2014/12/29 by A. Belhaj, Belhaj, A., M. Chabab +9
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Classical mechanics #Cosmology and Gravitation Theories #FOS: Physical sciences #Geometry #High Energy Physics - Theory (hep-th) #Mathematics #Noncommutative and Quantum Gravity Theories #Partition function (quantum field theory) #Physics #Quantum mechanics #Scalar (mathematics) #Scalar field #Statistical model #Statistical physics #Statistics #Theoretical physics #hep-th
paper · pdf · doi:10.48550/arxiv.1412.8322
10 pages, 6 figures, latex
arxiv created 2014/12/29 · openalex publication_date 2014/12/29 · arxiv updated 2014/12/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We investigate the statistical behaviors of 3D hairy black holes in the presence of a scalar field. The present study is made in terms of two relevant parameters: rotation parameter a and B parameter related to the scalar field. More precisely, we compute various statistical quantities including the partition function for non-charged and charged black hole solutions. Using a partition function calculation, we show that the probability is independent of a and B parameters.