ar X iv : g r - qc / 0 60 41 06 v 1 2 5 A pr 2 00 6 An explicit quantum weak energy inequality for Dirac fields in curved spacetimes
نویسنده
چکیده
The quantized Dirac field is known, by a result of Fewster and Verch, to satisfy a Quantum Weak Energy Inequality (QWEI) on its averaged energy density along time-like curves in arbitrary four-dimensional globally hyperbolic spacetimes. However, this result does not provide an explicit form for the bound. By adapting ideas from the earlier work, we give a simplified derivation of a QWEI for the Dirac field leading to an explicit bound. The bound simplifies further in the case of static curves in static spacetimes, and, in particular, coincides with a result of Fewster and Mistry in four-dimensional Minkowski spacetime. We also show that our QWEI is compatible with local covariance and derive a simple consequence.
منابع مشابه
ar X iv : g r - qc / 0 60 41 06 v 2 3 1 O ct 2 00 6 An explicit quantum weak energy inequality for Dirac fields in curved spacetimes
The quantized Dirac field is known, by a result of Fewster and Verch, to satisfy a Quantum Weak Energy Inequality (QWEI) on its averaged energy density along time-like curves in arbitrary four-dimensional globally hyperbolic spacetimes. However, this result does not provide an explicit form for the bound. By adapting ideas from the earlier work, we give a simplified derivation of a QWEI for the...
متن کامل0 30 70 98 v 1 2 3 Ju l 2 00 3 Quantum Weak Energy Inequalities for the Dirac field in Flat Spacetime
Quantum Weak Energy Inequalities (QWEIs) have been established for a variety of quantum field theories in both flat and curved spacetimes. Dirac fields are known (by a result of Fewster and Verch) to satisfy QWEIs under very general circumstances, although an explicit bound has hitherto been lacking. In this paper we present a new and explicit QWEI bound for Dirac fields of mass m 0 in four-dim...
متن کاملar X iv : g r - qc / 0 50 80 08 v 1 1 A ug 2 00 5 Observables for the polarized Gowdy model
We give an explicit characterization of all functions on the phase space for the polarized Gowdy 3-torus spacetimes which have weakly vanishing Poisson brackets with the Hamiltonian and momentum constraint functions.
متن کاملar X iv : g r - qc / 0 31 00 76 v 1 1 5 O ct 2 00 3 HOLONOMY GROUPS AND SPACETIMES
A study is made of the possible holonomy group types of a space-time for which the energy-momentum tensor corresponds to a null or non-null electromagnetic field, a perfect fluid or a massive scalar field. The case of an Einstein space is also included. The techniques developed are also applied to vacuum and conformally flat space-times and contrasted with already known results in these two cas...
متن کاملar X iv : m at h - ph / 0 41 20 64 v 3 1 3 A pr 2 00 5 Note on the energy - momentum tensor
This note provides an explicit proof of the equivalence of the Belinfante’s energy-momentum tensor and the metric energy-momentum tensor for general mixed tensor-spinor fields.
متن کامل