lecture 4 barometric formula and the boltzmann equation simple notions on free energy proteins

24
Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins Reading: Chapter 3

Upload: neveah

Post on 27-Jan-2016

60 views

Category:

Documents


2 download

DESCRIPTION

Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins Reading: Chapter 3. Barometric formula (let’s quickly derive…). a particle above the ground. h. h. a column of uniform fluid. pressure at the bottom. potential energy = - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Lecture 4

Barometric formula and the Boltzmann equation

Simple notions on Free Energy

Proteins

Reading: Chapter 3

Page 2: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

a column of uniform fluid

ghp

pressure at the bottom

Barometric formula (let’s quickly derive…)

pressure = density × gravitational const. × height

ghmEpot h

a particle above the ground

potential energy = mass × gravitational const. × height = work against the gravity

h

Page 3: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Now we have a column of compressible gas in the gravity field:

T is constant, but density depends on height

gdhhdp )(

dh

V

nm nkTpV

ideal gas equation

n – number of particlesm - mass

density

pdhkT

mgdp substituting:

hp

po

dhkT

mg

p

dp

0

kT

mgh

p

p

o

lnkTmgh

oepp /

dpp

p

Barometric formula

po

Page 4: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

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

Page 5: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

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 6: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

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 7: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Proteins

•Expression of genetic information: blueprint to structure/machine

•Should have emergent properties…catalytic, binding, motor, control, transport, …

Page 8: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins
Page 9: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Folding order Hierarchy

Page 10: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins
Page 11: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins
Page 12: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins
Page 13: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Alpha helix Beta sheet

Page 14: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Beta barrel channel: ompF (E. coli)

Page 15: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Dependent on the size and flexibility of side chains, only limited ranges of Phi (Φ) and Psy (Ψ) angles are permitted

Page 16: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins
Page 17: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins
Page 18: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Residues forming hairpins are not in helical or -sheet conformations

Glycines frequently occur in turns and loops because they can occupy essentially the entire Phi-Psy space

Page 19: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Different representations of structures (PDB coordinates)

Page 20: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

coiled coils are predicted by amphipathic character of helixes and heptad (7-residue repeats) organization

Page 21: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins
Page 22: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

1 mglsdgewql vlnvwgkvea dipghgqevl irlfkghpet41 lekfdkfkhl ksedemkase dlkkhgatvl talggilkkk81 ghheaeikpl aqshatkhki pvkylefise ciiqvlqskh 121 pgdfgadaqg amnkalelfr kdmasnykel gfqg

Primary sequence of human myoglobin

N-terminus (amino group) C-terminus (carboxyl group)

First Met is usually cleaved off

…go to protein database

Page 23: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

Myoglobin family tree

Page 24: Lecture 4 Barometric formula and the Boltzmann equation Simple notions on Free Energy Proteins

The 4-subunit association of Hb confers cooperativity of oxygen binding