Abstract
We discuss possible non-chiral extension of the Kerr/CFT correspondence. We
first consider the near horizon geometry of an extremal BTZ black hole and
study the asymptotic symmetry. In order to define it properly, we introduce a
regularization and show that the asymptotic symmetry becomes the desirable
non-chiral Virasoro symmetry with the same central charges for both left and
right sectors, which are independent of the regularization parameter. We then
investigate the non-chiral extension for general extremal black holes in the
zero entropy limit. Since the same geometric structure as above emerges in this
limit, we identify non-chiral Virasoro symmetry by a similar procedure. This
observation supports the existence of a hidden non-chiral CFT\_2 structure with
the same central charges for both left and right sectors dual to the rotating
black holes.
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