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Energy Cost to Make a Hole in the Fermi Sea

Rupert L. Frank, Mathieu Lewin, Elliott H. Lieb, and Robert Seiringer
Phys. Rev. Lett. 106, 150402 – Published 12 April 2011
Physics logo See Synopsis: Making a hole in a Fermi sea

Abstract

The change in energy of an ideal Fermi gas when a local one-body potential is inserted into the system, or when the density is changed locally, are important quantities in condensed matter physics. We show that they can be rigorously bounded from below by a universal constant times the value given by the semiclassical approximation.

  • Received 7 February 2011

DOI:https://doi.org/10.1103/PhysRevLett.106.150402

© 2011 American Physical Society

Synopsis

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Making a hole in a Fermi sea

Published 12 April 2011

A semiclassical approximation gives an accurate answer to a simply stated, but difficult to solve, quantum mechanical problem.

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Authors & Affiliations

Rupert L. Frank1, Mathieu Lewin2, Elliott H. Lieb1,3, and Robert Seiringer4

  • 1Department of Mathematics, Princeton University, Washington Road, Princeton, New Jersey 08544, USA
  • 2CNRS and Department of Mathematics (UMR CNRS 8088), University of Cergy-Pontoise, F-95 000 Cergy-Pontoise, France
  • 3Department of Physics, Princeton University, P.O. Box 708, Princeton, New Jersey 08542, USA
  • 4Department of Mathematics and Statistics, McGill University, 805 Sherbrooke Street West, Montréal, Québec, H3A 2K6, Canada

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Issue

Vol. 106, Iss. 15 — 15 April 2011

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