Redshift space distortions in the presence of non-minimally coupled dark matter | Paper Citation Record

Observation f1dfd21b-c2b6-4fac-b8e1-5618c3e202a3 · outbound

This paper cites This kind of interaction was ﬁrst proposed in the context of coupled quintessence in [53] and has been further investigated in [54–56].

Redshift space distortions in the presence of non-minimally coupled dark matter This kind of interaction was ﬁrst proposed in the context of coupled quintessence in [53] and has been further investigated in [54–56]

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T12:29:30.236537Z

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Observation 95bfb9ef-d34a-4d21-bb69-d91eee0919bf · outbound

This paper cites In the uncoupled case, the equation of state of the scalar ﬁeld follows the behavior of the dominant background ﬂuid according 12 (a) (b) FIG.

Redshift space distortions in the presence of non-minimally coupled dark matter In the uncoupled case, the equation of state of the scalar ﬁeld follows the behavior of the dominant background ﬂuid according 12 (a) (b) FIG

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T12:29:30.221771Z

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Observation cf9aeb11-901f-4e41-a031-be99417c0431 · outbound

This paper cites In this case, there is no interaction at the background level, Q0 = 0.

Redshift space distortions in the presence of non-minimally coupled dark matter In this case, there is no interaction at the background level, Q0 = 0

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T12:29:30.207314Z

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Observation 5a16905d-236b-42c1-8477-e1cb422bb1f2 · outbound

This paper cites (69), vanish and the equation of motion for the CDM growth function, Eq.

Redshift space distortions in the presence of non-minimally coupled dark matter (69), vanish and the equation of motion for the CDM growth function, Eq

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T12:29:30.192408Z

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Observation d0b2c61f-4236-437e-a1f3-6bafee17535f · outbound

This paper cites (106) As in conformal model I, the modiﬁcation to the Hubble friction term is related to the eﬀective CDM equation of state byE1 = 3weﬀ c /2.

Redshift space distortions in the presence of non-minimally coupled dark matter (106) As in conformal model I, the modiﬁcation to the Hubble friction term is related to the eﬀective CDM equation of state byE1 = 3weﬀ c /2

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T12:29:30.177172Z

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Observation 5f8f1a8c-46b8-480b-903e-680cc1c2a6e9 · outbound

This paper cites (90), one ﬁnds Υ 1 =−Υ2 =E2.

Redshift space distortions in the presence of non-minimally coupled dark matter (90), one ﬁnds Υ 1 =−Υ2 =E2

Reference 6

Resolution: malformed identifier; raw_fallback, observed 2026-08-14T12:29:30.161971Z

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Observation 5785ebb4-e52b-45f4-997f-526b4e7cde9f · outbound

This paper cites The power spectrum and bispectrum of SDSS DR11 BOSS galaxies I: bias and gravity.

Redshift space distortions in the presence of non-minimally coupled dark matter The power spectrum and bispectrum of SDSS DR11 BOSS galaxies I: bias and gravity

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.807239Z

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Observation f62232aa-29a4-4acd-b40e-b5b893b15786 · outbound

This paper cites The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints.

Redshift space distortions in the presence of non-minimally coupled dark matter The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.812395Z

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Observation 28fd3279-1b8d-45b3-a3af-6a802658736d · outbound

This paper cites Zwicky, Helvetica Physica Acta, 6, 110 (1933).

Redshift space distortions in the presence of non-minimally coupled dark matter Zwicky, Helvetica Physica Acta, 6, 110 (1933)

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T12:29:30.147111Z

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Observation 8ecb8ada-019c-4f68-a682-567a259ca124 · outbound

This paper cites an unresolved cited work.

Redshift space distortions in the presence of non-minimally coupled dark matter Unresolved cited work

Reference 10

Resolution: unresolved; raw_fallback, observed 2026-08-14T12:29:30.130960Z

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Observation f738c3e0-dccc-479f-af40-4ee8cacd1c96 · outbound

This paper cites an unresolved cited work.

Redshift space distortions in the presence of non-minimally coupled dark matter Unresolved cited work

Reference 11

Resolution: unresolved; raw_fallback, observed 2026-08-14T12:29:30.115754Z

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Observation 6d745920-f78f-4051-a1b0-0f1f3cd2766d · outbound

This paper cites Weak lensing mass reconstruction of the interacting cluster 1E0657-558: Direct evidence for the existence of dark matter.

Redshift space distortions in the presence of non-minimally coupled dark matter Weak lensing mass reconstruction of the interacting cluster 1E0657-558: Direct evidence for the existence of dark matter

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.830970Z

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Observation 6a3bc762-9161-4c8a-984e-59b62c17def9 · outbound

This paper cites Cosmology from Type Ia Supernovae.

Redshift space distortions in the presence of non-minimally coupled dark matter Cosmology from Type Ia Supernovae

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.835691Z

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Observation f03067d6-42ee-4af4-bda1-d9dbdfac524e · outbound

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

Redshift space distortions in the presence of non-minimally coupled dark matter Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.840205Z

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Observation b790fd58-8eab-498b-9bc6-e692ac8e4b98 · outbound

This paper cites Planck 2015 results. XIII. Cosmological parameters.

Redshift space distortions in the presence of non-minimally coupled dark matter Planck 2015 results. XIII. Cosmological parameters

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.844233Z

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Observation 2095dcba-ee4e-46de-9429-d13747c14b64 · outbound

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

Redshift space distortions in the presence of non-minimally coupled dark matter Quintessence, Cosmic Coincidence, and the Cosmological Constant

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.848629Z

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Observation 2875a1b3-4311-4849-a739-bd6aee5f7631 · outbound

This paper cites Kinetically Driven Quintessence.

Redshift space distortions in the presence of non-minimally coupled dark matter Kinetically Driven Quintessence

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.853070Z

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Observation c4fd25a8-2616-4892-8a96-7c6f3295eaf0 · outbound

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

Redshift space distortions in the presence of non-minimally coupled dark matter A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.857903Z

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Observation 8fe86061-a8d9-42f6-8200-79d5310b85e3 · outbound

This paper cites Is Cosmic Speed-Up Due to New Gravitational Physics?.

Redshift space distortions in the presence of non-minimally coupled dark matter Is Cosmic Speed-Up Due to New Gravitational Physics?

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.862681Z

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Observation f0934bc1-3923-4ac4-89ee-ff0656c37b16 · outbound

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

Redshift space distortions in the presence of non-minimally coupled dark matter Disappearing cosmological constant in f(R) gravity

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.867237Z

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Observation 4f2fce0c-78b8-4132-83e2-a396842cff7c · outbound

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

Redshift space distortions in the presence of non-minimally coupled dark matter Models of f(R) Cosmic Acceleration that Evade Solar-System Tests

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.871739Z

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Observation 7313fdee-1d99-41e4-bc85-5012568480a7 · outbound

This paper cites Quintessence without scalar fields.

Redshift space distortions in the presence of non-minimally coupled dark matter Quintessence without scalar fields

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.876855Z

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Observation 56ae2991-400d-405f-a41f-dfd3e971ef5a · outbound

This paper cites an unresolved cited work.

Redshift space distortions in the presence of non-minimally coupled dark matter Unresolved cited work

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.881569Z

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Observation c76649db-1224-4f88-8ddb-5624e4fdb38c · outbound

This paper cites From k-essence to generalised Galileons.

Redshift space distortions in the presence of non-minimally coupled dark matter From k-essence to generalised Galileons

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.887261Z

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Observation 38b29d00-e5c1-44cd-b795-3f026b244411 · outbound

This paper cites Generalized G-inflation: Inflation with the most general second-order field equations.

Redshift space distortions in the presence of non-minimally coupled dark matter Generalized G-inflation: Inflation with the most general second-order field equations

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.891803Z

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Observation 0f929b88-081a-4517-8c2c-0f427a32f295 · outbound

This paper cites Healthy theories beyond Horndeski.

Redshift space distortions in the presence of non-minimally coupled dark matter Healthy theories beyond Horndeski

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.896780Z

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Observation 75da2e09-460e-44b8-8170-b1b8f4cb500e · outbound

This paper cites Degenerate higher derivative theories beyond Horndeski: evading the Ostrogradski instability.

Redshift space distortions in the presence of non-minimally coupled dark matter Degenerate higher derivative theories beyond Horndeski: evading the Ostrogradski instability

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.901080Z

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Observation 82b8a4ff-685d-4ed5-bd9d-3bc2362c20d0 · outbound

This paper cites Modified gravity models of dark energy.

Redshift space distortions in the presence of non-minimally coupled dark matter Modified gravity models of dark energy

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.905420Z

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Observation 191a8199-299b-4669-abf4-bff6f1f20b0d · outbound

This paper cites Modified Gravity and Cosmology.

Redshift space distortions in the presence of non-minimally coupled dark matter Modified Gravity and Cosmology

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.909935Z

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Observation 52508a41-2f80-49a6-ab33-390ff5a9ed9d · outbound

This paper cites The Relation between Physical and Gravitational Geometry.

Redshift space distortions in the presence of non-minimally coupled dark matter The Relation between Physical and Gravitational Geometry

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.915322Z

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Observation f7c4ee0d-3d09-4cd8-a7ca-54711b3d6c23 · outbound

This paper cites Degenerate higher order scalar-tensor theories beyond Horndeski and disformal transformations.

Redshift space distortions in the presence of non-minimally coupled dark matter Degenerate higher order scalar-tensor theories beyond Horndeski and disformal transformations

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.919865Z

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Observation 26fec9fd-72e2-40ad-8b4f-383529dd76eb · outbound

This paper cites The fundamental constants and their variation: observational status and theoretical motivations.

Redshift space distortions in the presence of non-minimally coupled dark matter The fundamental constants and their variation: observational status and theoretical motivations

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.925404Z

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Observation 504c8b99-c4e8-423d-8be2-cde73342bf75 · outbound

This paper cites Tests of the Gravitational Inverse-Square Law below the Dark-Energy Length Scale.

Redshift space distortions in the presence of non-minimally coupled dark matter Tests of the Gravitational Inverse-Square Law below the Dark-Energy Length Scale

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.930298Z

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Observation b25a368c-e9b8-4b6a-900c-46ad7a269296 · outbound

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

Redshift space distortions in the presence of non-minimally coupled dark matter Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.935547Z

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Observation 4ed56772-e01f-4f3d-81a0-23ed2bfbc0c8 · outbound

This paper cites Equivalence Principle Implications of Modified Gravity Models.

Redshift space distortions in the presence of non-minimally coupled dark matter Equivalence Principle Implications of Modified Gravity Models

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.940210Z

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Observation 63ef81d7-78cd-4b0e-894e-a3ee3837fe67 · outbound

This paper cites Predictive Power of Strong Coupling in Theories with Large Distance Modified Gravity.

Redshift space distortions in the presence of non-minimally coupled dark matter Predictive Power of Strong Coupling in Theories with Large Distance Modified Gravity

Reference 36

Resolution: verified exact; local_arxiv, observed 2026-08-14T12:29:29.689819Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation ad08fb2b-c3b7-44af-af95-5d65679d0fd2 · outbound

This paper cites Beyond the Cosmological Standard Model.

Redshift space distortions in the presence of non-minimally coupled dark matter Beyond the Cosmological Standard Model

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.950276Z

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Observation 9bbf372d-c0c5-4832-80d2-19f9cb1373fa · outbound

This paper cites Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures.

Redshift space distortions in the presence of non-minimally coupled dark matter Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.955221Z

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Observation a8aedf55-385e-48fe-bc08-f1823fcd1438 · outbound

This paper cites Kaiser, Mon.

Redshift space distortions in the presence of non-minimally coupled dark matter Kaiser, Mon

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.959284Z

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Observation cdea5826-f9f4-48e1-8e58-35026e5348f5 · outbound

This paper cites Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS).

Redshift space distortions in the presence of non-minimally coupled dark matter Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.963487Z

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Observation 7c158f06-1816-48c5-b334-e0b5df01af62 · outbound

This paper cites The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering.

Redshift space distortions in the presence of non-minimally coupled dark matter The SDSS-IV eBOSS: emission line galaxy catalogues at z=0.8 and study of systematic errors in the angular clustering

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-08-14T12:29:29.626787Z

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Observation 3fcf6d5c-5aaf-4ebb-8a36-6ccaf4f7b767 · outbound

This paper cites The Euclid mission design.

Redshift space distortions in the presence of non-minimally coupled dark matter The Euclid mission design

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.973357Z

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Observation 9df76400-adc0-424a-919b-45b993b84ef5 · outbound

This paper cites Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report.

Redshift space distortions in the presence of non-minimally coupled dark matter Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.978130Z

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Observation c5f76b3c-de3f-4e6e-a1ab-178b67c838c5 · outbound

This paper cites Cosmology with the SKA -- overview.

Redshift space distortions in the presence of non-minimally coupled dark matter Cosmology with the SKA -- overview

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.983134Z

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Observation 303ba83a-a228-4eb1-985f-56f820aa7468 · outbound

This paper cites Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts.

Redshift space distortions in the presence of non-minimally coupled dark matter Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.988087Z

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Observation 57a9da48-3afd-456f-ae6e-ad680fa23ca8 · outbound

This paper cites Cosmology with the Square Kilometre Array by SKA-Japan.

Redshift space distortions in the presence of non-minimally coupled dark matter Cosmology with the Square Kilometre Array by SKA-Japan

Reference 46

Resolution: metadata mismatch; local_arxiv, observed 2026-08-14T12:29:29.548847Z

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Observation 4aab19f1-2be8-407f-b527-a0043d166bf4 · outbound

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

Redshift space distortions in the presence of non-minimally coupled dark matter Planck 2018 results. VI. Cosmological parameters

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:28.998579Z

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Observation c8b85ff4-3c1c-4969-888e-490fab375de7 · outbound

This paper cites Are redshift-space distortions actually a probe of growth of structure?.

Redshift space distortions in the presence of non-minimally coupled dark matter Are redshift-space distortions actually a probe of growth of structure?

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-08-14T12:29:29.512646Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 3b36b187-5297-4ae8-b7eb-ef12c0312449 · outbound

This paper cites Effective Theory of Dark Energy at Redshift Survey Scales.

Redshift space distortions in the presence of non-minimally coupled dark matter Effective Theory of Dark Energy at Redshift Survey Scales

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.007902Z

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Observation 9ae5f44a-5b61-4788-8229-7aa1d67d3c8d · outbound

This paper cites Limits of Quasi-Static Approximation in Modified-Gravity Cosmologies.

Redshift space distortions in the presence of non-minimally coupled dark matter Limits of Quasi-Static Approximation in Modified-Gravity Cosmologies

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.012675Z

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Observation c399870d-6816-4cd5-8eb1-fa4816aa34e3 · outbound

This paper cites The spatial and velocity bias of linear density peaks and proto-haloes in the Lambda cold dark matter cosmology.

Redshift space distortions in the presence of non-minimally coupled dark matter The spatial and velocity bias of linear density peaks and proto-haloes in the Lambda cold dark matter cosmology

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.017504Z

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Observation da1b4824-88e0-40b8-8476-50ae173cc33c · outbound

This paper cites Constraining higher-order parameters for primordial non-Gaussianities from power spectra and bispectra of imaging survey.

Redshift space distortions in the presence of non-minimally coupled dark matter Constraining higher-order parameters for primordial non-Gaussianities from power spectra and bispectra of imaging survey

Reference 52

Resolution: verified exact; local_arxiv, observed 2026-08-14T12:29:29.448035Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 7ca88ed3-7119-49b0-81b5-b7c2aa9fe84b · outbound

This paper cites Ratra and P.

Redshift space distortions in the presence of non-minimally coupled dark matter Ratra and P

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.025647Z

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Observation 9bce509d-b7c3-43c1-9d40-2779acf555e5 · outbound

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

Redshift space distortions in the presence of non-minimally coupled dark matter Cosmological Imprint of an Energy Component with General Equation of State

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.029476Z

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Observation fc9843bc-c305-4554-87eb-af5b65a6003e · outbound

This paper cites The Limits of Quintessence.

Redshift space distortions in the presence of non-minimally coupled dark matter The Limits of Quintessence

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.034655Z

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Observation 386d150e-e336-405b-90ea-f6e505cdadf9 · outbound

This paper cites Cosmological Tracking Solutions.

Redshift space distortions in the presence of non-minimally coupled dark matter Cosmological Tracking Solutions

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.040412Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 615614bb-cba2-4eca-915b-b758008f1400 · outbound

This paper cites Weinberg, Cosmology (Oxford University Press, Oxford New York, 2008), ISBN 978-0198526827.

Redshift space distortions in the presence of non-minimally coupled dark matter Weinberg, Cosmology (Oxford University Press, Oxford New York, 2008), ISBN 978-0198526827

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T12:29:30.073608Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 564acf98-7380-4e77-b8b3-af5b7243d793 · outbound

This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes.

Redshift space distortions in the presence of non-minimally coupled dark matter The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.049453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 69c1a017-d598-4900-8560-444458b9c1ce · outbound

This paper cites Coupled Quintessence.

Redshift space distortions in the presence of non-minimally coupled dark matter Coupled Quintessence

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.054776Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 57fc124e-5ce0-4338-aaaa-29df171584da · outbound

This paper cites Dark energy and the Boomerang data.

Redshift space distortions in the presence of non-minimally coupled dark matter Dark energy and the Boomerang data

Reference 60

Resolution: verified exact; local_arxiv, observed 2026-08-14T12:29:29.350547Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation c65b8b33-a23b-4f93-88e2-af4f4051ec3e · outbound

This paper cites Statefinder diagnostic for coupled quintessence.

Redshift space distortions in the presence of non-minimally coupled dark matter Statefinder diagnostic for coupled quintessence

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.064933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 240c5f85-87a1-4fc2-b543-835a782f89e8 · outbound

This paper cites Growing Matter.

Redshift space distortions in the presence of non-minimally coupled dark matter Growing Matter

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.069694Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 83b59cfb-39e5-41dd-a1dc-6859ff8bc5f0 · outbound

This paper cites Measuring cosmological parameters with galaxy surveys.

Redshift space distortions in the presence of non-minimally coupled dark matter Measuring cosmological parameters with galaxy surveys

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.075153Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c1e36f98-f873-4f27-be6d-f554dba5bf37 · outbound

This paper cites Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys.

Redshift space distortions in the presence of non-minimally coupled dark matter Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.079194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a53c2c6a-20a9-4831-9cad-d0a13d00b198 · outbound

This paper cites Alcock and B.

Redshift space distortions in the presence of non-minimally coupled dark matter Alcock and B

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.083805Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 54f42490-60de-4a75-a8fb-1da7088e297d · outbound

This paper cites Forecasting Cosmological Constraints from Redshift Surveys.

Redshift space distortions in the presence of non-minimally coupled dark matter Forecasting Cosmological Constraints from Redshift Surveys

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.087553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f170c30-8ee1-4872-99e2-8a34bd5dcaa3 · outbound

This paper cites Planck 2015 results. XIV. Dark energy and modified gravity.

Redshift space distortions in the presence of non-minimally coupled dark matter Planck 2015 results. XIV. Dark energy and modified gravity

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.092300Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8fe89fa5-3590-4d96-81e5-4ad092944c28 · outbound

This paper cites Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey.

Redshift space distortions in the presence of non-minimally coupled dark matter Luminosity dependence of the spatial and velocity distributions of galaxies: Semi-analytic models versus the Sloan Digital Sky Survey

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-08-14T12:29:29.242666Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 4790fbe0-214d-47dc-aeeb-42f7d8f737ee · outbound

This paper cites Late-time cosmology with 21cm intensity mapping experiments.

Redshift space distortions in the presence of non-minimally coupled dark matter Late-time cosmology with 21cm intensity mapping experiments

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.102274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7504ac77-9f0e-497c-8cbd-452c2a60de18 · outbound

This paper cites Cosmology and Fundamental Physics with the Euclid Satellite.

Redshift space distortions in the presence of non-minimally coupled dark matter Cosmology and Fundamental Physics with the Euclid Satellite

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.106838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d44d6b7d-306e-4cfd-9ec7-4d606982bfd5 · outbound

This paper cites Cosmological performance of SKA HI galaxy surveys.

Redshift space distortions in the presence of non-minimally coupled dark matter Cosmological performance of SKA HI galaxy surveys

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.111452Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 173e5484-fcd8-4f94-a90a-61b6c74d85b9 · outbound

This paper cites Stable clustering, the halo model and nonlinear cosmological power spectra.

Redshift space distortions in the presence of non-minimally coupled dark matter Stable clustering, the halo model and nonlinear cosmological power spectra

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.117200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8110d1fd-5f73-4584-a98f-1132ebbbd9aa · outbound

This paper cites Cosmology in the era of Euclid and the Square Kilometre Array.

Redshift space distortions in the presence of non-minimally coupled dark matter Cosmology in the era of Euclid and the Square Kilometre Array

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-14T12:29:29.122109Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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