2005/01/31 by Xin-Qin Gao, Jian-Yang Zhu · 2 citations
Physics and Astronomy · #Black hole (networking) #Casimir effect #Classical mechanics #Cosmology and Gravitation Theories #Dirac (video compression format) #Field (mathematics) #Massless particle #Mathematical physics #Noncommutative and Quantum Gravity Theories #Physics #Quantum #Quantum Electrodynamics and Casimir Effect #Quantum electrodynamics #Quantum mechanics #Unruh effect #gr-qc
paper · pdf · doi:10.1142/s0218271806008796
published in International Journal of Modern Physics D 15(09), 1473-1486 (World Scientific) · 10 pages, no figure. Accepted for publication in IJMPD
arxiv created 2006/04/11 · openalex publication_date 2006/09/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
In this paper, the two-dimensional Reissner–Nordström black hole is considered as a system of the Casimir type. In this background, the Casimir effect for the massless Dirac field is discussed. The massless Dirac field is confined between two "parallel plates" separated by a distance L and there is no particle current drilling through the boundaries. The vacuum expectation values of the stress tensor of the massless Dirac field at infinity are calculated separately in the Boulware state, the Hartle–Hawking state and the Unruh state.