Massive spin-2 theories
Sarah Folkerts, Cristiano Germani, Nico Wintergerst

TL;DR
This paper introduces massive spin-2 theories, discusses their non-linear completion challenges, reviews the Boulware-Deser ghost problem, and explores conditions to avoid it, highlighting the non-uniqueness of such theories.
Contribution
It provides an overview of massive spin-2 theories, examines the ghost problem, and identifies conditions under which the ghost can be avoided in truncated theories.
Findings
Boulware-Deser ghost can be avoided with non-Einsteinian derivative structures.
Massive spin-2 theories are not uniquely defined.
Circumventing no-go theorems requires specific derivative structures.
Abstract
We give an introduction to massive spin-2 theories and the problem of their non-linear completion. We review the Boulware-Deser ghost problem and two ways to circumvent classic no-go theorems. In turn, massive spin-2 theories are not uniquely defined. In the case of truncated theories, we show that the Boulware-Deser ghost may only be avoided if the derivative structure of the theory is not tuned to be Einsteinian.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Particle physics theoretical and experimental studies · Quantum Chromodynamics and Particle Interactions
