Recognition: unknown
Memory of Robinson-Trautman waves
Pith reviewed 2026-05-10 07:15 UTC · model grok-4.3
The pith
Robinson-Trautman waves exhibit an explicit gravitational memory effect after a frame rotation and coordinate shift renders them locally asymptotically flat at future null infinity.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The memory effect for Robinson-Trautman waves is worked out after constructing the combined frame rotation and coordinate transformation that renders them locally asymptotically flat at future null infinity; news-free solutions coincide with the vacuum sector of Euclidean Liouville theory and correspond to a boosted and rescaled Schwarzschild black hole.
What carries the argument
The combined frame rotation and coordinate transformation that makes Robinson-Trautman waves locally asymptotically flat at future null infinity, allowing direct use of existing memory formulas.
If this is right
- Displacement and nonlinear memory effects remain invariant under supertranslations.
- The same memory effects are covariant under BMS4 Lorentz transformations and constant rescalings.
- News-free Robinson-Trautman solutions describe boosted and rescaled Schwarzschild black holes.
- An improved generalized mass aspect supplies a manifestly positive local Lyapunov function for the wave evolution.
Where Pith is reading between the lines
- The same transformation technique could be tested on other exact vacuum solutions to check whether memory formulas extend without modification.
- The link to Euclidean Liouville theory opens a route to import 2D conformal methods into the study of 4D gravitational wave memory.
- The rest-frame flow interpretation may simplify the choice of reference frames when extracting memory from numerical relativity simulations.
Load-bearing premise
The constructed frame rotation and coordinate transformation truly renders Robinson-Trautman waves locally asymptotically flat at future null infinity so that standard memory formulas apply without further corrections.
What would settle it
A numerical extraction of the strain memory from an exact Robinson-Trautman metric both before and after the reported transformation; mismatch between the two would show that additional correction terms are required.
read the original abstract
The memory effect for Robinson-Trautman waves is explicitly worked out. In a first step, we construct the combined frame rotation and coordinate transformation in which Robinson-Trautman waves are manifestly locally asymptotically flat at future null infinity. This allows us to apply well-established results on how to derive the memory effect in this context. In a second step, we construct a suitably improved generalized mass aspect that provides a local Lyapunov function for the flow in the sense that it is manifestly positive. News-free solutions are studied in detail and shown to coincide with the vacuum sector of Euclidean Liouville theory. They correspond to a boosted and rescaled Schwarzschild black hole. As a by-product, we show that the displacement and non-linear memory effects in locally asymptotically flat spacetimes at future null infinity are invariant under supertranslations and covariant under $\mathrm{BMS}_4$ Lorentz transformations and constant rescalings. A novel interpretation of modified flows that control the low harmonics in terms of keeping the system in its instantaneous rest frame is provided.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript claims to explicitly compute the memory effect for Robinson-Trautman waves. It first constructs a combined frame rotation and coordinate transformation rendering the waves locally asymptotically flat at future null infinity, permitting direct application of established memory formulas. An improved generalized mass aspect is introduced as a manifestly positive local Lyapunov function for the flow. News-free solutions are shown to coincide with the vacuum sector of Euclidean Liouville theory and to correspond to a boosted and rescaled Schwarzschild black hole. As a by-product, displacement and non-linear memory effects are proven invariant under supertranslations and covariant under BMS4 Lorentz transformations and constant rescalings, with a novel interpretation of modified flows controlling low harmonics as keeping the system in its instantaneous rest frame.
Significance. If the transformation is shown to place the metric in the precise Bondi-Sachs gauge with standard peeling and no residual corrections to the memory integrals, the work would supply a concrete, exact-solution example of memory in radiative spacetimes, establish a direct link between Robinson-Trautman news-free sectors and Euclidean Liouville theory, and reinforce the BMS covariance of memory. The positive Lyapunov function could further inform stability analyses of these spacetimes.
major comments (2)
- [Section describing the frame rotation and coordinate transformation] The central construction of the combined frame rotation and coordinate transformation (described in the first step of the abstract and presumably detailed in the main text) is asserted to render Robinson-Trautman waves locally asymptotically flat at I+ in a form where established memory formulas apply directly. However, without explicit post-transformation metric components, verification of Bondi-Sachs gauge conditions, Weyl scalar peeling, and vanishing of non-standard terms at I+, it is impossible to confirm that no additional correction terms are required in the memory integrals. This is load-bearing for the primary claim.
- [Section on news-free solutions] The identification of news-free solutions with the vacuum sector of Euclidean Liouville theory and with a boosted and rescaled Schwarzschild black hole (second step of the abstract) rests on the post-transformation metric satisfying the required fall-offs exactly. Explicit matching of the metric functions, curvature scalars, or the news function to the Liouville vacuum and Schwarzschild form is needed to substantiate the correspondence.
minor comments (2)
- The definition and positivity proof of the 'suitably improved generalized mass aspect' should be stated with an explicit formula and a clear reference to the section where its Lyapunov property is demonstrated.
- Notation for BMS4 transformations and supertranslations should be cross-referenced to standard literature (e.g., Bondi-Sachs or Barnich-Troessaert conventions) for clarity.
Simulated Author's Rebuttal
We thank the referee for their careful reading of the manuscript and for highlighting the need for explicit verification of the key constructions. We address each major comment below and will incorporate additional details in the revised version to strengthen the presentation.
read point-by-point responses
-
Referee: [Section describing the frame rotation and coordinate transformation] The central construction of the combined frame rotation and coordinate transformation (described in the first step of the abstract and presumably detailed in the main text) is asserted to render Robinson-Trautman waves locally asymptotically flat at I+ in a form where established memory formulas apply directly. However, without explicit post-transformation metric components, verification of Bondi-Sachs gauge conditions, Weyl scalar peeling, and vanishing of non-standard terms at I+, it is impossible to confirm that no additional correction terms are required in the memory integrals. This is load-bearing for the primary claim.
Authors: We agree that explicit verification of the post-transformation metric is necessary to confirm the applicability of the standard memory formulas without corrections. In the revised manuscript we will add the full explicit expressions for the metric components following the combined frame rotation and coordinate transformation, verify that the metric satisfies the Bondi-Sachs gauge conditions with standard peeling of the Weyl scalars, and demonstrate the absence of non-standard terms at I+ that would affect the memory integrals. These additions will appear in the section detailing the transformation. revision: yes
-
Referee: [Section on news-free solutions] The identification of news-free solutions with the vacuum sector of Euclidean Liouville theory and with a boosted and rescaled Schwarzschild black hole (second step of the abstract) rests on the post-transformation metric satisfying the required fall-offs exactly. Explicit matching of the metric functions, curvature scalars, or the news function to the Liouville vacuum and Schwarzschild form is needed to substantiate the correspondence.
Authors: We acknowledge that explicit matching is required to fully substantiate the claimed correspondence. In the revised manuscript we will provide detailed comparisons, including explicit expressions for the metric functions, curvature scalars, and confirmation that the news function vanishes, matching both the vacuum sector of Euclidean Liouville theory and the form of a boosted and rescaled Schwarzschild black hole. These explicit identifications will be included in the section on news-free solutions. revision: yes
Circularity Check
No significant circularity; transformation and matching steps are independent
full rationale
The paper first constructs an explicit combined frame rotation and coordinate transformation to achieve local asymptotic flatness for Robinson-Trautman waves at future null infinity, then applies standard memory formulas to the resulting form. News-free solutions are matched by direct solution of the equations to the Euclidean Liouville vacuum sector and a boosted/rescaled Schwarzschild black hole. These steps are presented as constructive and verifiable rather than definitional or fitted by construction. Invariance properties follow as a by-product. No load-bearing self-citations, self-definitional reductions, or renamed known results reduce the central claims to inputs. The derivation remains self-contained against external benchmarks.
Axiom & Free-Parameter Ledger
axioms (2)
- domain assumption Existence of a combined frame rotation and coordinate transformation rendering Robinson-Trautman waves locally asymptotically flat at future null infinity
- standard math Standard BMS4 structure and memory formulas at future null infinity
Reference graph
Works this paper leans on
-
[1]
I. Robinson and A. Trautman. “Spherical Gravitational Waves”. In:Phys. Rev. Lett.4 (1960), pp. 431–432.DOI:10.1103/PhysRevLett.4.431
-
[2]
Some spherical gravitational waves in general relativity
I. Robinson and A. Trautman. “Some spherical gravitational waves in general relativity”. In:Proc. Roy. Soc. Lond.A265 (1962), pp. 463–473.DOI:10.1098/rspa.1962. 0036
-
[3]
Radiation of gravitational waves by a cluster of su- perdense stars
Y . B. Zeldovich and A. Polnarev. “Radiation of gravitational waves by a cluster of su- perdense stars”. In:Sov. Astron.18 (1974), pp. 17–23
1974
-
[4]
Nonlinear nature of gravitation and gravitational wave experiments
D. Christodoulou. “Nonlinear nature of gravitation and gravitational wave experiments”. In:Phys. Rev. Lett.67 (1991), pp. 1486–1489.DOI:10.1103/PhysRevLett.67. 1486
-
[5]
Contribution à l’étude du rayonnement gravitationnel émis par un système isolé
L. Blanchet. “Contribution à l’étude du rayonnement gravitationnel émis par un système isolé”. PhD thesis. Université Pierre et Marie Curie, Mar. 1990
1990
-
[6]
Christodoulou’s nonlinear gravitational wave memory: Evaluation in the quadrupole approximation
A. G. Wiseman and C. M. Will. “Christodoulou’s nonlinear gravitational wave memory: Evaluation in the quadrupole approximation”. In:Phys. Rev. D44.10 (1991), R2945– R2949.DOI:10.1103/PhysRevD.44.R2945
-
[7]
Gravitational-wave bursts with memory: The Christodoulou effect,
K. S. Thorne. “Gravitational-wave bursts with memory: The Christodoulou effect”. In: Phys. Rev. D45.2 (1992), pp. 520–524.DOI:10.1103/PhysRevD.45.520
-
[8]
Note on the memory effect
J. Frauendiener. “Note on the memory effect”. In:Classical and Quantum Gravity9.6 (1992), p. 1639
1992
-
[9]
Hereditary effects in gravitational radiation
L. Blanchet and T. Damour. “Hereditary effects in gravitational radiation”. In:Phys. Rev. D46 (1992), pp. 4304–4319.DOI:10.1103/PhysRevD.46.4304
-
[11]
Exact degenerate solutions of Einstein’s equations
I. Robinson and A. Trautman. “Exact degenerate solutions of Einstein’s equations”. In:Proceedings on Theory of Gravitation, Proc. Intern. GRG Conf., Jablonna. 1964, pp. 25–31
1964
-
[12]
A theorem on Petrov types
J. N. Goldberg and R. K. Sachs. “A theorem on Petrov types”. In:Acta Physica Polonica B, Proceedings Supplement22 (1962), p. 13
1962
-
[13]
An Approach to gravitational radiation by a method of spin coefficients
E. Newman and R. Penrose. “An Approach to gravitational radiation by a method of spin coefficients”. In:J. Math. Phys.3 (1962), pp. 566–578.DOI:10.1063/1.1724257
-
[14]
Empty Space Metrics Containing Hypersurface Orthogonal Geodesic Rays
E. T. Newman and L. A. Tamburino. “Empty Space Metrics Containing Hypersurface Orthogonal Geodesic Rays”. In:Journal of Mathematical Physics3.5 (1962), pp. 902– 907.DOI:10 . 1063 / 1 . 1724304.URL:http : / / link . aip . org / link / ?JMP/3/902/1. RTMEMORY73
1962
-
[15]
Note on the Robinson-Trautman solutions
J. Foster and E. Newman. “Note on the Robinson-Trautman solutions”. In:J. Math. Phys.8 (1967), p. 189
1967
-
[16]
Algebraically special perturbations of the Schwarzschild metric
W. E. Couch and E. T. Newman. “Algebraically special perturbations of the Schwarzschild metric”. In:J. Math. Phys.14 (1973), pp. 285–286.DOI:10.1063/1.1666311
-
[17]
On algebraically special perturbations of black holes
S. Chandrasekhar. “On algebraically special perturbations of black holes”. In:Proceed- ings of the Royal Society of London. A. Mathematical and Physical Sciences392.1802 (1984), pp. 1–13.DOI:10.1098/rspa.1984.0021
-
[18]
Robinson-Trautman equations and Chandrasekhar’s special perturbation of the Schwarzschild metric
G.-Y . Qi and B. F. Schutz. “Robinson-Trautman equations and Chandrasekhar’s special perturbation of the Schwarzschild metric”. In:Gen. Rel. Grav.25 (1993), pp. 1185– 1188.DOI:10.1007/BF00763761
-
[19]
Lyapunov functional approach to radiative metrics
B Lukacs et al. “Lyapunov functional approach to radiative metrics”. In:General rela- tivity and gravitation16 (1984), pp. 691–701
1984
-
[20]
Existence of solutions of the Robinson-Trautman equation and spatial infinity
B. Schmidt. “Existence of solutions of the Robinson-Trautman equation and spatial infinity”. English. In:General Relativity and Gravitation20.1 (1988), pp. 65–70.ISSN: 0001-7701.DOI:10.1007/BF00759256.URL:http://dx.doi.org/10. 1007/BF00759256
work page doi:10.1007/bf00759256.url:http://dx.doi.org/10 1988
-
[21]
Existence and asymptotic properties of global solutions of the Robinson- Trautman equation
A. D. Rendall. “Existence and asymptotic properties of global solutions of the Robinson- Trautman equation”. In:Classical and Quantum Gravity5.10 (1988), p. 1339
1988
-
[22]
The Robinson-Trautman equation and Lyapunov functions
A. Rendall. “The Robinson-Trautman equation and Lyapunov functions”. In:Proc. Fifth Marcel Grossmann Meeting on General Relativity. Ed. by D. Blair and M. Buckingham. World Scientific, Singapore, 1989, pp. 437–439
1989
-
[23]
On global existence and convergence of vacuum Robinson-Trautman solutions
D. Singleton. “On global existence and convergence of vacuum Robinson-Trautman solutions”. In:Classical and Quantum Gravity7.8 (1990), p. 1333.DOI:10.1088/ 0264 - 9381 / 7 / 8 / 012.URL:https : / / dx . doi . org / 10 . 1088 / 0264 - 9381/7/8/012
1990
-
[24]
Robinson-Trautman solutions of Einstein’s equations
D. B. Singleton. “Robinson-Trautman solutions of Einstein’s equations”. In: (Dec. 2020). DOI:10 . 26180 / 14876076 . v1.URL:https : / / bridges . monash . edu / articles/thesis/Robinson-Trautman_solutions_of_Einstein_s_ equations/14876076
-
[25]
Semi-global Existence and Convergence of Solutions of the Robinson- Trautman (2-Dimensional Calabi) Equation
P. Chrusciel. “Semi-global Existence and Convergence of Solutions of the Robinson- Trautman (2-Dimensional Calabi) Equation”. In:Commun. Math. Phys.137 (1991), pp. 289–313
1991
-
[26]
Analogues of the past horizon in the Robinson-Trautman metrics
K. P. Tod. “Analogues of the past horizon in the Robinson-Trautman metrics.” In:Clas- sical and Quantum Gravity6 (Aug. 1989), pp. 1159–1163
1989
-
[27]
Extremal Kähler Metrics
E. Calabi. “Extremal Kähler Metrics”. In:Seminar on Differential Geometry. Ed. by S. T. Yau. V ol. 102. Annals of Mathematics Studies. Princeton, NJ: Princeton University Press, 1982, pp. 259–290. 74G. BARNICH, A. SERAJ
1982
-
[28]
On the global structure of Robinson-Trautman space-times
P. T. Chrusciel. “On the global structure of Robinson-Trautman space-times”. In:Proc. Roy. Soc. Lond. A436 (1992), pp. 299–316.DOI:10.1098/rspa.1992.0019
-
[29]
Nonsmoothness of event horizons of Robinson- Trautman black holes
P. T. Chrusciel and D. B. Singleton. “Nonsmoothness of event horizons of Robinson- Trautman black holes”. In:Commun. Math. Phys.147 (1992), pp. 137–162.DOI:10. 1007/BF02099531
1992
-
[30]
The asymptotic structure of algebraically special spacetimes
L. Mason. “The asymptotic structure of algebraically special spacetimes”. In:Classical and Quantum Gravity15.4 (1998), p. 1019
1998
-
[31]
Quadratic perturbations of the Schwarzschild black hole: the algebraically special sector
J. Ben Achour and H. Roussille. “Quadratic perturbations of the Schwarzschild black hole: the algebraically special sector”. In:JCAP07 (2024), p. 085.DOI:10.1088/ 1475-7516/2024/07/085. arXiv:2406.08159 [gr-qc]
-
[32]
Algebraically special solutions in AdS/CFT
G. Bernardi de Freitas and H. S. Reall. “Algebraically special solutions in AdS/CFT”. In:JHEP06 (2014), p. 148.DOI:10.1007/JHEP06(2014)148. arXiv:1403. 3537 [hep-th]
-
[33]
Non-equilibrium dynamics andAdS 4 Robinson-Trautman
I. Bakas and K. Skenderis. “Non-equilibrium dynamics andAdS 4 Robinson-Trautman”. In:JHEP08 (2014), p. 056.DOI:10.1007/JHEP08(2014)056. arXiv:1404. 4824 [hep-th]
-
[34]
Robinson-Trautman spacetimes and gauge/gravity dual- ity
K. Skenderis and B. Withers. “Robinson-Trautman spacetimes and gauge/gravity dual- ity”. In:PoSCORFU2016 (2017), p. 097.DOI:10.22323/1.292.0097. arXiv: 1703.10865 [hep-th]
-
[35]
The Robinson-Trautman spacetime and its holographic fluid
L. Ciambelli et al. “The Robinson-Trautman spacetime and its holographic fluid”. In: PoSCORFU2016 (2017), p. 076.DOI:10 . 22323 /1 . 292 . 0076. arXiv:1707 . 02995 [hep-th]
2017
-
[36]
Heisenberg soft hair on Robinson-Trautman spacetimes
H. Adami et al. “Heisenberg soft hair on Robinson-Trautman spacetimes”. In:JHEP 05 (2024), p. 191.DOI:10 . 1007 / JHEP05(2024 ) 191. arXiv:2402 . 17658 [hep-th]
2024
-
[37]
G. Arenas-Henriquez et al. “Radiation in Fluid/Gravity and the Flat Limit”. In: (Aug. 2025). arXiv:2508.01446 [hep-th]
-
[38]
Gravitational charges and radiation in asymptot- ically locally de Sitter spacetimes
A. Poole, K. Skenderis, and M. Taylor. “Gravitational charges and radiation in asymptot- ically locally de Sitter spacetimes”. In: (Dec. 2025). arXiv:2512.14243 [hep-th]
-
[39]
On gravitational radiation from bounded sources
P. Hogan and A Trautman. “On gravitational radiation from bounded sources”. In:Grav- itation and Geometry(1987), p. 215
1987
-
[40]
Spacetimes admitting scri and the Robinson-Trautmann solutions
B. G. Schmidt. “Spacetimes admitting scri and the Robinson-Trautmann solutions”. In: Classical and Quantum Gravity5.8 (1988), p. 1153.URL:http://stacks.iop. org/0264-9381/5/i=8/a=011
1988
-
[41]
Penrose and W
R. Penrose and W. Rindler.Spinors and Space-Time, Volume 2: Spinor and Twistor Methods in Space-Time Geometry. Cambridge University Press, 1986. RTMEMORY75
1986
-
[42]
Symmetries of asymptotically flat 4 dimensional spacetimes at null infinity revisited
G. Barnich and C. Troessaert. “Symmetries of asymptotically flat 4 dimensional space- times at null infinity revisited”. In:Phys.Rev.Lett.105 (2010), p. 111103.DOI:10 . 1103/PhysRevLett.105.111103. arXiv:0909.2617 [gr-qc]
work page Pith review arXiv 2010
-
[43]
Aspects of the BMS/CFT correspondence
G. Barnich and C. Troessaert. “Aspects of the BMS/CFT correspondence”. In:JHEP 05 (2010), p. 062.DOI:10 . 1007 / JHEP05(2010 ) 062. arXiv:1001 . 1541 [hep-th]
2010
-
[44]
G. Barnich and C. Troessaert. “Finite BMS transformations”. In:JHEP03 (2016), p. 167.DOI:10.1007/JHEP03(2016)167. arXiv:1601.04090 [gr-qc]
-
[45]
On BMS Invariance of Gravitational Scattering
A. Strominger. “On BMS Invariance of Gravitational Scattering”. In:JHEP1407 (Dec. 2014), p. 152.DOI:10.1007/JHEP07(2014)152. eprint:1312.2229
-
[46]
Gravitational Memory, BMS Supertranslations and Soft Theorems
A. Strominger and A. Zhiboedov. “Gravitational Memory, BMS Supertranslations and Soft Theorems”. In:JHEP01 (2016), p. 086.DOI:10.1007/JHEP01(2016)086. arXiv:1411.5745 [hep-th]
-
[47]
S. Pasterski, A. Strominger, and A. Zhiboedov. “New Gravitational Memories”. In: JHEP12 (2016), p. 053.DOI:10.1007/JHEP12(2016)053. arXiv:1502.06120 [hep-th]
-
[48]
BMS Supertranslations and Memory in Four and Higher Dimensions
S. Hollands, A. Ishibashi, and R. M. Wald. “BMS Supertranslations and Memory in Four and Higher Dimensions”. In:Class. Quant. Grav.34.15 (2017), p. 155005.DOI: 10.1088/1361-6382/aa777a. arXiv:1612.03290 [gr-qc]
-
[49]
Spin memory effect for compact binaries in the post-Newtonian approx- imation
D. A. Nichols. “Spin memory effect for compact binaries in the post-Newtonian approx- imation”. In:Phys. Rev.D95.8 (2017), p. 084048.DOI:10.1103/PhysRevD.95. 084048. arXiv:1702.03300 [gr-qc]
-
[50]
P. Mao and X. Wu. “More on gravitational memory”. In:Journal of High Energy Physics 2019.5 (May 2019).ISSN: 1029-8479.DOI:10.1007/jhep05(2019)058.URL: http://dx.doi.org/10.1007/JHEP05(2019)058
-
[51]
Alpha-Vacuum and Inflationary Bispectrum.Phys
K. Mitman et al. “Computation of displacement and spin gravitational memory in nu- merical relativity”. In:Phys. Rev. D102.10 (2020), p. 104007.DOI:10.1103/PhysRevD. 102.104007. arXiv:2007.11562 [gr-qc]
-
[52]
Gyroscopic gravitational memory
A. Seraj and B. Oblak. “Gyroscopic gravitational memory”. In:JHEP11 (2023), p. 057. DOI:10.1007/JHEP11(2023)057. arXiv:2112.04535 [hep-th]
-
[53]
From shockwaves to the gravitational memory effect
T. He, A.-M. Raclariu, and K. M. Zurek. “From shockwaves to the gravitational memory effect”. In:JHEP01 (2024), p. 006.DOI:10.1007/JHEP01(2024)006. arXiv: 2305.14411 [hep-th]
-
[54]
The strong coupling constant: state of the art and the decade ahead,
K. Mitman et al. “A review of gravitational memory and BMS frame fixing in numerical relativity”. In:Class. Quant. Grav.41.22 (2024), p. 223001.DOI:10.1088/1361- 6382/ad83c2. arXiv:2405.08868 [gr-qc]. 76G. BARNICH, A. SERAJ
-
[55]
Asymptotically Flat Space-times
E. P. Newman and K. P. Tod. “Asymptotically Flat Space-times”. In:General Relativity and Gravitation. 100 Years after the Birth of Albert Einstein. Volume 2. Ed. by Plenum Press. 1980, pp. 1–36
1980
-
[56]
E. Newman and R. Penrose. “Spin-coefficient formalism”. In:Scholarpedia4.6 (2009), p. 7445.ISSN: 1941-6016.DOI:10.4249/scholarpedia.7445
-
[57]
Null Geodesic Congruences, Asymp- totically Flat Space-Times and Their Physical Interpretation
T. M. Adamo, C. N. Kozameh, and E. T. Newman. “Null Geodesic Congruences, Asymp- totically Flat Space-Times and Their Physical Interpretation”. In:Living Rev.Rel.12 (2009), p. 6. arXiv:0906.2155 [gr-qc]
-
[58]
Bondi mass in terms of the Penrose conformal factor
J. Tafel. “Bondi mass in terms of the Penrose conformal factor”. In:Classical and Quan- tum Gravity17.21 (2000), p. 4397
2000
-
[59]
On angular momentum at future null infinity
O. M. Moreschi. “On angular momentum at future null infinity”. In:Classical and Quantum Gravity3.4 (1986), p. 503.URL:http://stacks.iop.org/0264- 9381/3/i=4/a=006
1986
-
[60]
Supercenter of Mass System at Future Null Infinity
O. M. Moreschi. “Supercenter of Mass System at Future Null Infinity”. In:Class. Quant. Grav.5 (1988), pp. 423–435.DOI:10.1088/0264-9381/5/3/004
-
[61]
Stephani et al.Exact solutions of Einstein’s field equations
H. Stephani et al.Exact solutions of Einstein’s field equations. Cambridge University Press, 2003
2003
-
[62]
Behavior of Asymptotically Flat Empty Spaces
E. T. Newman and T. W. J. Unti. “Behavior of Asymptotically Flat Empty Spaces”. In: J. Math. Phys.3.5 (1962), p. 891.DOI:10.1063/1.1724303
-
[63]
Conserved quantities in the Einstein-Maxwell theory
A. Exton, E. Newman, and R. Penrose. “Conserved quantities in the Einstein-Maxwell theory”. In:J. Math. Phys.10 (1969), pp. 1566–1570.DOI:10.1063/1.1665006
-
[64]
F. Beyer et al. “Numerical evolutions of fields on the 2-sphere using a spectral method based on spin-weighted spherical harmonics”. In:Class. Quant. Grav.31 (2014), p. 075019. DOI:10.1088/0264-9381/31/7/075019. arXiv:1308.4729 [physics.comp-ph]
-
[65]
On the positivity of total gravitational energy at retarded times
M. Walker. “On the positivity of total gravitational energy at retarded times”. In:Ray- onnement gravitationnel – Gravitational radiation. Ed. by N. Deruelle and T. Piran. North-Holland, 1983, pp. 145–173
1983
-
[66]
Angular momentum at null infinity
T. Dray and M. Streubel. “Angular momentum at null infinity”. In:Classical and Quan- tum Gravity1.1 (1984), pp. 15–26.URL:http : / / stacks . iop . org / 0264 - 9381/1/15
1984
-
[67]
A. Held, E. T. Newman, and R. Posadas. “The Lorentz Group and the Sphere”. In: Journal of Mathematical Physics11.11 (1970), pp. 3145–3154.DOI:10.1063/1. 1665105.URL:http://link.aip.org/link/?JMP/11/3145/1
work page doi:10.1063/1 1970
-
[68]
Asymptotic symmetries in gravitational theory
R. K. Sachs. “Asymptotic symmetries in gravitational theory”. In:Phys. Rev.128 (1962), pp. 2851–2864. RTMEMORY77
1962
-
[69]
Note on the Bondi-Metzner-Sachs Group
E. T. Newman and R. Penrose. “Note on the Bondi-Metzner-Sachs Group”. In:J. Math. Phys.7 (1966), pp. 863–870.DOI:10.1063/1.1931221
-
[70]
Penrose and W
R. Penrose and W. Rindler.Spinors and Space-Time, Volume 1: Two-spinor Calculus and Relativistic Fields. Cambridge University Press, 1984
1984
-
[71]
I. M. Gelfand, M. I. Graev, and N. Y . Vilenkin.Generalized Functions, Volume 5: In- tegral Geometry and Representation Theory. Translated from the Russian by Eugene Saletan. New York and London: Academic Press, 1966
1966
-
[72]
BMS current algebra in the context of the Newman-Penrose formalism
G. Barnich, P. Mao, and R. Ruzziconi. “BMS current algebra in the context of the Newman-Penrose formalism”. In:Class. Quant. Grav.37.9 (2020), p. 095010.DOI: 10.1088/1361-6382/ab7c01. arXiv:1910.14588 [gr-qc]
-
[73]
Boosted Schwarzschild metrics from a Kerr–Schild per- spective
T. Mädler and J. Winicour. “Boosted Schwarzschild metrics from a Kerr–Schild per- spective”. In:Class. Quant. Grav.35.3 (2018), p. 035009.DOI:10 . 1088 / 1361 - 6382/aaa18e. arXiv:1708.08774 [gr-qc]
-
[74]
Coulombic contribution to angular momentum flux in general relativity
B. Bonga and E. Poisson. “Coulombic contribution to angular momentum flux in general relativity”. In:Phys. Rev. D99.6 (2019), p. 064024.DOI:10.1103/PhysRevD.99. 064024. arXiv:1808.01288 [gr-qc]
-
[75]
Quasinormal modes of black holes and black branes
E. Berti, V . Cardoso, and A. O. Starinets. “Quasinormal modes of black holes and black branes”. In:Class. Quant. Grav.26 (2009), p. 163001.DOI:10.1088/0264-9381/ 26/16/163001. arXiv:0905.2975 [gr-qc]
-
[76]
Flat Space Amplitudes and Conformal Symmetry of the Celestial Sphere
S. Pasterski, S.-H. Shao, and A. Strominger. “Flat Space Amplitudes and Conformal Symmetry of the Celestial Sphere”. In:Phys. Rev. D96.6 (2017), p. 065026.DOI:10. 1103/PhysRevD.96.065026. arXiv:1701.00049 [hep-th]
work page Pith review arXiv 2017
-
[77]
Conformal basis for flat space amplitudes
S. Pasterski and S.-H. Shao. “Conformal basis for flat space amplitudes”. In:Phys. Rev. D96.6 (2017), p. 065022.DOI:10.1103/PhysRevD.96.065022. arXiv:1705. 01027 [hep-th]
-
[78]
Spin-s Spherical Harmonics and eth
J. N. Goldberg et al. “Spin-s Spherical Harmonics and eth”. In:Journal of Mathematical Physics8.11 (1967), pp. 2155–2161.DOI:10 . 1063 / 1 . 1705135.URL:http : //link.aip.org/link/?JMP/8/2155/1
1967
-
[79]
L. Blanchet and T. Damour. “Radiative gravitational fields in general relativity I. general structure of the field outside the source”. In:Phil. Trans. Roy. Soc. Lond. A320 (1986), pp. 379–430.DOI:10.1098/rsta.1986.0125
-
[80]
Multipole expansions of gravitational radiation
K. S. Thorne. “Multipole expansions of gravitational radiation”. In:Rev. Mod. Phys. 52.2 (1980), pp. 299–339.DOI:10.1103/RevModPhys.52.299
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.