GR | # Login | Register
  GR9277 #73
GREPhysics.NET Official Solution    Alternate Solutions
A system in thermal equilibrium at temperature T consists of a large number $N_0$ of subsystems, each of which can exist only in two states of energy $E_1$ and $E_2$, where $E_2-E_1=\epsilon \gt 0$. In the expressions that follow, k is the Boltzmann constant.

Which of the following is true of the entropy of the system?

  1. It increases without limit with T from zero at T=0.
  2. It decreases with increasing T.
  3. It increases from zero at T=0 to $N_0k\ln 2$ at arbitrarily high temperatures.
  4. It is given by $N_0k\left(\frac{5}{2}\ln T - \ln \rho + constant\right)$
  5. It cannot be calculated from the information given.

Statistical Mechanics}Entropy

The third law of thermodynamics says that S(T\rightarrow 0) \rightarrow 0.

Also, the statistical definition of entropy is just S = Nk ln Z, where Z is the partition function. For this problem, one has Z=e^{-\epsilon/kT}+e^{-2\epsilon/kT}. For high temperatures, one has Z \rightarrow 1 + 1 = 2, since e^{x}\approx 1+x for small x (and then 1+x \approx 1 for very small x).

Thus the entropy behaves as in choice (C).

See below for user comments and alternate solutions! See below for user comments and alternate solutions!
Alternate Solutions
There are no Alternate Solutions for this problem. Be the first to post one!
2014-09-25 13:22:16
S = kln\Omega

At any arbitrarily high temperature, the system only has two accessible states, so S = kln(2). C is the only answer choice with this.

The third law of thermodynamics says that the change in entropy of a system approaches zero at absolute zero. Also because we cannot directly measure entropy, I think it is a bit of a misnomer to say that entropy is 0 at T = 0, but not according to ETS...
2009-10-08 06:44:31
the partition function is not as mantiond but:
2010-04-10 01:14:01
Why do we not just choose E1 to be zero? Simplifies things a bit.
2010-10-22 16:23:49

You are correct, but it's simpler to set E_1=0, which is perfectly OK and simplifies the algebra. Then

2009-10-05 00:03:34
What about the degrees of degeneracy in the partition function?
2009-10-08 16:00:41
one for each energy level for each system...
what's wrong with that?
Poop Loops
2008-10-25 17:38:11
You can also look at this conceptually. Remembering that S \right 0 as T \right 0, you already eliminate all but 2 choices.

It's tempting to think that Entropy can increase indefinitely, but think about what's going on here. Say this system is a perfect gas. As temperature increases, so does entropy because everything is getting more and more disordered. But, at really high temperatures, every particle is already zooming around everywhere really fast, so you can't really get *more* disorder.
2008-10-16 12:54:18
A simple way to see that C is the correct answer is that at low temps all the subsystems reduce into the lowest state E_1, and thus the number of accessible microstates of the whole system is just one at abs zero (so S=klnW=kln(1)=0). But at arb high temps, each system is equally likely to be in E_1 or E_2, so you have a two level system (just like the isolated spin-1/2 paramagnet at high temps), and to find the microstates of the whole system it's like finding how many ways to arrange O's and X's on a checkboard with N places. Thus there are W=2^N microstates at high temps, and entropy is S=kln2^N=kNln2.

2007-03-26 18:39:34
Not to be too nitty gritty but S = \frac{\partial}{\partial T}(Nk T ln Z). In our case at high T where Z = 2 then it reduces to the right answer.
2011-06-28 14:33:53
Yes, that was my problem with the original solution! Don't confuse the micro-canonical partition function with the canonical partition function (or the grand-canonical for that matter).

Post A Comment!
You are replying to:
Not to be too nitty gritty but S = \frac{\partial}{\partial T}(Nk T ln Z). In our case at high T where Z = 2 then it reduces to the right answer.

Click here to register.
This comment is best classified as a: (mouseover)
Mouseover the respective type above for an explanation of each type.

Bare Basic LaTeX Rosetta Stone

LaTeX syntax supported through dollar sign wrappers $, ex., $\alpha^2_0$ produces .
type this... to get...
$\langle my \rangle$
$\left( abacadabra \right)_{me}$
The Sidebar Chatbox...
Scroll to see it, or resize your browser to ignore it...