Paper Citation Record · LEDGER

Understanding acoustic scale observations: the one-sided fight against $\Lambda$

As of 11 August 2026, this Paper Citation Record lists 47 of 47 outbound references and 7 inbound Pith citation observations for arXiv:2412.13894.

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pith.paper-citation-record.v1
2412.13894 v3

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Outbound references

Observation 7cc5fc68-efc2-4a65-8b36-1e0e993add7b · outbound

This paper cites (2.3) combined with the Friedmann equation implies: Z z∗ 0 dzp ρm(z) + ρde(z) = Z z∗ 0 dzp ρm(z) + ρΛ.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ (2.3) combined with the Friedmann equation implies: Z z∗ 0 dzp ρm(z) + ρde(z) = Z z∗ 0 dzp ρm(z) + ρΛ

Reference 1

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Observation 6f2d1668-e8b9-4861-b184-fd96da19d042 · outbound

This paper cites 2.3) implies that DH (z) and DΛ H (z) must cross at some redshift zc: DH (zc) = DΛ H (zc) for some 0 < zc < z∗.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ 2.3) implies that DH (z) and DΛ H (z) must cross at some redshift zc: DH (zc) = DΛ H (zc) for some 0 < zc < z∗

Reference 2

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Observation a32b7282-63fc-4a44-8174-75aa2caf185d · outbound

This paper cites (2.12) At low redshift before the crossing point, z < zc, we have DH (z) > DΛ H (z), which implies that DM (z) = Z z 0 DH (z′) dz′ > Z z 0 DΛ H (z′) dz′ = DΛ M (z).

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ (2.12) At low redshift before the crossing point, z < zc, we have DH (z) > DΛ H (z), which implies that DM (z) = Z z 0 DH (z′) dz′ > Z z 0 DΛ H (z′) dz′ = DΛ M (z)

Reference 3

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Observation 0f6bcaff-cbb4-46cf-a498-cfd04f379bf5 · outbound

This paper cites (2.11) that DH /DΛ H ≤ 1.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ (2.11) that DH /DΛ H ≤ 1

Reference 4

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Observation c18450e2-d7f1-4793-be08-20889eddaed9 · outbound

This paper cites (2.21) Hence, DM (z)/DΛ M (z) decreases monotonically towards one at high redshift.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ (2.21) Hence, DM (z)/DΛ M (z) decreases monotonically towards one at high redshift

Reference 5

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Observation 6364ed42-3174-421d-a9c1-452c6024f3f2 · outbound

This paper cites However, we know DM (0) = DΛ M (0) = 0 and that at high redshift DM (z∗)3 = DΛ M (z∗)3, so we infer that the derivative must cross below one at some point if it starts above one.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ However, we know DM (0) = DΛ M (0) = 0 and that at high redshift DM (z∗)3 = DΛ M (z∗)3, so we infer that the derivative must cross below one at some point if it starts above one

Reference 6

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Observation a1e453f5-fbc8-4e0f-9852-1e7f92ccb16a · outbound

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

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Planck 2018 results. VI. Cosmological parameters

Reference 7

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Observation 8a7498ab-7c71-479d-ad72-9fb26049cd91 · outbound

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

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ CMB constraints on the early universe independent of late time cosmology

Reference 8

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Observation 8c386556-c0c7-4752-addb-26df0412ea08 · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 9

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Observation 944adc0e-6668-4459-9fd5-a91b74ec1560 · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 10

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Observation ad29c9d6-d255-4714-9de3-25486674a32f · outbound

This paper cites DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data

Reference 11

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Observation cc435d74-0181-4320-939f-9fccec313315 · outbound

This paper cites DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data

Reference 12

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Observation 1fe0dc59-92be-4c09-b1d3-5fc1b8e37531 · outbound

This paper cites Interpreting DESI's evidence for evolving dark energy.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Interpreting DESI's evidence for evolving dark energy

Reference 13

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Observation 2a0f5f65-98c0-4935-b1f2-79840d77b0be · outbound

This paper cites Interpreting Dark Energy Data Away from $\Lambda$.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Interpreting Dark Energy Data Away from $\Lambda$

Reference 14

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Observation 18c656b9-63d0-4a64-8390-b21e1c969f27 · outbound

This paper cites A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data

Reference 15

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Observation 38e3a989-3714-4bbb-8fe9-b0c67896eac8 · outbound

This paper cites Extended Dark Energy analysis using DESI DR2 BAO measurements.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 16

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Observation e857d3c6-ef02-445d-a70c-cb3b724ed5bb · outbound

This paper cites The Weak Energy Condition and the Expansion History of the Universe.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ The Weak Energy Condition and the Expansion History of the Universe

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Observation 77cb9730-9af4-432f-8546-d7519e0ea1f3 · outbound

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Accelerating Universes with Scaling Dark Matter

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Observation b84aa87a-83cc-4da5-9038-b29b182573d7 · outbound

This paper cites Exploring the Expansion History of the Universe.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Exploring the Expansion History of the Universe

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Observation b25c20f2-ce53-47ba-9fdf-f839d76d7279 · outbound

This paper cites Assessing observational constraints on dark energy.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Assessing observational constraints on dark energy

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Observation 07cd1c77-5843-4a0c-bde5-25b54de7b2ad · outbound

This paper cites Scant evidence for thawing quintessence.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Scant evidence for thawing quintessence

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Observation f5ab1433-93f2-443e-8142-1d7e343dd45a · outbound

This paper cites Do Observations Prefer Thawing Quintessence?.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Do Observations Prefer Thawing Quintessence?

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This paper cites Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry

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This paper cites Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes

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This paper cites JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ JWST Validates HST Distance Measurements: Selection of Supernova Subsample Explains Differences in JWST Estimates of Local H0

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Observation df59323b-c84c-4520-b37d-eb866eab1b4f · outbound

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Leveraging SN Ia spectroscopic similarity to improve the measurement of $H_0$

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This paper cites Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder

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Observation 36d90934-1a20-44e2-bd7b-52a353f156aa · outbound

This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

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Observation e8f42ce3-080b-4a32-ac1e-efdd47fc1918 · outbound

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Calibrating Dark Energy

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Underdetermination of dark energy

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Observation 6e088127-b5cf-4862-a7d2-64b474f317a7 · outbound

This paper cites Planck 2018 results. VIII. Gravitational lensing.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Planck 2018 results. VIII. Gravitational lensing

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Observation fc156cae-f1f0-4c26-bf90-219050cda125 · outbound

This paper cites DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements.

Understanding acoustic scale observations: the one-sided fight against $\Lambda$ DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Planck intermediate results. LVII. Joint Planck LFI and HFI data processing

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Observation d1869acf-15b3-4151-8a2b-b540ed692bdc · outbound

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ CMB power spectra and cosmological parameters from Planck PR4 with CamSpec

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Cobaya: Code for Bayesian Analysis of hierarchical physical models

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Efficient Computation of CMB anisotropies in closed FRW models

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ GetDist: a Python package for analysing Monte Carlo samples

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Observation 93ef1283-6969-481f-b140-7ce0a470d292 · outbound

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

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Observation 27b848f0-7208-414c-aadb-7271a482465e · outbound

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Evolving Dark Energy or Supernovae Systematics?

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ The axis of systematic bias in SN~Ia cosmology and implications for DESI 2024 results

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ BAO vs. SN evidence for evolving dark energy

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: Investigation based on "Evolving Dark Energy or Supernovae systematics?"

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ The Pantheon+ Analysis: Cosmological Constraints

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Testing for a Super-Acceleration Phase of the Universe

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Understanding acoustic scale observations: the one-sided fight against $\Lambda$ Scalar field dark energy models: Current and forecast constraints

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Pith citing papers

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Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations Understanding acoustic scale observations: the one-sided fight against $\Lambda$

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An overview of what current data can (and cannot yet) say about evolving dark energy Understanding acoustic scale observations: the one-sided fight against $\Lambda$

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DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints cites this paper.

DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints Understanding acoustic scale observations: the one-sided fight against $\Lambda$

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Observation 37058385-2bf0-44ce-9a04-26bf5eb4ee6c · inbound

Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.

Resolving the Planck-DESI tension by nonminimally coupled quintessence Understanding acoustic scale observations: the one-sided fight against $\Lambda$

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 006ec226-f9bc-4812-9ff9-0a55306a7c68 · inbound

Phenomenology of an Open Effective Field Theory of Dark Energy cites this paper.

Phenomenology of an Open Effective Field Theory of Dark Energy Understanding acoustic scale observations: the one-sided fight against $\Lambda$

Reference 1

Resolution: verified exact; arxiv_id, observed 2026-05-15T11:39:58.894161Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 53703ec6-4c9d-4946-865e-4250abaacdcf · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Understanding acoustic scale observations: the one-sided fight against $\Lambda$

Reference 196

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:51.261923Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 059fd1da-1797-4527-9950-98354bd41d05 · inbound

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide cites this paper.

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide Understanding acoustic scale observations: the one-sided fight against $\Lambda$

Reference 112

Resolution: unresolved; no resolver link, observed 2026-08-01T16:30:06.489198Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.