Finite-size energy of non-interacting Fermi gases
arXiv:1406.3739 · doi:10.1007/s11040-015-9198-1
Abstract
We prove the asymptotics of the difference of the ground-state energies of two non-interacting -particle Fermi gases on the half line of length in the thermodynamic limit up to order . We are particularly interested in subdominant terms proportional to , called finite-size energy. In the nineties Affleck and co-authors [Aff97, ZA97, AL94] claimed that the finite-size energy equals the decay exponent occuring in Anderson's orthogonality catastrophe. It turns out that the finite-size energy depends on the details of the thermodynamic limit and typically also includes a linear term in the scattering phase shift.
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References in corpus (4)
- Anderson's orthogonality catastrophe
- Anderson's Orthogonality Catastrophe for One-dimensional Systems
- Anderson's orthogonality catastrophe in one dimension induced by a magnetic field
- The asymptotics of an eigenfunction-correlation determinant for Dirac- perturbations (Anderson's Orthogonality Catastrophe for Dirac-)