Paper Citation Record · LEDGER

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets

As of 12 August 2026, this Paper Citation Record lists 44 of 44 outbound references and 2 inbound Pith citation observations for arXiv:2412.14342.

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

pith.paper-citation-record.v1
2412.14342 v1

Coverage vector

measured 44 of 44 reference resolution

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T06:07:22.048576Z

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

Source: arxiv_reference, observed 2026-07-03T02:57:35.038585Z

Reference resolution

44 of 44 outbound references displayed

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External citation measurements

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Outbound references

Observation a9aac5b7-696c-4677-b738-7d99da62f1d0 · outbound

This paper cites The DM temperature Tχ in this case is the average of the nucleon temperatures with which the DM is in thermal contact with, weighted by the local inter- action rate.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets The DM temperature Tχ in this case is the average of the nucleon temperatures with which the DM is in thermal contact with, weighted by the local inter- action rate

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.463005Z

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Observation 3abaa468-2ee1-4691-ac89-0c396a266cb9 · outbound

This paper cites Knudsen correction.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Knudsen correction

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.453620Z

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Observation b8221c6f-5f26-4d4a-b543-26840ce3636e · outbound

This paper cites [4, 8] ( mχ = 1 kg, R⋆ = 2.4 m), and a realistic solar model using temperature, density and composition data from the AGS05 Standard Solar Model.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets [4, 8] ( mχ = 1 kg, R⋆ = 2.4 m), and a realistic solar model using temperature, density and composition data from the AGS05 Standard Solar Model

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.444366Z

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Observation 86fa8129-570f-463d-830d-5d5e5509450a · outbound

This paper cites Po- sitions are drawn randomly from the radial distri- bution in Eq.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Po- sitions are drawn randomly from the radial distri- bution in Eq

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.435457Z

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Observation c4cbe758-59b7-47dd-b973-1f812ac3262e · outbound

This paper cites This is achieved by randomly choosing an optical depth τ , where dτ = X i ωi(⃗ v)dt.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets This is achieved by randomly choosing an optical depth τ , where dτ = X i ωi(⃗ v)dt

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.425726Z

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Observation 86965c88-cfc2-479b-938c-2aa1db6ad255 · outbound

This paper cites In our previous work [1], as per Refs.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets In our previous work [1], as per Refs

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.416455Z

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Observation 233c80a9-326f-47ec-ac6a-5c0e19fb0673 · outbound

This paper cites Whereas our previous work in Ref.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Whereas our previous work in Ref

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.406711Z

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Observation c218b7e6-a62f-438c-a6dd-7506a22a0196 · outbound

This paper cites (19) To do this we implement the sampling algorithm outlined in Ref.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets (19) To do this we implement the sampling algorithm outlined in Ref

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.397142Z

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Observation 61c352a4-3a4b-4a72-ac6c-74095aa692bd · outbound

This paper cites 1 Noting a missing square root in the conditional expression of Algorithm 1: ξ6 < p y2 + z − 2xyµ/(y + x).

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets 1 Noting a missing square root in the conditional expression of Algorithm 1: ξ6 < p y2 + z − 2xyµ/(y + x)

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.387668Z

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Observation 033acd38-a039-4d18-ba3e-b1bf4be9b62f · outbound

This paper cites Simulation of energy transport by dark matter scattering in stars.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Simulation of energy transport by dark matter scattering in stars

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T12:24:13.913138Z

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Observation 2c7bb628-963e-43f4-85e7-40386701b2ab · outbound

This paper cites First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-11T12:24:13.916952Z

Source-reported events for the cited work

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Observation 598e53ab-597d-404d-a651-1d1b2c32199f · outbound

This paper cites Effect of hypo- thetical, weakly interacting, massive particles on energy transport in the solar interior,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Effect of hypo- thetical, weakly interacting, massive particles on energy transport in the solar interior,

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.376926Z

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Observation f47aeed3-6b00-40bb-a5a9-375049ded5bb · outbound

This paper cites Thermal conduction by massive particles,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Thermal conduction by massive particles,

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.368002Z

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Observation 68279557-ee10-43ca-83dc-fc48035ec597 · outbound

This paper cites Non- relativistic effective theory of dark matter direct detec- tion,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Non- relativistic effective theory of dark matter direct detec- tion,

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.359524Z

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Observation 581a7d29-3d10-44a1-8f75-b8e8d54b8f53 · outbound

This paper cites The effective field theory of dark matter direct detection,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets The effective field theory of dark matter direct detection,

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.350672Z

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Observation 58af8f7f-3885-497d-a2cd-a8df12d1bbf3 · outbound

This paper cites Form factors for dark matter capture by the Sun in effective theories,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Form factors for dark matter capture by the Sun in effective theories,

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.341631Z

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Observation 70e9321f-36ce-42c1-822a-40e4aee66342 · outbound

This paper cites Cosmion energy transfer in stars - The Knudsen limit,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Cosmion energy transfer in stars - The Knudsen limit,

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.332762Z

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Observation aded7f52-327f-44a2-bfdd-0b97cbebbc07 · outbound

This paper cites Dark stars at the Galactic Centre - The main sequence,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Dark stars at the Galactic Centre - The main sequence,

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.323559Z

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Observation cf4a2923-1798-4c50-a3e5-ce9de1817f56 · outbound

This paper cites Energy transport and Evaporation of weakly interacting particles in the sun,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Energy transport and Evaporation of weakly interacting particles in the sun,

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.314454Z

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Observation 8c3919e4-7072-470c-9f52-91ed0d799bca · outbound

This paper cites An improved target velocity sampling algorithm for free gas elastic scattering,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets An improved target velocity sampling algorithm for free gas elastic scattering,

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.305068Z

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Observation 6e32297b-32a8-4203-983e-fa34173a0092 · outbound

This paper cites A new Generation of Standard Solar Models.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets A new Generation of Standard Solar Models

Reference 21

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Observation 526f1ea7-c08d-4f59-9c2f-031f91a8dd5c · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA).

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Modules for Experiments in Stellar Astrophysics (MESA)

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-11T12:24:13.954554Z

Source-reported events for the cited work

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Observation 1a665514-ba3b-4789-8107-cb8df4d3a153 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars

Reference 23

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Observation 658361f5-c6d9-400a-9409-f67d2d01057f · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions

Reference 24

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Observation 39828ef9-b6e2-4564-88d1-c7670d83d8d2 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions

Reference 25

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Source-reported events for the cited work

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Observation 821e7d98-c686-41a0-9854-e758d0edc029 · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation

Reference 26

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Observation e8f61cef-88e4-4d82-8fa6-1f7188bd343b · outbound

This paper cites Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-11T12:24:13.972107Z

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Observation 5fc69a7f-6e9d-4c53-8771-2ff34ac359da · outbound

This paper cites Preliminary ref- erence Earth model,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Preliminary ref- erence Earth model,

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.293688Z

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Observation a760120f-0159-4db9-b298-e4057f6331f9 · outbound

This paper cites 7.06 - temperatures, heat, and energy in the mantle of the Earth,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets 7.06 - temperatures, heat, and energy in the mantle of the Earth,

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.283595Z

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Observation db82743f-6be5-485b-be72-d9854a869edc · outbound

This paper cites The K/U ratio of the silicate Earth: Insights into mantle com- position, structure and thermal evolution,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets The K/U ratio of the silicate Earth: Insights into mantle com- position, structure and thermal evolution,

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.273712Z

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Observation b0e6b263-bab9-49a4-bdfb-d738bd8b10ee · outbound

This paper cites Earle, Physical Geology(BCcampus, 2015).

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Earle, Physical Geology(BCcampus, 2015)

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.264251Z

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Observation dbc4f112-4974-4998-9f95-a1139f55d671 · outbound

This paper cites Dark Matter, Destroyer of Worlds: Neutrino, Thermal, and Existential Signatures from Black Holes in the Sun and Earth.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Dark Matter, Destroyer of Worlds: Neutrino, Thermal, and Existential Signatures from Black Holes in the Sun and Earth

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-11T12:24:13.988534Z

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Observation ddc0e143-786a-4779-9a13-2a9d8d3b3830 · outbound

This paper cites Temperature and composition of the earth’s core,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Temperature and composition of the earth’s core,

Reference 33

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.254500Z

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Observation c733ffa2-7db7-4abd-9ded-1ae5f79c8414 · outbound

This paper cites Major and trace element composition of the depleted morb mantle (dmm),.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Major and trace element composition of the depleted morb mantle (dmm),

Reference 34

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.244591Z

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Observation 8a4eb7f7-4a99-4448-925e-84ebb81990b3 · outbound

This paper cites The elementary composition of the earth’s crust,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets The elementary composition of the earth’s crust,

Reference 35

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.235341Z

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Observation 8fb94f0f-b968-46ea-b83a-b63cf32f5946 · outbound

This paper cites Evaporation of WIMPs with arbitrary cross sections,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Evaporation of WIMPs with arbitrary cross sections,

Reference 36

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.226032Z

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Observation 0dd8522a-197c-489c-b304-baf8cb5ed856 · outbound

This paper cites Floating Dark Matter in Celestial Bodies.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Floating Dark Matter in Celestial Bodies

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-11T12:24:14.006900Z

Source-reported events for the cited work

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Observation 95d56e73-1827-434f-b857-518a8987f1c8 · outbound

This paper cites Evaporation and scattering of momentum- and velocity-dependent dark matter in the Sun,.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Evaporation and scattering of momentum- and velocity-dependent dark matter in the Sun,

Reference 38

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.216024Z

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Observation add3ffc0-ae0e-43ff-93ef-6be374459a05 · outbound

This paper cites Dark matter in the Sun: scattering off electrons vs nucleons.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Dark matter in the Sun: scattering off electrons vs nucleons

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-11T12:24:14.013511Z

Source-reported events for the cited work

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This paper cites This guide assumes the GNU Fortran compiler (gfortran).

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets This guide assumes the GNU Fortran compiler (gfortran)

Reference 40

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.206128Z

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Observation 5f04db51-8e60-4698-81f1-2531efa554ec · outbound

This paper cites s o make cosmion.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets s o make cosmion

Reference 41

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:24:14.195663Z

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Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets nucleonSI

Reference 42

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Observation a27545e7-97c8-44d2-ac3f-0393bd5783c1 · outbound

This paper cites an unresolved cited work.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Unresolved cited work

Reference 43

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Source-reported events for the cited work

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Observation 4cf6c232-0edc-4ce3-be8f-d400d9c61ce2 · outbound

This paper cites an unresolved cited work.

Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets Unresolved cited work

Reference 44

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Pith citing papers

Observation e81f666d-e192-4cae-8a3c-13ca6d9cb16d · inbound

Complementary Planetary Spectroscopy Probes of Dark Matter cites this paper.

Complementary Planetary Spectroscopy Probes of Dark Matter Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets

Reference 148

Resolution: unresolved; no resolver link, observed 2026-08-06T06:07:22.048576Z

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Observation f202ca16-94f0-4665-a677-a06a952736fb · inbound

Constraints and Projections for Millicharged Dark Matter in the Sun with Water Cherenkov Neutrino Detectors cites this paper.

Constraints and Projections for Millicharged Dark Matter in the Sun with Water Cherenkov Neutrino Detectors Simulation of thermal conduction by asymmetric dark matter in realistic stars and planets

Reference 98

Resolution: verified exact; arxiv_id, observed 2026-07-03T02:57:35.039956Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.