pith. machine review for the scientific record. sign in

arxiv: 2605.13804 · v1 · submitted 2026-05-13 · ✦ hep-th · gr-qc· math-ph· math.MP

Recognition: unknown

An algebra of proper observables at null infinity: Dirac brackets, Memory and Goldstone probes

Rodrigo Andrade e Silva, Simone Speziale

Pith reviewed 2026-05-14 17:36 UTC · model grok-4.3

classification ✦ hep-th gr-qcmath-phmath.MP
keywords null infinityDirac bracketsmemory effectsGoldstone probessupertranslationsproper observablesAshtekar-Streubel phase spacegravitational radiation
0
0 comments X

The pith

The conventional Goldstone mode at null infinity is not a proper observable, but an infinite family of Goldstone probes can measure it.

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

This paper identifies the algebra of proper observables on the phase space of radiative gravitational modes at null infinity. It works on the Ashtekar-Streubel phase space under boundary conditions of vanishing news and purely electric shear. Supertranslation charges are shown to generate the expected transformations on the shear. The standard definition of the Goldstone mode cannot be associated with a proper observable, defined as a function admitting a smooth symplectic flow, yet an infinite family of other proper observables called Goldstone probes can measure the mode. No Goldstone probes can be built solely from the shear or the news, and the paper derives distributional Dirac brackets between local shear and news that include non-local corrections.

Core claim

On the Ashtekar-Streubel phase space with vanishing news and purely electric shear, the conventional Goldstone mode cannot be associated with a proper observable, but an infinite family of proper observables called Goldstone probes exist that are capable of measuring the Goldstone mode. There are no Goldstone probes constructed only out of the shear or the news.

What carries the argument

Proper observables, defined as functions on the infinite-dimensional phase space that can be associated with smooth symplectic flows, together with the derived algebra and the Goldstone probes built from them.

If this is right

  • Supertranslation charges generate the correct transformations on the shear.
  • The Dirac brackets between local shear and news contain non-local corrections.
  • A separable Hilbert space with distinct memory states cannot be built using observables constructed only from shear or news.
  • Memory effects require observables that mix shear and news in non-local ways.

Where Pith is reading between the lines

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

  • Memory measurements in gravitational wave data may need to incorporate these non-local Goldstone probes rather than local field values.
  • The result suggests that quantum treatments of soft hair must track the full algebra of proper observables to separate memory sectors.
  • Similar analysis could be applied to other asymptotic symmetries such as superrotations to identify their corresponding probes.

Load-bearing premise

Boundary conditions in time require vanishing news and purely electric shear on the Ashtekar-Streubel phase space.

What would settle it

An explicit construction of even one Goldstone probe using only the shear or only the news, or a demonstration that the conventional Goldstone mode generates a smooth symplectic flow, would falsify the central claim.

read the original abstract

We develop a rigorous evaluation of Dirac brackets for classical observables on the phase space of radiative gravitational modes at null infinity that naturally incorporates memory effects. Considering the Ashtekar-Streubel phase space, with boundary conditions in time given by vanishing {\it news} and purely electric {\it shear}, and taking into account the infinite dimensionality of the phase space, we identify the algebra of proper observables (understood as functions on phase space that can be associated with smooth symplectic flows). We show that the action of supertranslation charges generate the correct transformations on the shear. We also show that the conventional definition of the ``Goldstone mode'' adopted in the literature cannot be associated with a proper observable, but nevertheless there exists an infinite family of proper observables, which we call {\it Goldstone probes}, that are capable of measuring the Goldstone mode. We notice that there are no Goldstone probes constructed only out of the shear {\it or} the news, providing a possible explanation for why attempts to construct a (separable) Hilbert space with different memory states have failed so far. Finally, we derive formulas for distributional Dirac brackets between local shear and news, and show that they contain non-local corrections.

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 / 1 minor

Summary. The paper develops the algebra of proper observables on the Ashtekar-Streubel phase space of radiative gravitational modes at null infinity, with boundary conditions of vanishing news and purely electric shear. It computes Dirac brackets for these observables, verifies that supertranslation charges generate the correct transformations on the shear, shows that the conventional Goldstone mode is not a proper observable, introduces an infinite family of Goldstone probes capable of measuring it, observes that no such probes exist constructed solely from shear or news, and derives distributional Dirac brackets between local shear and news that include non-local corrections.

Significance. If the central results hold, the work supplies a rigorous treatment of proper observables and Dirac brackets in asymptotic gravity that incorporates memory effects, clarifies why separable Hilbert-space constructions for distinct memory states have been difficult, and provides explicit formulas for non-local corrections in the brackets. The identification of Goldstone probes as an infinite family of proper observables is a concrete advance in the phase-space analysis of null-infinity symmetries.

major comments (2)
  1. [Discussion of Goldstone probes and boundary conditions] The claim that no Goldstone probes can be constructed solely from the shear or the news (abstract and final paragraph) rests on the time-boundary conditions of vanishing news and purely electric shear at all times. These conditions integrate the news to zero at late times and fix the memory sector; the paper does not show that the absence of shear-only or news-only probes survives under relaxed conditions (e.g., non-vanishing late-time news or magnetic shear components). This is load-bearing for the explanation offered for failed Hilbert-space constructions.
  2. [Definition of proper observables] The definition of a 'proper observable' as a function on phase space associated with a smooth symplectic flow is used to exclude the conventional Goldstone mode and to construct the probes. The infinite-dimensional character of the phase space makes the smoothness requirement delicate; the manuscript should supply an explicit check that the flows generated by the proposed Goldstone probes remain smooth under the stated boundary conditions.
minor comments (1)
  1. [Abstract] The abstract states that the supertranslation charges 'generate the correct transformations on the shear'; an explicit equation or section reference for this verification would improve readability.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We are grateful to the referee for their thorough review and valuable suggestions. We respond to the major comments point by point below.

read point-by-point responses
  1. Referee: The claim that no Goldstone probes can be constructed solely from the shear or the news (abstract and final paragraph) rests on the time-boundary conditions of vanishing news and purely electric shear at all times. These conditions integrate the news to zero at late times and fix the memory sector; the paper does not show that the absence of shear-only or news-only probes survives under relaxed conditions (e.g., non-vanishing late-time news or magnetic shear components). This is load-bearing for the explanation offered for failed Hilbert-space constructions.

    Authors: We agree that the claim regarding the absence of Goldstone probes constructed solely from shear or news is specific to the boundary conditions of vanishing news and purely electric shear at all times, as stated throughout the manuscript. These conditions are the standard choice for the Ashtekar-Streubel phase space of radiative modes and are essential for fixing the memory sector in the manner relevant to the Hilbert-space construction difficulties we discuss. We do not claim that the absence of such probes persists under relaxed conditions (e.g., non-vanishing late-time news or magnetic shear). We will add a clarifying paragraph emphasizing the dependence on these boundary conditions and noting that extensions to relaxed settings lie beyond the present scope. This constitutes a partial revision. revision: partial

  2. Referee: The definition of a 'proper observable' as a function on phase space associated with a smooth symplectic flow is used to exclude the conventional Goldstone mode and to construct the probes. The infinite-dimensional character of the phase space makes the smoothness requirement delicate; the manuscript should supply an explicit check that the flows generated by the proposed Goldstone probes remain smooth under the stated boundary conditions.

    Authors: We acknowledge that the infinite-dimensional nature of the phase space makes the smoothness of symplectic flows a delicate issue that merits explicit verification. The manuscript defines proper observables via association with smooth symplectic flows and constructs the Goldstone probes on that basis, but we agree that a direct check would strengthen the argument. In the revised version we will supply an explicit verification demonstrating that the flows generated by the proposed probes remain smooth under the stated boundary conditions of vanishing news and purely electric shear. This material will be added to the main text or as an appendix. revision: yes

Circularity Check

0 steps flagged

No significant circularity: claims follow from explicit Dirac bracket calculations on the stated phase space

full rationale

The paper takes the Ashtekar-Streubel phase space with explicitly stated boundary conditions (vanishing news and purely electric shear) as input and performs new calculations of Dirac brackets to define the algebra of proper observables (functions generating smooth symplectic flows). The result that the conventional Goldstone mode is not proper while an infinite family of Goldstone probes exists, and that none are built solely from shear or news, is obtained by direct evaluation of the brackets and the action of supertranslation charges on the shear; these steps do not reduce by definition or by construction to the input data or to any self-citation. The cited prior phase-space construction is independent (externally defined and falsifiable) and is not invoked as a uniqueness theorem that forces the new conclusions. No fitted parameters are renamed as predictions, and no ansatz is smuggled via self-citation.

Axiom & Free-Parameter Ledger

0 free parameters · 1 axioms · 1 invented entities

The paper rests on the Ashtekar-Streubel phase space together with specific boundary conditions; it introduces the new concept of Goldstone probes without independent evidence outside the construction itself.

axioms (1)
  • domain assumption Ashtekar-Streubel phase space with vanishing news and purely electric shear as boundary conditions in time
    Stated explicitly in the abstract as the setting for the analysis.
invented entities (1)
  • Goldstone probes no independent evidence
    purpose: Infinite family of proper observables capable of measuring the Goldstone mode
    Introduced in the paper as observables that can detect the mode even though the conventional Goldstone mode itself is not proper.

pith-pipeline@v0.9.0 · 5519 in / 1262 out tokens · 41550 ms · 2026-05-14T17:36:45.889795+00:00 · methodology

discussion (0)

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

Reference graph

Works this paper leans on

58 extracted references · 40 canonical work pages · 12 internal anchors

  1. [1]

    Ashtekar,Asymptotic Quantization of the Gravitational Field, Phys

    A. Ashtekar,Asymptotic Quantization of the Gravitational Field, Phys. Rev. Lett.46(1981) 573–576

  2. [2]

    Ashtekar,Asymptotic quantization : based on 1984 Naples lectures / Abhay Ashtekar

    A. Ashtekar,Asymptotic quantization : based on 1984 Naples lectures / Abhay Ashtekar. Monographs and textbooks in physical science. Bibliopolis, Napoli, 1987

  3. [3]

    T. He, V. Lysov, P. Mitra and A. Strominger,BMS supertranslations and Weinberg’s soft graviton theorem, JHEP05(2015) 151 [1401.7026]

  4. [4]

    Lectures on the Infrared Structure of Gravity and Gauge Theory

    A. Strominger,Lectures on the Infrared Structure of Gravity and Gauge Theory,1703.05448

  5. [5]

    Null infinity, the BMS group and infrared issues

    A. Ashtekar, M. Campiglia and A. Laddha,Null infinity, the BMS group and infrared issues, Gen. Rel. Grav.50(2018), no. 11 140–163 [1808.07093]. 72

  6. [6]

    Prabhu, G

    K. Prabhu, G. Satishchandran and R. M. Wald,Infrared finite scattering theory in quantum field theory and quantum gravity, Phys. Rev. D106(2022), no. 6 066005 [2203.14334]

  7. [7]

    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

  8. [8]

    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

  9. [9]

    Ashtekar, L

    A. Ashtekar, L. Bombelli and O. Reula,The covariant phase space of asymptotically flat gravitational fields, inMechanics, Analysis and Geometry: 200 Years After Lagrange(M. Francaviglia, ed.), North-Holland Delta Series, pp. 417 – 450. Elsevier, Amsterdam, 1991

  10. [10]

    C. G. Torre,Null Surface Geometrodynamics, Class. Quant. Grav.3(1986) 773

  11. [11]

    Light-Front Quantisation as an Initial-Boundary Value Problem

    T. Heinzl and E. Werner,Light front quantization as an initial boundary value problem, Z. Phys. C62(1994) 521–532 [hep-th/9311108]

  12. [12]

    Light-Cone Quantization: Foundations and Applications

    T. Heinzl,Light cone quantization: Foundations and applications, Lect. Notes Phys.572(2001) 55–142 [hep-th/0008096]

  13. [13]

    First order gravity on the light front

    S. Alexandrov and S. Speziale,First order gravity on the light front, Phys. Rev. D91(2015), no. 6 064043 [1412.6057]

  14. [14]

    Sachs' free data in real connection variables

    E. De Paoli and S. Speziale,Sachs free data in real connection variables, JHEP11(2017) 205 [1707.00667]

  15. [15]

    Barnich, S

    G. Barnich, S. Majumdar, S. Speziale and W.-D. Tan,Lessons from discrete light-cone quantization for physics at null infinity: bosons in two dimensions, JHEP05(2024) 326 [2401.14873]

  16. [16]

    Christodoulou,Nonlinear nature of gravitation and gravitational wave experiments, Phys

    D. Christodoulou,Nonlinear nature of gravitation and gravitational wave experiments, Phys. Rev. Lett.67(1991) 1486–1489

  17. [17]

    Global aspects of radiation memory

    J. Winicour,Global aspects of radiation memory, Class. Quant. Grav.31 (2014) 205003 [1407.0259]

  18. [18]

    Bieri,New Effects in Gravitational Waves and Memory, Phys

    L. Bieri,New Effects in Gravitational Waves and Memory, Phys. Rev. D103 (2021), no. 2 024043 [2010.09207]. 73

  19. [19]

    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

  20. [20]

    Sachs,Asymptotic symmetries in gravitational theory, Phys

    R. Sachs,Asymptotic symmetries in gravitational theory, Phys. Rev.128 (1962) 2851–2864

  21. [21]

    E. T. Newman and R. Penrose,Note on the Bondi-Metzner-Sachs group, J. Math. Phys.7(1966) 863–870

  22. [22]

    Geroch,Asymptotic Structure of Space-Time, ch

    R. Geroch,Asymptotic Structure of Space-Time, ch. 1, pp. 1–106. Springer US, Boston, MA, 1977

  23. [23]

    Speziale,GGI lectures on boundary and asymptotic symmetries, 2512.16810

    S. Speziale,GGI lectures on boundary and asymptotic symmetries, 2512.16810

  24. [24]

    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]

  25. [25]

    BMS charge algebra

    G. Barnich and C. Troessaert,BMS charge algebra, JHEP12(2011) 105 [1106.0213]

  26. [26]

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

  27. [27]

    A. M. Grant, K. Prabhu and I. Shehzad,The Wald-Zoupas prescription for asymptotic charges at null infinity in general relativity, Class. Quant. Grav. 39(2022), no. 8 085002 [2105.05919]

  28. [28]

    Chandrasekaran, E

    V. Chandrasekaran, E. E. Flanagan, I. Shehzad and A. J. Speranza,A general framework for gravitational charges and holographic renormalization, Int. J. Mod. Phys. A37(2022), no. 17 2250105 [2111.11974]

  29. [29]

    G. Odak, A. Rignon-Bret and S. Speziale,Wald-Zoupas prescription with soft anomalies, Phys. Rev. D107(2023), no. 8 084028 [2212.07947]

  30. [30]

    Rignon-Bret and S

    A. Rignon-Bret and S. Speziale,Centerless BMS charge algebra, Phys. Rev. D 110(2024), no. 4 044050 [2405.01526]

  31. [31]

    Ashtekar and S

    A. Ashtekar and S. Speziale,Null infinity and horizons: A new approach to fluxes and charges, Phys. Rev. D110(2024), no. 4 044049 [2407.03254]. 74

  32. [32]

    Penrose and W

    R. Penrose and W. Rindler,Spinors And Space-Time. Vol. 2: Spinor And Twistor Methods In Space-Time Geometry. CUP, 1986

  33. [33]

    Comp` ere, A

    G. Comp` ere, A. Fiorucci and R. Ruzziconi,Superboost transitions, refraction memory and super-Lorentz charge algebra, JHEP11(2018) 200 [1810.00377]. [Erratum: JHEP 04, 172 (2020)]

  34. [34]

    Rignon-Bret and S

    A. Rignon-Bret and S. Speziale,Spatially local energy density of gravitational waves, JHEP03(2025) 048 [2405.08808]

  35. [35]

    Bourbaki,Topological vector spaces: Chapters 1–5

    N. Bourbaki,Topological vector spaces: Chapters 1–5. Springer Science & Business Media, 2013

  36. [36]

    Rignon-Bret and S

    A. Rignon-Bret and S. Speziale,General covariance and boundary symmetry algebras, EPL149(2025), no. 6 69002 [2403.00730]

  37. [37]

    Supertranslations call for superrotations

    G. Barnich and C. Troessaert,Supertranslations call for superrotations, PoS CNCFG2010(2010) 010 [1102.4632]

  38. [38]

    Asymptotic symmetries and subleading soft graviton theorem

    M. Campiglia and A. Laddha,Asymptotic symmetries and subleading soft graviton theorem, Phys. Rev. D90(2014), no. 12 124028 [1408.2228]

  39. [39]

    Freidel, R

    L. Freidel, R. Oliveri, D. Pranzetti and S. Speziale,The Weyl BMS group and Einstein’s equations, JHEP07(2021) 170 [2104.05793]

  40. [40]

    Campiglia and A

    M. Campiglia and A. Sudhakar,Gravitational Poisson brackets at null infinity compatible with smooth superrotations, JHEP12(2024) 170 [2408.13067]

  41. [41]

    Himwich, S

    E. Himwich, S. A. Narayanan, M. Pate, N. Paul and A. Strominger,The Soft S-Matrix in Gravity, JHEP09(2020) 129 [2005.13433]

  42. [42]

    Arkani-Hamed, M

    N. Arkani-Hamed, M. Pate, A.-M. Raclariu and A. Strominger,Celestial amplitudes from UV to IR, JHEP08(2021) 062 [2012.04208]

  43. [43]

    Campiglia and A

    M. Campiglia and A. Laddha,BMS Algebra, Double Soft Theorems, and All That,2106.14717

  44. [44]

    Campiglia and J

    M. Campiglia and J. Peraza,Generalized BMS charge algebra, Phys. Rev. D 101(2020), no. 10 104039 [2002.06691]

  45. [45]

    Guevara, E

    A. Guevara, E. Himwich, M. Pate and A. Strominger,Holographic symmetry algebras for gauge theory and gravity, JHEP11(2021) 152 [2103.03961]. 75

  46. [46]

    Donnay, K

    L. Donnay, K. Nguyen and R. Ruzziconi,Loop-corrected subleading soft theorem and the celestial stress tensor, JHEP09(2022) 063 [2205.11477]

  47. [47]

    Ciambelli, L

    L. Ciambelli, L. Freidel and R. G. Leigh,Quantum null geometry and gravity, JHEP12(2024) 028 [2407.11132]

  48. [48]

    Freidel, D

    L. Freidel, D. Pranzetti and A.-M. Raclariu,A discrete basis for celestial holography, JHEP02(2024) 176 [2212.12469]

  49. [49]

    Riello and M

    A. Riello and M. Schiavina,Null Hamiltonian Yang-Mills theory: Soft symmetries and memory as superselection,2303.03531

  50. [50]

    Prabhu and G

    K. Prabhu and G. Satishchandran,Infrared finite scattering theory: scattering states and representations of the BMS group, JHEP08(2024) 055 [2402.00102]

  51. [51]

    Prabhu and G

    K. Prabhu and G. Satishchandran,Infrared finite scattering theory: Amplitudes and soft theorems, Phys. Rev. D110(2024), no. 8 085022 [2402.18637]

  52. [52]

    Agrawal and K

    S. Agrawal and K. Nguyen,Soft theorems and spontaneous symmetry breaking, Phys. Rev. D112(2025), no. 2 L021903 [2504.10577]

  53. [53]

    Donnay and Y

    L. Donnay and Y. Herfray,Infrared physics of QED and gravity from representation theory,2603.06297

  54. [54]

    Ashtekar and A

    A. Ashtekar and A. Magnon-Ashtekar,A Geometrical Approach To External Potential Problems In Quantum Field Theory, Gen. Rel. Grav.12(1980) 205–223

  55. [55]

    A. H. Najmi and A. C. Ottewill,Quantum States And The Hadamard Form. I. Energy Minimization For Scalar Fields, Phys. Rev. D30(1984) 1733–1741

  56. [56]

    A. H. Najmi and A. C. Ottewill,Quantum States And The Hadamard Form

  57. [57]

    Constraints In Cosmological Space-Times, Phys. Rev. D32(1985) 1942–1948

  58. [58]

    Henneaux and C

    M. Henneaux and C. Teitelboim,Quantization of gauge systems. Princeton university press, 1992. 76