Abstract
We review some motivation behind the introduction of chiral random matrix models in QCD, with particular emphasis on the importance of the Gell-Mann-Oakes-Renner (GOR) relation for these arguments. We show why the microscopic limit is universal in power counting, and present arguments for why the macroscopic limit is generic for a class of problems that defy power counting, examples being the strong CP and U(l) problems. We also discuss some of our new results in light of recent lattice simulations.
| Original language | English |
|---|---|
| Pages (from-to) | 3957-3988 |
| Number of pages | 32 |
| Journal | Acta Physica Polonica B |
| Volume | 29 |
| Issue number | 12 |
| State | Published - 1998 |
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