Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime | Paper Citation Record

Observation bbe4805f-04dd-46cb-83ec-3d4034a24746 · outbound

This paper cites It always exists and it verifies Ωm = 1.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists and it verifies Ωm = 1

Reference 1

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This paper cites Moreover, the evo- lution equation for H, given by the Raychaudhuri equation, decouples.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Moreover, the evo- lution equation for H, given by the Raychaudhuri equation, decouples

Reference 3

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Observation d27d423d-70c3-44db-af8f-3cfaef2b2837 · outbound

This paper cites This means that for each of the interactions (26)-(34), we obtain a different dynamical system when the corresponding values of α, β, δare substituted into (41)-(44).

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime This means that for each of the interactions (26)-(34), we obtain a different dynamical system when the corresponding values of α, β, δare substituted into (41)-(44)

Reference 4

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Observation c69d9e15-d7d9-423c-b4ef-10b62fbc0d59 · outbound

This paper cites They always exist and both represent an anisotropic Bianchi I vacuum solution.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime They always exist and both represent an anisotropic Bianchi I vacuum solution

Reference 5

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Observation ceff70db-13be-4efa-ad3d-cb403b31d9a8 · outbound

This paper cites It always exists and we verify that Ωm = 1.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists and we verify that Ωm = 1

Reference 6

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Observation 17d8f258-c022-4d14-acc4-653bf22bf63c · outbound

This paper cites It always exists It always exists and represents a scalar field dominated flat FLRW solution.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists It always exists and represents a scalar field dominated flat FLRW solution

Reference 7

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Observation cb1a2da9-e85f-4c38-94a0-c200720f46b3 · outbound

This paper cites These points are anisotropic vacuum Bianchi I solutions.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime These points are anisotropic vacuum Bianchi I solutions

Reference 8

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This paper cites an unresolved cited work.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Unresolved cited work

Reference 9

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Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Unresolved cited work

Reference 11

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Observation d4d3c655-3b96-4219-b7f7-e32ef8d633a7 · outbound

This paper cites It always exists and is i) sink for 0 ≤ γ <2, ¯Γ < −3(γ − 1), ii) saddle for 0 ≤ γ <2, ¯Γ > −3(γ − 1), iii) non-hyperbolic for ¯Γ = −3(γ − 1) or γ = 2.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists and is i) sink for 0 ≤ γ <2, ¯Γ < −3(γ − 1), ii) saddle for 0 ≤ γ <2, ¯Γ > −3(γ − 1), iii) non-hyperbolic for ¯Γ = −3(γ − 1) or γ = 2

Reference 12

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Observation 5e7627bd-7d31-4bf7-a358-4a8056caa84b · outbound

This paper cites They always exist and are i) sources for 0 ≤ γ <2, ¯Γ > −3, ii) saddles for 0 ≤ γ <2, ¯Γ < −3, iii) non-hyperbolic for ¯Γ = −3 or γ = 2.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime They always exist and are i) sources for 0 ≤ γ <2, ¯Γ > −3, ii) saddles for 0 ≤ γ <2, ¯Γ < −3, iii) non-hyperbolic for ¯Γ = −3 or γ = 2

Reference 13

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Observation 5d93c7f0-e6fa-45e1-9a73-270c088a8ec0 · outbound

This paper cites This point verifies Ωm = ¯Γ 3−3γ.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime This point verifies Ωm = ¯Γ 3−3γ

Reference 14

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Observation 6c53ea7f-66c8-422e-a063-a1e76b08ff0a · outbound

This paper cites They belong to the singular line ¯Ω = 0 and are non-hyperbolic.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime They belong to the singular line ¯Ω = 0 and are non-hyperbolic

Reference 15

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Observation 569f7a54-fbf8-44bb-a85f-4eb08e812876 · outbound

This paper cites It has Ωm = 1 6 3 − √ 9γ+12¯Γ−9√γ−1 and it exists exists for 0 ≤ γ < 1, 0 ≤ ¯Γ ≤ 1 4 (3 − 3γ) or 1 < γ ≤ 2, 1 4 (3 − 3γ) ≤ ¯Γ ≤ 0.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It has Ωm = 1 6 3 − √ 9γ+12¯Γ−9√γ−1 and it exists exists for 0 ≤ γ < 1, 0 ≤ ¯Γ ≤ 1 4 (3 − 3γ) or 1 < γ ≤ 2, 1 4 (3 − 3γ) ≤ ¯Γ ≤ 0

Reference 16

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Observation 15021203-a64b-4ee0-93e0-03e49b799b55 · outbound

This paper cites It has Ωm = 1 6 √ 9γ+12¯Γ−9√γ−1 + 3 , it exists for 0 ≤ γ <1, 0 ≤ ¯Γ ≤ 1 4 (3 − 3γ) or 1 < γ≤ 2, 1 4 (3 − 3γ) ≤ ¯Γ ≤ 0.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It has Ωm = 1 6 √ 9γ+12¯Γ−9√γ−1 + 3 , it exists for 0 ≤ γ <1, 0 ≤ ¯Γ ≤ 1 4 (3 − 3γ) or 1 < γ≤ 2, 1 4 (3 − 3γ) ≤ ¯Γ ≤ 0

Reference 17

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Observation 1febb70f-54ab-457f-b2e2-192e95ee4350 · outbound

This paper cites It exist for i) m <0, 1 ≤ γ ≤ 2 or ii) m = 0, 0 ≤ γ <1 or iii) m = 0, 1 < γ≤ 2 or iv) m >0, 0 ≤ γ ≤ 1.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It exist for i) m <0, 1 ≤ γ ≤ 2 or ii) m = 0, 0 ≤ γ <1 or iii) m = 0, 1 < γ≤ 2 or iv) m >0, 0 ≤ γ ≤ 1

Reference 20

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Observation faf948dd-0a20-47bb-81cf-dfdfa7ab668e · outbound

This paper cites It always exists and it verifies Ωm = 1.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists and it verifies Ωm = 1

Reference 21

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Observation a7a8824b-c5f7-4972-852d-c20c9b2537f6 · outbound

This paper cites It always exists and represents a scalar field domi- nated solution.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists and represents a scalar field domi- nated solution

Reference 22

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Observation 92b78682-21dd-448c-8a9c-fb09c5712cb9 · outbound

This paper cites They always exist and both represent an anisotropic Bianchi I vacuum solution.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime They always exist and both represent an anisotropic Bianchi I vacuum solution

Reference 23

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Observation b0cc5ceb-0dd1-481b-a0ca-275609739635 · outbound

This paper cites The points M1,2 = ± q γ+m−1 m , q 2−γ m only exist for γ = 2 and m ≤ −1.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime The points M1,2 = ± q γ+m−1 m , q 2−γ m only exist for γ = 2 and m ≤ −1

Reference 24

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Observation 19bfce06-b7b0-491d-92a7-6167d321b81a · outbound

This paper cites It always exists and it verifies Ωm = 1.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists and it verifies Ωm = 1

Reference 25

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Observation 4cc1f344-5ffa-41b8-b16c-765174650bcc · outbound

This paper cites It always exists and represents a scalar field dominated flat FLRW solution.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists and represents a scalar field dominated flat FLRW solution

Reference 26

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Observation 1aa9afa9-9ee9-4286-8a37-38fe10985e82 · outbound

This paper cites They always exist and both represent an anisotropic Bianchi I vacuum solution.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime They always exist and both represent an anisotropic Bianchi I vacuum solution

Reference 27

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Observation dfaaf535-19e9-4c4e-9bcf-381e97382e60 · outbound

This paper cites It always exists and it verifies Ωm = 1.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists and it verifies Ωm = 1

Reference 28

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Observation 94d98d12-682d-4600-b4f7-0194dabe8204 · outbound

This paper cites It always exists and represents a scalar field domi- nated solution.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It always exists and represents a scalar field domi- nated solution

Reference 29

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Observation 9c27d056-4742-45ef-8027-87f8b9611651 · outbound

This paper cites They always exist, to study their stability we substitute ¯Ω = 0 in the Jacobian matrix and then take the limit as Σ → ±1.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime They always exist, to study their stability we substitute ¯Ω = 0 in the Jacobian matrix and then take the limit as Σ → ±1

Reference 30

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Observation a8a4f835-a764-4340-8102-425ec6eabafe · outbound

This paper cites The point exists for m > 0, 0 ≤ γ ≤ 1 or m <0, 1 ≤ γ ≤ 2 and is a i) sink for 0 ≤ γ <1, −γ2+2γ−1 γ−2 < m <1 − γ or 1 < γ≤ 2, m <1 − γ, ii) saddle for i.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime The point exists for m > 0, 0 ≤ γ ≤ 1 or m <0, 1 ≤ γ ≤ 2 and is a i) sink for 0 ≤ γ <1, −γ2+2γ−1 γ−2 < m <1 − γ or 1 < γ≤ 2, m <1 − γ, ii) saddle for i

Reference 31

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Observation a28aa2bd-7f61-4eb4-8e11-b0b0a0174476 · outbound

This paper cites The definition of the deceleration parameter q is as follows q := −1 − ˙H(t) H 2(t).

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime The definition of the deceleration parameter q is as follows q := −1 − ˙H(t) H 2(t)

Reference 32

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Observation d911cb4d-b969-4f1d-9d18-2309939772de · outbound

This paper cites It describes acceleration for 0 ≤ γ < 2 3.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime It describes acceleration for 0 ≤ γ < 2 3

Reference 33

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Observation 22b565f9-2502-4c37-8b20-89df724d3021 · outbound

This paper cites (152) In Figure 21 we see that qseries oscillates between deceleration and acceleration.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime (152) In Figure 21 we see that qseries oscillates between deceleration and acceleration

Reference 34

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Observation 90c6175b-f741-4bbc-88b2-c619d7c54988 · outbound

This paper cites The Hubble function is H(t) = 1 3t.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime The Hubble function is H(t) = 1 3t

Reference 35

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Observation 047ef38a-c392-4cfd-9d20-9a83f108331d · outbound

This paper cites (154) We focus on qaveraged, it describes acceleration for ¯Γ < 2 − 3γ.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime (154) We focus on qaveraged, it describes acceleration for ¯Γ < 2 − 3γ

Reference 36

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Observation d262e8ae-a1eb-4887-aab6-0e95054705ed · outbound

This paper cites (157) We focus on qaveraged, it describes acceleration for ¯Γ > 1.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime (157) We focus on qaveraged, it describes acceleration for ¯Γ > 1

Reference 37

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Observation 9319a71c-ab33-4e63-93ca-56f1fde7f0cd · outbound

This paper cites (160) We focus on qaveraged.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime (160) We focus on qaveraged

Reference 38

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Observation f089a3c6-bd84-4e78-8a67-314273062a3d · outbound

This paper cites (163) We focus on qaveraged.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime (163) We focus on qaveraged

Reference 39

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Observation b56c694b-5157-4ef5-9681-b7ab2a31ae18 · outbound

This paper cites (166) We focus on qaveraged.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime (166) We focus on qaveraged

Reference 40

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Observation 0d787b85-6c9d-46f7-be6d-b352b0f39d22 · outbound

This paper cites They describe acceleration for 0 ≤ γ <2, 1 4 (3γ − 6) < m <0.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime They describe acceleration for 0 ≤ γ <2, 1 4 (3γ − 6) < m <0

Reference 41

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Observation ad282bc8-ceda-4a53-9dad-75e2e09ba8bc · outbound

This paper cites (170) We focus on qaveraged.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime (170) We focus on qaveraged

Reference 42

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Observation f33e4322-773f-4e5f-9a58-11d79b8e4296 · outbound

This paper cites StiffnessSwitching.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime StiffnessSwitching

Reference 43

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Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Unresolved cited work

Reference 44

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This paper cites Coupled Quintessence.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Coupled Quintessence

Reference 45

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Observation 51debe04-2cb7-424d-9b01-375b0d21c1df · outbound

This paper cites Interacting Dark Energy -- constraints and degeneracies.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting Dark Energy -- constraints and degeneracies

Reference 46

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This paper cites Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters

Reference 47

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Observation f1a8856e-1a4d-4e5a-9574-971e3d2d806c · outbound

This paper cites Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem

Reference 48

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This paper cites Interaction in the dark sector: a phenomenological approach.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interaction in the dark sector: a phenomenological approach

Reference 49

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Observation 9233e1d4-bf8e-4fc9-a5b8-09078f837af2 · outbound

This paper cites Compartmentalization and Coexistence in the Dark Sector of the Universe.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Compartmentalization and Coexistence in the Dark Sector of the Universe

Reference 50

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This paper cites Perturbations in the interacting vacuum.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Perturbations in the interacting vacuum

Reference 51

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Observation ecae731f-ac48-4d97-a39b-f78fd8de2d54 · outbound

This paper cites Looking for interactions in the cosmological dark sector.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Looking for interactions in the cosmological dark sector

Reference 52

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Observation f045838d-eedd-4ebf-ab59-7f2e3bc90bd1 · outbound

This paper cites Modeling dark energy through an Ising fluid with network interactions.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Modeling dark energy through an Ising fluid with network interactions

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T05:28:59.128323Z

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Observation 11cc10ab-63a0-48a9-987b-dbf713bf8d17 · outbound

This paper cites The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-06T05:28:59.273736Z

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Observation a8b43846-c1d1-4154-bccb-58792836b042 · outbound

This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-06T05:28:59.388019Z

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Observation fd5022d4-6bc8-43cb-aee1-afd18c8f0813 · outbound

This paper cites Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-06T05:28:59.482509Z

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Observation bd750522-5d90-4622-ba07-ff800e44466e · outbound

This paper cites Update on Coupled Dark Energy and the $H_0$ tension.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Update on Coupled Dark Energy and the $H_0$ tension

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-06T05:28:59.585298Z

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Observation ec6d6515-d8ac-413d-83e9-d2f6128065cd · outbound

This paper cites Linear and non-linear perturbations in dark energy models.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Linear and non-linear perturbations in dark energy models

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-06T05:28:59.710092Z

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Observation e55833c5-6aa5-474b-b9de-c8428cad290c · outbound

This paper cites Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-06T05:28:59.809102Z

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Observation 58c72245-faca-4465-b5f9-fac0bfd6a421 · outbound

This paper cites Dark sector interaction: a remedy of the tensions between CMB and LSS data.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Dark sector interaction: a remedy of the tensions between CMB and LSS data

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-06T05:28:59.934875Z

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Observation 9ad79361-2de8-4cc8-a0ce-d16892c77657 · outbound

This paper cites Carloni, O.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Carloni, O

Reference 61

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Observation 7dfb7f55-4276-4fc6-a73b-b85d1d88b83f · outbound

This paper cites Observational constraints of a new unified dark fluid and the $H_0$ tension.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Observational constraints of a new unified dark fluid and the $H_0$ tension

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:00.143128Z

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Observation 16d76090-1bf2-406f-a86a-5bed88c92fe5 · outbound

This paper cites Multi-interacting dark energy and its cosmological implications.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Multi-interacting dark energy and its cosmological implications

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:00.246942Z

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Observation 05d301e8-2778-4d08-b7bd-e35c1161a0ea · outbound

This paper cites Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_{0}$ tension.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_{0}$ tension

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:00.381382Z

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Observation 9f538751-3a3f-4993-92e9-24e970e519bb · outbound

This paper cites Smoothing the $H_0$ tension with a dynamical dark energy model.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Smoothing the $H_0$ tension with a dynamical dark energy model

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:00.517706Z

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Observation 45c7aab6-34b4-40f6-97d9-9e8bfe4edd28 · outbound

This paper cites Relieving the $H_0$ tension with a new interacting dark energy model.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Relieving the $H_0$ tension with a new interacting dark energy model

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:00.615033Z

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Observation aeaabf5e-4cc9-45ed-9afc-49ec2bd7ff6d · outbound

This paper cites Cosmological implications of an interacting model of dark matter \& dark energy.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Cosmological implications of an interacting model of dark matter \& dark energy

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:00.732394Z

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Observation e9cfe380-33ab-49a3-a4a4-7de3139219d1 · outbound

This paper cites Interacting dark energy: clarifying the cosmological implications and viability conditions.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting dark energy: clarifying the cosmological implications and viability conditions

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:00.850445Z

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Observation b7992508-e649-43f5-95ad-1a9c25bb5495 · outbound

This paper cites Late time interacting cosmologies and the Hubble constant tension.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Late time interacting cosmologies and the Hubble constant tension

Reference 69

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Observation 62724885-5ac0-4d85-a97d-ecd48a95b30c · outbound

This paper cites Some Classes of Interacting Two-Fluid Model of the Expanding Universe.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Some Classes of Interacting Two-Fluid Model of the Expanding Universe

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:01.100292Z

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Observation 43c14924-a39b-4618-8515-39dec55cbcb3 · outbound

This paper cites Reconciling $S_8$: Insights from Interacting Dark Sectors.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Reconciling $S_8$: Insights from Interacting Dark Sectors

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:01.205976Z

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Observation c3d0989d-07b8-4c2b-bab8-8c1158ab1214 · outbound

This paper cites Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:01.353564Z

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Observation 423bccd1-a2ce-4d53-9178-17d6c2db99be · outbound

This paper cites J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:01.485032Z

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Observation aa3ae12b-23aa-4234-a764-a901733074a9 · outbound

This paper cites Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:01.623476Z

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Observation f3b3fd0d-bb88-4a50-9257-47f957da1471 · outbound

This paper cites Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Extended Analysis of Neutrino-Dark Matter Interactions with Small-Scale CMB Experiments

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:01.709828Z

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Observation fc3aca07-458b-4ab9-b88f-3bd85bd62173 · outbound

This paper cites Chakraborty, T.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Chakraborty, T

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:01.813045Z

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Observation c006d971-c973-4e23-8da8-16efbc43dd5a · outbound

This paper cites Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:01.892565Z

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Observation ad815fa9-5887-4f99-88a4-7e868a3072d5 · outbound

This paper cites Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:02.010016Z

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Observation f63b7d5f-0ea4-4499-8e69-90d2faa0a0f4 · outbound

This paper cites Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

Reference 79

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Observation ebf91d30-c1de-4bc1-94b0-174b788fd3ac · outbound

This paper cites Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements

Reference 80

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Observation 7e5b8f9e-86dd-40fb-946c-f4b0b4d330bc · outbound

This paper cites Interacting dark sector with quadratic coupling: theoretical and observational viability.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting dark sector with quadratic coupling: theoretical and observational viability

Reference 81

Resolution: verified exact; local_arxiv, observed 2026-08-06T05:29:18.500205Z

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Observation aded0440-68fd-450c-93dd-53e0db2340a8 · outbound

This paper cites Cosmological constraints on two vacuum decay models.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Cosmological constraints on two vacuum decay models

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:02.425542Z

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Observation 4b74d059-6719-472e-a3e2-5fd4147f6f0b · outbound

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

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting Dark Sectors in light of DESI DR2

Reference 83

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Observation 45e27586-f073-4249-b29b-81386e38c0ff · outbound

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

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime New constraints on interacting dark energy from DESI DR2 BAO observations

Reference 84

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Observation 6bc727ac-65dd-4a4d-87ca-837f73e41eae · outbound

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

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Dynamical Dark Energy Implies a Coupled Dark Sector: Insights from DESI DR2 via a Data-Driven Approach

Reference 85

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Observation f14da499-3227-489d-9dfa-e76c99adcadd · outbound

This paper cites New cosmological constraints on the evolution of dark matter energy density.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime New cosmological constraints on the evolution of dark matter energy density

Reference 86

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Observation b00d8804-5541-4a8c-89e4-dff5962c6cf4 · outbound

This paper cites van der Westhuizen, D.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime van der Westhuizen, D

Reference 87

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Observation 34075756-de46-4ef4-bc00-0111981fb50f · outbound

This paper cites Constraint on Momentum-coupled Dark Energy using DESI DR2.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Constraint on Momentum-coupled Dark Energy using DESI DR2

Reference 88

Resolution: verified exact; local_arxiv, observed 2026-08-06T05:29:17.908374Z

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Observation 48c9aa2c-7286-4026-953e-dbdbeec21ecb · outbound

This paper cites Paliathanasis (2025), 2503.20896.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Paliathanasis (2025), 2503.20896

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:03.066621Z

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Observation 7f9c33e9-24db-46c3-a5e0-928625377506 · outbound

This paper cites Observational Constraints on Scalar Field--Matter Interaction in Weyl Integrable Spacetime.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Observational Constraints on Scalar Field--Matter Interaction in Weyl Integrable Spacetime

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:03.143295Z

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Observation c11ccf52-bf0a-4381-bc2c-a412225403f2 · outbound

This paper cites Li and X.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Li and X

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:03.212372Z

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Observation 7f86fe27-65bb-4651-94db-e2241c6e0652 · outbound

This paper cites an unresolved cited work.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Unresolved cited work

Reference 92

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Observation 921d20a7-401d-4b85-8833-a113aa100c5b · outbound

This paper cites General Relativity and Weyl Geometry.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime General Relativity and Weyl Geometry

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:03.460981Z

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Observation 3977328a-11ee-4480-b7f2-6cd85377c841 · outbound

This paper cites Interacting dark energy in curved FLRW spacetime from Weyl Integrable Spacetime.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting dark energy in curved FLRW spacetime from Weyl Integrable Spacetime

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:03.524844Z

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Observation c2997d30-2d25-43b5-abaf-0494948e03b3 · outbound

This paper cites Integrable Weyl Geometry in Multidimensional Cosmology. Numerical Investigation.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Integrable Weyl Geometry in Multidimensional Cosmology. Numerical Investigation

Reference 95

Resolution: verified exact; local_arxiv, observed 2026-08-06T05:29:17.265153Z

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No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 262d45e9-b62f-463c-835f-d64bee91d03d · outbound

This paper cites Quintom cosmology and modified gravity after DESI 2024.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Quintom cosmology and modified gravity after DESI 2024

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:03.744635Z

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Observation f4de0fae-fd6c-43c6-90f0-21f1812246a2 · outbound

This paper cites Cosmic Duality in Quintom Universe.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Cosmic Duality in Quintom Universe

Reference 97

Resolution: verified exact; local_arxiv, observed 2026-08-06T05:29:16.999452Z

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No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation b60a7e3d-7bf8-4996-a9f2-6d9a074baaea · outbound

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

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Quantum Gravity Meets DESI: Dynamical Dark Energy in Light of the Trans-Planckian Censorship Conjecture

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:03.928886Z

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Observation 11dd371a-7793-4d12-a71f-9bc6da59ea55 · outbound

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

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Modified gravity realizations of quintom dark energy after DESI DR2

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:04.039842Z

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Observation 663285bd-341d-4e22-900c-eeea17a85783 · outbound

This paper cites Equivalence of $f(Q)$ cosmology with quintom-like scenario: the phantom field as effective realization of the non-trivial connection.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Equivalence of $f(Q)$ cosmology with quintom-like scenario: the phantom field as effective realization of the non-trivial connection

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:04.134717Z

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Observation f9eacbba-b0bb-42be-86c4-90ad711424a4 · outbound

This paper cites Quintom Cosmology: Theoretical implications and observations.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Quintom Cosmology: Theoretical implications and observations

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:04.222183Z

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Observation 698ebfb2-0b6d-4e1b-853c-c8482fc7c14f · outbound

This paper cites The dynamics of scalar-field Quintom cosmological models.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime The dynamics of scalar-field Quintom cosmological models

Reference 102

Resolution: verified exact; local_arxiv, observed 2026-08-06T05:29:16.714485Z

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No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation a611b045-058b-4894-a691-5999c4018646 · outbound

This paper cites The past and future dynamics of quintom dark energy models.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime The past and future dynamics of quintom dark energy models

Reference 103

Resolution: verified exact; local_arxiv, observed 2026-08-06T05:29:16.478734Z

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This paper cites Quintom phase-space: beyond the exponential potential.

Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Quintom phase-space: beyond the exponential potential

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