Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:29:45.776075Z
Paper Citation Record · LEDGER
The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory
As of 21 August 2026, this Paper Citation Record lists 26 of 26 outbound references and 0 inbound Pith citation observations for arXiv:2608.09897.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
26 of 26 outbound references displayed
- verified exact1
- verified fuzzy8
- unresolved17
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
No inbound Pith citation observations are available.