Paper Citation Record · LEDGER

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory

As of 16 August 2026, this Paper Citation Record lists 26 of 26 outbound references and 0 inbound Pith citation observations for arXiv:2608.09897.

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pith.paper-citation-record.v1
2608.09897 v1

Coverage vector

measured 26 of 26 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:29:45.776075Z

measured 26 of 26 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

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Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

Reference resolution

26 of 26 outbound references displayed

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verified fuzzy8
unresolved17
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External citation measurements

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Outbound references

Observation 49004049-e810-4e56-b877-181bcac05083 · outbound

This paper cites (B6) For future convenience, note that the trace of the latter reads Ci i =−3ψ+∇ 2E.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory (B6) For future convenience, note that the trace of the latter reads Ci i =−3ψ+∇ 2E

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T14:29:46.091428Z

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Observation a78eddb1-a2da-4748-a8ff-ad05c21f5d14 · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-08-15T14:29:46.122858Z

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Observation 34cde29a-abaf-47b5-b136-08ae9fee73d9 · outbound

This paper cites Note that the Bianchi identity relates the 00, 0i,ijtrace, and energy conservation equations, and so of these 5 equations, only 4 are independent.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Note that the Bianchi identity relates the 00, 0i,ijtrace, and energy conservation equations, and so of these 5 equations, only 4 are independent

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T14:29:46.112401Z

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Observation 0996417d-2373-400d-9d7e-54ba8d092c51 · outbound

This paper cites weight function.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory weight function

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T14:29:46.102086Z

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Observation ae65fbaf-1a38-44f3-bbda-24f959ed2667 · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 5

Resolution: unresolved; raw_fallback, observed 2026-08-15T14:29:46.080883Z

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No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation c8bac61e-cfaf-4511-836a-9209f549dbc9 · outbound

This paper cites Lettingx µ(τ) be a fluid element’s worldline, withτthe proper time comoving with the fluid, one has uµ = dxµ dτ.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Lettingx µ(τ) be a fluid element’s worldline, withτthe proper time comoving with the fluid, one has uµ = dxµ dτ

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T14:29:46.070203Z

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Observation 87dbbb4b-a5f4-424a-a715-1aa616dcf794 · outbound

This paper cites energy” and “momentum.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory energy” and “momentum

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T14:29:46.058922Z

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Observation 5d8a24be-cc7e-4c97-9d53-ef87e188ce5d · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 8

Resolution: unresolved; raw_fallback, observed 2026-08-15T14:29:46.048011Z

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Observation 4292468f-4f83-4511-9181-eb098478c79f · outbound

This paper cites For the scalar perturbations, the energy and momentum constraints are 3H ψ′ 1 +Hϕ 1 −∇ 2ψ1−H∇ 2 E′ 1−B 1 =−4πGa 2δρ1, (C6) ψ′ 1 +Hϕ 1 =−4πGa 2 ρ0 +p 0 v1 +B 1.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory For the scalar perturbations, the energy and momentum constraints are 3H ψ′ 1 +Hϕ 1 −∇ 2ψ1−H∇ 2 E′ 1−B 1 =−4πGa 2δρ1, (C6) ψ′ 1 +Hϕ 1 =−4πGa 2 ρ0 +p 0 v1 +B 1

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T14:29:46.037045Z

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Observation 3277b1c7-37f8-4021-a5df-bf4b56efe54f · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 10

Resolution: unresolved; raw_fallback, observed 2026-08-15T14:29:46.024814Z

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Observation 2a8d631a-481b-45ac-940c-05c2fd439cfa · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 11

Resolution: unresolved; raw_fallback, observed 2026-08-15T14:29:46.013502Z

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Observation dff8f3f0-6a77-4838-9ef0-c520cd705309 · outbound

This paper cites (C17) For the Einstein equations, Eq.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory (C17) For the Einstein equations, Eq

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T14:29:46.002518Z

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Observation c33cdc9c-bd8a-486d-a39c-4a3fa29b20cf · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 13

Resolution: unresolved; raw_fallback, observed 2026-08-15T14:29:45.991248Z

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Observation 50d16b09-6069-48ac-a656-5f69cca93464 · outbound

This paper cites (E1e) 25.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory (E1e) 25

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T14:29:45.980571Z

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Observation 415694c9-1db7-441d-b53a-85b983d3b9e1 · outbound

This paper cites Large Scale White Noise and Cosmology.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Large Scale White Noise and Cosmology

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-15T14:29:45.733578Z

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Observation d24d0029-0dec-49c1-a5ca-53a2f024ada0 · outbound

This paper cites The Noisy Universe.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory The Noisy Universe

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-15T14:29:45.737509Z

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Observation 2d1ad1a3-8d85-47c9-a579-386e859e3042 · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 17

Resolution: unresolved; raw_fallback, observed 2026-08-15T14:29:45.969580Z

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Observation b7480c38-ed1e-4cfa-bb41-27ba0842e7cd · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-15T14:29:45.745335Z

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Observation e5ebd211-cbc2-4cf6-9f95-8f14e8dd4ee9 · outbound

This paper cites Cosmological perturbations.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Cosmological perturbations

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-15T14:29:45.748809Z

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Observation dd512cc5-0277-471c-a6b6-5e159bc224a8 · outbound

This paper cites Applications of Cosmological Perturbation Theory.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Applications of Cosmological Perturbation Theory

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-15T14:29:45.752657Z

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Observation 9ceee897-2651-4f61-8577-8a1a432c58f9 · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 21

Resolution: unresolved; raw_fallback, observed 2026-08-15T14:29:45.952953Z

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No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 28687c0c-2ed3-46c0-b8c8-6ea617be3707 · outbound

This paper cites CMB Anisotropies at Second Order I.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory CMB Anisotropies at Second Order I

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-15T14:29:45.760055Z

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Observation e27c1938-8f0d-4938-9d5a-724821f744d8 · outbound

This paper cites CMB Anisotropies at Second-Order II: Analytical Approach.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory CMB Anisotropies at Second-Order II: Analytical Approach

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-15T14:29:45.764088Z

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Observation 24560233-570a-4f30-8c66-b02ea9029d8e · outbound

This paper cites Evolution of non-linear cosmological perturbations.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Evolution of non-linear cosmological perturbations

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-15T14:29:45.768443Z

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Observation 23d9e36f-91eb-4e83-9d68-8fe474ba4cfc · outbound

This paper cites Langlois and F.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Langlois and F

Reference 25

Resolution: verified exact; raw_fallback, observed 2026-08-15T14:29:45.864527Z

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Observation 7c42fb4d-5ac8-41de-8546-35fd85962713 · outbound

This paper cites an unresolved cited work.

The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory Unresolved cited work

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-15T14:29:45.776075Z

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