Chiral Morphing
Abstract
Chiral symmetry undergoes a metamorphosis at . For , the usual Noether charge, , is dynamically broken by the vacuum. Above , chiral symmetry undergoes a subtle change, and the Noether charge \underline{{\em morphs}} into , with the thermal vacuum now becoming invariant under . This vacuum is however not invariant under the old transformations. As a result, the pion remains strictly massless at high . The pion propagates in the early universe with a halo. New order parameters are proposed to probe the structure of the new thermal vacuum.
Cite
@article{arxiv.hep-ph/9403309,
title = {Chiral Morphing},
author = {Ngee Pong Chang},
journal= {arXiv preprint arXiv:hep-ph/9403309},
year = {2008}
}
Comments
14 pages, LaTeX, CCNY-HEP-94-6 Invited contribution to the Marshak Memorial volume, edited by E.C.G. Sudarshan, to be published by World Scientific Publishing Co., Singapore, 1994. **** Earlier version had email bug due to transmission problem