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Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics
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Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

Dec 14, 2015

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Page 1: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

Lecture 5

Barometric formula and the Boltzmann equation(continued)

Notions on Entropy and Free Energy

Intermolecular interactions: Electrostatics

Page 2: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

kTmgh

o

ep

p /Barometric formula

kTE

o

potec

c /

kTmgh

o

en

n / n = number of particles per unit volume

c = concentration (which is probability)

because pressure is proportional to the number of

particles p ~ n

normalizing to the volume c = n/V

potEUH kTH

o

ec

c /

in our case U is constant because T is constant

Boltzmann:

Page 3: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

Boltzmann equation uses probabilities

kTEE

j

i jiep

p /)(

the relative populations of particles in states i and j separated by an energy gap

t

j

kTE

kTE

jj

j

e

ep

1

/

/

t

j

kTE je1

/- partition function

the fraction of particles in each state:

E2-1

E3-2

1

3

2

Page 4: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

S = k lnW

Free energy difference G = H - TS

W is the number of micro-states

e-1 = 0.37

e-2 = 0.135

e-3 = 0.05

e-4 = 0.018

e-5 = 0.007

H

entropic advantage

The energy difference here represents enthalpyH = U + W (internal energy +work)

kTG

j

i ep

p /

For two global states which can be ensembles of microstates:

H

pi/pj

pi

pj

kTH

j

i ep

p /

Page 5: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

Carnot cycle and Entropy

V

p

T1

T2

Q1 - Q2 = W (reversible work)

2

2

1

1

T

Q

T

Q

0 Ti

Qi

0T

dQ T

dTC

T

dQdS

prev

B

A

revT

dQASBS )()( S = k lnW

W = number of accessible configurations

Q1

Q2

Page 6: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

B

A

revdQASBST )]()([

At constant T

QUW

)]()([)()( ASBSTBUAUW

)()( BFAFW

)()()( ATSAUAF

)()()( BTSBUBF

STUFW

HelmholtzFreeEnergy

Page 7: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

TSUF HelmholtzFreeEnergy

TSPVUG

PVUH

TSHG GibbsFreeEnergy

Page 8: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.
Page 9: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

What determines affinity and specificity?

Tight stereochemical fitand Van der Waals forces Electrostatic interactionsHydrogen bondingHydrophobic effect

All forces add up giving the total energy of binding:

Gbound– Gfree= RT

lnKd

Page 10: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

What are all these interactions?

Page 11: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

Electrostatic (Coulombic) interactions

20

21

4 r

qqF

r

qqFdrU

r 0

21

4

(in SI)

r

q1 q2

charge - charge

dielectric constant of the medium that attenuates the field≥

kTelB 02 4/

The Bjerrum length is the distance between two charges at which the

energy of their interactions is equal to kT

When T = 20oC, = 80 lB = 7.12 Ǻ

Page 12: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

rq

Electrostatic self-energy, effects of size and dielectric constant

r

qqGel

04

q

r

qqdqG

q

el 0

2

00 84

1

brought from infinity

rq

?

Consider effects of 1. charge2. size3. value of 2 relative to 1

on the partitioning between the two phases

Page 13: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

r

q+q-

What if there are many ions around as in electrolytes?

02 / Poisson eqn

)exp()( 1 KrArr Solution in the Debye approximation:

The radial distribution function shows the probabilities of finding counter-ions and similar ions in the vicinity of a particular charge

Point charge and radial symmetry predict a decay that is steeper than exponential

K – Debye length, a function of ion concentration

same charge ions

counter-ions

Page 14: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

Charge-Dipole and Dipole-Dipole interactions

+ q’

- q’

a

charge - dipole

r

204

cos

r

qdU

qad

dipole moment

static

420

22

3)4( kTr

dqU

with Brownian tumbling

30

21

4 r

KddU

d1 d2

K – orientation factor dependent on angles

620

22

21

)4(32

rkT

ddU

with Brownian motion

static

q

r

Page 15: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

Induced dipoles and Van der Waals (dispersion) forcesE

Ed -

+ a - polarizability

dr 6

02

2

)4( r

dU

constant dipole

induced dipole

r64

21

2121

3)( rnII

IIU

I1,2 – ionization energies

1,2 – polarizabilities

n – refractive index of the medium

induced dipoles(all polarizable molecules

are attracted by dispersion forces)

neutral molecule in the field

d – dipole moment

Large planar assemblies of dipoles are capable of generating long-range interactions

Page 16: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

0 2 4 6 8 100

0.2

0.4

0.6

0.8

U1 r( )

U2 r( )

U4 r( )

U6 r( )

r

1/r2

1/r6

1/r

Long-range and short-range interactions

Even without NET CHARGES on the molecules, attractive interactions always exist. In the presence of random thermal forces all charge-dipole or dipole-dipole interactions decay steeply (as 1/r4 or 1/r6)

1/r4

Page 17: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

Interatomic interaction: Lennard-Jones potential describes both repulsion and attraction

Uo 1

U x( ) Uo x12

2x6

0.6 0.8 1 1.2 1.4 1.6 1.8

1

0

1

2

U x( )

x

600

1200 )/(2)/()( rrErrErEp

r = r0 (attraction=minimum)

r = 0.89r0

r = r0

steric repulsion

Bond stretching is often considered in the harmonic approximation:

202

1 )()( xxxU

Page 18: Lecture 5 Barometric formula and the Boltzmann equation (continued) Notions on Entropy and Free Energy Intermolecular interactions: Electrostatics.

desolvdispstericeltot EBAqE

Van der Waals

Here is a typical form in which energy of interactions between two proteins or protein and small molecule can be written Ionic pairs +

H-bondingremoval of waterfrom the contact