Fermionic condensate and the mean energy-momentum tensor in the Fulling-Rindler vacuum
S. Bellucci, V. Kh. Kotanjyan, A. A. Saharian

TL;DR
This paper analyzes the properties of the fermionic Fulling-Rindler vacuum for massive Dirac fields across various dimensions, focusing on condensate and energy-momentum tensor behaviors, revealing thermal properties and isotropic stresses.
Contribution
It provides a detailed evaluation of the fermionic condensate and energy-momentum tensor in the Fulling-Rindler vacuum, including massless and massive cases, and explores their thermal and dimensional properties.
Findings
Fermion condensate vanishes for massless fields and is negative for massive fields.
Vacuum stresses are isotropic for fermions, with negative energy density and pressures.
Thermal distributions exhibit Unruh temperature, with Bose-Einstein type in even dimensions.
Abstract
We investigate the properties of the fermionic Fulling-Rindler vacuum for a massive Dirac field in a general number of spatial dimensions. As important local characteristics, the fermionic condensate and the expectation value of the energy-momentum tensor are evaluated. The renormalization is reduced to the subtraction of the corresponding expectation values for the Minkowski vacuum. It is shown that the fermion condensate vanishes for a massless field and is negative for nonzero mass. Unlike the case of scalar fields, the fermionic vacuum stresses are isotropic for general case of massive fields. The energy density and the pressures are negative. For a massless field the corresponding spectral distributions exhibit thermal properties with the standard Unruh temperature. However, the density-of-states factor is not Planckian for general number of spatial dimensions. Another interesting…
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Taxonomy
TopicsQuantum Electrodynamics and Casimir Effect · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
