English

Bounds on negative energy densities in flat spacetime

General Relativity and Quantum Cosmology 2008-11-26 v2 High Energy Physics - Theory

Abstract

We generalise results of Ford and Roman which place lower bounds -- known as quantum inequalities -- on the renormalised energy density of a quantum field averaged against a choice of sampling function. Ford and Roman derived their results for a specific non-compactly supported sampling function; here we use a different argument to obtain quantum inequalities for a class of smooth, even and non-negative sampling functions which are either compactly supported or decay rapidly at infinity. Our results hold in dd-dimensional Minkowski space (d2d\ge 2) for the free real scalar field of mass m0m\ge 0. We discuss various features of our bounds in 2 and 4 dimensions. In particular, for massless field theory in 2-dimensional Minkowski space, we show that our quantum inequality is weaker than Flanagan's optimal bound by a factor of 3/2.

Keywords

Cite

@article{arxiv.gr-qc/9805024,
  title  = {Bounds on negative energy densities in flat spacetime},
  author = {C. J. Fewster and S. P. Eveson},
  journal= {arXiv preprint arXiv:gr-qc/9805024},
  year   = {2008}
}

Comments

REVTeX, 13 pages and 2 figures. Minor typos corrected, one reference added