Abstract
Classifying consistent effective field theories for the gravitational interaction has recently been the subject of intense research. Demanding the absence of causality violation in high energy graviton scattering processes has led to a hierarchy of constraints on higher derivative terms in the Lagrangian. Most of these constraints have relied on analysis that is performed in general relativistic backgrounds, as opposed to a generic solution to the equations of motion which are perturbed by higher curvature operators. Hence, these constraints are necessary but may not be sufficient to ensure that the theory is consistent. In this context, we explore the so-called CEMZ causality constraints on Quadratic Gravity in a space of shock wave solutions beyond GR. We show that the Shapiro time delay experienced by a graviton is polarization-independent and positive, regardless of the strength of the gravitational couplings. Our analysis shows that as far as the causality constraints are concerned, albeit inequivalent to General Relativity due to additional propagating modes, Quadratic Gravity is causal as per as the diagnostic proposed by CEMZ.
Highlights
JHEP09(2021)150 terms in the gravitational sector below the Planck scale
Our analysis shows that as far as the causality constraints are concerned, albeit inequivalent to General Relativity due to additional propagating modes, Quadratic Gravity is causal as per as the diagnostic proposed by CEMZ
Such terms are not amenable to causality constraints probed by the sign of the Shapiro time shift, which is only sensitive to the three-point graviton couplings
Summary
We make a quick review on the propagation of a probe particle in the shock wave background of General Relativity [2, 23, 24]. We consider a classical probe particle of momentum pv propagating in the shock wave background, and assume that it crosses the shock localized at u = 0 with impact parameter b. The subscript indicates that this result is for a scalar particle scattering off the shock wave background which is a solution of Einstein’s equations. Few comments on this result are in order. One can generate the same result by performing an eikonal scattering amplitude computation in the deflectionless limit [2]
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