
>geometries and calculating energies for the cations and anions of these
>molecules.  To make these calculations more accurate (hopefully) we are
>using the configuration interaction options in MOPAC 6, but have encountered
>some problems with convergence.  After reducing the gradient to below 1.0,

It's a great idea, one that i've tried to rationalize myself. It's also
a double correction, since parameterization adjusts the energies to 
include the 'correlation' piece once already, and what that means for
transition states is anyone's guess.

>the optimization begins to oscillate, and shows no sign of convergence
>after running for several hours.  A typical command line is as follows:
>
>AM1 PRECISE CHARGE=-1 C.I.=(4,2) VECTORS NODIIS

Indeed, I saw the same thing, and EF only makes it worse. NLLSQ was the
one that did the trick, and occasionally I would use SIGMA as well. Also,
you have to be very careful about picking your ci levels. sometimes (5,2)
is a much better choice due to near degeneracies which don't cause it
to abort with errors, but oscillate instead. 

Also, try dummy atoms, and define your geometries in different ways. A
well chosen zmatrix cured some, not all, of my ills. Part of my problem
turned out to be I was attributing more symmetry to the molecule than was 
true by a bad zmatrix definition. XYZ was right out because I was studying
a cyclization, and the orchestrated nature of the reaction required good
control of the zmatrix. I assume for porphyrin analogs you're using 
symmetry to cut down on the number of dependent variables. what I found was 
the forced symmetry led me to a multiple saddle point, not a minimum or
transition state.

>Kristopher Wise
>University of Oklahoma
>Department of Chemistry and Biochemistry
>KEWISE@aardvark.ucs.uoknor.edu

matt harbowy
tea chemist, thomas j lipton.
-- 
matt harbowy               |  
o-cha@cnj.digex.net        | "I'm the bear that went
greentea@eden.rutgers.edu  |  over the mountain."
harbowy@aol.com            |

