Superluminality and UV Completion

TL;DR

This paper critically examines how superluminal propagation relates to the UV completion of effective field theories, analyzing specific models and emphasizing the importance of high-frequency phase velocity and causality constraints.

Contribution

It provides a detailed analysis of superluminality in quantum field theories, highlighting the role of dispersion relations and the imaginary part of the refractive index in causality and UV completion.

Findings

Numerical evaluation of dispersion relations in QED with background fields.

Superluminal phase velocities can arise in certain conditions.

Negative imaginary parts of the refractive index may be necessary to preserve causality.

Abstract

The idea that the existence of a consistent UV completion satisfying the fundamental axioms of local quantum field theory or string theory may impose positivity constraints on the couplings of the leading irrelevant operators in a low-energy effective field theory is critically discussed. Violation of these constraints implies superluminal propagation, in the sense that the low-frequency limit of the phase velocity $v_{\rm ph}(0)$ exceeds $c$. It is explained why causality is related not to $v_{\rm ph}(0)$ but to the high-frequency limit $v_{\rm ph}(\infty)$ and how these are related by the Kramers-Kronig dispersion relation, depending on the sign of the imaginary part of the refractive index $\Ima n(\w)$ which is normally assumed positive. Superluminal propagation and its relation to UV completion is investigated in detail in three theories: QED in a background electromagnetic field, where the full dispersion relation for $n(\w)$ is evaluated numerically for the first time and the role of the null energy condition $T_{\m\n}k^\m k^\n \ge 0$ is highlighted; QED in a background gravitational field, where examples of superluminal low-frequency phase velocities arise in violation of the positivity constraints; and light propagation in coupled laser-atom $\L$-systems exhibiting Raman gain lines with $\Ima n(\w) < 0$. The possibility that a negative $\Ima n(\w)$ must occur in quantum field theories involving gravity to avoid causality violation, and the implications for the relation of IR effective field theories to their UV completion, are carefully analysed.