A Carroll-covariant energy-momentum-news complex at future null infinity yields Ward identities that generalise the Bondi loss equations, with an anomalous Carroll boost.
Non-Boost Invariant Fluid Dynamics
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abstract
We consider uncharged fluids without any boost symmetry on an arbitrary curved background and classify all allowed transport coefficients up to first order in derivatives. We assume rotational symmetry and we use the entropy current formalism. The curved background geometry in the absence of boost symmetry is called absolute or Aristotelian spacetime. We present a closed-form expression for the energy-momentum tensor in Landau frame which splits into three parts: a dissipative (10), a hydrostatic non-dissipative (2) and a non-hydrostatic non-dissipative part (4), where in parenthesis we have indicated the number of allowed transport coefficients. The non-hydrostatic non-dissipative transport coefficients can be thought of as the generalization of coefficients that would vanish if we were to restrict to linearized perturbations and impose the Onsager relations. For the two hydrostatic and the four non-hydrostatic non-dissipative transport coefficients we present a Lagrangian description. Finally when we impose scale invariance, thus restricting to Lifshitz fluids, we find 7 dissipative, 1 hydrostatic and 2 non-hydrostatic non-dissipative transport coefficients.
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hep-th 2years
2026 2representative citing papers
Nonlinear analysis of relativistic viscous fluid relaxation yields an asymptotic attractor with frequency locking to n times the fundamental and amplitude cascading J_n = α_J^{n-1} J_1^n fixed by EOS and viscosity.
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The Energy-Momentum-News Complex near Future Null Infinity
A Carroll-covariant energy-momentum-news complex at future null infinity yields Ward identities that generalise the Bondi loss equations, with an anomalous Carroll boost.
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Nonlinear nature of near-equilibrium viscous fluids
Nonlinear analysis of relativistic viscous fluid relaxation yields an asymptotic attractor with frequency locking to n times the fundamental and amplitude cascading J_n = α_J^{n-1} J_1^n fixed by EOS and viscosity.