Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model | Paper Citation Record

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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This paper cites For ξ1 to be a critical point, ϵ3 must be exactly 6 .4581.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model For ξ1 to be a critical point, ϵ3 must be exactly 6 .4581

Reference 15

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This paper cites For ξ3 to be a critical point, β must satisfy the condition β = 1.0074.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model For ξ3 to be a critical point, β must satisfy the condition β = 1.0074

Reference 16

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This paper cites For ξ6 to be a critical point, ϵ2 must be related to ϵ1 by ϵ2 = −0.924.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model For ξ6 to be a critical point, ϵ2 must be related to ϵ1 by ϵ2 = −0.924

Reference 17

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Observation bbd27be4-4f02-4070-8e00-b1aa9cd2e873 · outbound

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

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Measurements of Omega and Lambda from 42 High-Redshift Supernovae

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model The Cosmological Constant

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model The Cosmological Constant Problem

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Dynamics of Dark Energy

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Dark Energy and the Accelerating Universe

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This paper cites Cosmic Growth History and Expansion History.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Cosmic Growth History and Expansion History

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

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Five-Year Wilkinson Microwave Anisotropy Probe Observations: Data Processing, Sky Maps, and Basic Results

Reference 27

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This paper cites Energy Stored on a Cosmological Horizon and Its Thermodynamic Fluctuations in Holographic Equipartition Law.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Energy Stored on a Cosmological Horizon and Its Thermodynamic Fluctuations in Holographic Equipartition Law

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This paper cites Observational Signatures of f (R) DE Models That Satisfy Cosmological and Local Gravity Constraints.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Observational Signatures of f (R) DE Models That Satisfy Cosmological and Local Gravity Constraints

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This paper cites Cosmological Fluids in the Equivalence between Rastall and Einstein Gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Cosmological Fluids in the Equivalence between Rastall and Einstein Gravity

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Late-Time Cosmology in a Model of Modified Gravity with an Exponential Function of the Curvature

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This paper cites Accretion disk around Reissner-Nordstr\"{o}m black hole coupled with a nonlinear electrodynamics field.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Accretion disk around Reissner-Nordstr\"{o}m black hole coupled with a nonlinear electrodynamics field

Reference 32

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This paper cites Tunneling analysis of null aether black hole theory in the background of Newman-Janis algorithm.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Tunneling analysis of null aether black hole theory in the background of Newman-Janis algorithm

Reference 33

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This paper cites Strong Gravitational Lensing by Sgr A* and M87* Black Holes embedded in Dark Matter Halo exhibiting string cloud and quintessential field.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Strong Gravitational Lensing by Sgr A* and M87* Black Holes embedded in Dark Matter Halo exhibiting string cloud and quintessential field

Reference 34

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This paper cites Mustafa, Xia Tiecheng, and Farruh Atamurotov.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Mustafa, Xia Tiecheng, and Farruh Atamurotov

Reference 35

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Observation 7e89ba11-0d43-4f89-a76f-74ed8e2c3cba · outbound

This paper cites Models of f (R) Cosmic Acceleration That Evade Solar-System Tests.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Models of f (R) Cosmic Acceleration That Evade Solar-System Tests

Reference 36

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This paper cites Constraining study of charged gravastars solutions in symmetric teleparallel gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Constraining study of charged gravastars solutions in symmetric teleparallel gravity

Reference 37

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This paper cites Exploring Tidal Force Effects and Shadow Constraints for Schwarzschild-like Black Hole in Starobinsky-Bel-Robinson Gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Exploring Tidal Force Effects and Shadow Constraints for Schwarzschild-like Black Hole in Starobinsky-Bel-Robinson Gravity

Reference 38

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Observation fce96eb4-a6c7-4c34-90ea-78e2fb413eeb · outbound

This paper cites Ricci Inverse Gravity Wormholes.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Ricci Inverse Gravity Wormholes

Reference 39

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This paper cites Deflection of light by wormholes and its shadow due to dark matter within modified symmetric teleparallel gravity formalism.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Deflection of light by wormholes and its shadow due to dark matter within modified symmetric teleparallel gravity formalism

Reference 40

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This paper cites New embedded wormhole solutions in Ricci inverse gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model New embedded wormhole solutions in Ricci inverse gravity

Reference 41

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Observation 2eaeb26a-d9da-47ff-b6ab-ac0d0e692c10 · outbound

This paper cites Imprints of dark energy models on structural properties of charged gravastars in extended teleparallel gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Imprints of dark energy models on structural properties of charged gravastars in extended teleparallel gravity

Reference 42

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Observation 91e43572-84e9-4251-9f3b-755749286924 · outbound

This paper cites Matter accretion onto the magnetically charged Euler-Heisenberg black hole with scalar hair.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Matter accretion onto the magnetically charged Euler-Heisenberg black hole with scalar hair

Reference 43

Resolution: verified exact; local_arxiv, observed 2026-08-10T21:04:56.716044Z

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Observation e6a353d4-2384-47bf-b2dc-df8d953ae731 · outbound

This paper cites Thermal Analysis and Joule-Thomson Expansion of Black Hole Exhibiting Metric-Affine Gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Thermal Analysis and Joule-Thomson Expansion of Black Hole Exhibiting Metric-Affine Gravity

Reference 44

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Observation 871a2a73-7e92-4395-9a53-44b8085e1cc9 · outbound

This paper cites Unified Cosmic History in Modified Gravity: From f (R) Theory to Lorentz Non-Invariant Models.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unified Cosmic History in Modified Gravity: From f (R) Theory to Lorentz Non-Invariant Models

Reference 45

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

Reference 46

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Observation db5125b7-1f6d-40e7-9326-df6b9290a065 · outbound

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

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-Time Evolution

Reference 47

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Observation cc766b2f-0f1e-481b-804f-db84a321adfb · outbound

This paper cites f (R) Theories.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model f (R) Theories

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:04:59.080608Z

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Observation 8529faec-04ee-4498-bd85-9deff1282641 · outbound

This paper cites f (R) and f(T) Theories of Modified Gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model f (R) and f(T) Theories of Modified Gravity

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Resolution: verified exact; doi, observed 2026-08-10T21:04:55.839813Z

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Observation 85699bf6-b938-4d72-a5f1-332eb0506b6d · outbound

This paper cites Exact Solutions for Bianchi Type-I Cosmological Models in f (R) Theory of Gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Exact Solutions for Bianchi Type-I Cosmological Models in f (R) Theory of Gravity

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:04:59.030193Z

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Observation b498c691-1e73-441f-8369-286e5924e94d · outbound

This paper cites Exact Solutions of Bianchi Types I and V Spacetimes in f (R) Theory of Gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Exact Solutions of Bianchi Types I and V Spacetimes in f (R) Theory of Gravity

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Resolution: unresolved; no resolver link, observed 2026-08-10T21:04:53.634751Z

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Observation 9ec43d65-3d33-48f8-b698-ece7197bb87b · outbound

This paper cites A New f (R) Gravity Model and Properties of Gravitational Waves in It.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model A New f (R) Gravity Model and Properties of Gravitational Waves in It

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Resolution: verified exact; doi, observed 2026-08-10T21:04:55.790181Z

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Observation 99147307-6a8f-4f5c-9b51-428cafe8521a · outbound

This paper cites Exponential Gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Exponential Gravity

Reference 53

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:04:58.986842Z

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Observation 0935c0bf-d077-4068-82f0-ddd44aa1d1a3 · outbound

This paper cites Toward a Better Understanding of Cosmic Chronometers: A new measurement of H(z) at z~0.7.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Toward a Better Understanding of Cosmic Chronometers: A new measurement of H(z) at z~0.7

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Resolution: unresolved; no resolver link, observed 2026-08-10T21:04:54.664671Z

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Observation d7ee549e-360d-4709-a646-164aaf820f4c · outbound

This paper cites Measuring cosmic bulk flow with Pantheon catalogue in perturbed f (R) gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Measuring cosmic bulk flow with Pantheon catalogue in perturbed f (R) gravity

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Resolution: verified exact; doi, observed 2026-08-10T21:04:55.692721Z

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Observation c9979396-8a98-4902-aed4-9b9d27cd4a70 · outbound

This paper cites Generalization of the Einstein Theory.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Generalization of the Einstein Theory

Reference 57

Resolution: malformed identifier; no resolver link, observed 2026-08-10T21:04:53.854754Z

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Observation 6974ea87-ffbf-4c0e-815f-ed778d51f759 · outbound

This paper cites Third gravitational wave polarization mode in Rastall theory and analogy with f(R) theories.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Third gravitational wave polarization mode in Rastall theory and analogy with f(R) theories

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Resolution: verified exact; local_arxiv, observed 2026-08-10T21:04:56.611860Z

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Observation cde508ba-fbc2-40ef-b90f-1112625b36b4 · outbound

This paper cites A Resolution of the Cosmological Age Puzzle.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model A Resolution of the Cosmological Age Puzzle

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Resolution: verified exact; doi, observed 2026-08-10T21:04:55.664754Z

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Observation f1ec5bfa-561e-4a97-8f7c-a72272aa6177 · outbound

This paper cites D., and P.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model D., and P

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Resolution: unresolved; no resolver link, observed 2026-08-10T21:04:53.995359Z

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This paper cites Comments on the Scalar-Tensor Theory.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Comments on the Scalar-Tensor Theory

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-10T21:04:54.060658Z

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Observation ff89598d-d15a-47e8-af39-b42ffb6b28be · outbound

This paper cites f (R) Gravities, Killing Spinor Equations, ‘BPS’ Domain Walls and Cosmology.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model f (R) Gravities, Killing Spinor Equations, ‘BPS’ Domain Walls and Cosmology

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Resolution: unresolved; no resolver link, observed 2026-08-10T21:04:54.095175Z

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Observation d33bf93c-1f62-4274-8db5-be2b72ad132a · outbound

This paper cites Non-Linear Lagrangians and Cosmological Theory.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Non-Linear Lagrangians and Cosmological Theory

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Resolution: unresolved; no resolver link, observed 2026-08-10T21:04:54.148265Z

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Observation a1502350-6328-4560-ac71-01df45b16ae0 · outbound

This paper cites On Continued Gravitational Contraction.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model On Continued Gravitational Contraction

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Observation 36a6e454-a41b-4141-9d68-6aa79dc212c4 · outbound

This paper cites Einstein Static Universe in Rastall Theory of Gravity.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Einstein Static Universe in Rastall Theory of Gravity

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:04:58.912481Z

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Observation f3de0d31-64da-447b-8b68-af484a237ab0 · outbound

This paper cites Note on the Evolution of the Gravitational Potential in Rastall Scalar Field Theories.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Note on the Evolution of the Gravitational Potential in Rastall Scalar Field Theories

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Resolution: unresolved; raw_fallback, observed 2026-08-10T21:04:58.837811Z

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Observation c42cf1cd-44cc-4ddf-a715-fd216c12df11 · outbound

This paper cites Planck 2018 results. V. CMB power spectra and likelihoods.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Planck 2018 results. V. CMB power spectra and likelihoods

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Observation 99f48460-d901-4b5b-bdfb-4c77d4a881bc · outbound

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Resolution: unresolved; raw_fallback, observed 2026-08-10T21:04:58.794747Z

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Observation af6b2f0d-ac12-464b-ac4e-bd67c2072472 · outbound

This paper cites J., Howlett, C., et al.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model J., Howlett, C., et al

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:04:58.737058Z

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Observation 669b396a-6cb7-4ea5-8bf8-63252233150e · outbound

This paper cites 2017,The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample, MNRAS, 470, 2617.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model 2017,The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample, MNRAS, 470, 2617

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T21:04:58.704743Z

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

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Resolution: unresolved; raw_fallback, observed 2026-08-10T21:04:58.544825Z

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Observation 11beebb1-4ecf-4f85-a287-ca545ce66ed3 · outbound

This paper cites Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope

Reference 75

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Observation b8d4cf65-9f31-442e-9497-cacd1453a2d2 · outbound

This paper cites Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements

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Observation bb0aece7-946e-44dd-993d-b32575e3af92 · outbound

This paper cites Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix

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Observation bbfa8a25-6271-4d64-95c0-0be9ff93dd8f · outbound

This paper cites Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers

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Observation f6666687-a8e4-46c5-a39c-174fe5105a2a · outbound

This paper cites Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2

Reference 79

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Observation c6564350-7d09-4ce5-9c22-039a11dd4665 · outbound

This paper cites A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration

Reference 80

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Observation 38fc754a-f41c-46a5-b9e3-b76af586668b · outbound

This paper cites Jeans Type Instability of a Complex Self-Interacting Scalar Field in GR.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Jeans Type Instability of a Complex Self-Interacting Scalar Field in GR

Reference 81

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Observation 6de50dab-2220-4476-8386-49d18b51262a · outbound

This paper cites Massive Neutrinos in Cosmology: Analytic Solutions and Fluid Approxi- mation.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Massive Neutrinos in Cosmology: Analytic Solutions and Fluid Approxi- mation

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Resolution: verified exact; doi, observed 2026-08-10T21:04:55.468089Z

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Observation f699c9c3-487a-487f-b634-bfeeec84b696 · outbound

This paper cites The Peculiar Jeans Length.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model The Peculiar Jeans Length

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Resolution: verified exact; doi, observed 2026-08-10T21:04:55.434216Z

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Observation 47049c28-10fc-46d9-b172-c30f309fab5a · outbound

This paper cites The Interaction of Neutrinos with Phantom, Quintessence, and Quintum Scalar Fields and Its Effect on the Formation of Structures in the Early Universe.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model The Interaction of Neutrinos with Phantom, Quintessence, and Quintum Scalar Fields and Its Effect on the Formation of Structures in the Early Universe

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Resolution: verified exact; doi, observed 2026-08-10T21:04:55.388336Z

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Observation a2425ef3-d56c-4705-8c68-cba433755094 · outbound

This paper cites Hubble Parameter Measurement Constraints on the Cosmological Deceleration- Acceleration Transition Redshift.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Hubble Parameter Measurement Constraints on the Cosmological Deceleration- Acceleration Transition Redshift

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Resolution: unresolved; no resolver link, observed 2026-08-10T21:04:55.021847Z

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Observation 646e6c79-a39d-4fc0-b468-75fbe9f454ae · outbound

This paper cites Communications in Theoretical Physics 75 - 055401(2023)).

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Communications in Theoretical Physics 75 - 055401(2023))

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Resolution: unresolved; no resolver link, observed 2026-08-10T21:04:55.029323Z

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

Reference 87

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:04:58.384896Z

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

Reference 88

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:04:58.276390Z

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Observation 10d80cec-0422-4108-901f-fff8ca15845a · outbound

This paper cites and Loh, Y.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model and Loh, Y

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Resolution: unresolved; no resolver link, observed 2026-08-10T21:04:55.144755Z

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Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Unresolved cited work

Reference 90

Resolution: unresolved; raw_fallback, observed 2026-08-10T21:04:58.204749Z

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Observation 7efd040f-4e11-480f-8c59-81c131ff776b · outbound

This paper cites Joule-Thomson expansion and tidal force effects of AdS black holes surrounded by Chaplygin dark fluid.

Comparative Analysis of Perturbed $f(R)$ Gravity and Perturbed Rastall Gravity Models in Describing Cosmic Evolution from Early to Late Universe Relative to the $\Lambda$CDM Model Joule-Thomson expansion and tidal force effects of AdS black holes surrounded by Chaplygin dark fluid

Reference 2023

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