ArXiv TLDR

Necessary conditions for causality from linearized stability at ultra-high boosts

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2605.12291

Shuvayu Roy, Sukanya Mitra, Rajeev Singh

hep-thnucl-th

TLDR

New method uses linear stability at ultra-high boosts to constrain causality in relativistic hydrodynamics, exploiting Lorentz-invariant stability.

Key contributions

  • Introduces a novel method to constrain causality in relativistic hydrodynamic systems.
  • Exploits Lorentz-invariant stability and "γ-suppression" at ultra-high boosts.
  • Shows stability at the spatially homogeneous limit suffices for causality at near-luminal boosts.
  • Validated the method using conformal Müller-Israel-Stewart theory.

Why it matters

This paper provides an efficient and novel method to derive necessary conditions for causality in relativistic hydrodynamics. It simplifies complex analysis by leveraging high-boost stability, remaining within the low-energy regime. This is crucial for accurately modeling extreme physical phenomena.

Original Abstract

In this work, we provide a novel method to constrain the causal parameter space of a relativistic hydrodynamic system exclusively from its linear stability analysis at non-zero momenta. Our approach exploits the Lorentz-invariant stability property of causal theories. In boosted frames, the dispersion relation exhibits a feature that we call ``$γ$-suppression,'' whereby the higher-order terms in the wavenumber expansion are increasingly suppressed beyond leading order at large boosts. As a consequence, at near-luminal values of Lorentz boost, stability criteria at the spatially homogeneous limit are sufficient to identify the region of the parameter space that satisfies the necessary conditions of causality, even at non-zero momenta. After presenting the general hydrodynamic framework, we test the method in conformal Müller-Israel-Stewart theory and show that it provides an efficient way of deriving the necessary conditions of causality while remaining within the low-energy regime of hydrodynamic validity.

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