We calculated the chiral condensate and the dressed Polyakov loop in the space-time R × S3 and R × H3. The chiral condensate is the order parameter for the chiral phase transition, whereas the dressed Polyakov loop is the order parameter for the deconfinement phase transition. When there is a current mass, critical points for the chiral and deconfinement phase transitions are different in the crossover region. We show that the difference is changed by the gravitational effect. Copyright © Progress of Theoretical Physics 2012.
CITATION STYLE
Sasagawa, S., & Tanaka, H. (2012). Separation of chiral and deconfinement phase transitions in curved space-time. Progress of Theoretical Physics, 128(5), 925–939. https://doi.org/10.1143/PTP.128.925
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