Abstract
We note the following: The quark model implies that superdense matter (found in neutron-star cores, exploding black holes, and the early big-bang universe) consists of quarks rather than of hadrons. Bjorken scaling implies that the quarks interact weakly. An asymptotically free gauge theory allows realistic calculations taking full account of strong interactions.
- Received 6 January 1975
DOI:https://doi.org/10.1103/PhysRevLett.34.1353
©1975 American Physical Society
