Spontaneous Lorentz violation and asymptotic flatness
Yuri Bonder, Christian Peterson

TL;DR
This paper investigates spontaneous Lorentz violation within the minimal gravity sector of the SME, revealing that the $t$ term uniquely prevents asymptotically flat solutions in static, spherically symmetric spacetimes without matter.
Contribution
It demonstrates that the $t$ term in the minimal gravity sector uniquely obstructs asymptotic flatness, clarifying the $t$ puzzle in Lorentz-violating gravity models.
Findings
The $t$ term fixes the asymptotic behavior of the curvature tensor.
No asymptotically flat solutions exist for the $t$ term in the studied scenario.
The $t$ puzzle is linked to the unique properties of the $t$ term.
Abstract
The Standard Model Extension (SME) is a generic parametrization for Lorentz violation and the phenomenological consequences of the minimal gravity sector of the SME are usually studied using a post-Newtonian expansion that requires spacetime to be asymptotically flat. However, there is a term in this sector for which these approximations are unable to make predictions; this is known as the puzzle. The present paper studies a model of spontaneous Lorentz violation in the minimal gravity sector of the SME in a static and spherically symmetric situation, when no additional matter fields are present. It is shown that, under the above mentioned assumptions, is the only term in the minimal gravity sector for which no asymptotically flat solutions exist. This stems from the fact that the term fixes the asymptotic behavior of all the pieces of the curvature tensor.
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