2020/05/01 by C. A. Escobar, Leonardo Medel, A. Martín-Ruiz
Mathematics · Physics and Astronomy · #Casimir effect #Classical field theory #Classical mechanics #Cosmology and Gravitation Theories #Field (mathematics) #Field theory (psychology) #Geometry #Lorentz transformation #Mathematical physics #Mathematics #Noncommutative and Quantum Gravity Theories #Physics #Pure mathematics #Quantum Electrodynamics and Casimir Effect #Quantum electrodynamics #Quantum gravity #Quantum mechanics #Scalar (mathematics) #Scalar field #Scalar field theory #Scalar theories of gravitation #Theoretical physics #Theory of relativity #hep-th
paper · pdf · doi:10.1103/physrevd.101.095011
published as Phys. Rev. D 101, 095011 (2020) · 13 pages, 2 figures, Accepted for publication in PRD
arxiv created 2020/05/01 · openalex publication_date 2020/05/11 · arxiv updated 2020/05/20 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We study the Casimir effect in the classical geometry of two parallel conductive plates, separated by a distance L, for a Lorentz-breaking extension of the scalar field theory. The Lorentz-violating part of the theory is characterized by the term \ensuremathλ(u\ifmmode⋅\else\textperiodcentered\fi\ensuremath∂\ensuremathφ)2, where the parameter \ensuremathλ and the background four-vector u^\ensuremathμ codify Lorentz symmetry violation. We use Green's function techniques to study the local behavior of the vacuum stress-energy tensor in the region between the plates. Closed analytical expressions are obtained for the Casimir energy and pressure. We show that the energy density EC (and hence the pressure) can be expressed in terms of the Lorentz-invariant energy density E0 as follows EC(L)=√\frac1\ensuremath-\ensuremathλun21+\ensuremathλu2E0(\stackrel\texttildelowL), where \stackrel\texttildelowL=L/√1\ensuremath-\ensuremathλun2 is a rescaled plate-to-plate separation and un is the component of \stackrel\ensuremath→u along the normal to the plates. As usual, divergences of the local Casimir energy do not contribute to the pressure.