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Paper Citation Record · LEDGER

Light path averages in spacetimes with non-vanishing average spatial curvature

As of 15 August 2026, this Paper Citation Record lists 61 of 61 outbound references and 0 inbound Pith citation observations for arXiv:1909.00610.

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pith.paper-citation-record.v1
1909.00610 v2

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measured 61 of 61 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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61 of 61 outbound references displayed

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Outbound references

Observation f808fe6f-a26c-448a-99e6-563378519757 · outbound

This paper cites On average properties of inhomogeneous fluids in general relativity I: dust cosmologies.

Light path averages in spacetimes with non-vanishing average spatial curvature On average properties of inhomogeneous fluids in general relativity I: dust cosmologies

Reference 1

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Observation 060aa651-d732-44c7-ba3b-fc8678864bce · outbound

This paper cites an unresolved cited work.

Light path averages in spacetimes with non-vanishing average spatial curvature Unresolved cited work

Reference 2

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Observation 8df778a5-cf45-4241-9ab3-7d5d3591c439 · outbound

This paper cites Backreaction in late-time cosmology.

Light path averages in spacetimes with non-vanishing average spatial curvature Backreaction in late-time cosmology

Reference 3

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Observation 2cf96255-3f06-4c1b-ba89-ac3a0be250e3 · outbound

This paper cites Does the growth of structure affect our dynamical models of the universe? The averaging, backreaction and fitting problems in cosmology.

Light path averages in spacetimes with non-vanishing average spatial curvature Does the growth of structure affect our dynamical models of the universe? The averaging, backreaction and fitting problems in cosmology

Reference 4

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Observation cab1ac9f-8c17-41f7-8be8-f642b2b6888b · outbound

This paper cites The effect of inhomogeneities on the distance to the last scattering surface and the accuracy of the CMB analysis.

Light path averages in spacetimes with non-vanishing average spatial curvature The effect of inhomogeneities on the distance to the last scattering surface and the accuracy of the CMB analysis

Reference 5

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Observation e0ecaac1-eee7-44c0-bc34-b00dc1df6653 · outbound

This paper cites (Mis-)Interpreting supernovae observations in a lumpy universe.

Light path averages in spacetimes with non-vanishing average spatial curvature (Mis-)Interpreting supernovae observations in a lumpy universe

Reference 6

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Observation 034f64f1-2bee-484e-8890-ffc464f893b6 · outbound

This paper cites Transition from Clumpy to Smooth Angular Diameter Distances.

Light path averages in spacetimes with non-vanishing average spatial curvature Transition from Clumpy to Smooth Angular Diameter Distances

Reference 7

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Observation 37746888-21ec-40a0-b0b6-156d8baada35 · outbound

This paper cites Ray tracing and Hubble diagrams in post-Newtonian cosmology.

Light path averages in spacetimes with non-vanishing average spatial curvature Ray tracing and Hubble diagrams in post-Newtonian cosmology

Reference 8

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Observation 245c322a-c3e1-4347-92a4-266b60b7b30f · outbound

This paper cites Swiss-cheese models and the Dyer-Roeder approximation.

Light path averages in spacetimes with non-vanishing average spatial curvature Swiss-cheese models and the Dyer-Roeder approximation

Reference 9

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Observation 3ea09fb2-238b-4bd8-8878-872651884a3c · outbound

This paper cites Interpretation of the Hubble diagram in a nonhomogeneous universe.

Light path averages in spacetimes with non-vanishing average spatial curvature Interpretation of the Hubble diagram in a nonhomogeneous universe

Reference 10

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Observation e20d76d6-82f7-4df5-8e5c-bf84136220df · outbound

This paper cites The theory of stochastic cosmological lensing.

Light path averages in spacetimes with non-vanishing average spatial curvature The theory of stochastic cosmological lensing

Reference 11

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Observation 7579c7f1-5dbc-4162-83cc-7689957307f8 · outbound

This paper cites Cosmological ensemble and directional averages of observables.

Light path averages in spacetimes with non-vanishing average spatial curvature Cosmological ensemble and directional averages of observables

Reference 12

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Observation 339a08c1-56bf-435c-b31d-f0883f632c4e · outbound

This paper cites Average magnification effect of clumping of matter.

Light path averages in spacetimes with non-vanishing average spatial curvature Average magnification effect of clumping of matter

Reference 13

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Observation ec4afaa7-d32f-4f74-bd22-b7563e08e64b · outbound

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Light path averages in spacetimes with non-vanishing average spatial curvature Unresolved cited work

Reference 14

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Observation e7dc0217-6ab6-44f0-a13a-b9e97d15db81 · outbound

This paper cites Average and dispersion of the luminosity-redshift relation in the concordance model.

Light path averages in spacetimes with non-vanishing average spatial curvature Average and dispersion of the luminosity-redshift relation in the concordance model

Reference 15

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Observation 802db732-f357-4060-9f6a-4ea7f432f4a4 · outbound

This paper cites Do stochastic inhomogeneities affect dark-energy precision measurements?.

Light path averages in spacetimes with non-vanishing average spatial curvature Do stochastic inhomogeneities affect dark-energy precision measurements?

Reference 16

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Observation 106c1b75-0f77-4c7e-abd6-2564062c79c4 · outbound

This paper cites Do we care about the distance to the CMB? Clarifying the impact of second-order lensing.

Light path averages in spacetimes with non-vanishing average spatial curvature Do we care about the distance to the CMB? Clarifying the impact of second-order lensing

Reference 17

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Observation f9616295-cd16-4934-9d93-6948471e3aec · outbound

This paper cites On the Bias of the Distance-Redshift Relation from Gravitational Lensing.

Light path averages in spacetimes with non-vanishing average spatial curvature On the Bias of the Distance-Redshift Relation from Gravitational Lensing

Reference 18

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Observation 6f2cdcb8-dc5e-475c-9f73-1b257f96ed09 · outbound

This paper cites close-ups.

Light path averages in spacetimes with non-vanishing average spatial curvature close-ups

Reference 19

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Observation 6c0fa3da-2087-4880-a9eb-7fb533562d84 · outbound

This paper cites Luminosity distance in "Swiss cheese" cosmology with randomized voids: I. Single void size.

Light path averages in spacetimes with non-vanishing average spatial curvature Luminosity distance in "Swiss cheese" cosmology with randomized voids: I. Single void size

Reference 20

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Observation 3cd0b472-faca-4858-afee-5f467acb921b · outbound

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Light path averages in spacetimes with non-vanishing average spatial curvature Effect of inhomogeneities on high precision measurements of cosmological distances

Reference 21

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Observation cc295637-ee06-454f-894e-ecb63b9772d1 · outbound

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Light path averages in spacetimes with non-vanishing average spatial curvature CMB seen through random Swiss Cheese

Reference 22

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Observation fbecb05b-5464-4b84-98f2-e78557166a07 · outbound

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Light path averages in spacetimes with non-vanishing average spatial curvature The Effect of Large-Scale Inhomogeneities on the Luminosity Distance

Reference 23

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Observation 54e4782c-7a38-4c7d-aa69-74cdce18c5d9 · outbound

This paper cites Hubble Diagram Dispersion From Large-Scale Structure.

Light path averages in spacetimes with non-vanishing average spatial curvature Hubble Diagram Dispersion From Large-Scale Structure

Reference 24

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Light path averages in spacetimes with non-vanishing average spatial curvature Unresolved cited work

Reference 25

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Observation 2eea8e04-f9a9-48ec-8539-52e8500d1bd4 · outbound

This paper cites Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe.

Light path averages in spacetimes with non-vanishing average spatial curvature Ricci focusing, shearing, and the expansion rate in an almost homogeneous Universe

Reference 26

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Observation c651294a-7238-41e7-bd0a-0e520534c6e0 · outbound

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Light path averages in spacetimes with non-vanishing average spatial curvature Planck 2018 results. VI. Cosmological parameters

Reference 27

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Light path averages in spacetimes with non-vanishing average spatial curvature Light propagation in Swiss cheese models of random close-packed Szekeres structures: Effects of anisotropy and comparisons with perturbative results

Reference 28

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Observation 09ab9a0b-430d-4138-ad37-3eba6e3a0155 · outbound

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Light path averages in spacetimes with non-vanishing average spatial curvature Average expansion rate and light propagation in a cosmological Tardis spacetime

Reference 29

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Light path averages in spacetimes with non-vanishing average spatial curvature Light propagation in statistically homogeneous and isotropic dust universes

Reference 30

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Observation d717464f-82ae-4fb8-958a-44ad2bcd7618 · outbound

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Light path averages in spacetimes with non-vanishing average spatial curvature Spatial Curvature in Cosmology Revisited

Reference 31

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Light path averages in spacetimes with non-vanishing average spatial curvature On the local variation of the Hubble constant

Reference 32

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Observation 0b913f07-e7a1-4dcb-a21a-0a2979aa8e09 · outbound

This paper cites The Local Value of $H_0$ in an Inhomogeneous Universe.

Light path averages in spacetimes with non-vanishing average spatial curvature The Local Value of $H_0$ in an Inhomogeneous Universe

Reference 33

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Light path averages in spacetimes with non-vanishing average spatial curvature The value of H_0 in the inhomogeneous Universe

Reference 34

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Light path averages in spacetimes with non-vanishing average spatial curvature Cosmic variance of the local Hubble flow in large-scale cosmological simulations

Reference 35

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Light path averages in spacetimes with non-vanishing average spatial curvature Expectations for the Difference Between Local and Global Measurements of the Hubble Constant

Reference 36

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Observation d31a8604-46c7-4073-a84c-f80685e897a8 · outbound

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Light path averages in spacetimes with non-vanishing average spatial curvature The variance of the locally measured Hubble parameter explained with different estimators

Reference 37

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source=pdf_text observed=2026-08-14T05:52:30.480371Z digest=sha256:211244b4b57dfe81da31d01f7401b723dbc3437fe0b97a2e96fa0c8189c41027

Observation 7a9c1a6d-47be-45cc-8082-ffac89bf8385 · outbound

This paper cites Lemaitre: L’Universe en expansion, Annales de la So- ciete Scienti que de Bruxelles A 53, 51 (1933), English translation: The expanding universe, Gen.

Light path averages in spacetimes with non-vanishing average spatial curvature Lemaitre: L’Universe en expansion, Annales de la So- ciete Scienti que de Bruxelles A 53, 51 (1933), English translation: The expanding universe, Gen

Reference 38

Resolution
verified fuzzy
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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation 64cb7c39-0f3a-4d86-9bba-dba6074cf735 · outbound

This paper cites an unresolved cited work.

Light path averages in spacetimes with non-vanishing average spatial curvature Unresolved cited work

Reference 39

Resolution
unresolved
raw_fallback, observed 2026-08-14T05:52:31.386824Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation 28aaf813-9bd2-44e6-a2c7-2927ad7cbe4e · outbound

This paper cites Emergence of spatial curvature.

Light path averages in spacetimes with non-vanishing average spatial curvature Emergence of spatial curvature

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-08-14T05:52:30.822842Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.491591Z digest=sha256:de26810cd2337183f49873d96f5f1ef91eb57479281bd4fb4b469106b7a4da5c

Observation 9de089d8-e76d-401f-889b-592cbd44c94a · outbound

This paper cites Scalar Perturbations on Lemaitre-Tolman-Bondi Spacetimes.

Light path averages in spacetimes with non-vanishing average spatial curvature Scalar Perturbations on Lemaitre-Tolman-Bondi Spacetimes

Reference 41

Resolution
verified exact
local_arxiv, observed 2026-08-14T05:52:30.808086Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.506849Z digest=sha256:7143594ac8b958075942517017647096d34d0cc647fa8831f071f6b730a51c39

Observation 55ee2608-1480-4aa6-9cd5-cb51ae71a7ec · outbound

This paper cites Radiation in the process of the formation of voids.

Light path averages in spacetimes with non-vanishing average spatial curvature Radiation in the process of the formation of voids

Reference 42

Resolution
verified exact
local_arxiv, observed 2026-08-14T05:52:30.793949Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.510670Z digest=sha256:9ccd5d45dcfcaf442775240d8a5f7223edc112fea3fca694c1cfd356c7f52f49

Observation abba972c-6a23-4701-8b8a-62295d15683e · outbound

This paper cites Bondi: Spherically Symmetrical Models in General Relativity, Month.

Light path averages in spacetimes with non-vanishing average spatial curvature Bondi: Spherically Symmetrical Models in General Relativity, Month

Reference 43

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T05:52:31.376000Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.502931Z digest=sha256:309192ec862ded0b792405e6481961dc3f1f59886a405f47ba910c803abb7fb1

Observation 7364c154-42b8-4c2c-9d39-734f136cc3c5 · outbound

This paper cites Szekeres: A class of inhomogeneous cosmological mod- els , Communications in Mathematical Physics 41 (1975), no.

Light path averages in spacetimes with non-vanishing average spatial curvature Szekeres: A class of inhomogeneous cosmological mod- els , Communications in Mathematical Physics 41 (1975), no

Reference 44

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T05:52:31.364150Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.517774Z digest=sha256:7783985c13915be033b1622735c91623ce4e1ffd293d0495f9355a261c6d0026

Observation 267602bf-2edf-479f-ac73-18ae4f8eb511 · outbound

This paper cites The Size and Shape of Local Voids.

Light path averages in spacetimes with non-vanishing average spatial curvature The Size and Shape of Local Voids

Reference 45

Resolution
verified exact
local_arxiv, observed 2026-08-14T05:52:30.764403Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.521049Z digest=sha256:212e61383ed752f2c083799eb201e428e88a774c4e8ce572f07263de0eeebf83

Observation e2c3f41d-567a-457a-a782-4de726883bcc · outbound

This paper cites Pressure gradients, shell crossing singularities and acoustic oscillations - application to inhomogeneous cosmological models.

Light path averages in spacetimes with non-vanishing average spatial curvature Pressure gradients, shell crossing singularities and acoustic oscillations - application to inhomogeneous cosmological models

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-08-14T05:52:30.779031Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.514259Z digest=sha256:f74018c6b1df8ab8a6f83c36fb9b2fdc992aab56c3ece2ac60a01a097775672e

Observation 53479435-5473-4813-852c-5caa99b0913f · outbound

This paper cites Voids in the 2dF Galaxy Redshift Survey.

Light path averages in spacetimes with non-vanishing average spatial curvature Voids in the 2dF Galaxy Redshift Survey

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-14T05:52:30.529362Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:52:30.529362Z digest=sha256:afeb17c9f00fc376bdf050efa5ed2c3629de8507714b40081a5e44641725f440

Observation 95eb0bd4-8b1d-4005-bd6d-565eb2ee0bbb · outbound

This paper cites Simulating the joint evolution of quasars, galaxies and their large-scale distribution.

Light path averages in spacetimes with non-vanishing average spatial curvature Simulating the joint evolution of quasars, galaxies and their large-scale distribution

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-14T05:52:30.534089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:52:30.534089Z digest=sha256:a17fcda43823fe289ebfe199774d212e37d7fe016bdc44dfeb16edb4b5f5ec5b

Observation 1f50e10d-d3ef-41b3-9b83-a3d7897949b0 · outbound

This paper cites Vogeley: Voids in the PSCz Survey and the Updated Zwicky Cata- log, Astrophys.J.566:641-651,2002, arXiv:astro- ph/0109357v2.

Light path averages in spacetimes with non-vanishing average spatial curvature Vogeley: Voids in the PSCz Survey and the Updated Zwicky Cata- log, Astrophys.J.566:641-651,2002, arXiv:astro- ph/0109357v2

Reference 49

Resolution
verified exact
raw_fallback, observed 2026-08-14T05:52:30.747172Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.525742Z digest=sha256:3b49a8a88c8e21c5cba5037614893c538a232ed4ebd3e864bfbebdd7a898154a

Observation eadc3464-c4b3-425e-a3b1-7b0b22cd37ce · outbound

This paper cites an unresolved cited work.

Light path averages in spacetimes with non-vanishing average spatial curvature Unresolved cited work

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-14T05:52:30.541915Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:52:30.541915Z digest=sha256:b34fbadc33f5534207646cbf130cd495081ab41ec07063f35e901674255e9409

Observation 5e31b6d8-257d-44ef-9b48-144a408433ff · outbound

This paper cites an unresolved cited work.

Light path averages in spacetimes with non-vanishing average spatial curvature Unresolved cited work

Reference 51

Resolution
unresolved
raw_fallback, observed 2026-08-14T05:52:31.352907Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.545524Z digest=sha256:eac58ad6efc5df7c85b4a7c04d2037eeefac7f9878125e8200a642a052bb45bf

Observation b36d5a14-f4a3-41c5-9419-d95c4a1667e1 · outbound

This paper cites an unresolved cited work.

Light path averages in spacetimes with non-vanishing average spatial curvature Unresolved cited work

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-14T05:52:30.538244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:52:30.538244Z digest=sha256:fa75e364d9ded12ae40a38438e40c0135b3ed2e3f960083db3d3bed735de5d1d

Observation 642a06e7-4c42-4a02-9eb3-c9699a97a3c3 · outbound

This paper cites Accurately computing weak lensing convergence.

Light path averages in spacetimes with non-vanishing average spatial curvature Accurately computing weak lensing convergence

Reference 53

Resolution
verified exact
local_arxiv, observed 2026-08-14T05:52:30.662651Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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Observation f2492d93-b487-4114-96f1-707a31e1ffc3 · outbound

This paper cites Periodic boundary conditions on the pseudosphere.

Light path averages in spacetimes with non-vanishing average spatial curvature Periodic boundary conditions on the pseudosphere

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-08-14T05:52:30.646458Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.556031Z digest=sha256:ce84edddc955f8eedbed1e3588f9ec9309de1a2f182ca28017d1c914c0d09249

Observation 16064d40-32ef-4a12-96e9-d6e2965be360 · outbound

This paper cites an unresolved cited work.

Light path averages in spacetimes with non-vanishing average spatial curvature Unresolved cited work

Reference 55

Resolution
unresolved
raw_fallback, observed 2026-08-14T05:52:31.341079Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.549001Z digest=sha256:b1d5305466d7d1531b2883b3b771887bc367c0ed29c101552d4a6376d95224e5

Observation c5aa3042-9a67-4832-bdb0-f0e8ee922768 · outbound

This paper cites Towards statistically homogeneous and isotropic perfect fluid universes with cosmic backreaction.

Light path averages in spacetimes with non-vanishing average spatial curvature Towards statistically homogeneous and isotropic perfect fluid universes with cosmic backreaction

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-14T05:52:30.564001Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T05:52:30.564001Z digest=sha256:2835826bd0814f04075ca7fad3d0506b0a8381a31856fcf2636bb61f659431a3

Observation dd700d81-4af0-4675-a4d4-626ff233ecf2 · outbound

This paper cites an unresolved cited work.

Light path averages in spacetimes with non-vanishing average spatial curvature Unresolved cited work

Reference 57

Resolution
unresolved
raw_fallback, observed 2026-08-14T05:52:31.330322Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.567594Z digest=sha256:cfc965b6764148da34193540c8e07ec6e5e0522e2beeefdd799796937b7365e2

Observation b741e61b-d5b6-44b3-b85e-94c07b55064b · outbound

This paper cites This was also suggested in 2 This explanation was suggested by the anonymous referee and later confirmed by the author by looking through the numerical data.

Light path averages in spacetimes with non-vanishing average spatial curvature This was also suggested in 2 This explanation was suggested by the anonymous referee and later confirmed by the author by looking through the numerical data

Reference 58

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T05:52:31.429958Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.343300Z digest=sha256:ac109f1ef4b1f966680bfb07523bf4e2e0ac3b2afd2eb3567eeb531463bab8e3

Observation b4e7ec9c-9142-4d11-9cc0-f394bf5acde4 · outbound

This paper cites Light propagation and the average expansion rate in near-FRW universes.

Light path averages in spacetimes with non-vanishing average spatial curvature Light propagation and the average expansion rate in near-FRW universes

Reference 59

Resolution
verified exact
local_arxiv, observed 2026-08-14T05:52:30.630873Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.560170Z digest=sha256:5f29848e8ff34a419e7e387a46ee549857669181eede7812fb61e19267ef5c9f

Observation 293ba68a-9027-4bd7-b195-47fe9e581717 · outbound

This paper cites Rees and D.

Light path averages in spacetimes with non-vanishing average spatial curvature Rees and D

Reference 61

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T05:52:31.319837Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.571072Z digest=sha256:c9d914e86972c7216f602707cc860c28dc98ac3bba8e3ccd8e3d33c26742201b

Observation 85595619-1462-4021-b142-98d61b983562 · outbound

This paper cites Setting A(t1200,r ) = 1 1200r is a convenient way to ensure (for conceptual convenience) that A = ar in spacetime regions that are FLRW i.e.

Light path averages in spacetimes with non-vanishing average spatial curvature Setting A(t1200,r ) = 1 1200r is a convenient way to ensure (for conceptual convenience) that A = ar in spacetime regions that are FLRW i.e

Reference 1200

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T05:52:31.441122Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T05:52:30.337032Z digest=sha256:a76591c75ea17e738c29cdf22d9d841c2434bda922a71c97bf6557b032fed4fa

Pith citing papers

No inbound Pith citation observations are available.