Researchers examine the effects of gravity on an ideal Fermi gas, revealing key insights about energy states and density distribution.
We consider an ideal Fermi gas in a container subject to a uniform gravitational field at absolute zero temperature. Under a semiclassical approximation, we examine the density profile of the particles and derive an expression for the chemical potential. A critical value of the chemical potential separates the weak- and strong-gravity regimes, and the kinetic and potential energies of the Fermi gas are determined in both regimes.
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Tanalikhit et al. (2026) studied this question.
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