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Paper Citation Record · LEDGER

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$

As of 18 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 0 inbound Pith citation observations for arXiv:2504.17798.

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

pith.paper-citation-record.v1
2504.17798 v1

Coverage vector

measured 51 of 51 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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Reference resolution

51 of 51 outbound references displayed

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External citation measurements

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Outbound references

Observation 0e97c0b1-1272-4a35-b7d7-ce4b6d8ed711 · outbound

This paper cites Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35

Reference 1

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Observation 3539b6d4-8438-47bb-9486-625935316f42 · outbound

This paper cites Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications

Reference 2

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Observation 78a2b10d-a671-4a48-890a-588b2df967a6 · outbound

This paper cites Measurements of Omega and Lambda from 42 High-Redshift Supernovae.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Measurements of Omega and Lambda from 42 High-Redshift Supernovae

Reference 3

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Observation 789fa334-1bd3-4a38-bacd-00a2327898e1 · outbound

This paper cites Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis

Reference 4

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Observation 899149fa-6c91-42f0-a4a5-105eec10d180 · outbound

This paper cites Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis

Reference 5

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Observation 82627af7-aef4-4dbe-99dc-5faa1cb6fb7e · outbound

This paper cites First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results

Reference 6

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Observation 95ce5bf5-842e-4731-8087-d02d7132b376 · outbound

This paper cites Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology

Reference 7

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Observation 4f3ec58a-d787-4040-88cc-6bd7bb64d21d · outbound

This paper cites Anderson et al.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Anderson et al

Reference 8

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Observation 341df8a6-3053-4ea3-acc7-17c941fe92b5 · outbound

This paper cites Aubourg et al.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Aubourg et al

Reference 9

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Observation 4bdbee78-e447-4a12-b2f9-ec51a3e964ba · outbound

This paper cites Blake, S.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Blake, S

Reference 10

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Observation 4a47d234-5e89-4477-9d9d-8fe36550357d · outbound

This paper cites Louis, E.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Louis, E

Reference 11

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An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

Reference 12

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Observation e2ef8c4d-9924-449c-940f-a156d47501bf · outbound

This paper cites Grøn, and S.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Grøn, and S

Reference 13

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Observation 448f377e-ba0e-4dee-88f3-cc27e07ae053 · outbound

This paper cites Abazajian, J.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Abazajian, J

Reference 14

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Observation 08b0a3fd-102b-4b6a-919e-ef2fcdfc3bf1 · outbound

This paper cites Sahni and A.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Sahni and A

Reference 15

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Observation 6727666e-92f8-41dd-979f-541bcbee0bd7 · outbound

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An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

Reference 16

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An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

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Observation ceb1609c-04cb-429c-b076-71817061b290 · outbound

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An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

Reference 18

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Observation c7702b60-43d5-454b-b5ff-ec5a76a6a718 · outbound

This paper cites Szydlowski, Cosmological model with decaying vacuum energy from quantum mechanics, Phys.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Szydlowski, Cosmological model with decaying vacuum energy from quantum mechanics, Phys

Reference 19

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Observation c81ffc47-0a99-45e4-94d4-1ab55cc9f2c4 · outbound

This paper cites Koussour , N.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Koussour , N

Reference 20

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An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

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An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

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An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

Reference 23

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An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

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An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

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Observation 11ec4300-b3b7-480d-b4d2-1c99f6073a56 · outbound

This paper cites Ratra and P.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Ratra and P

Reference 26

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Observation 15edde23-8630-46b5-8214-6fa98e58c72d · outbound

This paper cites An f(R,T) Gravity Based FLRW Model and Observational Constraints.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ An f(R,T) Gravity Based FLRW Model and Observational Constraints

Reference 27

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Observation 7cd1d565-7beb-4341-8ac3-36ab547bfb78 · outbound

This paper cites The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity in Bianchi-I spacetime.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity in Bianchi-I spacetime

Reference 28

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Observation d4a955ad-7409-45f4-82d9-fc37bc542005 · outbound

This paper cites The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity

Reference 29

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Observation 9e44c6fa-ac07-41d0-a22d-e822fdea0260 · outbound

This paper cites Reconstruction of an Observationally Constrained $f(R, T)$ gravity model.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Reconstruction of an Observationally Constrained $f(R, T)$ gravity model

Reference 30

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Observation f4ed2b02-e444-4c54-b0b7-692e9503ef16 · outbound

This paper cites Suzuki et al., The Hubble space telescope cluster supernova survey V improving the dark energy constraints above z >1 and building an early-type-hosted supernova sample, Astrophys.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Suzuki et al., The Hubble space telescope cluster supernova survey V improving the dark energy constraints above z >1 and building an early-type-hosted supernova sample, Astrophys

Reference 31

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Observation 2b80b3dd-d569-4482-ad3f-f3b4a0039a15 · outbound

This paper cites Scolnic, D.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Scolnic, D

Reference 32

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Observation dfa74e34-2894-4510-993e-36bb4053512d · outbound

This paper cites The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

Reference 33

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Observation 8074fecb-2dff-47d3-ae77-c9126a732972 · outbound

This paper cites Giostri, M.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Giostri, M

Reference 34

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation e12afa5a-3437-4e77-a7a5-fa89cbfe8c8e · outbound

This paper cites Goswami, and Anirudh Pradhan, An axially symmetric transi- tioning model with observational constraints, Chin J Phys, 80, 261–274(2022).

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Goswami, and Anirudh Pradhan, An axially symmetric transi- tioning model with observational constraints, Chin J Phys, 80, 261–274(2022)

Reference 35

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raw_fallback, observed 2026-08-16T12:36:11.540106Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-16T12:36:11.178450Z digest=sha256:7db80f41908780ad68e67acfa84f9c2fabda385a937a044c159d26f48e37cfab

Observation c3a5d312-cdb9-4612-a103-01827abe0997 · outbound

This paper cites A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - I : Methods and Application to the Sloan Digital Sky Survey.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - I : Methods and Application to the Sloan Digital Sky Survey

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-16T12:36:11.181351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:36:11.181351Z digest=sha256:9efbb5f3ef5f200270d8267ae9162493deb458f79445c4888dbe858f27c61a19

Observation ceaa5476-eb4c-4969-9436-60c62166a82e · outbound

This paper cites The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-16T12:36:11.184946Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:36:11.184946Z digest=sha256:14c4e3f053a7aa368ed7488f9ef9d44ef03335b70d8c272c2ac80e2bbbb9e880

Observation 364c9389-dc98-4a23-ba3c-cd105cf79510 · outbound

This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-16T12:36:11.188213Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:36:11.188213Z digest=sha256:58732f2a6956099e2d2fd97635ddb880fa4f30d7239bf6b004ba34948bc39a96

Observation 2dbba94f-6b16-4d85-85bf-7f660eeff264 · outbound

This paper cites The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-16T12:36:11.191670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:36:11.191670Z digest=sha256:b8ac06f62a93714065cb9feaa02ef64f1c02793fb060206ba9b062494aeca101

Observation 6c70b25b-4dd4-441c-b5c7-9f5d1bce48fe · outbound

This paper cites The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-16T12:36:11.195189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:36:11.195189Z digest=sha256:be28bd9d00f9930251ef4305091fd86f1d7a301a61c75994619294f989a4c59a

Observation f8022912-a33d-47d9-8f2f-7841a898c2c1 · outbound

This paper cites Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-16T12:36:11.199337Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:36:11.199337Z digest=sha256:a38eb32a16c0f3448c1ef210059bbe4e571e5cbe5804c9e5070197d4a703bd38

Observation 8569b71c-8275-4a8f-9ec9-709a2357b5fc · outbound

This paper cites Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-16T12:36:11.203052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:36:11.203052Z digest=sha256:7c98901a8c855e4e0b1de35c86107412fcf4c152ef982ff06e86f2dd4a6629aa

Observation 17402e3e-0068-471d-a219-79be0e98b164 · outbound

This paper cites Progress in Direct Measurements of the Hubble Constant.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Progress in Direct Measurements of the Hubble Constant

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-16T12:36:11.206562Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:36:11.206562Z digest=sha256:75a95d13e70ae904dd7ee97cdfea6c828f31e78f00af5a4a738129a78c1e406d

Observation 0a5f2e35-1212-44a8-939d-d7e1363d0e27 · outbound

This paper cites Mann, One Number Shows Something Is Fundamentally Wrong with Our Conception of the Universe – This fight has universal implications”, Live Science, Retrieved 26 August 2019.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Mann, One Number Shows Something Is Fundamentally Wrong with Our Conception of the Universe – This fight has universal implications”, Live Science, Retrieved 26 August 2019

Reference 44

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T12:36:11.528494Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-16T12:36:11.210024Z digest=sha256:854da23aed3393e232d5abddd0c4e0d8d58b547191c0d0776897049d152459cc

Observation 6be65eb8-9a76-42e9-8aeb-4fe8b7a4d67c · outbound

This paper cites In the Realm of the Hubble tension $-$ a Review of Solutions.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-16T12:36:11.213567Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:36:11.213567Z digest=sha256:65857fb2e72c3ffb12d77c99806cebe0b1bffa5aad308976acdc620aa73a74b0

Observation cc850a0d-7ddf-4431-aa27-ee0e60ad6296 · outbound

This paper cites Brout, D.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Brout, D

Reference 46

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T12:36:11.517905Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-16T12:36:11.217038Z digest=sha256:cd356047aa0534fb8245ea825aab2d2152ecc717bc6090f3c8656ce47b8df869

Observation bbc35b14-9294-450f-b29d-a74037bc78ca · outbound

This paper cites de Jaeger, L.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ de Jaeger, L

Reference 47

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T12:36:11.508243Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-16T12:36:11.220510Z digest=sha256:a66200c2645e6bc5cf6fae01c3b24c7e35c1640b74208faa4cb3e4993712327a

Observation 1742f1e0-ddc9-40ef-96dd-0b78e42da231 · outbound

This paper cites an unresolved cited work.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Unresolved cited work

Reference 48

Resolution
unresolved
raw_fallback, observed 2026-08-16T12:36:11.499245Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-16T12:36:11.223521Z digest=sha256:b734fc4d8ffd61ad2bcc9675626986abbd5d2d6b398484343c85e7d62df44143

Observation 39ae8320-e338-40fe-8853-058524f83d3a · outbound

This paper cites Contarini, A.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Contarini, A

Reference 49

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T12:36:11.489011Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-16T12:36:11.227201Z digest=sha256:e502bb7e3a1fafb78a65fbfc93c14e9dc27a0a7e640b2f422ae690a90462e3df

Observation 2413829f-eebb-45b8-8db4-9632783af432 · outbound

This paper cites Sneppen, D.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Sneppen, D

Reference 50

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T12:36:11.479203Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-16T12:36:11.230492Z digest=sha256:3a16b428ae175cbe96ddd46e7f7a39f1bab9f4cf2ea78f10e5d948559811be7b

Observation f64c8cf7-9e10-43f8-94de-830335aa4aab · outbound

This paper cites Balkenhol, D.

An Accelerating Flat FLRW Model with Observation Constraints and Dynamic $\Lambda$ Balkenhol, D

Reference 51

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T12:36:11.469163Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-16T12:36:11.233935Z digest=sha256:51e7c29c546e10dcf633d7d4aefdbae983f018e0e469a41ac7e367ea0cbf4ba4

Pith citing papers

No inbound Pith citation observations are available.