Paper Citation Record · LEDGER

Topological defects as effective dynamical dark energy

As of 7 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 2 inbound Pith citation observations for arXiv:2506.10075.

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

pith.paper-citation-record.v1
2506.10075 v1

Coverage vector

measured 74 of 74 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T04:41:33.794114Z

measured 76 of 76 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-29T05:39:36.647189Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-29T05:43:08.242636Z

Reference resolution

74 of 74 outbound references displayed

verified exact4
verified fuzzy2
unresolved68
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 3e76b706-2dfb-4c39-b4b9-3461b486e6c3 · outbound

This paper cites Cosmological Evolution of a Quintom Model of Dark Energy.

Topological defects as effective dynamical dark energy Cosmological Evolution of a Quintom Model of Dark Energy

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.534677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4098a4fd-2944-4184-9b16-ba01b8e20bf9 · outbound

This paper cites Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom.

Topological defects as effective dynamical dark energy Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.539510Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2e0fb7c9-5a6f-4d64-9be1-ad9a7b613bd2 · outbound

This paper cites The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae.

Topological defects as effective dynamical dark energy The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.543751Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 55320898-2ba4-4329-b558-1c88458a31a2 · outbound

This paper cites Late-time cosmic acceleration from quantum gravity.

Topological defects as effective dynamical dark energy Late-time cosmic acceleration from quantum gravity

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.547613Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a384f8b5-d218-427b-828c-fcf9295ccccf · outbound

This paper cites Comparison of dynamical dark energy with {\Lambda}CDM in light of DESI DR2.

Topological defects as effective dynamical dark energy Comparison of dynamical dark energy with {\Lambda}CDM in light of DESI DR2

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.551299Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1da33b0f-2abf-4739-b23f-91781238def7 · outbound

This paper cites Dynamical dark energy from an ultralight axion.

Topological defects as effective dynamical dark energy Dynamical dark energy from an ultralight axion

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.555260Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 86c69dec-e9b2-405b-b318-93ad4bb68581 · outbound

This paper cites Isotropic cosmic birefringence from string axion domain walls without cosmic strings, and DESI results.

Topological defects as effective dynamical dark energy Isotropic cosmic birefringence from string axion domain walls without cosmic strings, and DESI results

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.558958Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f9914a5-7a56-4746-9495-391187a89b67 · outbound

This paper cites Interpreting Cosmic Birefringence and DESI Data with Evolving Axion in $\Lambda$CDM.

Topological defects as effective dynamical dark energy Interpreting Cosmic Birefringence and DESI Data with Evolving Axion in $\Lambda$CDM

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.562824Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 566de9c0-27e7-4be3-896f-564dfcec5c79 · outbound

This paper cites S-dual Quintessence, the Swampland, and the DESI DR2 Results.

Topological defects as effective dynamical dark energy S-dual Quintessence, the Swampland, and the DESI DR2 Results

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.566843Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f711d1a1-a0a3-4300-ab6d-d5d34ad2f283 · outbound

This paper cites Dynamical Dark Energy, Dual Spacetime, and DESI.

Topological defects as effective dynamical dark energy Dynamical Dark Energy, Dual Spacetime, and DESI

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.570593Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 551a55d0-c88e-4cd2-a03a-f619fba2b61a · outbound

This paper cites The Impact of the Hubble Tension on the Evidence for Dynamical Dark Energy.

Topological defects as effective dynamical dark energy The Impact of the Hubble Tension on the Evidence for Dynamical Dark Energy

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.574514Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 21e9aa56-e589-440f-9d3c-306575ef9e68 · outbound

This paper cites To CPL, or not to CPL? What we have not learned about the dark energy equation of state.

Topological defects as effective dynamical dark energy To CPL, or not to CPL? What we have not learned about the dark energy equation of state

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.578311Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c27fc521-a21e-4475-bb93-09238cf36edf · outbound

This paper cites Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO.

Topological defects as effective dynamical dark energy Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.581825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dc236eda-172a-4649-826c-b79d4d34b15d · outbound

This paper cites Dynamical Dark Energy Implies a Coupled Dark Sector: Insights from DESI DR2 via a Data-Driven Approach.

Topological defects as effective dynamical dark energy Dynamical Dark Energy Implies a Coupled Dark Sector: Insights from DESI DR2 via a Data-Driven Approach

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.585676Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0cf01886-b1c9-476d-ae6f-4100a3289936 · outbound

This paper cites One-parameter dynamical dark energy: Hints for oscillations.

Topological defects as effective dynamical dark energy One-parameter dynamical dark energy: Hints for oscillations

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.589096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c4762e60-e2dc-4f45-b1f8-3264951ee51d · outbound

This paper cites Has DESI detected exponential quintessence?.

Topological defects as effective dynamical dark energy Has DESI detected exponential quintessence?

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.592658Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 29940736-2c74-4c4b-a21e-1b3b91fb4fb9 · outbound

This paper cites Whyw̸=−1? Anthropic Selection in a Λ + Axion Dark Energy Model,.

Topological defects as effective dynamical dark energy Whyw̸=−1? Anthropic Selection in a Λ + Axion Dark Energy Model,

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.596430Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1c95c4ed-2fe9-4352-b447-32f031e23359 · outbound

This paper cites Thawing quintessence and transient cosmic acceleration in light of DESI,.

Topological defects as effective dynamical dark energy Thawing quintessence and transient cosmic acceleration in light of DESI,

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.600005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b6ebbdf-c3fb-4a80-bc16-475cd66343f3 · outbound

This paper cites Physical vs phantom dark energy after DESI: thawing quintessence in a curved background.

Topological defects as effective dynamical dark energy Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.603337Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ed8e550d-0946-441b-81c4-dad4208df1b7 · outbound

This paper cites Implications of distance duality violation for the $H_0$ tension and evolving dark energy.

Topological defects as effective dynamical dark energy Implications of distance duality violation for the $H_0$ tension and evolving dark energy

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.606617Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a1d39d0-e365-4427-a382-2b59cb208616 · outbound

This paper cites Assessing cosmological evidence for non-minimal coupling.

Topological defects as effective dynamical dark energy Assessing cosmological evidence for non-minimal coupling

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.610393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94732e5f-90c2-4b3c-a4f6-c0a75e87b427 · outbound

This paper cites Quantum Gravity Meets DESI: Dynamical Dark Energy in Light of the Trans-Planckian Censorship Conjecture.

Topological defects as effective dynamical dark energy Quantum Gravity Meets DESI: Dynamical Dark Energy in Light of the Trans-Planckian Censorship Conjecture

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.614073Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd3e2e67-d93a-44c3-8133-7dbdac792248 · outbound

This paper cites Testing Quintessence Axion Dark Energy with Recent Cosmological Results,.

Topological defects as effective dynamical dark energy Testing Quintessence Axion Dark Energy with Recent Cosmological Results,

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.617600Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95c22741-d0b6-40d7-99fb-a2a0477b1c2c · outbound

This paper cites Screened Axio-dilaton Cosmology: Novel Forms of Early Dark Energy.

Topological defects as effective dynamical dark energy Screened Axio-dilaton Cosmology: Novel Forms of Early Dark Energy

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.621837Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ac0013f3-d38d-4c97-a778-4aeb09768ef0 · outbound

This paper cites Quintessence Dark Matter.

Topological defects as effective dynamical dark energy Quintessence Dark Matter

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.625484Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d8cc6a6d-ea98-4ccd-ab4f-72128f463cc4 · outbound

This paper cites Geometric formulation of $k$-essence and late-time acceleration.

Topological defects as effective dynamical dark energy Geometric formulation of $k$-essence and late-time acceleration

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.629052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb9536bd-5283-4017-8c5b-6472cdd48878 · outbound

This paper cites Examining Quintessence Models with DESI Data.

Topological defects as effective dynamical dark energy Examining Quintessence Models with DESI Data

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.632820Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c15a6ee2-e953-4c59-8cab-2aef76dfd972 · outbound

This paper cites Dynamical Dark Energy at Late Time $\Lambda$CDM.

Topological defects as effective dynamical dark energy Dynamical Dark Energy at Late Time $\Lambda$CDM

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.636189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e77dcac9-4be2-46d3-8734-08cfbff6bc43 · outbound

This paper cites The Quintom theory of dark energy after DESI DR2.

Topological defects as effective dynamical dark energy The Quintom theory of dark energy after DESI DR2

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.639868Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bc909804-4248-49da-af36-8a98cd4ef6a2 · outbound

This paper cites Evidence for non-cold dark matter from DESI DR2 measurements.

Topological defects as effective dynamical dark energy Evidence for non-cold dark matter from DESI DR2 measurements

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.643128Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 930182db-8e22-41a6-ade5-b37347fd077f · outbound

This paper cites When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior,.

Topological defects as effective dynamical dark energy When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior,

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.646487Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d8662ae2-491a-47fc-82d6-43338f4c0b95 · outbound

This paper cites Evidence for Dynamical Dark Matter.

Topological defects as effective dynamical dark energy Evidence for Dynamical Dark Matter

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.649426Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3ca83fea-574d-4bf7-9dce-b0ca774bccae · outbound

This paper cites Evolving Dark Energy or Evolving Dark Matter?.

Topological defects as effective dynamical dark energy Evolving Dark Energy or Evolving Dark Matter?

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.652949Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 711c0148-13f5-461b-8bb6-bc069deb7927 · outbound

This paper cites Interacting Quintessence, Cosmic Acceleration and the Coincidence Problem.

Topological defects as effective dynamical dark energy Interacting Quintessence, Cosmic Acceleration and the Coincidence Problem

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.656158Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 774e35bb-258e-44e7-ae76-e490e8c648d2 · outbound

This paper cites Super-acceleration as Signature of Dark Sector Interaction.

Topological defects as effective dynamical dark energy Super-acceleration as Signature of Dark Sector Interaction

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.659837Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f044c63-f0da-4416-8e98-c0faed9f60cd · outbound

This paper cites Upper limits on dark energy-dark matter interaction from DESI DR2 in a field-theoretic analysis.

Topological defects as effective dynamical dark energy Upper limits on dark energy-dark matter interaction from DESI DR2 in a field-theoretic analysis

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.663195Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ded406ed-af18-4a92-97f1-b924e5e80b1c · outbound

This paper cites DESI results: Hint towards coupled dark matter and dark energy,.

Topological defects as effective dynamical dark energy DESI results: Hint towards coupled dark matter and dark energy,

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.666520Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 33570af3-c004-4624-beaa-9cf9d65d92a4 · outbound

This paper cites Apparent w <−1 and a LowerS 8 from Dark Axion and Dark Baryons Interactions,.

Topological defects as effective dynamical dark energy Apparent w <−1 and a LowerS 8 from Dark Axion and Dark Baryons Interactions,

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.669487Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1c1a5f1a-95da-44c2-8ac8-ce016664417c · outbound

This paper cites Interacting Dark Sectors in light of DESI DR2.

Topological defects as effective dynamical dark energy Interacting Dark Sectors in light of DESI DR2

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.672684Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50d493d4-67ec-4723-a142-48f75f69600b · outbound

This paper cites New constraints on interacting dark energy from DESI DR2 BAO observations.

Topological defects as effective dynamical dark energy New constraints on interacting dark energy from DESI DR2 BAO observations

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.675837Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09642a04-08aa-4e2c-9c41-0262f26d45a6 · outbound

This paper cites Interacting dark energy after DESI DR2: a challenge for ΛCDM paradigm?,.

Topological defects as effective dynamical dark energy Interacting dark energy after DESI DR2: a challenge for ΛCDM paradigm?,

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.679379Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 31a6a164-050c-44f7-a12f-b2c7245ccb30 · outbound

This paper cites Optimal parameterizations for observational constraints on thawing dark energy.

Topological defects as effective dynamical dark energy Optimal parameterizations for observational constraints on thawing dark energy

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.682404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7052afd6-88f0-42b2-a546-23345efeba25 · outbound

This paper cites Modified gravity realizations of quintom dark energy after DESI DR2.

Topological defects as effective dynamical dark energy Modified gravity realizations of quintom dark energy after DESI DR2

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.685582Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ba1c0850-c03b-41c1-a5d2-48218de01243 · outbound

This paper cites Forecasts for interacting dark energy with time-dependent momentum exchange,.

Topological defects as effective dynamical dark energy Forecasts for interacting dark energy with time-dependent momentum exchange,

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.688742Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 997587ef-7b0f-4c78-afc8-77c983d513f8 · outbound

This paper cites Compartmentalization in the Dark Sector of the Universe after DESI DR2 BAO data,.

Topological defects as effective dynamical dark energy Compartmentalization in the Dark Sector of the Universe after DESI DR2 BAO data,

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.691751Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7acc92bc-6857-4701-ae17-5b579160718b · outbound

This paper cites Cosmic curvature on large-scale structures with homogeneous dark energy.

Topological defects as effective dynamical dark energy Cosmic curvature on large-scale structures with homogeneous dark energy

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-08-07T04:41:34.428871Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a0faa318-723b-4309-af37-1cf1f8e0f573 · outbound

This paper cites Bumblebee cosmology: Tests using distance- and time-redshift probes,.

Topological defects as effective dynamical dark energy Bumblebee cosmology: Tests using distance- and time-redshift probes,

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.698093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b82c35d-f145-4a7e-a613-87f210822278 · outbound

This paper cites Non-minimally coupled gravity constraints from DESI DR2 data.

Topological defects as effective dynamical dark energy Non-minimally coupled gravity constraints from DESI DR2 data

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.700986Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 777aba84-2353-4758-b968-b5aac7bb198e · outbound

This paper cites Dark Energy within the Generalized Uncertainty Principle in Light of DESI DR2,.

Topological defects as effective dynamical dark energy Dark Energy within the Generalized Uncertainty Principle in Light of DESI DR2,

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.704556Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6fabdfba-85c2-4738-9130-152b81bc3208 · outbound

This paper cites Testing f(R)-gravity models with DESI DR2 2025-BAO and other cosmological data.

Topological defects as effective dynamical dark energy Testing f(R)-gravity models with DESI DR2 2025-BAO and other cosmological data

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.707696Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6aade71c-b0ab-499d-9600-a96a7f0add48 · outbound

This paper cites Testing Non-Coincidentf(Q)-gravity with DESI DR2 BAO and GRBs,.

Topological defects as effective dynamical dark energy Testing Non-Coincidentf(Q)-gravity with DESI DR2 BAO and GRBs,

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.710930Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37af0ecd-6dcb-4c85-ac60-dcd9d27d8f84 · outbound

This paper cites Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition.

Topological defects as effective dynamical dark energy Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.713790Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37993655-f299-4caf-9982-397e7e82487d · outbound

This paper cites Dynamical Dark Energy Emerges from Massive Gravity.

Topological defects as effective dynamical dark energy Dynamical Dark Energy Emerges from Massive Gravity

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.716914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6d77a3fd-0c57-4912-99dd-57384aa844c9 · outbound

This paper cites Non-minimally coupled scalar field dark sector of the universe: in-depth (Einstein frame) case study.

Topological defects as effective dynamical dark energy Non-minimally coupled scalar field dark sector of the universe: in-depth (Einstein frame) case study

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.720008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37d699c9-e0c2-471c-a8d5-bdaee3f00e3d · outbound

This paper cites Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years.

Topological defects as effective dynamical dark energy Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years

Reference 58

Resolution: verified exact; local_arxiv, observed 2026-08-07T04:41:34.153080Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 06f07253-f672-45af-9786-7283f1651e24 · outbound

This paper cites Void and Density Walls Inhomogeneous Cosmic Web And Dark Energy.

Topological defects as effective dynamical dark energy Void and Density Walls Inhomogeneous Cosmic Web And Dark Energy

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-08-07T04:41:34.136998Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 18ff8b8c-a59b-4dd4-98c5-f043d781005d · outbound

This paper cites Is Dynamical Dark Energy Necessary? DESI BAO and Modified Recombination,.

Topological defects as effective dynamical dark energy Is Dynamical Dark Energy Necessary? DESI BAO and Modified Recombination,

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.731155Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c577f00f-1e7d-407b-bdad-26e0ef560c27 · outbound

This paper cites Contribution of domain wall networks to the CMB power spectrum.

Topological defects as effective dynamical dark energy Contribution of domain wall networks to the CMB power spectrum

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-08-07T04:41:33.978783Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation cd448d0f-435c-46bc-8479-4f1d06754ae8 · outbound

This paper cites Cosmic Microwave Background anisotropies generated by domain wall networks.

Topological defects as effective dynamical dark energy Cosmic Microwave Background anisotropies generated by domain wall networks

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.738358Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a83849c-8552-4973-9447-d6890b0d8d13 · outbound

This paper cites Cobaya: Code for Bayesian Analysis of hierarchical physical models.

Topological defects as effective dynamical dark energy Cobaya: Code for Bayesian Analysis of hierarchical physical models

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.741988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 691200e2-e50d-41c7-8bde-43971207c8de · outbound

This paper cites Efficient Computation of CMB anisotropies in closed FRW models.

Topological defects as effective dynamical dark energy Efficient Computation of CMB anisotropies in closed FRW models

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.745316Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3518053e-577e-4de9-8b6c-8c1541bb6b2a · outbound

This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.

Topological defects as effective dynamical dark energy The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.748758Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 05ffc42f-8a15-4810-b9ab-39bc35c170fc · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Topological defects as effective dynamical dark energy The Pantheon+ Analysis: Cosmological Constraints

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.752049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b4155625-687a-49df-9c9b-810844d824a0 · outbound

This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.

Topological defects as effective dynamical dark energy Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.757511Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 92555d86-b4c5-467a-9e12-6192526ea6d1 · outbound

This paper cites CMB constraints on the early universe independent of late time cosmology.

Topological defects as effective dynamical dark energy CMB constraints on the early universe independent of late time cosmology

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.761718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bce51d28-61d5-464b-9bb8-2d7699eeef43 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Topological defects as effective dynamical dark energy Planck 2018 results. VI. Cosmological parameters

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.765086Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aa5c6e50-d889-4d18-a208-e96668c9e841 · outbound

This paper cites GetDist: a Python package for analysing Monte Carlo samples.

Topological defects as effective dynamical dark energy GetDist: a Python package for analysing Monte Carlo samples

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.768856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 73888d1b-7c43-4896-a755-97b934846462 · outbound

This paper cites scikit-hep/iminuit,.

Topological defects as effective dynamical dark energy scikit-hep/iminuit,

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.772263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3bf876cd-4141-43f7-9d9c-03d7aaf80d8a · outbound

This paper cites Bayesian measures of model complexity and fit,.

Topological defects as effective dynamical dark energy Bayesian measures of model complexity and fit,

Reference 75

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T04:41:35.417966Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation fc5153a7-dade-4ad1-b8ca-ef20f2cb5a59 · outbound

This paper cites Information criteria for astrophysical model selection,.

Topological defects as effective dynamical dark energy Information criteria for astrophysical model selection,

Reference 76

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T04:41:35.407663Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 0a21022d-a29f-48e7-b2b2-16db9be5fb1b · outbound

This paper cites PolyChord: nested sampling for cosmology.

Topological defects as effective dynamical dark energy PolyChord: nested sampling for cosmology

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.783695Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 04008bfe-cfbc-4c89-9ec3-a49a0b540fa6 · outbound

This paper cites PolyChord: next-generation nested sampling.

Topological defects as effective dynamical dark energy PolyChord: next-generation nested sampling

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.787004Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e3894cf3-72df-4983-8f1a-3910a7781dc7 · outbound

This paper cites anesthetic: nested sampling visualisation.

Topological defects as effective dynamical dark energy anesthetic: nested sampling visualisation

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.790796Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 89deccaf-b8ab-4f69-aef9-f81071aa3cbf · outbound

This paper cites Cosmic Strings as Dynamical Dark Energy: Novel Constraints.

Topological defects as effective dynamical dark energy Cosmic Strings as Dynamical Dark Energy: Novel Constraints

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.794114Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation f751afac-740c-4dde-9761-d6ccaa90b968 · inbound

Domain-wall Quintessence cites this paper.

Domain-wall Quintessence Topological defects as effective dynamical dark energy

Reference 24

Resolution: verified exact; arxiv_id, observed 2026-05-20T02:07:58.778251Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 380d4def-b7e8-4b11-948e-58aecf7a28ea · inbound

Late-time Quantum Vacuum Decay and its Cosmological Implications cites this paper.

Late-time Quantum Vacuum Decay and its Cosmological Implications Topological defects as effective dynamical dark energy

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-06-29T05:43:08.244089Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.