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Paper Citation Record · LEDGER

The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:astro-ph/0505395.

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

pith.paper-citation-record.v1
astro-ph/0505395 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

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 2026-08-16T06:30:59.297886+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T20:26:05.987245Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T13:24:40.514568Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation d1760981-e805-48a4-95c3-97f9b1a43bc9 · inbound

MeV-scale reheating temperature and thermalization of oscillating neutrinos by radiative and hadronic decays of massive particles cites this paper.

MeV-scale reheating temperature and thermalization of oscillating neutrinos by radiative and hadronic decays of massive particles The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

Reference 4

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unresolved
no resolver link, observed 2026-08-14T12:17:12.117530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 2157bc52-07d8-4111-be1b-c1b86fd9638a · inbound

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter cites this paper.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

Reference 103

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unresolved
no resolver link, observed 2026-08-12T12:24:03.981730Z

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Unavailable: canonical work link unavailable.

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Observation a019100a-8787-4e5c-a004-c80d0bf90f26 · inbound

Two Micron-Size Dark Dimensions cites this paper.

Two Micron-Size Dark Dimensions The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-10T18:05:28.999835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 3d6c95a9-28aa-43eb-b1c7-fc1e3548fbec · inbound

Searching for coupled, hyperlight scalars across cosmic history cites this paper.

Searching for coupled, hyperlight scalars across cosmic history The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-08T22:50:24.344041Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation f2ad7a94-4995-47e6-a140-315398fb251b · inbound

Viability of post-inflationary freeze-in with precision cosmology cites this paper.

Viability of post-inflationary freeze-in with precision cosmology The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-15T20:26:05.987245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 49a855d0-6fba-4f7e-8013-c77e02b7e3a3 · inbound

Exponential Quintessence Model: Analytical Quantification of the Fine-Tuning Problem in Dark Energy cites this paper.

Exponential Quintessence Model: Analytical Quantification of the Fine-Tuning Problem in Dark Energy The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

Reference 13

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verified exact
local_arxiv, observed 2026-05-15T21:10:18.695831Z

Source-reported events for the cited work

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

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Observation 2a382294-bc09-4609-9aaf-f19ee0fa4721 · inbound

Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations cites this paper.

Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

Reference 57

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verified exact
arxiv_id, observed 2026-05-11T17:16:10.135471Z

Source-reported events for the cited work

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

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Observation d4cc09b6-832c-4dfb-b9b3-33d9c21af0de · inbound

Exponential Quintessence: Analytic Relationship Between the Current Equation of State Parameter and the Potential Parameter cites this paper.

Exponential Quintessence: Analytic Relationship Between the Current Equation of State Parameter and the Potential Parameter The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

Reference 48

Resolution
verified exact
arxiv_id, observed 2026-05-11T18:01:05.181000Z

Source-reported events for the cited work

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

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Observation 4c702572-bdd0-4c4a-828f-ce5f7869def2 · inbound

Freeze-in $SU(2)$ vector dark matter at low reheating temperature cites this paper.

Freeze-in $SU(2)$ vector dark matter at low reheating temperature The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature

Reference 13

Resolution
verified exact
local_arxiv, observed 2026-06-30T13:24:40.515745Z

Source-reported events for the cited work

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

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