How to Compute Specific Heat for a 1-D Lattice?

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SUMMARY

The discussion focuses on computing the specific heat (c_v) for a one-dimensional lattice of N particles interacting via spring-like forces. For the limit as temperature T approaches infinity, the energy U is expressed in terms of the normal node frequencies, leading to a specific heat that does not explicitly depend on T. As T approaches zero, the specific heat is characterized by the relationship c_v ∝ A ω^{-\alpha} T^{\gamma}, where the exponents α and γ need to be determined. The partition function is suggested as a method to derive thermodynamic properties, particularly in the limits of T approaching zero and infinity.

PREREQUISITES
  • Understanding of harmonic oscillators and their energy equations
  • Familiarity with statistical mechanics concepts, particularly partition functions
  • Knowledge of thermodynamic limits and behavior at extreme temperatures
  • Basic grasp of lattice dynamics and normal mode frequencies
NEXT STEPS
  • Study the derivation of the partition function for harmonic oscillators
  • Research the behavior of specific heat in low and high-temperature limits
  • Explore the relationship between energy states and temperature in quantum systems
  • Investigate the implications of the exponents α and γ in specific heat equations
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Students and researchers in condensed matter physics, particularly those studying thermal properties of lattice systems and specific heat calculations.

Cryg9
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Homework Statement


A 1-D lattice consists of a linear array of N particles (N>>1) interacting via spring-like nearest neighbor forces. The normal node frequencies are given by
\omega_n=\omega_0\sqrt{\,\,2-2\cos\left(2\pi n/N\right)}
where \omega_0 is a constant and n an integer ranging from -N/2 and +N/2. The system is in thermal equilibrium at temperature T. Let cv be the constant length specific heat.

a) Compute cv for the T -> infinity.

b) For T -> 0, c_v\rightarrow A \omega^{-\alpha}T^{\gamma} where A is a constant you need not compute. Compute the exponents \alpha\text{ and }\gamma.


Homework Equations


U=(1/2+n)\hbar\omega\\\\c_v=\left.\frac{d U}{d T}\right|_V



The Attempt at a Solution


a) Using the energy of a harmonic oscillator listed above, we have
U=N(1/2+n)\hbar\omega_0\sqrt{\,\,2-2\cos\left(2\pi n/N\right)}
which does not have T in it explicitly. It seems n should depend on T, that in order to cause it to go to the next excited mode, one would have to add enough energy to increment n but I am not sure how to express that.

b) For T->0, the lowest energy state is when n=0 -> wn=0, no motion/energy. That does not really tell me anything useful though. I feel its the same question, how does the energy (or n) depend on T?
 
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Cryg9 said:

The Attempt at a Solution


a) Using the energy of a harmonic oscillator listed above, we have
U=N(1/2+n)\hbar\omega_0\sqrt{\,\,2-2\cos\left(2\pi n/N\right)}
which does not have T in it explicitly. It seems n should depend on T, that in order to cause it to go to the next excited mode, one would have to add enough energy to increment n but I am not sure how to express that.

b) For T->0, the lowest energy state is when n=0 -> wn=0, no motion/energy. That does not really tell me anything useful though. I feel its the same question, how does the energy (or n) depend on T?

You are confusing your formulas here. U_1 = \hbar\omega_n = \hbar \omega_0 \sqrt{2-2 \cos\left( \frac{2 \pi n}{N} \right) }

is the energy for a single oscillator

What you would usually do here is to calculate the partition function, and then find the thermodynamics from that. In this case, you cannot really calculate it explicitly, but you can find T->0 and T-> infinity limits.
 

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