You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
In reality, in a wide range of pH values the substance is zwitterionic. My guess is that the sigma profiles of the zwitterion will look quite different from the un-ionized version of the molecule and I would expect a different phase equilibrium to be predicted.
What's the correct way of modelling this?
The text was updated successfully, but these errors were encountered:
Definitely the scripts were not set up to operate on such complex species. A pull request that thoughtfully addresses such a case would be welcomed by the community.
I just tried using the to_sigma.py script on a molecule that is zwitterionic (and simulated as such in my DFT calculations) and I ran into this line:
COSMOSAC/profiles/to_sigma.py
Line 407 in dd10c53
This line flat out not does allow quaternary nitrogens - is this intentional, because COSMO-SAC was never intended to be used on such species?
My real case is more complicated, but imagine we are looking at L-glutamic acid (https://en.wikipedia.org/wiki/Glutamic_acid). This molecule is in fact in the database, but with the COOH and NH2 group in their unionized state: https://github.com/usnistgov/COSMOSAC/blob/dd10c53d5248dd26321cdecd9c77569bc1f4d3f2/profiles/UD/cosmo/WHUUTDBJXJRKMK-VKHMYHEASA-N.cosmo
In reality, in a wide range of pH values the substance is zwitterionic. My guess is that the sigma profiles of the zwitterion will look quite different from the un-ionized version of the molecule and I would expect a different phase equilibrium to be predicted.
What's the correct way of modelling this?
The text was updated successfully, but these errors were encountered: