Notes on Boltzmann Distribution - Thermal Physics | PHYS 213, Study notes of Physics

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Physics 213: Lecture 7, Pg 1
213 Midterm coming up
213 Midterm coming up
Monday Nov. 10, 7 pm (5:15pm)
Covers:
Lectures 1-7+ ~8 (no thermal radiation)
HW 1-4
Discussion 1-4
Labs 1-2
NOTE: Different coverage than <2008! (see extra
problems online)
Review Session
Sun. Nov. 9, 3-5 PM Lincoln Hall Theater
Conflicts? Sign up (or email Prof. Dahmen) by Wed.
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Physics 213: Lecture 7, Pg 1

213 Midterm coming up

213 Midterm coming up

Monday Nov. 10,

7 pm (5:15pm)

Covers:

Lectures 1-7+ ~8 (no thermal radiation)HW 1-4Discussion 1-4Labs 1-

NOTE: Different coverage than <2008! (see extraproblems online)Review Session

Sun. Nov. 9, 3-5 PM Lincoln Hall Theater

Conflicts? Sign up (or email Prof. Dahmen) by Wed.

Physics 213: Lecture 7, Pg 2

Lecture 7 Lecture 7

The Boltzmann Distribution The Boltzmann Distribution

Concept of a thermal reservoir

The Boltzmann distribution

Paramagnetic Spins – MRI

Elasticity of a Polymer

Supplement: Proof ofequipartition, showing its limits

Reference for this Lecture:

Elements

Ch 8

Reference for Lecture 8:

Elements

Ch 9

Physics 213: Lecture 7, Pg 4

Averages from Probabilities of States

Averages from Probabilities of States

If you could list every quantum state of some system. 1, 2..n…

o

Realistic for small, independent parts (e.g., a SHO, an atom)

And knew the properties of each state

(E

n

, magnetic moment, optical density, etc)

And knew the probability of each state (P

1

, P

2

, ...P

n

IF

You could calculate the average of E, magnetic moment, opticaldensity, etc. for each part. E.g.,

= P

1

E

1

+P

2

E

2

+ ...P

n

E

n

o

And their s.d., etc. too, if you want.

Now if you have a big system, made up of simple little parts asabove, to get , , etc. for the big system,

you just add all

the parts

THEN

We can figure out how things behave starting from scratch.The key step is 3: the Boltzmann factor gets us the probabilities.

Physics 213: Lecture 7, Pg 5

Concept of a Thermal Reservoir Concept of a Thermal Reservoir



Consider a small system in thermal contact with a largesystem (

a thermal reservoir

E

n

E
+ E

m

+ E

q

= U

R

= energy of reservoir

ε

ε

ε

ε

Total energy U = E

n

+ U

R

Set

U = 3

.

R

= # microstates of

reservoir

Key problem

: What is the probability,

P

n

, that the small system is in

the state n with energy

E

n

? (Here E

n

= n

ε ε

ε ε

, i.e., n quanta)?

Answer

: The probability of finding the small system in state n is

proportional to the corresponding

R

Small

Reservoir

system

R

n

P

Ω

Physics 213: Lecture 7, Pg 7

The Boltzmann Distribution

The Boltzmann Distribution



Consider a

small system

exchanging E with a

big reservoir

n = label of state n (quantum #)E

n

= energy of system in state n

(not necessarily an oscillator)

U

tot

= E

n

+ U

R

E

n

U

R

R

R

n

Basic Question:

What is the probability that the small system is

in a particular state

(labeled n) with energy E

n

R

n

R

R

i

n

P

n

i

Ω Ω

Ω Ω

R

=

ΩΩΩΩ

R

(U

tot

  • E

n

) = # states of reservoir

when the particle has energy E

n

.

(See previous table.)

The probability of finding thesmall system in a state withenergy E

n

is proportional to the

corresponding number of statesin the

reservoir

P

n

E

n

The entropy of thereservoir decreases whenthe small system extractsE

n

from it. But T

R

is ~ fixed.

Physics 213: Lecture 7, Pg 8

ln(

entropy

of

reservoir

when

(Taylor expansion)

so

because

R

n

R

n

R

R

R

o R

R

tot

o

R

R

tot

n

R

n

R

o

n

R

R

R

R

R

E kT

n

P

e

remember

let

E

U

U

U

E

E

U

E

kT

kT

U

P

e

e

σ

σ

σ

σ

σ

σ

σ

σ

σ

σ

Derivation of the Boltzmann Distribution

Derivation of the Boltzmann Distribution

n

n

E

kT

E

kT

n

e

P

Ce

Z

=

Boltzmann

Factor:

n

/

1

Z

n

n

E

kT

n

P

e

=

=

“Partition

function”

Physics 213: Lecture 7, Pg 10

Example: Boltzmann Factor

A particular molecule has three states, with energy spacing

ε ε

ε ε

= 10

-

J, as

shown; the molecule is in contact with the environment (reservoir), which hasa temperature of 1000K.

a) What is P

1

, the probability that the molecule is in the middle energy

state?

1

n

E / kT

/ kT

1

E

/ kT

0 / kT

/ kT

2

/ kT

23

3

e

e

J
P

e

e

e

e

kT

10 J

−ε

−ε

− ε

ε

×

e

e

e

b) What is P

2

, the probability that it is in the highest energy state?

E

E

2

E

1

E

o

Physics 213: Lecture 7, Pg 11

Example: Boltzmann Factor

A particular molecule has three states, with energy spacing

ε ε

ε ε

= 10

-

J, as

shown; the molecule is in contact with the environment (reservoir), which hasa temperature of 1000K.

a) What is P

1

, the probability that the molecule is in the middle energy

state?

b) What is P

2

, the probability that it is in the highest energy state?

kT

/

E

kT

/

E

kT

/

E

kT

/

E

2

2

1

0

2

e

e

e

e

P

E

E

2

E

1

E

o

1

n

E / kT

/ kT

1

E

/ kT

0 / kT

/ kT

2

/ kT

23

3

e

e

J
P

e

e

e

e

kT

10 J

−ε

−ε

− ε

ε

×

e

e

e

Physics 213: Lecture 7, Pg 13

Act 1 Act 1

Since P

1

and P

2

both

0 as T

0, P

0

must

At zero temperature, the molecule is always

in the ground state.

) What is P

0

at T = 0?

a)

b)

c) 1

A particular molecule has three states, withenergy spacing

εεεε

= 10

-

J, as shown; the

molecule is in contact with the environment(reservoir

),),),),

at temperature T.at temperature T.at temperature T.at temperature T.

E

E

2

E

1

E

o

) What is P

2

as T

a)

b)

c) 1

Physics 213: Lecture 7, Pg 14

Act 1 Act 1

A particular molecule has three states, withenergy spacing

εεεε

= 10

-

J, as shown; the

molecule is in contact with the environment(reservoir)

at temperature T

.

E

E

2

E

1

E

o

) What is P

2

as T

a)

b)

c) 1

2

0

1

2

/

0

2

/

/

/

0

0

0

1 3

E

kT

E

kT

E

kT

E

kT

e

e

P

e

e

e

e

e

e

=

=

For very high temperatures, all states are equally likely to be occupied,because the reservoir entropy doesn’t depend much on energy.

a) decreases

b) increases

c) increases, thendecreases

  1. What happens to P

2

as we decrease T?

Physics 213: Lecture 7, Pg 16

The probability of finding the particle with energy E

equals

the number of single-particle states at that energy

(

ΩΩΩΩ

1

) TIMES

the probability that one state is occupied

:

How to apply the Boltzmann Factor

How to apply the Boltzmann Factor

(if there are degenerate states)

(if there are degenerate states)

3 states

1 state

E

/

P(E)

3

/

E

kT

e

Z

=

0 /

P(0)

/

1/

kT

e

Z

Z

=

=

/

1

3

E

kT

Z

e

=

P(E) depends

on the # ofstates at E.

/

n

P

/

n

E

kT

e

Z

=

Thermal reservoir

temperature T

Small system (single atom, oscillator, spin…)

Probability

one

particular state (n) is occupied:

You may come across a system that is “degenerate”, which means thatmore than one state has the same energy. In this case, you simply needto count the number of degenerate states.

Physics 213: Lecture 7, Pg 17

Paramagnet: Paramagnet:

System of Independent Magnetic Spins System of Independent Magnetic Spins



In a magnetic field, electron spins can point parallel oranti-parallel to the field --- a result of quantum mechanics.

B

N spins, each with magnetic

moment m , in contact with athermal bath at temperature T.

Each spin has potential energy:

B

E

n

μ

±

=

The probability P

n

that a spin will have energy E

n

is given

by the Boltzmann distribution:

kT

E

n

n

Ce

P

=

Physics 213: Lecture 7, Pg 19

Apply Boltzmann Statistics

Apply Boltzmann Statistics

P

P

n n

= e

-E

n

kT

/Z



Determine the constant C from the condition:



The total magnetic moment

M

of the spin system is:

)

kT

/

B

tanh(

N

M

μ

μ

=

Let’s plot this function:

P

P

down

up

/

/

B kT

B kT

C

e

e

Z

μ

μ

kT

B

kT

B

kT

B

kT

B

down

up

e

e

e e N ) P P ( N M

μ

μ

μ

μ

− +

μ

=

μ

=

kT

/

B

down

Ce

P

μ

=

B

E

down

μ

=

B

E

up

μ

=

kT

/

B

up

Ce

P

μ

=

B

PartitionFunction

Physics 213: Lecture 7, Pg 20

Paramagnetism

Paramagnetism

At sufficiently high temperatures, the ratio

x =

μμμμ

B / kT

is much less than

unity. Using

for small x:

Curie’s Law

Total magnetic moment

of the spin system:

T

B T

kT

B

N

M

2

M

B/T

x

)

x

tanh(

N
N

B/kT

)

/

tanh(

kT

B

N

M

μ

μ

=

M

High-B, low-T,spins lined up“saturation”

Low-B, high-T,few spins lined upLinear response