Paper Citation Record · LEDGER

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential

As of 15 August 2026, this Paper Citation Record lists 65 of 65 outbound references and 3 inbound Pith citation observations for arXiv:2412.02519.

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pith.paper-citation-record.v1
2412.02519 v1

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Reference resolution

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Outbound references

Observation cab4cc5a-9cb8-4a2e-aa24-15fbdffa51de · outbound

This paper cites an unresolved cited work.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

Reference 1

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This paper cites The Thomas- Fermi regime no longer exists and the soliton is deter- mined by the balance between gravity and the quantum pressure.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential The Thomas- Fermi regime no longer exists and the soliton is deter- mined by the balance between gravity and the quantum pressure

Reference 2

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This paper cites (44) We recover the scaling (32).

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential (44) We recover the scaling (32)

Reference 3

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This paper cites (33) This bypasses the numerical computation of the soliton profiles and should provide the correct scalings and be- haviors.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential (33) This bypasses the numerical computation of the soliton profiles and should provide the correct scalings and be- haviors

Reference 4

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This paper cites (42) Up to factors of order unity, we recover the exact result (30).

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential (42) Up to factors of order unity, we recover the exact result (30)

Reference 5

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This paper cites The Waning of the WIMP? A Review of Models, Searches, and Constraints.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential The Waning of the WIMP? A Review of Models, Searches, and Constraints

Reference 6

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

Reference 12

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This paper cites V A 1, we first set the threshold ρc = 500 to a very high value so that the self-interaction potential always takes the form Φ I = λρ.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential V A 1, we first set the threshold ρc = 500 to a very high value so that the self-interaction potential always takes the form Φ I = λρ

Reference 13

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This paper cites 9 the case of a small thresh- old, ρc = 0.5.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential 9 the case of a small thresh- old, ρc = 0.5

Reference 14

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential 13 the intermediate case ρc = 80

Reference 18

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Supersymmetric Dark Matter

Reference 19

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Drees, R

Reference 20

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Steigman and M

Reference 21

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Direct Detection of WIMP Dark Matter: Concepts and Status

Reference 22

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Indirect Detection of WIMP Dark Matter: a compact review

Reference 23

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Phase transitions between dilute and dense axion stars

Reference 24

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Cold dark matter: controversies on small scales

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Small scale problems of the $\Lambda$CDM model: a short review

Reference 26

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Shedding light on the small-scale crisis with CMB spectral distortions

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential The landscape of QCD axion models

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Cold and Fuzzy Dark Matter

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This paper cites Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential

Reference 30

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Ultralight scalars as cosmological dark matter

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Goodman, New Astron

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Scalar Field as Dark Matter in the Universe

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Cosmic Structure as the Quantum Interference of a Coherent Dark Wave

Reference 34

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Ultra-Light Dark Matter

Reference 35

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Cosmological Constraints on Bose-Einstein-Condensed Scalar Field Dark Matter

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Do Dark Matter Axions Form a Condensate with Long-Range Correlation?

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Bose-Einstein Condensation of Dark Matter Axions

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Axion Cosmology

Reference 40

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Formation and structure of ultralight bosonic dark matter halos

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: I. Analytical results

Reference 42

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Core-Envelope Haloes in Scalar Field Dark Matter with Repulsive Self-Interaction: Fluid Dynamics Beyond the de Broglie Wavelength

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Cosmological structure formation in scalar field dark matter with repulsive self-interaction: The Incredible Shrinking Jeans Mass

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Weinberg, Phys

Reference 46

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Wilczek, Phys

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Unresolved cited work

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Monodromy in the CMB: Gravity Waves and String Inflation

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Gravity Waves and Linear Inflation from Axion Monodromy

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Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Impact of kinetic and potential self-interactions on scalar dark matter

Reference 51

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Observation c77fca79-45ac-44bf-a740-2874f2f0f848 · outbound

This paper cites Madelung, Z.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Madelung, Z

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-11T23:27:52.095817Z

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Observation 1ab4ac0d-0e0f-4292-8731-f08f98af3b85 · outbound

This paper cites Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: II. Numerical results.

Reference 53

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Observation 6869b293-3ca7-4219-8270-6ebe59c8b561 · outbound

This paper cites Evolution of cosmological perturbations in Bose-Einstein condensate dark matter.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Evolution of cosmological perturbations in Bose-Einstein condensate dark matter

Reference 54

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Observation a45437f9-cbfc-4ea9-af71-5b7eaaf4d5a3 · outbound

This paper cites Non-Relativistic Formation of Scalar Clumps as a Candidate for Dark Matter.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Non-Relativistic Formation of Scalar Clumps as a Candidate for Dark Matter

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-08-11T23:27:52.301192Z

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Observation 26e23500-0fa0-4566-a097-3f4992d75ef6 · outbound

This paper cites Self-consistent construction of virialized wave dark matter halos.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Self-consistent construction of virialized wave dark matter halos

Reference 56

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Observation 596338da-09aa-4ed5-ad93-87dfbcbfd2c3 · outbound

This paper cites Construction of Wave Dark Matter Halos: Numerical Algorithm and Analytical Constraints.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Construction of Wave Dark Matter Halos: Numerical Algorithm and Analytical Constraints

Reference 57

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Observation 46393341-d571-4274-b846-b5fe08d19310 · outbound

This paper cites Binney and S.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Binney and S

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T23:27:52.769258Z

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Observation 331cc734-8676-4a7d-89eb-1899acc97b03 · outbound

This paper cites Pathria and J.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Pathria and J

Reference 59

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Observation d9f242f7-6bb7-410c-a2b9-5976742db216 · outbound

This paper cites Zhang and M.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Zhang and M

Reference 60

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Observation 2d1038f8-2baf-4e3f-8120-e7de342a5fd2 · outbound

This paper cites PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics

Reference 61

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Observation e7d6af8f-d1d6-4832-a425-f826bf3c4f4b · outbound

This paper cites Solitons and halos for self-interacting scalar dark matter.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Solitons and halos for self-interacting scalar dark matter

Reference 62

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Observation a2bc70e1-f3d7-491f-a644-2576054c4aee · outbound

This paper cites Gravitational Bose-Einstein condensation in the kinetic regime.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Gravitational Bose-Einstein condensation in the kinetic regime

Reference 63

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Observation e258c3ba-63d9-460f-9f67-1cefe3a5270d · outbound

This paper cites Condensation and Evaporation of Boson Stars.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Condensation and Evaporation of Boson Stars

Reference 64

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Observation e6689980-479b-4dcc-87ee-70b49ce1e120 · outbound

This paper cites Kinetic relaxation and Bose-star formation in multicomponent dark matter- I.

Formation of solitons and their transitions in scalar-field dark matter models with a non-polynomial self-interaction potential Kinetic relaxation and Bose-star formation in multicomponent dark matter- I

Reference 65

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Observation 0ba31398-3d6f-4c28-a875-c822018ab886 · inbound