A note on spin two fields in curved backgrounds

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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5 pages - Minor misprints corrected - Version accepted by Class. Quant. Grav

Scientific paper

10.1088/0264-9381/24/6/N01

We reconsider the consistency constraints on a free massless symmetric, rank
2, tensor field in a background and confirm that they uniquely require it to be
the linear deviation about (cosmological) Einstein gravity. Neither adding
non-minimal higher derivative terms nor changing the gauge transformations by
allowing terms non-analytic in the cosmological constant alters this fact.

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