CCL: translational entropy in solution
- From: "VITORGE Pierre 094605"
<Pierre.VITORGE!A!cea.fr>
- Subject: CCL: translational entropy in solution
- Date: Sun, 14 Dec 2008 12:03:54 +0100
Sent to CCL by: "VITORGE Pierre 094605" [Pierre.VITORGE,cea.fr]
A dimmer with very long distance between the 2 monomers is meaningless.
Deciding you have a dimmer (or any chemical species) means you make an
approximation where you split atomic interactions between (strong)
intramolecular and (weak or even zero for the ideal systems) intermolecular
ones: when the dimmer is formed there is a strong enough bound between the
monomers and they are at short distance.
This difference between strong/zero interatomic interactions is at the basis of
the thermodynamic demonstration of the law of mass action and the corresponding
equilibrium "constant" (actually a function of P and T) K, where
delta_G° = -RTlnK (G°, not G) and so on...
Besides this thermodynamic feature, note that solvation often has a huge
contribution to the total energy with eventually both enthalpic and entropic
contributions.
--
Pierre Vitorge
http://www.vitorge.name
-----Message d'origine-----
De : owner-chemistry+pierre.vitorge==cea.fr_+_ccl.net [mailto:owner-chemistry+pierre.vitorge==cea.fr_+_ccl.net] De la part de
Andreas Klamt klamt/./cosmologic.de
Envoyé : vendredi 12 décembre 2008 08:46
À : VITORGE Pierre 094605
Objet : CCL: translational entropy in solution
Sent to CCL by: Andreas Klamt [klamt%a%cosmologic.de]
> > Let us for a moment assume that A = B i.e. consider
>
>> A +A --> AA
>>
>> and the interactions and surface of AA are just twice the interactions
>> of A. We may consider the case of 2 cyclohexane molecules getting bound
>> together by a virtual stiff bond which is long enough so that there are
>> no relevant interactions between the 2 parts. In the gasphase this
leads
>> to a large loss of free energy due to the loss of the translational and
>> rotational free energy (not just entropy) of one of the particles
>>
>
> Actually if there is a loss in the entropy of the system its free energy
increases:
>
> dG = dH - TdS
> dS < 0 , dG increases.
>
Sorry for being a little unprecise here regardig the sign, but I think
it is clear what I am talking about.
> Also, there is an increase in the enthalpy of the system(considering that
no kind of interaction is going on between A and A,what is quite contradictory
anyway) after the reaction. The new vibrational modes in AA are going to have a
zero point energy that is bigger than the rotational and translational energies
of the reagents, increasing the enthalpy of the system, which is another reason
for an increase in G and for this reaction to be non-spontaneous
>
>
>> I believe that the physics is correct here. The solvent definitely
>> reduces the motional (kinetic) phase space. The molecules cannot move
>> and rotate as freely as they can in the gasphase, and hence the part of
>> the free energy arising from the integration over momentum and
>> rotational momentum must be reduced in solution. Obviously, and here I
>> agree with the other people in the discussion, the solute can take all
>> positions and orientations, as in the gasphase, and hence the free
>> energy arsing from these integrals are the same as in the gasphase.
>>
>
> Actually, although the solute can take all positions and orientations, in
solution some of these are going to be very disfavored energetically, while
others are going to be more favored, and that is introduced by the term U
(potential energy) in the integral used to calculate the molecular partition
function. So the molecular partition function is not going to be the same as in
the gas phase.
>
Indeed, I mentioned this in the next partof my last CCL entry (see
below) . My argument is that these contributions are unlikely to cancel.
Indeed, I have no estimate which contribution is stronger. We have no
chance to sest that, because my virtual case of a dimerization with a
virtual long connection between the two parts will never be realized in
nature. Association here alway goes along with interactions and hence
with large changes in the interaction integrals. Usually the overall
external polarity of the dimer will be strongly reduced in association.
Hence we will never be able to proof my arguments in reality.
>
>
>> Obviously, in reality, if we generate real close contact associates or
>> even product molecules, the loss of the external degrees of freedom
will
>> be partly compensated by additional internal vibrational modes. But it
>> is unlikely that this exactly matches the loss of external degrees of
>> freedom. Please note, that usually the change in the vibrational free
>> energies upon solvation is parameterized int the surface proportinal
>> part of solvation models, i.e. the non-electrostatic parts.
>>
>
> Non-electrostactic contributions in most of the solvent models
also(actually they should, but in most cases don't) account for the change in
all of the other components of free energy. What about COSMO-RS? I don't have
access to your book and I'm going to read a paper on COSMO-RS soon, but I'm very
curious on the physical foundations of the 2 extra terms (the one proportional
to lnV and the one that depends on the temperature) you've mentioned. Where does
these terms come from? What is parametrized in the model?
>
There are typically 3 contributions to the non-electrostatic terms:
1) the "cavitation energy" often expressed as a kind of solvent
specific
surface tension. This part is not required in COSMO-RS but it
automatically aises from the statistical thermodynamics for the slute
and solvent surface interactions. The free energy required to break the
solvent-solvent contacts in order to enable solute-solvent contacts
automatically and termodynamically consistently follows rom that. Hence
COSMO-RS does not need such a thing as a solvent surface tension: This
automatically follows from the sigma-profile (COSMO charges) of the solvent.
2) the non-electrostatic interactions: The hydrogen bond interations in
COSMO-RS are part of the surface interations taken into account in the
statistical thermodynamics, quantified approximately based on the
surface polarities (COSMO polarization charge densities) of donor and
acceptor. The vdW-interactions are the weekest part of COSMO-RS: They
are just taken into account as surface proportial with element specific
vdW-surface tensions (one of the 2 element specific parameters of
COSMO-RS, the other being the element specific radius). We assume that
the the vdW-interactions have a generic temperature dependence (hence a
split into enthalpic and entropic contributions).
Other solvation models need to parameterize all this into empirical
corrections or solvent specific radii scaling, ...
>
>> This
>> allows for the treatment of phase diagrams, vapor pressures, .... the
>> entire fluid phase equilibrium thermodynamics. And in difference to
>> dielectric solavtion models COSMO-RS yields entropic and enthalpic
>> contributions of the solvation energy (because it does a statistical
>> thermodynamics!!!) For example, it correctly describes the solvation of
>> alkanes n water as a mainly entropic effect, in best agreement with the
>> experiment.
>>
>
> Do you mean that COSMO-RS yields each
component(translational/rotational/vibrational/electronic) of entropy and
enthalpy or that it only separates the free energy of solvation in enthalpy and
entropy contributions?
No, COSMO-RS does not yield all the contributions separately. What we
can separate are the electrostatic, hydrogen bonding and vdWs
contribution to the interaction enthalpy. The other components are
essentially parameterized into the few adjusted pareters of COSMO-RS.
Since there is no fundamental theory of the translations, rotations and
vibrations in solution, there is no chance to do this rigorously. And
fitting to exp. free energies of solvation does not allow us to split
the contributions with respect to the physical origin. But we can quite
clearly say that we find a significant (~3 kcal/mol at 298 K)
contribution to the free energy of solvation which is directly connected
to the molecule and not indirectly via its interactions and surface.
Best regards
Andreas
--
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Dr. habil. Andreas Klamt
COSMOlogic GmbH&CoKG
Burscheider Str. 515
51381 Leverkusen, Germany
Tel.: +49-2171-73168-1 Fax: +49-2171-73168-9
e-mail: klamt],[cosmologic.de
web: www.cosmologic.de
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