From chemistry-request@ccl.net Fri Aug  7 03:44:52 1992
From: Dan Severance <dan@omega.chem.yale.edu>
Subject: Re: your mail
To: rak@igor.caltech.edu (Robert A. Kumpf)
Date: Thu, 6 Aug 92 20:38:01 EDT
Organization: Laboratory for Computational Chemistry
Status: R

> 
>    We have been trying to run a PMF calcuation for a system of two 
> solutes in a box of TIP3P water using BOSS version 2.7.  The first 
> step of the simulation appears to work fine; however, all attempts
> to continue the simulation using the option ISTART=3 have resulted
> in values of 'Infinity' being written to the UP file. The ISTART=3
> option is the recommended choice for beginning the next step in a
> free energy perturbation calculation. Has anyone encountered this
> problem as well?  Any suggestions for a fix would be  greatly
> appreciated.  
> 
    Hi Bob,
       Try running the 311 simulation for 50,000 configs or so, and
  then instead of using 001 on the next step, use 011 to restart
  averaging (this will recreate the upfile).  By that point the initial
  bad interactions which led to the infinities will have been resolved
  and furthur writes to the upfile will be fine.  You can then do your
  normal 001 starts for the rest of the equilibration as usual...

       Dan Severance
       dan@omega.chem.yale.edu  ! No big .sigs !


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From chemistry-request@ccl.net Fri Aug  7 04:23:31 1992
Date: 06 Aug 1992 22:50:46 -0400 (EDT)
From: "DR. DOUGLAS A. SMITH, UNIVERSITY OF TOLEDO" <DSMITH@uoft02.utoledo.edu>
Subject: new MacroModel mail exploder now available
To: chemistry@ccl.net
Status: R

MMODINFO:     THE  MACROMODEL   INFORMATION  MAIL  EXPLODER  WITH
ASSOCIATED ANONYMOUS  FTP ARCHIVES.

WHAT IS THE MMODINFO LIST?

     The  MMODINFO  LIST  is  an  e-mail  exploder  which  allows
MacroModel  users  and  computational  chemistry  researchers  to
exchange information  and experience.    The  list  and  archives
reside on  a VAX  6420 running  the VMS  operating system  at the
University of  Toledo.  This list is not restricted and anyone is
welcome to  subscribe.   It works on the principle, "WHAT ANYBODY
POSTS, EVERYBODY  GETS." All  postings to  this list are archived
and available  for downloading  as described in the  rules of the
list which are automatically sent when you subscribe.

HOW TO SUBSCRIBE.

     To subscribe  to the  MMODINFO List,  send e-mail containing
     the message 

	 SUBSCRIBE MMODINFO   
     to
	 MMODINFO-REQUEST@UOFT02.UTOLEDO.EDU.

ARCHIVES OF THE MMODINFO LIST.

     Currently, archives are accessible only via anonymous ftp at
     FTP.UTOLEDO.EDU (131.183.1.1)

     all mail sent to the list (in [.MMOD]).
     software and  utility programs submitted by list subscribers
     (in [.CHEMISTRY.SOFTWARE]).
     positions         offerred         announcements         (in
     [.CHEMISTRY.POSITIONS.OFFERRED]).
     positions         wanted          announcements          (in
     [.CHEMISTRY.POSITIONS.WANTED]).

DISCLAIMERS

     The  list   is  organized   as  a   service  to   MacroModel
researchers.   By posting to this list you agree that the content
represents your  personal opinion.   In  no event should the list
administrator (Doug Smith), the University of Toledo, the authors
of  MacroModel   (WCS  et  al.),  its  distributors  (Distributed
Chemical Graphics)  or Columbia  University  be  liable  for  the
opinions or  materials posted.  The list administrator and others
listed above  are not  reviewing the  materials submitted to this
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LIST ADMINISTRATOR

     This list is operated by:

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     Assistant Professor of Chemistry
     The University of Toledo
     Toledo, OH  43606-3390
     USA

     voice     (419)537-2116
     fax  (419)537-4033
     email     dsmith@uoft02.utoledo.edu

     Additional support  and problem  solving by  our VAX systems
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     or   shenkin@cunixf.BITNET

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From chemistry-request@ccl.net Fri Aug  7 09:33:06 1992
Date: 07 Aug 1992 07:17:08 -0400 (EDT)
From: "DR. DOUGLAS A. SMITH, UNIVERSITY OF TOLEDO" <DSMITH@uoft02.utoledo.edu>
Subject: ACS Symposium on H-Bonding
To: chemistry@ccl.net
Status: R

At the ACS National Meeting in Chicago, August 22-27, 1993 (a year from now)
I will be chairing a symposium entitled "Modeling the Hydrogen Bond."  We
are now entering the planning stages for that symposium.  If there is 
sufficient interest, I hope to have invited speakers, submitted oral 
papers, and a poster session.

In order to assist in planning, I would ask that you, the readers of this
mail exploder, help by letting me know if you are interested in speaking
and/or presenting at this symposium.  The more I know now, the more time
and money I can ask for and the better the symposium will be.

Please reply to me directly.  I will summarize the invited speakers list
at the appropriate time.  Thank you.

Doug Smith
Assistant Professor of Chemistry
The University of Toledo
Toledo, OH  43606-3390

voice    419-537-2116
fax      419-537-4033
email    dsmith@uoft02.utoledo.edu

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From chemistry-request@ccl.net Fri Aug  7 15:37:05 1992
Date: Fri, 7 Aug 92 11:40:39 -0400
From: kxb3@po.CWRU.Edu (Kenneth Butenhof)
To: chemistry@ccl.net
Subject: CHARMm .DCD distance extraction
Status: RO



Dear CHARMm user(s),

	I have a CHARMm MD data file (.DCD) from which I would like to
extract a set of interatomic distances (for all frames).  I have used the
CORREL command for bond distance extractions, however this requires that
the atoms be bonded (or at least have a atom types compatible for bonding).
Of course, I could add new entries into the  .PRM  (.bin) file but this 
seems messy, and possibly dangerous.  Is there a way to extract distances of
unbonded sets of atoms, and generate statistics on the fluctuations?

	Unfortunately the CHARMm "package", on the CRAY at OSC, does not 
include the analysis modual - that would make it too easy.

	Yes, of course I should get Quanta -- but I don't have it now.

	-- any (other) suggestions would be greatly appreciated!

--
					Ken Butenhof
					Department of Pediatrics
					Case Western Reserve University
					Cleveland, Ohio  44106

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From chemistry-request@ccl.net Fri Aug  7 15:07:55 1992
Date: Fri, 07 Aug 1992 10:59:50 EDT
From: breneman@XRAY.CHEM.RPI.EDU
To: chemistry@ccl.net
Subject: SYBYL User's Group BBS Invitation
Status: RO

From:	MX%"<breneman@quant.chem.rpi.edu>"  7-AUG-1992 10:53:35.05
To:	BRENEMAN
CC:	
Subj:	

Return-Path: <@XRAY.CHEM.RPI.EDU:breneman@quant.chem.rpi.edu>
From: <breneman@quant.chem.rpi.edu>
Date: Fri, 7 Aug 92 10:54:47 EDT
To: breneman@quant.chem.rpi.edu
Date: Fri, 7 Aug 92 13:07:10 -0400
From: jle@world.std.com (Joe M Leonard)
To: chemistry@ccl.net
Subject: Wanted: Info on Sybyl atom type(s)
Status: R


For all you Sybyl guru's out there...

What is the Sybyl atom type for the N in the nitro group?  I can see
N-pl3, since it's trigonal planar, or N-ar, which would be reasonable
for nitrobenzene, or...?  Looking at the published force field parameters
seems to suggest that it really doesn't matter which I choose (even N-sp2
would work), but I'm interested in picking the type "correctly"..

Thanks in advance,

Joe
jle@world.std.com

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From chemistry-request@ccl.net Fri Aug  7 17:30:51 1992
Date: Fri, 7 Aug 92 14:06:55 EDT
From: Weigang Huang <whuang@sodium.mps.ohio-state.edu>
To: CHEMISTRY@ccl.net
Subject: help needed using gaussian 92: calculate istp freq.
Status: R


I am using gaussian 92 to calculate the vibrational frequency modes of
boranes. I got the frequency modes of bh2sh , saved in a check point
file. But I am having trouble using the 'ReadFc' and 'ReadIsotopes'
options to get the frequency modes of different isotopomers of bh2sh.
Since we don't have the manual for g92, my input file follows the
manual of g90. Here are the input and part of the output:


input:
------
$RunGauss
%Chk=bh2sh.chk
#freq=(ReadFc,ReadIsotopes) geom=checkpoint ChkBas

bh2sh isotop#1 freq  pvtz

0  1

no
11
32
1
1
2
------

output:
-------
........

 WANTED A FLOATING POINT NUMBER AS INPUT
 FOUND A STRING AS INPUT
no

?
Error termination in Lnk1e.
.......
-------

Once I tried  'freq=ReadIsotopes' only, no error message about the
input format but re-calculate frequecy from the scratch.

Could somebody help me with this problem?  BTW, does anybody know where
can we get the manual of gaussian 92?


Weigang Huang Chemistry department,the Ohio State University




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From chemistry-request@ccl.net Fri Aug  7 18:23:50 1992
Date: Fri, 7 Aug 92 12:09:27 PDT
From: d3f012@gator.pnl.gov
Subject: Free Software
To: CHEMISTRY@ccl.net
Status: R



 8/7/92


The semi-empirical electronic structure program Argus
version 1.0 is now available by anonymous ftp 
on pnlg.pnl.gov

When you get into the system you should go to the
argus directory. 

The file is argus.tar

I've included compiled executables for Sun4,
SGI, IBM/6000, and Cray YMP.

(Remember to use binary ftp)




Additional notes:
----------------

I've disabled the geometry optimization in version 1.0. 
This code is being completely restructured to work 
better with the MD code (also not in version 1.0).

I'd be happy to receive any constructive criticism on 
the program.

I strongly encourage you to print the User Manual.

Argus is free.  However, it is Copyrighted and distributed
under license. Make sure to read the CopyRight file and the 
License agreement included in the tar file.


Enjoy.



----------------------------------------------------------------
Mark A. Thompson                    email:  d3f012@pnlg.pnl.gov
Sr. Research Scientist              
Molecular Science Research Center
Pacific Northwest Laboratory
PO Box 999, Mail Stop K1-90
Richland, WA.  99352
----------------------------------------------------------------



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From chemistry-request@ccl.net Fri Aug  7 21:35:50 1992
Date: 7-AUG-1992 17:11:38.61
From: WSONNEN@EAGLE.WESLEYAN.EDU
Subject: Re: CHARMm .DCD distance extraction
To: chemistry@ccl.net
Status: R

One solution to extracting atomic distances from a CHARMm .DCD trajectory
file is provided by the following:

------------------------
Note. The following example reads a .PSF file for your system and
      calculates the distances between atoms 1:6 and 530:542.
      This is a straight forward application of the DIST command
      (page 8 of Lecture #5,  CHARMM COURSE by Bernie Brooks at
       the NIH---you'll have to contact him for your own copy of
       the notes [about 500 pages]. I'll fax you a copy of the relevant
       page if you need it).

Good luck,
Wayne Sonnen
-------------------
* Script file produced by WAYNE
* 
open write unit 7 Card name JUNK.LOG line
outu 7
bomlev -2
bann
 
OPEN READ UNIT 63 FILE NAME DNA_PSF.PSF
READ PSF UNIT 63
OPEN READ UNIT 52 FILE NAME SI1_NO.DCD

TRAJ IREAD 52 NREAD 1 EXPA NFILE 20

SET 1 1
LABEL L1
  TRAJ READ
  COOR DIST CUT 11.0 SELE BYNUM 1:6 END SELE BYNUM 530:542 END
  INCR 1 BY 1
IF 1 LT 20.5 GOTO L1

STOP

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From chemistry-request@ccl.net Fri Aug  7 22:54:33 1992
Date: Fri, 7 Aug 92 18:39:48 EDT
From: m10!frisch@uunet.UU.NET (Michael Frisch)
Subject: Re: help needed using gaussian 92: calculate istp freq.
To: chemistry@ccl.net
Status: R

Weigang Huang <uunet!sodium.mps.ohio-state.edu!whuang> asked:
    
    I am using gaussian 92 to calculate the vibrational frequency modes of
    boranes. I got the frequency modes of bh2sh , saved in a check point
    file. But I am having trouble using the 'ReadFc' and 'ReadIsotopes'
    options to get the frequency modes of different isotopomers of bh2sh.
    Since we don't have the manual for g92, my input file follows the
    manual of g90. Here are the input and part of the output:
    
    
    input:
    ------
    $RunGauss
    %Chk=bh2sh.chk
    #freq=(ReadFc,ReadIsotopes) geom=checkpoint ChkBas
    
    bh2sh isotop#1 freq  pvtz
    
    0  1
    
    no
    11
    32
    1
    1
    2
    
    Once I tried  'freq=ReadIsotopes' only, no error message about the
    input format but re-calculate frequecy from the scratch.
    
    Could somebody help me with this problem?  BTW, does anybody know where
    can we get the manual of gaussian 92?
    
    
    Weigang Huang Chemistry department,the Ohio State University
    
This is an input incompatibility between Gaussian 90 and Gaussian 92, but we
hope it is a change in the right direction.  Instead of the silly line
containing "no", for G92 you provide the temperature in kelvin and the
pressure in atmospheres at which the thermochemical calculations are to be
done.  A value of zero for either quantity implies the default (standard
temperature or pressure).  Many G90 users requested the capability of
reading in these values, hence the change.  In hindsight, we should have
continued to accept "no" as equivalent to 0.0,0.0 but we didn't think of that.

You can order a manual from Gaussian, Inc.  Call 412-621-2050.  Questions
about ordering Gaussian's products can be sent to info@gaussian.com.
Questions about using the program and bug reports can be sent to
help@gaussian.com

Mike Frisch
-------

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