Paper Citation Record · LEDGER

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades

As of 6 August 2026, this Paper Citation Record lists 34 of 34 outbound references and 0 inbound Pith citation observations for arXiv:2605.23317.

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

pith.paper-citation-record.v1
2605.23317 v1

Coverage vector

measured 34 of 34 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-25T04:15:35.829969Z

measured 34 of 34 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

34 of 34 outbound references displayed

verified exact9
verified fuzzy18
unresolved7
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation a1e59048-d26a-43f3-bd67-2f0985dae444 · outbound

This paper cites Jaeckel and A.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Jaeckel and A

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.301711Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 43bf3f5f-2815-4c65-aee4-cfebc3b677f0 · outbound

This paper cites Ringwald, Exploring the Role of Axions and Other WISPs in the Dark Universe, Phys.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Ringwald, Exploring the Role of Axions and Other WISPs in the Dark Universe, Phys

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.322613Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation edbe909c-bb85-4fe2-8032-a12fbc57d55c · outbound

This paper cites Antelet al., Feebly-interacting particles: FIPs 2022 Workshop Report, Eur.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Antelet al., Feebly-interacting particles: FIPs 2022 Workshop Report, Eur

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.311337Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation ff928ed7-7837-4476-bae3-ab7988fb5e31 · outbound

This paper cites Agrawalet al., Feebly-interacting particles: FIPs 2020 workshop report, Eur.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Agrawalet al., Feebly-interacting particles: FIPs 2020 workshop report, Eur

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.316906Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 0b6ac864-c9c8-41dc-8dee-f27a0502ce30 · outbound

This paper cites Arzaet al., The COSMIC WISPers White Paper: The physics case for Weakly Interacting Slim Particles, arXiv:2603.03433 [hep-ph] (2026).

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Arzaet al., The COSMIC WISPers White Paper: The physics case for Weakly Interacting Slim Particles, arXiv:2603.03433 [hep-ph] (2026)

Reference 5

Resolution: verified exact; arxiv_id, observed 2026-05-25T04:16:36.028225Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation c9f6d65c-459b-4aa3-993d-6e24c6980a15 · outbound

This paper cites an unresolved cited work.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Unresolved cited work

Reference 6

Resolution: unresolved; raw_fallback, observed 2026-05-25T04:16:36.295686Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation ed7d7c73-cfde-4fc1-8c40-fb77c3681f13 · outbound

This paper cites Axion Astrophysics.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Axion Astrophysics

Reference 7

Resolution: verified exact; arxiv_id, observed 2026-05-25T04:16:36.038079Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 0927c74d-dcca-4d46-924b-421d077a2c0c · outbound

This paper cites Andriamonjeet al., Search for solar axion emission from 7LiandD(p, γ) 3Henuclear decays with the CAST γ-ray calorimeter, JCAP03, 032.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Andriamonjeet al., Search for solar axion emission from 7LiandD(p, γ) 3Henuclear decays with the CAST γ-ray calorimeter, JCAP03, 032

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.292917Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation fa726ab1-fe98-4a60-808c-d0d8f1e4dc0d · outbound

This paper cites Belliniet al., Search for Solar Axions Produced in p(d, 3He)A Reaction with Borexino Detector, Phys.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Belliniet al., Search for Solar Axions Produced in p(d, 3He)A Reaction with Borexino Detector, Phys

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.315332Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation de5fe072-f8c0-41a4-b70a-ef2ac147a4af · outbound

This paper cites Bhusal, N.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Bhusal, N

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.279327Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 64f5882e-da6d-48c5-b766-6f3b27b47df6 · outbound

This paper cites D’Eramo, G.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades D’Eramo, G

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.312427Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation dcb406ac-66c8-42ff-8f08-58b78dec5b69 · outbound

This paper cites an unresolved cited work.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Unresolved cited work

Reference 12

Resolution: unresolved; raw_fallback, observed 2026-05-25T04:16:36.309749Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation bb6b9c5e-7e0d-4982-b748-874db624d5d6 · outbound

This paper cites Holdom, Two U(1)’s and Epsilon Charge Shifts, Phys.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Holdom, Two U(1)’s and Epsilon Charge Shifts, Phys

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.302061Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 7c33ee1e-8179-4b1e-908c-a117d1bf3e83 · outbound

This paper cites Fabbrichesi, E.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Fabbrichesi, E

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.307026Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 005bd016-6ad9-4d77-b5b3-2995289412a6 · outbound

This paper cites an unresolved cited work.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Unresolved cited work

Reference 15

Resolution: unresolved; raw_fallback, observed 2026-05-25T04:16:36.299270Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation a2dc9b73-0da2-458b-ac48-bddcc02c124f · outbound

This paper cites Covariant Compton Scattering Kernel in General Relativistic Radiative Transfer.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Covariant Compton Scattering Kernel in General Relativistic Radiative Transfer

Reference 16

Resolution: verified exact; local_arxiv, observed 2026-05-25T04:16:36.052370Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation cdbafe26-091c-4309-b62c-daaba019fac8 · outbound

This paper cites plasma conditions or specific couplings related to the WISP considered.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades plasma conditions or specific couplings related to the WISP considered

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.269120Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 18790869-b321-426f-a490-7eba0d76d9ec · outbound

This paper cites an unresolved cited work.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Unresolved cited work

Reference 18

Resolution: unresolved; raw_fallback, observed 2026-05-25T04:16:36.276397Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 7122ba0a-ed0e-401d-bcbd-8a696feb6a77 · outbound

This paper cites an unresolved cited work.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Unresolved cited work

Reference 19

Resolution: unresolved; raw_fallback, observed 2026-05-25T04:16:36.279039Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation d2516725-5bb7-41b2-9925-59fc99a02b7b · outbound

This paper cites an unresolved cited work.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Unresolved cited work

Reference 20

Resolution: unresolved; raw_fallback, observed 2026-05-25T04:16:36.286438Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 92dbd547-7ee1-46c3-990c-f797aab7f452 · outbound

This paper cites Redondo and G.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Redondo and G

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.261955Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation ad999d64-a257-468d-b28b-c95772bcacfd · outbound

This paper cites Hardy and R.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Hardy and R

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.271083Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 01e5f3ad-f234-404d-8778-b00664fd301a · outbound

This paper cites Redondo, Helioscope Bounds on Hidden Sector Pho- tons, JCAP07, 008.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Redondo, Helioscope Bounds on Hidden Sector Pho- tons, JCAP07, 008

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.289508Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation e3ba0872-d729-4eb9-90fa-2b90e15c8e74 · outbound

This paper cites The XENONnT Dark Matter Experiment.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades The XENONnT Dark Matter Experiment

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-25T04:16:36.055893Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 9d88aab6-e759-47a5-b67b-5b1f9ce55ca2 · outbound

This paper cites Direct detection of solar chameleons with electron recoil data from XENONnT.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Direct detection of solar chameleons with electron recoil data from XENONnT

Reference 25

Resolution: verified exact; arxiv_id, observed 2026-05-26T03:04:07.320045Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 1de44e91-81a0-498f-875c-9821285f764a · outbound

This paper cites Physics potential of the International Axion Observatory (IAXO).

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Physics potential of the International Axion Observatory (IAXO)

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-05-25T04:16:36.058864Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 87aba9d7-57fe-41e9-ae7e-289a1dbbc1aa · outbound

This paper cites Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-05-25T04:16:36.044485Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation cf7edbbf-77de-45ac-9d4d-66bb3a79840d · outbound

This paper cites An accurate solar axions ray-tracing response of BabyIAXO.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades An accurate solar axions ray-tracing response of BabyIAXO

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-05-25T04:16:36.035131Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 9f65c17e-55a4-44b6-bc1d-d96e297c09c7 · outbound

This paper cites Herrera and A.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Herrera and A

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.319451Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation a1d0ebc8-5879-4b85-8303-5047e6113a1b · outbound

This paper cites number per second.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades number per second

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.313868Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation cb6eaf3e-5c1f-4ad7-b651-b2fcc64c4f07 · outbound

This paper cites The 511 keV emission from positron annihilation in the Galaxy.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades The 511 keV emission from positron annihilation in the Galaxy

Reference 31

Resolution: verified exact; local_arxiv, observed 2026-05-25T04:16:36.041145Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 8823cbef-509b-4491-b99f-b80151f23e08 · outbound

This paper cites Agostinelliet al.(GEANT4), GEANT4 - A Simulation Toolkit, Nucl.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Agostinelliet al.(GEANT4), GEANT4 - A Simulation Toolkit, Nucl

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.304671Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 8d362ef9-2a3c-4a60-b032-16dee609ebcd · outbound

This paper cites [34]K th denotes the thermalization energy scale in the Sun, of the order of the solar-core thermal energy.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades [34]K th denotes the thermalization energy scale in the Sun, of the order of the solar-core thermal energy

Reference 33

Resolution: verified fuzzy; raw_fallback, observed 2026-05-25T04:16:36.318118Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation c890f9fa-c792-4269-89c0-0a5ac2e9bcc8 · outbound

This paper cites an unresolved cited work.

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades Unresolved cited work

Reference 34

Resolution: unresolved; raw_fallback, observed 2026-05-25T04:16:36.307705Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Pith citing papers

No inbound Pith citation observations are available.