statistical mechanics Flashcards

1
Q

Definition of Temperature

A

1/KT =(dlng(E)/de)

where K : boltzmanns constnant converts j to k

E: energy of microsttes
g(E) :density of microstates, g(E) e = no. of microstates between E and dE

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

PEEP

A

principle of equal equilibrium probability

For isolated system exploring W microstates with the same energy, each is equally probable

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Mean energy of a system equation

A

mean E = sum (EiPi)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Energy when T is small

A

when T –> 0 E—> 0 at low T system is frozen in ground state which has energy =0

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Energy when T is large

A

when T–> infinity E–>sum of states/number of states

As high T all states have equal boltzmann factors so all equally likely and E is just 1/no. of staates (sum of states)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Gibbs expression for the entropy of a general system

A

S= -K sumPi (ln) pi
where
pi is the probability that the system is in microstate i
K is the boltzman constant

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Entropy of isolated system

A

by PEEP
pi=1/w for each of w states
0 fo other states

S= -kw(1/w)ln(1/w) = Klnw

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Meaning of entropy (based on Gibbs and Boltzmann expression)

A

s measures (logorithmically) the no. of microstates being explored (klnW) are, more generally (gibbs) the extent to which many microstates are being explored with significant probability.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

S at low temps

A

by third law of thermodynamics s–>0 most real systems have a unique ground state, into which the system will be ‘frozen’ (boltzmann) at low T, w=1

therefore : S=KlnW=0

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

pressure of a system is given by…?

A

the thermodynamic relation

P=-(df/dv)T,N

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

pressure of ideal gas

A

PV=NRT

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

relate pressure of a system to pressure of a ideal gas

A

P=-(df/dv)T,N =+NKT(1/V) –> PV=NKT

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Thermodynamic expression for chemical potential

A

mu = (df/dN)T,V

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

chemical potential of ideal gas

A

mu = KT ln (N/V [2πhbar^2/mkT]^3/2)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

State the Pauli exclusion principle which applies to identical fermions

A

Spin S= integers are bosons, integer +1/2 is a fermion, you can’t put more than 1 fermion in each sinlge particle state

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

fermi dirac equation

A

f(epsilon) = 1/ e^(epsilon-mu)/KT + 1

17
Q

what is fermi dirac

A

The Fermi-Dirac distribution that gives the mean occupation f(c) of a single-particle state of energy ε, in a system of identical non-interacting fermions at temperature T

18
Q

micro state

A

quantum state of the entire system. isolated system has fixed energy so only has access to those microstates that have same energy as one another.

19
Q

g(E) density of microstates in energy

A

g(E)dE= no. of microstates in range E–> E+dE if E is fixed to within deltaE, W=gdeltaE but for large systems g approx 10^10^23 where as deltaE approaches 10^-20 -10^-1 J so lnw approx lng as -20 –1 are negligable by comparison with 10^23

20
Q

a physical system that has g(E)=AE^n density of microstates

A

A system of n harmonics oscillators has, at high temp (KT»hbarW) on energy nKT (classically equipartition) and hence has g(E) of the form given (at high energies)

21
Q

partition function

A

Z = sum j exp (-Ei/KT)

Ei : energy of microstates

22
Q

boltmann function

A

Pi = exp(-Ei/KT)/Z

23
Q

no. of q points per unit vol of Q space (sphere)

A

(L/π)^3)^-1 = V/π^3.

becausse q points form a cubic lattice with spacing π/L

therefore no. points per unit vol of q-space is
((π/L)^3)^-1 = V/π^3. where V=L^3

24
Q

energy density in q space, sphere ignoring zero point

A

no. of modes in +ive octant of sphere radius q thickness dq

vol of +ive octant X no of q puv X no. of q modes X energy per mode

25
Q

vol of +ive octant

A

4piq^2/8 dq

26
Q

no of q per unit vol of q modes

A

v/pi^3

27
Q

graph epsilon(omega )omega for different temps

A

at low T, epsilon(omega) is exponentially small throughout visible range

At high T, epsilon(omega is large at red end of visible range but falls off

28
Q

what is a boson

A

has a interger of spin and certain atoms and photons

29
Q

what is a fermion

A

integer +1/2 of spin electron and proton

30
Q

For a system of many non-interacting identical particles, state how a fundamental principle of quantum mechanics, depending on whether the particles are bosons or fermions, affects the possible values of the number of particles in a given single-particle quantum state.

A

Pauli exclusion principle

only one or zero fermions in each single particle state, no restrictions for bosons so 0,1,2,3…

31
Q

mu in the gibbs disrtibution

A

mu: chemical potential ith microstate in which energy is Ei

32
Q

heat resevoir

A

large system (large heat capacity) whose temperature changes negligibly when energy on the energy scale ofout system is added/subtracted. allowed to exchange energy with our system

33
Q

microstate

A

quantum state of our entire system

34
Q

pi

A

is the probability that the system is in a microstate i