Venue: Physics Building, Max-von-Laue-Str. 1, Seminar
Room PHYS 2.116
Time: Tuesday, August 09,
3:00 pm (s.t.)
Contact: hees@fias.uni-frankfurt.de
In
non-central heavy-ion collisions or in neutron star cores finite
rotation effects should be as important as magnetic field effects, or
their interplay is quite non-trivial. Recently some possible
effects of rotation on chiral condensate are discussed, but we found
that no effects appear as long as the temperature is zero. This
situation is qualitatively changed by the magnetic field or the finite
temperature; the former is easy to understand from the triangle gauge
anomaly, while the latter is highly non-trivial, especially a
microscopic connection to the mixed anomaly is still not very
clear. Some controversies will be discussed.