Abstract
An argument is presented to explain the observed increase in the density of states at low energy of a hamiltonian describing a charged particle with spin 1 2 and with a g-factor = 2 in the presence of a random magnetic field in two dimensions. This effect is equivalent to chiral symmetry breaking in the quenched massless euclidean Schwinger model.
| Original language | English |
|---|---|
| Pages (from-to) | 67-69 |
| Number of pages | 3 |
| Journal | Physics Letters B |
| Volume | 139 |
| Issue number | 1-2 |
| DOIs | |
| State | Published - 3 May 1984 |