How Does Phonon Contribution Affect Heat Capacity in Liquid Helium Below 0.6K?

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SUMMARY

The heat capacity of liquid helium below 0.6K is accurately described by the equation Cv=(9.819 x 10^-3 K^-3)NkT^3, where N represents the number of molecules, k is Boltzmann's constant, and T is the temperature in Kelvin. The discussion highlights that transverse shear waves cannot propagate in a liquid, which is crucial for understanding phonon contributions to heat capacity. The speed of sound in liquid helium is given as c=238 m/s, and its density is p=0.145 g cm^-3. The confusion regarding the T^3 dependence of specific heat for massless bosons is noted, emphasizing the relationship between internal energy U and temperature.

PREREQUISITES
  • Understanding of thermodynamics, specifically heat capacity concepts.
  • Familiarity with phonon theory and its application to bosonic systems.
  • Knowledge of Boltzmann's constant and its role in statistical mechanics.
  • Basic principles of fluid dynamics, particularly in relation to sound propagation in liquids.
NEXT STEPS
  • Study the derivation of the heat capacity equation for liquid helium at low temperatures.
  • Explore the relationship between internal energy and temperature for massless bosons.
  • Investigate the implications of sound speed and density on phonon contributions in liquids.
  • Learn about the behavior of specific heat in quantum systems, particularly at low temperatures.
USEFUL FOR

Physicists, materials scientists, and researchers studying low-temperature phenomena in quantum fluids, particularly those interested in the thermal properties of liquid helium.

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Below 0.6K the heat capacity of liquid He is well represented by the equation
Cv=(9.819 x 10^-3 K^-3)NkT^3
Given that transverse shear waves cannot propagate in a liquid, predict the phonon contribution to the heat capacity of He from the data
c=238 m/s (speed of sound in liquid He)
p=0.145 g cm^-3 (density of liquid He)

......difficult...T_T
 
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x is supposed to be multiplication
N number of molecules
k Boltzmann's constant
T temperature in kelvin
Cv heat capacity
 
I find this rather hard to follow since I'm not getting that the specific heat has a T^3 dependence at low temperatures for a system of massless bosons (read: the phonons). I'm getting that U ~ T^3 and, then C_v ~ T^2, so I'm a little confused. I also haven't slept much the past two weeks so I could be doing something silly here.
 

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