Pith. sign in

Paper Citation Record · LEDGER

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach

As of 11 August 2026, this Paper Citation Record lists 85 of 85 outbound references and 0 inbound Pith citation observations for arXiv:2412.20209.

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

pith.paper-citation-record.v1
2412.20209 v2

Coverage vector

measured 85 of 85 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-10T23:40:11.793648Z

measured 85 of 85 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

85 of 85 outbound references displayed

  • verified exact14
  • verified fuzzy0
  • unresolved66
  • parse uncertain0
  • malformed identifier5
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 5ce7606d-870b-4e7b-9f52-d5a1c12720fa · outbound

This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.434664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.434664Z digest=sha256:665fe03a331be0e3983f9656898e3ae2ec43f4a91ced6018c550221a82f8ddbf

Observation 93ec5761-4a7d-4a08-b655-6244a423bd60 · outbound

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

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Measurements of Omega and Lambda from 42 High-Redshift Supernovae

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.439589Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.439589Z digest=sha256:d9490474b7aef954da1bb4d0282e6a1913b4d5e204a5d3e489e4c20863c10103

Observation 1479d225-2ffb-45bf-ac8c-d1d8d7d2b2c2 · outbound

This paper cites First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters

Reference 3

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.443732Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.443732Z digest=sha256:23ee73a764fb8d89ed94b7b02a53462dc25900ef90f25ed5304b9c69c9c34e51

Observation f7d5c39d-6315-4e0f-b19a-727eca3443d0 · outbound

This paper cites Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results

Reference 4

Resolution
malformed identifier
no resolver link, observed 2026-08-10T23:40:11.448607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.448607Z digest=sha256:2ec5baf4618bd628d3da4fdf9438ea2c7bb8e8dfbfacf8f362e234a53888b3dd

Observation a46f2555-17d0-4436-bb0f-4d7b11db5701 · outbound

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

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.453232Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.453232Z digest=sha256:0261524e7b2df2f1bb274233d7027d799eff3cbbdb7f88d5f1f0c191915c2fe7

Observation 0adf8abe-d54b-46a3-b350-28cb655fc8ae · outbound

This paper cites Sofue and V.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Sofue and V

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.457881Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.457881Z digest=sha256:9016aa1c790eea067687fb031f918e4eac1c2a640a8a830692cc6cfcb526a467

Observation 4c348f9d-ce0e-4dbd-8bfd-0f492e344832 · outbound

This paper cites Bartelmann and P.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Bartelmann and P

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.462794Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.462794Z digest=sha256:ac9499c51424412e8579c70b47082641289c1149b88cb4848c4b61a03fd7d8e3

Observation ab5957b1-d465-446c-ae57-7457892db97d · outbound

This paper cites Clowe, A.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Clowe, A

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.466703Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.466703Z digest=sha256:063755c4717bc9fb1e31e35dadfdc47265d486c8b9f9c3d45180b0ca3cc38486

Observation 98b656f1-f814-49d3-bbcf-74b9f809d85c · outbound

This paper cites Planck 2013 results. XVI. Cosmological parameters.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Planck 2013 results. XVI. Cosmological parameters

Reference 9

Resolution
malformed identifier
no resolver link, observed 2026-08-10T23:40:11.471053Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.471053Z digest=sha256:976f1f1cfa1ba45f24fdc4bf2d93ddade1abdef78ab72f6e967ae1b65103f72e

Observation 456cf0cd-3ec3-4a27-ac96-43f41d1cebee · outbound

This paper cites Quintessence, Cosmic Coincidence, and the Cosmological Constant.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Quintessence, Cosmic Coincidence, and the Cosmological Constant

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.475460Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.475460Z digest=sha256:f6f4c34e7c5659855bdd6f21b17cb3a735fc4a49750bbe073ccb8b0d38fedf37

Observation 3d70f2b4-910a-4098-b088-2d6d1f0e5064 · outbound

This paper cites Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask).

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.479674Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.479674Z digest=sha256:41cfb474da8d5e96a0230f5e31ce667bdb030b5221bffe19dc7f657e35aedd7a

Observation 6f431494-aed7-4493-b593-584598634406 · outbound

This paper cites an unresolved cited work.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Unresolved cited work

Reference 12

Resolution
malformed identifier
no resolver link, observed 2026-08-10T23:40:11.485094Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.485094Z digest=sha256:b2f84250064625603a731e24e191ddfda4e74f2e81ab3a11c5a9400b9b235363

Observation 64f5cfbf-4fbe-412d-9d9e-c2ecc2d8910b · outbound

This paper cites an unresolved cited work.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Unresolved cited work

Reference 13

Resolution
verified exact
doi, observed 2026-08-10T23:40:11.857167Z

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.

source=pdf_text observed=2026-08-10T23:40:11.489250Z digest=sha256:3d36e4fbd98abc028e31c15837c08c78769e92536ec68d5b5c4b283f1fadfe3f

Observation 480c116b-877e-40c8-a02f-1adae5823087 · outbound

This paper cites The Cosmological Constant and Dark Energy.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach The Cosmological Constant and Dark Energy

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.493803Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.493803Z digest=sha256:0c995f0234f70e8ef6f080b8e2f533b119c26bf1901f0defa6470b16bf8bac3e

Observation f347ab5f-7321-4595-afdd-4eb8555f6192 · outbound

This paper cites Nishioka and Y.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Nishioka and Y

Reference 15

Resolution
verified exact
doi, observed 2026-08-10T23:40:11.844212Z

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.

source=pdf_text observed=2026-08-10T23:40:11.498139Z digest=sha256:800704ca669828d193f52694f7b6fd57d6290e5d426131778ee138cc071d224d

Observation a9f8a83d-0699-443a-a293-600825a6426b · outbound

This paper cites Structure formation with a self-tuning scalar field.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Structure formation with a self-tuning scalar field

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.502188Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.502188Z digest=sha256:87cbe173e4f9e67dcece1d324394ca1259dc75b09606a0dae7f2bceab52c86a1

Observation 0f0c550a-cb8e-4688-82b3-ba2e44db2e97 · outbound

This paper cites Cosmology with a Primordial Scaling Field.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Cosmology with a Primordial Scaling Field

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.506406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.506406Z digest=sha256:1fd20691acb847a3a87a3eac1c0220781f5cf36c0b901b64bf274cda17996a5f

Observation b14b4eba-cd3f-440e-b015-98b84042b2fb · outbound

This paper cites Cosmological Imprint of an Energy Component with General Equation of State.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Cosmological Imprint of an Energy Component with General Equation of State

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.510532Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.510532Z digest=sha256:92dd110b120af0cdeb2f886d93288f65eba473effc6739d44de92125a9d4cf0e

Observation 220c4f57-a69d-47c4-95ae-2b3c37986343 · outbound

This paper cites Quintessence and the Rest of the World.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Quintessence and the Rest of the World

Reference 19

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.514778Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.514778Z digest=sha256:027d294477988367bd67c1448ce2f4b16f518289d7278a92dacaad5129457c43

Observation 516e4896-a163-413b-9fea-df01cc00588d · outbound

This paper cites Exponential potentials and cosmological scaling solutions.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Exponential potentials and cosmological scaling solutions

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.518975Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.518975Z digest=sha256:4c1b85f5e2a63d63315e4eccfb4a3a7f81e2c7166a0153ef9c653b3975c788d8

Observation 3f4e693d-cd06-4c20-9f4d-a73958f37049 · outbound

This paper cites Full Investigation on the Dynamics of Power-Law Kinetic Quintessence.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Full Investigation on the Dynamics of Power-Law Kinetic Quintessence

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.523376Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.523376Z digest=sha256:45678fe7ffc656391a61c2b410b01d42aa92ba37cfcf2de6938622074e9f8d0d

Observation bae6baa1-37f9-4d30-b877-6ec0defd8472 · outbound

This paper cites k-Inflation.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach k-Inflation

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.527553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.527553Z digest=sha256:81f0c6e6d7c3ae5210e6a74a716e43b03260eda437c940fcd53904c9c41504f5

Observation 6a2cb563-151f-4589-af2e-ce040f3714cf · outbound

This paper cites Essentials of k-essence.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Essentials of k-essence

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.531717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.531717Z digest=sha256:50bb5f72ee7954bcf116bf4b98c6a0fa961ec992f333ab5871ef42220047d1f7

Observation f67429b8-40b3-48d5-80b3-8db033196184 · outbound

This paper cites A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.535614Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.535614Z digest=sha256:545d6d6a2e5a1e599bfc2344494fa6aaf2a8b126c8534a03bc20ab38e2ac1afe

Observation 30d2637f-cf6f-44a3-9168-3f4ebef01946 · outbound

This paper cites Haloes of k-Essence.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Haloes of k-Essence

Reference 25

Resolution
malformed identifier
no resolver link, observed 2026-08-10T23:40:11.540183Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.540183Z digest=sha256:66a76ac7bea32a3c8c668708f2e53a15fc9b6fb15b611c43879304cea4f0b9f6

Observation e32ecba9-6751-4e3e-b86d-788b373392d4 · outbound

This paper cites Kinetically Driven Quintessence.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Kinetically Driven Quintessence

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.544143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.544143Z digest=sha256:d23b9b4787eb6aff87e567da86c874901e58b0ca8a85b17b3ad3fc8ba34b9eb0

Observation 20adfea5-2ad4-4aff-9afa-66c09814e5f8 · outbound

This paper cites Ghost Condensation and a Consistent Infrared Modification of Gravity.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Ghost Condensation and a Consistent Infrared Modification of Gravity

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.548330Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.548330Z digest=sha256:30021a412d08c437535029ef26daaafe2a6b360940bf57136a7b36a4605a5043

Observation f7c802a6-327e-4433-a0c5-d8a5a2af13d4 · outbound

This paper cites A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.553226Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.553226Z digest=sha256:0b98098d8c65c4accb7490c27bf0c5a7951671507f6481e765e6d62578bee9ba

Observation 9b191a43-b551-43eb-8a5c-fcea3ec38ad5 · outbound

This paper cites Realising Interactions Between Dark Matter and Dark Energy Using $k$-essence Cosmology.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Realising Interactions Between Dark Matter and Dark Energy Using $k$-essence Cosmology

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.557678Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.557678Z digest=sha256:9679a15968effc24cbe7667707ec4b35b3a93bc278584d2458c63021fa8063f0

Observation b14022f1-5281-4b9c-82dc-dab508c6ab15 · outbound

This paper cites Diffusive dark matter and dark energy scenario and $k-$essence in the context of Supernova Ia observations.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Diffusive dark matter and dark energy scenario and $k-$essence in the context of Supernova Ia observations

Reference 30

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:12.556421Z

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.

source=pdf_text observed=2026-08-10T23:40:11.561846Z digest=sha256:7ddf27cfd13fa5b142c94868ff70c65417cce2b12b7be19cc62dd51a5a5918f6

Observation 7b928158-3e44-4b36-a98f-973acef1cd04 · outbound

This paper cites Implications of JLA data for $k-$essence model of dark energy with given equation of state.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Implications of JLA data for $k-$essence model of dark energy with given equation of state

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.566450Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.566450Z digest=sha256:764c3fa4520b79e0aecf0b8ffca816f233737a4ef22f2d05af9c1ec5c3e7ec07

Observation 04cba874-0ec5-47be-a345-17b169ed3dbd · outbound

This paper cites Time-dependent diffusive interactions between dark matter and dark energy in the context of $k-$essence cosmology.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Time-dependent diffusive interactions between dark matter and dark energy in the context of $k-$essence cosmology

Reference 32

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:12.526803Z

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.

source=pdf_text observed=2026-08-10T23:40:11.570204Z digest=sha256:7ea1f497cab765eab0015d9ddaf88d6d8e625cddbf04827591c55ef1d277763f

Observation 3e4a2603-7295-4581-8939-74e1991cff45 · outbound

This paper cites Modified scaling in $k$-essence model in interacting dark energy - dark matter scenario.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Modified scaling in $k$-essence model in interacting dark energy - dark matter scenario

Reference 33

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:12.508768Z

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.

source=pdf_text observed=2026-08-10T23:40:11.574008Z digest=sha256:b0f4611ba6971340ef06a5981f72900323bcf87dcf7353e68b5d50d2644c19ea

Observation 985bad89-6410-4bb7-8c18-c048076d4cd8 · outbound

This paper cites Curvature Quintessence.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Curvature Quintessence

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.577849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.577849Z digest=sha256:d404288de2c3d07341ccd1b2b14ce1e4999e0b7e028a74c8e5d9c32fe91c02b2

Observation d626237f-1007-4fda-abe3-bc9e0fb7ed47 · outbound

This paper cites Curvature quintessence matched with observational data.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Curvature quintessence matched with observational data

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.582133Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.582133Z digest=sha256:fb961a982f5f3a2282b810bc520e621d83e131637396ab7afa6f361f539371d8

Observation d4dc0110-e49c-45c8-828f-47320e75635d · outbound

This paper cites Modified gravity with negative and positive powers of the curvature: unification of the inflation and of the cosmic acceleration.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Modified gravity with negative and positive powers of the curvature: unification of the inflation and of the cosmic acceleration

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.586199Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.586199Z digest=sha256:f37bb653ebc088e561a172040f664b910e71c56a3258df9b858fad01eefa1832

Observation 8392d3ea-87dc-4639-bd0a-e5e66f482168 · outbound

This paper cites Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.589924Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.589924Z digest=sha256:03485362f2a1fe03ef354f992711858f33bb73438a98e59a475bed3ab64e4aba

Observation 80f737d0-731a-4038-a9ee-cee328ec6b6a · outbound

This paper cites Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.593644Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.593644Z digest=sha256:8f46a5b85d891c187dbbb703af80897ed49a9eb3771a6d7cba948015643273f2

Observation 01f3ee8d-5d37-43d9-abbd-64a2a208f430 · outbound

This paper cites Observational constraints on non-minimally coupled curvature-matter models of gravity from the analysis of Pantheon data.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Observational constraints on non-minimally coupled curvature-matter models of gravity from the analysis of Pantheon data

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.597366Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.597366Z digest=sha256:7ba2c54ec501b9b4c5184255ad9044dcf8bd1825ff352297f0e38072e9b5d1f7

Observation 573d05d1-c7a9-4ac1-a132-c4b273f2b7d1 · outbound

This paper cites Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Investigating the accelerated expansion of the Universe through updated constraints on viable $f(R)$ models within the metric formalism

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.600894Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.600894Z digest=sha256:5af3ef4562912f1db30c5356b5930e8fd2a72907ed07076489f957f4c32190b3

Observation e00d89c0-de28-474c-9bc9-2101400a110b · outbound

This paper cites Observational constraints on generic models of non-minimal curvature-matter coupling.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Observational constraints on generic models of non-minimal curvature-matter coupling

Reference 41

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:12.414246Z

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.

source=pdf_text observed=2026-08-10T23:40:11.604793Z digest=sha256:02d3f65674f0f4b25afb79f500dce9cd76f2f6ec3302de066ef4e426423a94be

Observation d4f16cd0-137c-4543-bcf3-0a7a1fc4f52f · outbound

This paper cites Extra force in $f(R)$ modified theories of gravity.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Extra force in $f(R)$ modified theories of gravity

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.608987Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.608987Z digest=sha256:664ec877eec591d2f5557cc62019b4736e320a6ae5fe881feb150816f2cd2d05

Observation 8d0de1f4-cfc0-420a-9540-969b1b145fc8 · outbound

This paper cites Is cosmological data suggesting a nonminimal coupling between matter and gravity?.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Is cosmological data suggesting a nonminimal coupling between matter and gravity?

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.613049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.613049Z digest=sha256:af16e73fbf0b7a472630991eaf3754aa3ef054f6ee4688276ab794307a9ce49b

Observation 5c43eece-65e7-4b24-a6d8-4b24ad716d54 · outbound

This paper cites Exploring the evolution of structure growth in the universe with field-fluid interactions through dynamical stability analysis.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Exploring the evolution of structure growth in the universe with field-fluid interactions through dynamical stability analysis

Reference 44

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:12.374077Z

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.

source=pdf_text observed=2026-08-10T23:40:11.617504Z digest=sha256:cf497f780b48d6ef7dd32d25f830f0400be96fbc37de136ff25057ea2c9d2e6f

Observation 9f2de8a7-ecbc-4bdb-b088-783fefb8c623 · outbound

This paper cites Dynamical stability of K-essence field interacting non-minimally with a perfect fluid.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical stability of K-essence field interacting non-minimally with a perfect fluid

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.622100Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.622100Z digest=sha256:14afaf5ddc211597ae60e04d11d6c8ed19a3bdc6109a2e52703c2b72022a48a3

Observation 99f5bc08-d33b-4a31-b752-df77fde8d5b9 · outbound

This paper cites Dynamical analysis of $k$-essence cosmology in the light of Supernova Ia observations.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical analysis of $k$-essence cosmology in the light of Supernova Ia observations

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.626501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.626501Z digest=sha256:53138683a95d46b3a8f90610cf16ca44a96dfec1bd122a1778a926ecaf9c49ad

Observation dcd58238-2ba5-4e58-8f5a-2e0a53272519 · outbound

This paper cites Ghost condensates and pure kinetic $k$-essence condensates in presence of field-fluid non-minimal coupling in the dark sector.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Ghost condensates and pure kinetic $k$-essence condensates in presence of field-fluid non-minimal coupling in the dark sector

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.631220Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.631220Z digest=sha256:8746f9330e20cfa31527cd6522d2f240912e0876cd361a2e9bf05a6a53ea4677

Observation 38b3a3d7-4110-4519-a0bb-c51d1f2945e6 · outbound

This paper cites Dynamical Stability in presence of non-minimal derivative dependent coupling of $k$-essence field with a relativistic fluid.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical Stability in presence of non-minimal derivative dependent coupling of $k$-essence field with a relativistic fluid

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.635862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.635862Z digest=sha256:0abc118011e225c657d29bfb8d1f5fd00635a83ed60e65adf74aeb69bdda93bf

Observation 9425c3f0-8ad2-4163-8350-2ff06b32855f · outbound

This paper cites Dynamical stability in models where dark matter and dark energy are non-minimally coupled to curvature.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical stability in models where dark matter and dark energy are non-minimally coupled to curvature

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.640479Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.640479Z digest=sha256:3c160be48a77f1ac2bf48b615678bf7094d04d7972adea27abde74e532a27db0

Observation f13e8c9f-8d06-4b53-82c1-83deaff6ceab · outbound

This paper cites f(R) theories.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach f(R) theories

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.645046Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.645046Z digest=sha256:013cf1652f49c9c963baaed0c2cf3bd48cfe8b2fddcd067e4b31803eff29024e

Observation 8c113121-ca89-4544-9e6b-3449ddbb3dbc · outbound

This paper cites f(R) Theories Of Gravity.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach f(R) Theories Of Gravity

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.649412Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.649412Z digest=sha256:9bfd214eadb9392051e2beaf12cdf2bfd4cdc34267b48282fe166984c76e6fe2

Observation 7ea4e7ca-cc5c-442e-a3ce-e753ddbbe990 · outbound

This paper cites Conditions for the cosmological viability of f(R) dark energy models.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Conditions for the cosmological viability of f(R) dark energy models

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.653917Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.653917Z digest=sha256:27738a7db0a0e8e3b0946bca8761040cb3ffcc3b96334ab75afac6a1bbf7f500

Observation d9a1db7f-84f1-4aa7-bd40-32592f1c3296 · outbound

This paper cites Energy Conditions and Stability in $f(R)$ theories of gravity with non-minimal coupling to matter.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Energy Conditions and Stability in $f(R)$ theories of gravity with non-minimal coupling to matter

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.658981Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.658981Z digest=sha256:279b25c325fea645d03e3d50ac06d9d34cdc602cfb413f1956b5f25c6a82a87d

Observation 657712a3-7c3e-4612-8806-a5583da83a02 · outbound

This paper cites Gunzig, V.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Gunzig, V

Reference 54

Resolution
verified exact
doi, observed 2026-08-10T23:40:11.830440Z

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.

source=pdf_text observed=2026-08-10T23:40:11.663499Z digest=sha256:b03b63349655b36194c20b986d2ce007b13c497fbc03c26653944126a20a061e

Observation 12396643-cc1d-4695-8c3d-94d87d59d46e · outbound

This paper cites Autonomous Dynamical System Approach for $f(R)$ Gravity.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Autonomous Dynamical System Approach for $f(R)$ Gravity

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.668558Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.668558Z digest=sha256:c4cf0ad8175d75c01bb03f0072b515f5633bd5ebcacb5818158dee12a2b875b3

Observation 4a5dc3b9-1f41-4e45-9a15-a3912c379be5 · outbound

This paper cites Cosmology in symmetric teleparallel gravity and its dynamical system.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Cosmology in symmetric teleparallel gravity and its dynamical system

Reference 56

Resolution
malformed identifier
no resolver link, observed 2026-08-10T23:40:11.672815Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.672815Z digest=sha256:27d8bde259357c16d4f66e9aa74c47fd0fbb9c2acd619f91852336f24df0b47d

Observation 6f89e90d-dcc0-4e42-9aa5-467995222a75 · outbound

This paper cites Dynamical Systems Perspective of Cosmological Finite-time Singularities in $f(R)$ Gravity and Interacting Multifluid Cosmology.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical Systems Perspective of Cosmological Finite-time Singularities in $f(R)$ Gravity and Interacting Multifluid Cosmology

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.676872Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.676872Z digest=sha256:6d42c965712290bcd9c997cf71a1422202fc1ac7e1415aa7e47682a7d6ae5029

Observation 911739e6-a37b-4676-be73-0dc38b17e8c9 · outbound

This paper cites Dynamical systems applied to cosmology: dark energy and modified gravity.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical systems applied to cosmology: dark energy and modified gravity

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.680835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.680835Z digest=sha256:eb3eb7f64c70a9b5c258dc28a8e67d7c126082bd75c867ffd5785f496442444a

Observation 2a7184c3-e1ad-4cb1-9134-f195ee6df696 · outbound

This paper cites Dynamical system analysis of generalized energy-momentum-squared gravity.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical system analysis of generalized energy-momentum-squared gravity

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.684956Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.684956Z digest=sha256:0721c9fedb6c6c903ebca5598ee656ffa097bcb7a7e93ab4ebfb65b2883b93ef

Observation 9c665672-ac90-4f45-aa27-3a8038827195 · outbound

This paper cites Dynamical analysis of generalized Galileon cosmology.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical analysis of generalized Galileon cosmology

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.688790Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.688790Z digest=sha256:d14ebb9697b1170a2f376b898ffd15eb93d93a3c2b32a0bb6fbd00a09a50b1a6

Observation f96aa9a4-7966-4abb-808e-ac53c6ad715a · outbound

This paper cites Phase-Space analysis of Teleparallel Dark Energy.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Phase-Space analysis of Teleparallel Dark Energy

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.692585Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.692585Z digest=sha256:bace4efe129e0cfef738202ca88cc0b63520277e1574c1c28bd2f095760ed70c

Observation 96dccbbb-e041-4f22-af9e-b51b0bdac722 · outbound

This paper cites Phantom dark energy with varying-mass dark matter particles: acceleration and cosmic coincidence problem.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Phantom dark energy with varying-mass dark matter particles: acceleration and cosmic coincidence problem

Reference 62

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:12.165847Z

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.

source=pdf_text observed=2026-08-10T23:40:11.696721Z digest=sha256:2eb9b464ac32b266a421c707651a7a1d8c8cbf883c27321717e2052af12ac22e

Observation 939c4ff8-ffbb-4da6-9452-724fd279921a · outbound

This paper cites Phase-space analysis of Horava-Lifshitz cosmology.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Phase-space analysis of Horava-Lifshitz cosmology

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.701212Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.701212Z digest=sha256:d667f4aa87032e0b6fdda7396990857a2f13949dfbe329752a59818594b83d0f

Observation 05bc5c51-65d1-488e-b163-6d65f6eaf14e · outbound

This paper cites Dynamical behavior in $f(T,T_G)$ cosmology.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical behavior in $f(T,T_G)$ cosmology

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.705174Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.705174Z digest=sha256:b31a74eee1d3d1dc1854b87abe44dfc2e36e8f42c2783485be25083e7d708000

Observation 86ce931d-8396-46ca-8076-cc2f6966d29f · outbound

This paper cites Dynamical system analysis at background and perturbation levels: Quintessence in severe disadvantage comparing to $\Lambda$CDM.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical system analysis at background and perturbation levels: Quintessence in severe disadvantage comparing to $\Lambda$CDM

Reference 65

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:12.127989Z

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.

source=pdf_text observed=2026-08-10T23:40:11.709124Z digest=sha256:11cd33bc624f3394f2621a30fe49a0d4e7370c4b2534f28a5fd283712b81ae34

Observation d41f7ca3-8a22-4edc-b002-0d32bd04cda7 · outbound

This paper cites Cosmological dynamics of interacting dark energy and dark matter in viable models of f(R) gravity.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Cosmological dynamics of interacting dark energy and dark matter in viable models of f(R) gravity

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.713193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.713193Z digest=sha256:ef46b7918dd7f2ffdb6fd40551111bb0d1342030f43e8d63f9e6ad1d833ada21

Observation 134928d8-0375-48dd-a5d5-6e9dab7b05f7 · outbound

This paper cites Dynamical analysis of modified gravity with nonminimal gravitational coupling to matter.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical analysis of modified gravity with nonminimal gravitational coupling to matter

Reference 67

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:12.098399Z

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.

source=pdf_text observed=2026-08-10T23:40:11.717042Z digest=sha256:30e669798fa58d61cba1253108724f03cc13efdfe243b900e1050f1c594bc7a0

Observation 544b7354-b723-43c7-bbff-05b61ed80ba6 · outbound

This paper cites Are f(R) dark energy models cosmologically viable ?.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Are f(R) dark energy models cosmologically viable ?

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.722121Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.722121Z digest=sha256:1512ad815c3ab7b6a823492ac994c8d9ce17fb1a5274263ded8dae5e453751a5

Observation 8942e200-7b54-4a05-95d5-6949c64cd010 · outbound

This paper cites Power-laws f(R) theories are cosmologically unacceptable.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Power-laws f(R) theories are cosmologically unacceptable

Reference 69

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:12.071012Z

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.

source=pdf_text observed=2026-08-10T23:40:11.726417Z digest=sha256:ad048ebb10c580609b025bb5aa1c5390bd28e47f8c25d6a12c491d58240cdb91

Observation 0ee57154-2099-4915-905d-70bf3aee431e · outbound

This paper cites Phantom crossing, equation-of-state singularities, and local gravity constraints in f(R) models.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Phantom crossing, equation-of-state singularities, and local gravity constraints in f(R) models

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.730528Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.730528Z digest=sha256:675f7e857e17d4c2399a5b18e1f9e418fafa61b505dba01c15a94a0d39ef51f5

Observation 043f45f4-7844-4afc-b69c-005a5703778f · outbound

This paper cites Dynamical analysis of coupled curvature-matter scenario in viable $f(R)$ dark energy models at de Sitter phase.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dynamical analysis of coupled curvature-matter scenario in viable $f(R)$ dark energy models at de Sitter phase

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.734758Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.734758Z digest=sha256:4331f5bb31fa595ddcc5e35752e8566ff948d0a8b19cd55b47015629b1c35ec5

Observation 7d89a2b4-24ae-4470-889c-0ce3aa03f03a · outbound

This paper cites f(R) gravity: successes and challenges.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach f(R) gravity: successes and challenges

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.738719Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.738719Z digest=sha256:48eb4045d91359c3dbd425a84e62fb6d1709526f12b3de44e67cdae561a71510

Observation 47228393-b5a1-444e-b626-5b75c8310c92 · outbound

This paper cites Dark energy: investigation and modeling.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Dark energy: investigation and modeling

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.742901Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.742901Z digest=sha256:bf6eeacacb6a8a3b36eae16c69f857ad45f2483a5d6f9156f2583673e8addb61

Observation 795f2362-4b7c-4bf3-bd7e-7e914fd22b06 · outbound

This paper cites The Cosmology of f(R) Gravity in the Metric Variational Approach.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach The Cosmology of f(R) Gravity in the Metric Variational Approach

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.746904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.746904Z digest=sha256:96d9eac578a37e67ada72d878f065e8db2011465facce9f8c873494fded9fce7

Observation 32b0eef3-abbc-40cc-81dc-85b05887fed8 · outbound

This paper cites Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.750912Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.750912Z digest=sha256:85ca2a4b26fbedf01997f733ab4885715182092c159591b86f9e3fa7d2673366

Observation 92186414-ca70-44c6-86a0-e05b87ae9d28 · outbound

This paper cites f(R) Gravity and Chameleon Theories.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach f(R) Gravity and Chameleon Theories

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.755254Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.755254Z digest=sha256:8c6603340db5904d54f074ff347003f1329d0ae63a5882dca4abfa176d8a9b51

Observation 604701aa-6088-4d47-b9e6-aab5628a9e16 · outbound

This paper cites Disappearing cosmological constant in f(R) gravity.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Disappearing cosmological constant in f(R) gravity

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.759504Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.759504Z digest=sha256:4139fa348297294bf17065c6f9fe0332df7be047987583ebb5254e67150f8edc

Observation 82baa176-341f-4877-afcf-506b7519beac · outbound

This paper cites Cosmological Constraints from Hubble Parameter on f(R) Cosmologies.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Cosmological Constraints from Hubble Parameter on f(R) Cosmologies

Reference 78

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:11.970897Z

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.

source=pdf_text observed=2026-08-10T23:40:11.763446Z digest=sha256:dc9672a4fc41c1025e48daf2f1909cd4b52c1289b9d6aeb8c66e18e3cc948d14

Observation 58e7b36d-4e32-4156-88b3-98dbcaaa0a3f · outbound

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

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Planck 2018 results. VI. Cosmological parameters

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.767580Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.767580Z digest=sha256:fce040373f1ad68316654fa53bc239a18961143dba2a4f51b2dacc84506a7b9c

Observation c438d5de-ea95-4ff1-a8ca-db056d9056cf · outbound

This paper cites Transition redshift in $f(T)$ cosmology and observational constraints.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Transition redshift in $f(T)$ cosmology and observational constraints

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.771744Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.771744Z digest=sha256:7af34135b91f98588f8a5548a36f570ef84f0bc543c17d65153e904adc204b47

Observation 0cea635a-92f7-4007-8a48-9de57f70f387 · outbound

This paper cites Cosmology Based on f(R) Gravity Admits 1 eV Sterile Neutrinos.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Cosmology Based on f(R) Gravity Admits 1 eV Sterile Neutrinos

Reference 81

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:40:11.930846Z

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.

source=pdf_text observed=2026-08-10T23:40:11.776022Z digest=sha256:386b6dab4edb70b665fce51097bbbbd9e39d927a7693fd158096cef5a65aef57

Observation fa19f89e-f623-4475-9b4a-5fbb9a50328d · outbound

This paper cites Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.780231Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.780231Z digest=sha256:591069ec431da9ae9583b02f09a1a45c0a25cd2c0121b03866ef9ae357f5f2e0

Observation 28531bc8-e6d0-4fb8-adf6-d316cd97db79 · outbound

This paper cites Unifying inflation with LambdaCDM epoch in modified f(R) gravity consistent with Solar System tests.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Unifying inflation with LambdaCDM epoch in modified f(R) gravity consistent with Solar System tests

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.785097Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.785097Z digest=sha256:6d734b2b18656bfd4b77b0f3301a1552367875624a95f0e4fac9e8863a2960f3

Observation f820db80-e814-4efe-8930-34a85270df4c · outbound

This paper cites Solar System constraints to general f(R) gravity.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Solar System constraints to general f(R) gravity

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.789385Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.789385Z digest=sha256:d8481ec5d283510532547dd318ac4491a8d282ea8fbaa34e40332f3ceb990f31

Observation ca0921ae-4995-42fb-a1b5-f0e215ddcce0 · outbound

This paper cites Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase.

Understanding curvature-matter interaction in viable $f(R)$ dark energy models: A dynamical analysis approach Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-10T23:40:11.793648Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:40:11.793648Z digest=sha256:0f6840605d30a15f23a0e9778f0d8e7d7cd4a2884d75214af5b09cfadceee52e

Pith citing papers

No inbound Pith citation observations are available.