Why Does Boltzmann Distribution Depend Only on Temperature?

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SUMMARY

The Boltzmann distribution is fundamentally dependent on temperature rather than total energy, as it describes the probability of a system's particles occupying various energy states in thermal equilibrium. In a closed system, energy is conserved on average, and temperature serves as a Lagrange parameter that maximizes entropy while maintaining a fixed mean energy. For an ideal monatomic gas, the total internal energy is expressed as U = (3/2) N k T, where T is the absolute temperature, N is the number of particles, and k is Boltzmann's constant. This relationship illustrates that even with high energy levels, the probability of finding particles in lower energy states remains significant at a given temperature.

PREREQUISITES
  • Understanding of Boltzmann distribution
  • Familiarity with thermal equilibrium concepts
  • Knowledge of ideal monatomic gas properties
  • Basic grasp of statistical mechanics
NEXT STEPS
  • Study the derivation of the Boltzmann distribution in statistical mechanics
  • Explore the implications of temperature in thermodynamic systems
  • Investigate the concept of entropy maximization in closed systems
  • Learn about the relationship between energy states and temperature in quantum mechanics
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Students and professionals in physics, particularly those focusing on statistical mechanics, thermodynamics, and quantum mechanics, will benefit from this discussion.

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Why is the Boltzmann distribution for a collection of atoms independent of their total energy? (it only depends on their temperature)

One would assume that if the energy is high there'd be a greater tendency to be in excited states or am I wrong?
 
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The Boltzmann distribution is valid for a subsystem of a larger closed system in thermal equilibrium, which allows the exchange of energy but not the exchange of particles. Energy is thus conserved on average, and the total value of energy is fixed by the temperature, which is the Lagrange parameter introduced into the problem to maximize entropy under the constraint that the mean energy has this given value. Thus, there is a one-to-one correspondence between the average energy and temperature. E.g. for an ideal monatomic gas non-degenerate gas, the total internal energy is given by

[tex]U=\langle E \rangle=\frac{3}{2} N k T,[/tex]


where [itex]T[/itex] is the absolute temperature, [itex]N[/itex] the particle number contained in the subsystem, and [itex]k[/itex] Boltzmann's constant.
 
hmm okay, but consider this:

If you try to find the probability of an atom in hot resevoir of other atoms appearing in an excited state at T=300K you find that the probability of finding the atom in the ground state is overwhelmingly more probable.

But what if the energy of the system of N particles is so big, that E/N is far larger than the energy of the ground state. How can the ground state then still be so probable? We still assume that T=300K (temperature isn't directly the same as energy, so isn't this possible?)
 

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