pith. sign in

arxiv: 2508.01446 · v3 · pith:CEC2GG5Unew · submitted 2025-08-02 · ✦ hep-th · gr-qc

Radiation in Fluid/Gravity and the Flat Limit

Gabriel Arenas-Henriquez , Luca Ciambelli , Felipe Diaz , Weizhen Jia , David Rivera-Betancour This is my paper

Pith reviewed 2026-05-21 23:51 UTC · model grok-4.3

classification ✦ hep-th gr-qc
keywords fluid/gravity dualitygravitational radiationasymptotically locally AdSCarrollian holographyentropy productiondissipative hydrodynamicsBondi newsnull gauges
0
0 comments X

The pith

Bulk radiation in asymptotically locally anti-de Sitter spacetimes maps directly to dissipative corrections and entropy production in the dual boundary fluid for algebraically special solutions.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper shows how gravitational radiation in the bulk of certain anti-de Sitter spacetimes can be read from the boundary Cotton tensor and stress tensor. It collects this information into a radiative vector and reinterprets the vector in terms of fluid variables in the dual theory. For algebraically special solutions the vector lines up with viscous terms in the stress tensor, producing a direct correspondence between radiation and entropy production. The same null gauges that capture the radiation also support a flat limit, in which a Carrollian version of the vector sources viscous stress and heat current while encoding Bondi news. Explicit examples such as Robinson-Trautman spacetimes and accelerating black holes are used to check the mapping.

Core claim

For algebraically special solutions we uncover a close connection between bulk radiation and dissipative corrections in the boundary stress tensor, demonstrating a direct link between radiation and entropy production in the boundary fluid. The radiative content is captured by a boundary radiative vector assembled from the Cotton and stress tensors and reinterpreted holographically in fluid variables. In the flat limit a Carrollian analogue of the radiative vector is constructed, and bulk radiation is shown to source the Carrollian viscous stress tensor and heat current that encodes the Bondi news.

What carries the argument

The radiative vector, assembled from the boundary Cotton tensor and stress tensor, which encodes bulk radiation and is reinterpreted in fluid variables for the dual theory and in a Carrollian analogue for the flat limit.

If this is right

  • Bulk radiation corresponds to dissipative corrections in the boundary stress tensor.
  • These dissipative corrections generate entropy production in the dual fluid.
  • In the flat limit bulk radiation sources the Carrollian viscous stress tensor and heat current.
  • The radiative structure naturally produces celestial observables such as energy detectors.
  • The mapping holds for Robinson-Trautman spacetimes and accelerating black holes.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The link suggests that known radiating bulk solutions could be used to generate explicit out-of-equilibrium states in conformal fluids.
  • If the gauge condition can be relaxed, the correspondence might extend beyond algebraically special solutions.
  • The Carrollian construction offers a route to extract Bondi news from boundary fluid data in flat-space holography.

Load-bearing premise

Null gauges must exist that simultaneously capture radiative behavior in asymptotically locally anti-de Sitter spacetimes and admit a well-defined flat limit so the radiative vector can be reinterpreted in both fluid and Carrollian terms.

What would settle it

An explicit algebraically special solution in which the dissipative corrections extracted from the boundary stress tensor fail to reproduce the entropy production rate implied by the bulk radiative vector would falsify the claimed direct link.

read the original abstract

We explore asymptotically locally anti-de Sitter spacetimes exhibiting gravitational radiative behavior, employing null gauges that allow for a well-defined flat limit. The radiative content in the bulk is captured by the boundary Cotton and stress tensor, which we collect into a radiative vector. We reinterpret this vector holographically in terms of fluid variables in the dual boundary theory. For algebraically special solutions, we uncover a close connection between bulk radiation and dissipative corrections in the boundary stress tensor, demonstrating a direct link between radiation and entropy production in the boundary fluid. This reveals a rich interplay between radiative dynamics in the bulk and out-of-equilibrium conformal physics at the boundary. We then investigate the flat limit of this correspondence in the context of flat-space holography. In this setting, we construct a Carrollian analogue of the radiative vector and introduce Celestial observables, such as energy detectors, which emerge naturally from the bulk's radiative structure. Our analysis shows that bulk radiation sources the Carrollian viscous stress tensor and heat current, which encodes the Bondi news in this framework. We illustrate our results with explicit examples, including Robinson-Trautman spacetimes and accelerating black holes.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript explores asymptotically locally anti-de Sitter spacetimes with gravitational radiative behavior, employing null gauges that permit a well-defined flat limit. Radiative content is encoded in a boundary radiative vector constructed from the Cotton tensor and stress tensor, which is reinterpreted in fluid/gravity variables. For algebraically special solutions the work claims a direct link between bulk radiation and dissipative corrections to the boundary stress tensor, implying a connection to entropy production. The flat limit is then taken to construct a Carrollian analogue of the radiative vector, relating bulk radiation to the Carrollian viscous stress tensor and heat current that encodes Bondi news; explicit illustrations are given for Robinson-Trautman spacetimes and accelerating black holes.

Significance. If the gauge construction and the claimed link hold, the result would supply a concrete holographic dictionary connecting bulk gravitational radiation to out-of-equilibrium dissipative processes and entropy production in the dual fluid, while also furnishing a Carrollian counterpart relevant to flat-space holography and celestial observables. The explicit examples supply concrete test cases.

major comments (2)
  1. [Abstract and algebraically special solutions section] Abstract and § on algebraically special solutions: the central claim that bulk radiation (via the radiative vector) is directly linked to dissipative corrections and entropy production rests on the existence of null gauges that simultaneously capture radiative degrees of freedom in asymptotically locally AdS geometries and admit a clean flat limit. No general construction or existence proof for such gauges is supplied beyond the specific examples; if the gauge family does not exist for generic radiative solutions or introduces singularities in the flat limit, the claimed direct connection fails to hold.
  2. [Flat limit and Carrollian section] Flat-limit discussion: the reinterpretation of the radiative vector as a Carrollian analogue that sources the viscous stress tensor and heat current encoding Bondi news assumes the flat limit preserves radiative information without loss or singularity. The manuscript does not demonstrate that this limit is well-defined for the full class of solutions considered, which is load-bearing for the Carrollian holography claim.
minor comments (2)
  1. [Notation and definitions] Clarify the precise definition of the radiative vector (its components in terms of Cotton and stress tensors) and its Carrollian counterpart, including any index conventions or normalizations, to facilitate verification.
  2. [Examples section] In the Robinson-Trautman and accelerating black hole examples, explicitly state the coordinate ranges and asymptotic fall-off conditions used when taking the flat limit so that readers can reproduce the Bondi-news encoding.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their careful reading of the manuscript and for the constructive comments. We address each major point below, clarifying the scope of our results while agreeing to revisions that strengthen the presentation.

read point-by-point responses

  1. Referee: [Abstract and algebraically special solutions section] Abstract and § on algebraically special solutions: the central claim that bulk radiation (via the radiative vector) is directly linked to dissipative corrections and entropy production rests on the existence of null gauges that simultaneously capture radiative degrees of freedom in asymptotically locally AdS geometries and admit a clean flat limit. No general construction or existence proof for such gauges is supplied beyond the specific examples; if the gauge family does not exist for generic radiative solutions or introduces singularities in the flat limit, the claimed direct connection fails to hold.

    Authors: We appreciate the referee drawing attention to the foundational role of the gauge choice. The manuscript constructs the required null gauges explicitly for the algebraically special solutions under consideration (Robinson-Trautman spacetimes and accelerating black holes), where the radiative vector built from the Cotton and stress tensors is well-defined and the flat limit proceeds without introducing singularities. We do not claim a general existence theorem applicable to arbitrary radiative asymptotically locally AdS geometries; our results demonstrate the holographic link between bulk radiation and boundary dissipative corrections (including entropy production) within this concrete class of solutions that admit the necessary gauges. To clarify the scope and avoid any overstatement, we will revise the abstract and the algebraically special solutions section to state explicitly that the direct connection is established for solutions possessing such gauges. revision: yes

  2. Referee: [Flat limit and Carrollian section] Flat-limit discussion: the reinterpretation of the radiative vector as a Carrollian analogue that sources the viscous stress tensor and heat current encoding Bondi news assumes the flat limit preserves radiative information without loss or singularity. The manuscript does not demonstrate that this limit is well-defined for the full class of solutions considered, which is load-bearing for the Carrollian holography claim.

    Authors: We agree that the well-definedness of the flat limit is central to the Carrollian extension. In the manuscript the limit is carried out explicitly for the same algebraically special solutions (Robinson-Trautman and accelerating black holes), where the Carrollian analogue of the radiative vector is shown to source the viscous stress tensor and heat current that encodes the Bondi news, with no loss of radiative information or singularities encountered. While a general demonstration for every possible radiative solution would be desirable, the paper focuses on the class where the limit is manifestly well-defined and the Carrollian observables (including energy detectors) emerge naturally. We will add a brief discussion of the conditions under which the flat limit preserves the radiative data, together with a note on the illustrative nature of the examples. revision: partial

Circularity Check

0 steps flagged

No significant circularity; derivation remains self-contained.

full rationale

The paper's central results for algebraically special solutions are obtained by explicit computation in chosen null gauges applied to concrete examples (Robinson-Trautman, accelerating black holes). The radiative vector is assembled from the boundary Cotton tensor and stress tensor, then reinterpreted in fluid variables; the link to dissipative corrections and entropy production is presented as an outcome of this analysis rather than an identity built into the definitions. Gauge existence and flat-limit well-definedness are stated as working assumptions enabling the setup, not as derived claims that loop back on themselves. No self-citations, fitted parameters renamed as predictions, or ansatzes smuggled via prior work are invoked to force the main correspondence. The Carrollian flat-space extension follows the same pattern of construction from bulk data. The derivation chain therefore stands on independent content once the gauges are adopted.

Axiom & Free-Parameter Ledger

0 free parameters · 2 axioms · 2 invented entities

The central claims rest on the standard fluid/gravity and AdS/CFT correspondences as background assumptions, plus the new definitions of the radiative vector and its Carrollian counterpart introduced to organize the radiation data.

axioms (2)
  • domain assumption Asymptotically locally anti-de Sitter spacetimes can exhibit gravitational radiative behavior that is captured by boundary Cotton and stress tensors.
    This is the starting point for collecting the radiative content into a single vector.
  • domain assumption Null gauges exist that permit a well-defined flat limit while preserving the radiative structure.
    Required for the second half of the analysis.
invented entities (2)
  • radiative vector no independent evidence
    purpose: To collect the boundary Cotton tensor and stress tensor into a single object that encodes bulk radiation.
    New packaging introduced to enable the holographic reinterpretation.
  • Carrollian analogue of the radiative vector no independent evidence
    purpose: To carry the radiative information into the flat-space limit and source the viscous stress tensor and heat current.
    Constructed to extend the correspondence to Carrollian hydrodynamics.

pith-pipeline@v0.9.0 · 5746 in / 1689 out tokens · 71986 ms · 2026-05-21T23:51:45.309477+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Lean theorems connected to this paper

Citations machine-checked in the Pith Canon. Every link opens the source theorem in the public Lean library.

  • IndisputableMonolith/Foundation/AlexanderDuality.lean alexander_duality_circle_linking echoes
    ?
    echoes

    ECHOES: this paper passage has the same mathematical shape or conceptual pattern as the Recognition theorem, but is not a direct formal dependency.

    The radiative content in the bulk is captured by the boundary Cotton and stress tensor, which we collect into a radiative vector... bulk radiation sources the Carrollian viscous stress tensor and heat current, which encodes the Bondi news

  • IndisputableMonolith/Cost/FunctionalEquation.lean washburn_uniqueness_aczel unclear
    ?
    unclear

    Relation between the paper passage and the cited Recognition theorem.

    For algebraically special solutions, we uncover a close connection between bulk radiation and dissipative corrections in the boundary stress tensor, demonstrating a direct link between radiation and entropy production

What do these tags mean?
matches
The paper's claim is directly supported by a theorem in the formal canon.
supports
The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
extends
The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
uses
The paper appears to rely on the theorem as machinery.
contradicts
The paper's claim conflicts with a theorem or certificate in the canon.
unclear
Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Memory of Robinson-Trautman waves

    gr-qc 2026-04 unverdicted novelty 7.0

    Robinson-Trautman waves exhibit an explicit memory effect, with their news-free sector matching boosted rescaled Schwarzschild black holes and the vacuum sector of Euclidean Liouville theory.

  2. Quasinormal Modes of pp-Wave Spacetimes and Zero Temperature Dissipation

    gr-qc 2026-04 unverdicted novelty 7.0

    Scalar quasinormal modes on pp-wave spacetimes show zero-temperature dissipation for d >= 3 via an irregular singular point acting as absorber, with exact non-dissipative spectrum for d=2 and gapped modes proven by re...

  3. Entanglement Entropy and Thermodynamics of Dynamical Black Holes

    hep-th 2025-09 unverdicted novelty 5.0

    In f(R) theories, the replica-method gravitational entropy computed on the apparent horizon matches the Hollands-Wald-Zhang dynamical black hole entropy and satisfies the first law, while the event horizon does not; t...

Reference graph

Works this paper leans on

269 extracted references · 269 canonical work pages · cited by 3 Pith papers · 93 internal anchors

  1. [1]

    Dimensional Reduction in Quantum Gravity

    G. ’t Hooft,Dimensional reduction in quantum gravity, Conf. Proc. C930308 (1993) 284–296, [gr-qc/9310026]

    work page internal anchor Pith review Pith/arXiv arXiv 1993

  2. [2]

    The World as a Hologram

    L. Susskind,The World as a hologram, J. Math. Phys.36 (1995) 6377–6396, [hep-th/9409089]

    work page internal anchor Pith review Pith/arXiv arXiv 1995

  3. [3]

    J. M. Maldacena,The Large N limit of superconformal field theories and supergravity, Adv. Theor. Math. Phys.2 (1998) 231–252, [hep-th/9711200]

    work page internal anchor Pith review Pith/arXiv arXiv 1998

  4. [4]

    S. S. Gubser, I. R. Klebanov, and A. M. Polyakov,Gauge theory correlators from noncritical string theory, Phys. Lett. B428 (1998) 105–114, [hep-th/9802109]

    work page internal anchor Pith review Pith/arXiv arXiv 1998

  5. [5]

    Anti De Sitter Space And Holography

    E. Witten,Anti-de Sitter space and holography, Adv. Theor. Math. Phys.2 (1998) 253–291, [hep-th/9802150]

    work page internal anchor Pith review Pith/arXiv arXiv 1998

  6. [6]

    Robin,Conformal invariants, in ´Elie Cartan et les math´ ematiques d’aujourd’hui - Lyon, 25-29 juin 1984, no

    Fefferman, Charles and Graham, C. Robin,Conformal invariants, in ´Elie Cartan et les math´ ematiques d’aujourd’hui - Lyon, 25-29 juin 1984, no. S131 in Ast´ erisque. Soci´ et´ e math´ ematique de France, 1985

    work page 1984

  7. [7]

    Fefferman and C

    C. Fefferman and C. R. Graham,The ambient metric (AM-178). Princeton University Press, 2012

    work page 2012

  8. [8]

    AdS/CFT correspondence and Geometry

    I. Papadimitriou and K. Skenderis,AdS / CFT correspondence and geometry, IRMA Lect. Math. Theor. Phys.8 (2005) 73–101, [hep-th/0404176]

    work page internal anchor Pith review Pith/arXiv arXiv 2005

  9. [9]

    Quantum effective action from the AdS/CFT correspondence

    K. Skenderis and S. N. Solodukhin,Quantum effective action from the AdS / CFT correspondence, Phys. Lett. B472 (2000) 316–322, [hep-th/9910023]

    work page internal anchor Pith review Pith/arXiv arXiv 2000

  10. [10]

    Holographic Reconstruction of Spacetime and Renormalization in the AdS/CFT Correspondence

    S. de Haro, S. N. Solodukhin, and K. Skenderis,Holographic reconstruction of space-time and renormalization in the AdS / CFT correspondence, Commun. Math. Phys.217 (2001) 595–622, [hep-th/0002230]

    work page internal anchor Pith review Pith/arXiv arXiv 2001

  11. [11]

    M. T. Anderson,On the structure of conformally compact einstein metrics, 2010

    work page 2010

  12. [12]

    M. T. Anderson,Geometric aspects of the AdS / CFT correspondence, IRMA Lect. Math. Theor. Phys. 8 (2005) 1–31, [hep-th/0403087]

    work page internal anchor Pith review Pith/arXiv arXiv 2005

  13. [13]

    M. T. Anderson,On the uniqueness and global dynamics of AdS spacetimes, Class. Quant. Grav. 23 (2006) 6935–6954, [hep-th/0605293]

    work page internal anchor Pith review Pith/arXiv arXiv 2006

  14. [14]

    Serantes and B

    A. Serantes and B. Withers,Convergence of the Fefferman-Graham expansion and complex black hole anatomy, Class. Quant. Grav.39 (2022), no. 24 245010, [arXiv:2207.07132]

    work page arXiv 2022

  15. [15]

    J. D. Brown and M. Henneaux,Central Charges in the Canonical Realization of Asymptotic Symmetries: An Example from Three-Dimensional Gravity, Commun. Math. Phys.104 (1986) 207–226

    work page 1986

  16. [16]

    The Holographic Weyl anomaly

    M. Henningson and K. Skenderis,The Holographic Weyl anomaly, JHEP 07 (1998) 023, [hep-th/9806087]

    work page internal anchor Pith review Pith/arXiv arXiv 1998

  17. [17]

    A Stress Tensor for Anti-de Sitter Gravity

    V. Balasubramanian and P. Kraus,A Stress tensor for Anti-de Sitter gravity, Commun. Math. Phys. 208 (1999) 413–428, [hep-th/9902121]

    work page internal anchor Pith review Pith/arXiv arXiv 1999

  18. [18]

    Diffeomorphisms and Holographic Anomalies

    C. Imbimbo, A. Schwimmer, S. Theisen, and S. Yankielowicz,Diffeomorphisms and holographic anomalies, Class. Quant. Grav.17 (2000) 1129–1138, [hep-th/9910267]

    work page internal anchor Pith review Pith/arXiv arXiv 2000

  19. [19]

    Holonomies, anomalies and the Fefferman-Graham ambiguity in AdS3 gravity

    M. Rooman and P. Spindel,Holonomies, anomalies and the Fefferman-Graham ambiguity in AdS(3) gravity, Nucl. Phys. B594 (2001) 329–353, [hep-th/0008147]. – 57 –

    work page internal anchor Pith review Pith/arXiv arXiv 2001

  20. [20]

    Nonlinear Fluid Dynamics from Gravity

    S. Bhattacharyya, V. E. Hubeny, S. Minwalla, and M. Rangamani,Nonlinear Fluid Dynamics from Gravity, JHEP 02 (2008) 045, [arXiv:0712.2456]

    work page internal anchor Pith review Pith/arXiv arXiv 2008

  21. [21]

    V. E. Hubeny, M. Rangamani, and T. Takayanagi,A Covariant holographic entanglement entropy proposal, JHEP 07 (2007) 062, [arXiv:0705.0016]

    work page internal anchor Pith review Pith/arXiv arXiv 2007

  22. [22]

    D. T. Son and A. O. Starinets,Viscosity, Black Holes, and Quantum Field Theory, Ann. Rev. Nucl. Part. Sci.57 (2007) 95–118, [arXiv:0704.0240]

    work page internal anchor Pith review Pith/arXiv arXiv 2007

  23. [23]

    Local Fluid Dynamical Entropy from Gravity

    S. Bhattacharyya, V. E. Hubeny, R. Loganayagam, G. Mandal, S. Minwalla, T. Morita, M. Rangamani, and H. S. Reall,Local Fluid Dynamical Entropy from Gravity, JHEP 06 (2008) 055, [arXiv:0803.2526]

    work page internal anchor Pith review Pith/arXiv arXiv 2008

  24. [24]

    Nonlinear viscous hydrodynamics in various dimensions using AdS/CFT

    M. Haack and A. Yarom,Nonlinear viscous hydrodynamics in various dimensions using AdS/CFT, JHEP 10 (2008) 063, [arXiv:0806.4602]

    work page internal anchor Pith review Pith/arXiv arXiv 2008

  25. [25]

    Hydrodynamics from charged black branes

    N. Banerjee, J. Bhattacharya, S. Bhattacharyya, S. Dutta, R. Loganayagam, and P. Surowka,Hydrodynamics from charged black branes, JHEP 01 (2011) 094, [arXiv:0809.2596]

    work page internal anchor Pith review Pith/arXiv arXiv 2011

  26. [26]

    Gravity & Hydrodynamics: Lectures on the fluid-gravity correspondence

    M. Rangamani,Gravity and Hydrodynamics: Lectures on the fluid-gravity correspondence, Class. Quant. Grav.26 (2009) 224003, [arXiv:0905.4352]

    work page internal anchor Pith review Pith/arXiv arXiv 2009

  27. [27]

    V. E. Hubeny, S. Minwalla, and M. Rangamani,The fluid/gravity correspondence, in Theoretical Advanced Study Institute in Elementary Particle Physics: String theory and its Applications: From meV to the Planck Scale, pp. 348–383, 2012.arXiv:1107.5780

    work page internal anchor Pith review Pith/arXiv arXiv 2012

  28. [28]

    From Navier-Stokes To Einstein

    I. Bredberg, C. Keeler, V. Lysov, and A. Strominger,From Navier-Stokes To Einstein, JHEP 07 (2012) 146, [arXiv:1101.2451]

    work page internal anchor Pith review Pith/arXiv arXiv 2012

  29. [29]

    The holographic fluid dual to vacuum Einstein gravity

    G. Compere, P. McFadden, K. Skenderis, and M. Taylor,The Holographic fluid dual to vacuum Einstein gravity, JHEP 07 (2011) 050, [arXiv:1103.3022]

    work page internal anchor Pith review Pith/arXiv arXiv 2011

  30. [30]

    The relativistic fluid dual to vacuum Einstein gravity

    G. Compere, P. McFadden, K. Skenderis, and M. Taylor,The relativistic fluid dual to vacuum Einstein gravity, JHEP 03 (2012) 076, [arXiv:1201.2678]

    work page internal anchor Pith review Pith/arXiv arXiv 2012

  31. [31]

    M. M. Caldarelli, J. Camps, B. Gout´ eraux, and K. Skenderis,AdS/Ricci-flat correspondence, JHEP 04 (2014) 071, [arXiv:1312.7874]

    work page internal anchor Pith review Pith/arXiv arXiv 2014

  32. [32]

    Towards a general fluid/gravity correspondence

    N. Pinzani-Fokeeva and M. Taylor,Towards a general fluid/gravity correspondence, Phys. Rev. D 91 (2015), no. 4 044001, [arXiv:1401.5975]

    work page internal anchor Pith review Pith/arXiv arXiv 2015

  33. [33]

    Second-order transport, quasinormal modes and zero-viscosity limit in the Gauss-Bonnet holographic fluid

    S. Grozdanov and A. O. Starinets,Second-order transport, quasinormal modes and zero-viscosity limit in the Gauss-Bonnet holographic fluid, JHEP 03 (2017) 166, [arXiv:1611.07053]

    work page internal anchor Pith review Pith/arXiv arXiv 2017

  34. [34]

    Holographic Thermodynamics of Accelerating Black Holes

    A. Anabal´ on, M. Appels, R. Gregory, D. Kubizˇ n´ ak, R. B. Mann, and A. Ovg¨ un, Holographic Thermodynamics of Accelerating Black Holes, Phys. Rev. D98 (2018), no. 10 104038, [arXiv:1805.02687]

    work page internal anchor Pith review Pith/arXiv arXiv 2018

  35. [35]

    R. E. Hoult and P. Kovtun,Causal first-order hydrodynamics from kinetic theory and holography, Phys. Rev. D106 (2022), no. 6 066023, [arXiv:2112.14042]

    work page arXiv 2022

  36. [36]

    Ciambelli and L

    L. Ciambelli and L. Lehner,Fluid-gravity correspondence and causal first-order relativistic viscous hydrodynamics, Phys. Rev. D108 (2023), no. 12 126019, [arXiv:2310.15427]

    work page arXiv 2023

  37. [37]

    From AdS/CFT correspondence to hydrodynamics

    G. Policastro, D. T. Son, and A. O. Starinets,From AdS / CFT correspondence to hydrodynamics, JHEP 09 (2002) 043, [hep-th/0205052]. – 58 –

    work page internal anchor Pith review Pith/arXiv arXiv 2002

  38. [38]

    Energy-momentum/Cotton tensor duality for AdS4 black holes

    I. Bakas,Energy-momentum/Cotton tensor duality for AdS(4) black holes, JHEP 01 (2009) 003, [arXiv:0809.4852]

    work page internal anchor Pith review Pith/arXiv arXiv 2009

  39. [39]

    V. E. Hubeny and M. Rangamani,A Holographic view on physics out of equilibrium, Adv. High Energy Phys.2010 (2010) 297916, [arXiv:1006.3675]

    work page internal anchor Pith review Pith/arXiv arXiv 2010

  40. [40]

    M. M. Caldarelli, R. G. Leigh, A. C. Petkou, P. M. Petropoulos, V. Pozzoli, and K. Siampos,Vorticity in holographic fluids, PoS CORFU2011 (2011) 076, [arXiv:1206.4351]

    work page internal anchor Pith review Pith/arXiv arXiv 2011

  41. [41]

    R. G. Leigh, A. C. Petkou, and P. M. Petropoulos,Holographic Fluids with Vorticity and Analogue Gravity, JHEP 11 (2012) 121, [arXiv:1205.6140]

    work page internal anchor Pith review Pith/arXiv arXiv 2012

  42. [42]

    Holographic perfect fluidity, Cotton energy-momentum duality and transport properties

    A. Mukhopadhyay, A. C. Petkou, P. M. Petropoulos, V. Pozzoli, and K. Siampos, Holographic perfect fluidity, Cotton energy-momentum duality and transport properties, JHEP 04 (2014) 136, [arXiv:1309.2310]

    work page internal anchor Pith review Pith/arXiv arXiv 2014

  43. [43]

    Non-equilibrium dynamics and $AdS_4$ Robinson-Trautman

    I. Bakas and K. Skenderis,Non-equilibrium dynamics andAdS4 Robinson-Trautman, JHEP 08 (2014) 056, [arXiv:1404.4824]

    work page internal anchor Pith review Pith/arXiv arXiv 2014

  44. [44]

    P. M. Petropoulos and K. Siampos,Integrability, Einstein spaces and holographic fluids, arXiv:1510.06456

    work page internal anchor Pith review Pith/arXiv arXiv

  45. [45]

    J. Gath, A. Mukhopadhyay, A. C. Petkou, P. M. Petropoulos, and K. Siampos,Petrov Classification and holographic reconstruction of spacetime, JHEP 09 (2015) 005, [arXiv:1506.04813]

    work page internal anchor Pith review Pith/arXiv arXiv 2015

  46. [46]

    The Robinson-Trautman spacetime and its holographic fluid

    L. Ciambelli, A. C. Petkou, P. M. Petropoulos, and K. Siampos,The Robinson-Trautman spacetime and its holographic fluid, PoS CORFU2016 (2017) 076, [arXiv:1707.02995]

    work page internal anchor Pith review Pith/arXiv arXiv 2017

  47. [47]

    Robinson-Trautman spacetimes and gauge/gravity duality

    K. Skenderis and B. Withers,Robinson-Trautman spacetimes and gauge/gravity duality, PoS CORFU2016 (2017) 097, [arXiv:1703.10865]

    work page internal anchor Pith review Pith/arXiv arXiv 2017

  48. [48]

    Asymptotically Anti-de Sitter Space-times: Conserved Quantities

    A. Ashtekar and S. Das,Asymptotically Anti-de Sitter space-times: Conserved quantities, Class. Quant. Grav.17 (2000) L17–L30, [hep-th/9911230]

    work page internal anchor Pith review Pith/arXiv arXiv 2000

  49. [49]

    ´E. Cotton,Sur les vari´ et´ es ` a trois dimensions, Annales de la Facult´ e des sciences de l’Universit´ e de Toulouse pour les sciences math´ ematiques et les sciences physiques1 (1899), no. 4 385–438

    work page

  50. [50]

    Algebraically special solutions in AdS/CFT

    G. Bernardi de Freitas and H. S. Reall,Algebraically special solutions in AdS/CFT, JHEP 06 (2014) 148, [arXiv:1403.3537]

    work page internal anchor Pith review Pith/arXiv arXiv 2014

  51. [51]

    P. M. Petropoulos,Gravitational duality, topologically massive gravity and holographic fluids, Lect. Notes Phys.892 (2015) 331–367, [arXiv:1406.2328]

    work page internal anchor Pith review Pith/arXiv arXiv 2015

  52. [52]

    Dual Gravitons in AdS4/CFT3 and the Holographic Cotton Tensor

    S. de Haro,Dual Gravitons in AdS(4) / CFT(3) and the Holographic Cotton Tensor, JHEP 01 (2009) 042, [arXiv:0808.2054]

    work page internal anchor Pith review Pith/arXiv arXiv 2009

  53. [53]

    R. G. Leigh, A. C. Petkou, and P. M. Petropoulos,Holographic Three-Dimensional Fluids with Nontrivial Vorticity, Phys. Rev. D85 (2012) 086010, [arXiv:1108.1393]

    work page internal anchor Pith review Pith/arXiv arXiv 2012

  54. [54]

    Kalamakis, R

    G. Kalamakis, R. G. Leigh, and A. C. Petkou,Aspects of holography of Taub-NUT- AdS4 spacetimes, Phys. Rev. D103 (2021), no. 12 126012, [arXiv:2009.08022]

    work page arXiv 2021

  55. [55]

    Ciambelli, C

    L. Ciambelli, C. Corral, J. Figueroa, G. Giribet, and R. Olea,Topological Terms and the Misner String Entropy, Phys. Rev. D103 (2021), no. 2 024052, [arXiv:2011.11044]

    work page arXiv 2021

  56. [56]

    Kalamakis and A

    G. Kalamakis and A. C. Petkou,Remarks on the quasinormal modes of Taub-NUT-AdS4, arXiv:2503.21001. – 59 –

    work page arXiv

  57. [57]

    Adami, M

    H. Adami, M. M. Sheikh-Jabbari, and V. Taghiloo,Gravitational stress tensor and current at null infinity in three dimensions, Phys. Lett. B855 (2024) 138835, [arXiv:2405.00149]

    work page arXiv 2024

  58. [58]

    Arenas-Henriquez, F

    G. Arenas-Henriquez, F. Diaz, and D. Rivera-Betancour,Generalized Fefferman-Graham gauge and boundary Weyl structures, JHEP 02 (2025) 007, [arXiv:2411.12513]

    work page arXiv 2025

  59. [59]

    Roychowdhury,Metallic transports from accelerating black holes, JHEP 01 (2025) 134, [arXiv:2411.15474]

    D. Roychowdhury,Metallic transports from accelerating black holes, JHEP 01 (2025) 134, [arXiv:2411.15474]

    work page arXiv 2025

  60. [60]

    Luo,Holography dual of accelerating and rotating black hole in Nariai limit, arXiv:2412.21013

    S. Luo,Holography dual of accelerating and rotating black hole in Nariai limit, arXiv:2412.21013

    work page arXiv

  61. [61]

    R. G. Leigh and A. C. Petkou,Gravitational duality transformations on (A)dS(4), JHEP 11 (2007) 079, [arXiv:0704.0531]

    work page internal anchor Pith review Pith/arXiv arXiv 2007

  62. [62]

    Bondi,Gravitational Waves in General Relativity, Nature 186 (1960), no

    H. Bondi,Gravitational Waves in General Relativity, Nature 186 (1960), no. 4724 535–535

    work page 1960

  63. [63]

    R. K. Sachs,Gravitational waves in general relativity. 6. The outgoing radiation condition, Proc. Roy. Soc. Lond. A264 (1961) 309–338

    work page 1961

  64. [64]

    Bondi, M

    H. Bondi, M. G. J. van der Burg, and A. W. K. Metzner,Gravitational waves in general relativity. 7. Waves from axisymmetric isolated systems, Proc. Roy. Soc. Lond. A269 (1962) 21–52

    work page 1962

  65. [65]

    R. K. Sachs,Gravitational waves in general relativity. 8. Waves in asymptotically flat space-times, Proc. Roy. Soc. Lond. A270 (1962) 103–126

    work page 1962

  66. [66]

    Newman and R

    E. Newman and R. Penrose,An Approach to gravitational radiation by a method of spin coefficients, J. Math. Phys.3 (1962) 566–578

    work page 1962

  67. [67]

    Geroch,Asymptotic Structure of Space-Time, inSymposium on Asymptotic Structure of Space-Time, 1977

    R. Geroch,Asymptotic Structure of Space-Time, inSymposium on Asymptotic Structure of Space-Time, 1977

    work page 1977

  68. [68]

    Ashtekar and M

    A. Ashtekar and M. Streubel,Symplectic Geometry of Radiative Modes and Conserved Quantities at Null Infinity, Proc. Roy. Soc. Lond. A376 (1981) 585–607

    work page 1981

  69. [69]

    Ashtekar,Radiative Degrees of Freedom of the Gravitational Field in Exact General Relativity, J

    A. Ashtekar,Radiative Degrees of Freedom of the Gravitational Field in Exact General Relativity, J. Math. Phys.22 (1981) 2885–2895

    work page 1981

  70. [70]

    R. M. Wald and A. Zoupas,A General definition of ’conserved quantities’ in general relativity and other theories of gravity, Phys. Rev. D61 (2000) 084027, [gr-qc/9911095]

    work page internal anchor Pith review Pith/arXiv arXiv 2000

  71. [71]

    Geometry and Physics of Null Infinity

    A. Ashtekar,Geometry and physics of null infinity, Surveys Diff. Geom.20 (2015), no. 1 99–122, [arXiv:1409.1800]

    work page internal anchor Pith review Pith/arXiv arXiv 2015

  72. [72]

    ´E. ´E. Flanagan and D. A. Nichols,Conserved charges of the extended Bondi-Metzner-Sachs algebra, Phys. Rev. D95 (2017), no. 4 044002, [arXiv:1510.03386]. [Erratum: Phys.Rev.D 108, 069902 (2023)]

    work page arXiv 2017

  73. [73]

    Fern´ andez-´Alvarez and J

    F. Fern´ andez-´Alvarez and J. M. M. Senovilla,Novel characterization of gravitational radiation in asymptotically flat spacetimes, Phys. Rev. D101 (2020), no. 2 024060, [arXiv:1909.13796]

    work page arXiv 2020

  74. [74]

    Bondi-Sachs Formalism

    T. M¨ adler and J. Winicour,Bondi-Sachs Formalism, Scholarpedia 11 (2016) 33528, [arXiv:1609.01731]

    work page internal anchor Pith review Pith/arXiv arXiv 2016

  75. [75]

    Fern´ andez-´Alvarez and J

    F. Fern´ andez-´Alvarez and J. M. M. Senovilla,Gravitational radiation condition at infinity with a positive cosmological constant, Phys. Rev. D102 (2020), no. 10 101502, [arXiv:2007.11677]. – 60 –

    work page arXiv 2020

  76. [76]

    Fern´ andez-´Alvarez and J

    F. Fern´ andez-´Alvarez and J. M. M. Senovilla,Asymptotic structure with a positive cosmological constant, Class. Quant. Grav.39 (2022), no. 16 165012, [arXiv:2105.09167]

    work page arXiv 2022

  77. [77]

    Fern´ andez-´Alvarez and J

    F. Fern´ andez-´Alvarez and J. M. M. Senovilla,Asymptotic structure with vanishing cosmological constant, Class. Quant. Grav.39 (2022), no. 16 165011, [arXiv:2105.09166]

    work page arXiv 2022

  78. [78]

    Fern´ andez-´Alvarez, J

    F. Fern´ andez-´Alvarez, J. Podolsk´ y, and J. M. M. Senovilla,Analysis of gravitational radiation generated by type D black holes with positive cosmological constant, Phys. Rev. D 110 (2024), no. 10 104029, [arXiv:2407.14863]

    work page arXiv 2024

  79. [79]

    Ciambelli, S

    L. Ciambelli, S. Pasterski, and E. Tabor,Radiation in holography, JHEP 09 (2024) 124, [arXiv:2404.02146]

    work page arXiv 2024

  80. [80]

    Fern´ andez-´Alvarez and J

    F. Fern´ andez-´Alvarez and J. M. M. Senovilla,Gravitational radiation at infinity with negative cosmological constant and AdS4 holography, arXiv:2507.05826

    work page arXiv

Showing first 80 references.