Massive symmetric tensor field in spacetimes with a positive cosmological constant

Atsushi Higuchi*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

We quantize the free massive symmetric tensor field in arbitrary vacuum spacetime with a positive cosmological constant. We find that the theory with (mass)2 between 0 (linearized gravity) and 2 3 × (cosmological constant) is non-unitary if we require that it locally resemble the flat-spacetime counterpart. This is the generalization of the result obtained earlier in de Sitter spacetime.

Original languageEnglish
Pages (from-to)745-765
Number of pages21
JournalNuclear Physics B
Volume325
Issue number3
DOIs
Publication statusPublished - 23 Oct 1989

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