2012/09/13 by Shuji Sasagawa, S. Sasagawa, H. Tanaka +1
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Quantum Chromodynamics and Particle Interactions #hep-ph
paper · pdf · doi:10.1143/ptp.128.925
published as Prog. Theor. Phys. 128 (2012), 925-939 · 14 pages, 14 figures
arxiv created 2012/09/13 · openalex publication_date 2012/11/01 · arxiv updated 2012/12/03 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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.