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Paper Citation Record · LEDGER

Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2407.09341.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2407.09341 v4

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T20:39:02.115444Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-27T05:20:35.731895Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 47cb9eb7-cc8b-4919-9384-830ecd1a23f3 · inbound

Convective mixing in distant and close-in giant planets -- Dependences on the initial composition, luminosity, bloating and semi-convection cites this paper.

Convective mixing in distant and close-in giant planets -- Dependences on the initial composition, luminosity, bloating and semi-convection Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-12T11:04:05.040900Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T11:04:05.040900Z digest=sha256:c16e96d5b8e6129bab667f0f0a75c1e41a33d8e7b6f79b36a788752cb5b53562

Observation 78551290-7b0f-4b4e-bfb0-44d3567d22d6 · inbound

Simultaneous Evolutionary Fits for Jupiter and Saturn Incorporating Fuzzy Cores cites this paper.

Simultaneous Evolutionary Fits for Jupiter and Saturn Incorporating Fuzzy Cores Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Reference 38

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unresolved
no resolver link, observed 2026-08-11T05:51:36.905603Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7ddaf005-5141-4155-b17b-26c09b992f21 · inbound

Formation of Giant Planets cites this paper.

Formation of Giant Planets Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Reference 75

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unresolved
no resolver link, observed 2026-08-10T16:24:08.583988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7cfdcc1f-1e95-44ef-bf18-a554808aa62f · inbound

Determination of Jupiter's Primordial Physical State cites this paper.

Determination of Jupiter's Primordial Physical State Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-15T20:39:02.115444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T20:39:02.115444Z digest=sha256:9edc41bb9347d8261862eb1438ca54e12926ad0113e149b27fe1826819e2078a

Observation d3ddfcd9-02d0-4cf4-9c07-756940766dd5 · inbound

Different Inhomogeneous Evolutionary Histories for Uranus and Neptune cites this paper.

Different Inhomogeneous Evolutionary Histories for Uranus and Neptune Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-07T00:31:48.972040Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:31:48.972040Z digest=sha256:58bc39fce0b7a57bda5381c6ca0e59e3b8af0b9e02db307ce943e66ddf17a28a

Observation fcaa25db-f8bb-45a7-a1e6-45db6cb759fc · inbound

ORCHARD: A General Planetary Evolution Code cites this paper.

ORCHARD: A General Planetary Evolution Code Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Reference 11

Resolution
verified exact
arxiv_id, observed 2026-05-11T23:11:18.477496Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-05-07T17:57:49.490609Z digest=sha256:046175b82febcb9f9989dd47d06908cc8c668ef7adc447edd528d048f4bf136c

Observation a7ef8108-a7e8-40b1-bf2b-7abae8ce6d3a · inbound

Next-Generation Atmosphere Models for Giant Planets with Application to Coupled Interior Composition and Spectral Evolution I: Cloudless Models with Equilibrium Chemistry cites this paper.

Next-Generation Atmosphere Models for Giant Planets with Application to Coupled Interior Composition and Spectral Evolution I: Cloudless Models with Equilibrium Chemistry Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Reference 35

Resolution
verified exact
arxiv_id, observed 2026-06-27T05:20:35.733977Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-06-27T05:19:04.102830Z digest=sha256:f66efabbc76b859d69db0d9e2d07b170b64377d01875bfb98386cf1b0f31671a

Observation 173fe56b-dd1b-4df3-9dca-ec38d67b5b90 · inbound

The influence of composition gradients on giant planet radii cites this paper.

The influence of composition gradients on giant planet radii Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Reference 37

Resolution
unresolved
no resolver link, observed 2026-07-12T02:17:19.814114Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation c70b72c1-4321-4a2f-99dc-285965a8269b · inbound

The atmospheric vertical structure of Uranus and Neptune from thermochemical models: the impact of model assumptions cites this paper.

The atmospheric vertical structure of Uranus and Neptune from thermochemical models: the impact of model assumptions Convective Mixing in Gas Giant Planets with Primordial Composition Gradients

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-15T15:37:35.573479Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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