Matter influence on large-scale scalar dynamics | Paper Citation Record

Observation b747fbcc-f408-40a4-af97-4d3b8fc0aacf · outbound

This paper cites At lowest order, the scalar perturbations on large scales obey the linear response theory.

Matter influence on large-scale scalar dynamics At lowest order, the scalar perturbations on large scales obey the linear response theory

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This paper cites This is useful as an illustration compared to the full complexity of the matter power spectrum deduced from the growth of cosmological perturbations.

Matter influence on large-scale scalar dynamics This is useful as an illustration compared to the full complexity of the matter power spectrum deduced from the growth of cosmological perturbations

Reference 2

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This paper cites In this context, ⃗kis just the usual comoving wavevector.

Matter influence on large-scale scalar dynamics In this context, ⃗kis just the usual comoving wavevector

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Observation b85b0d13-827f-4a4a-9dc3-f9abc4c75ea9 · outbound

This paper cites Screening takes places when the Compton wavelength of the scalar field is much shorter than the size of the local matter over-densities.

Matter influence on large-scale scalar dynamics Screening takes places when the Compton wavelength of the scalar field is much shorter than the size of the local matter over-densities

Reference 5

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Observation f562e50e-e569-4ebf-8cfd-682581d8a140 · outbound

This paper cites This implies that A(L) =− iβ mPl Z |⃗ p|≥1 L /d3p P(⃗ p, ω(p))−P(⃗ p,−ω(p)) 2ω(p) (81) which depends onL.

Matter influence on large-scale scalar dynamics This implies that A(L) =− iβ mPl Z |⃗ p|≥1 L /d3p P(⃗ p, ω(p))−P(⃗ p,−ω(p)) 2ω(p) (81) which depends onL

Reference 7

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Observation 6dd29270-f6e6-4cc2-a82d-77ff97b0c4e5 · outbound

This paper cites This can be written as Veff(¯ϕ) = 1 2 m2 ϕ(¯ϕ− ˆϕ)− 1 2 m2 ϕ ˆϕ2 (93) where ˆϕ=− βρ0 mPlm2 ϕ andm 2 ϕ =m 2 0 + β2 m2 Pl B2ρ0 is the mass squared of the cosmological field.

Matter influence on large-scale scalar dynamics This can be written as Veff(¯ϕ) = 1 2 m2 ϕ(¯ϕ− ˆϕ)− 1 2 m2 ϕ ˆϕ2 (93) where ˆϕ=− βρ0 mPlm2 ϕ andm 2 ϕ =m 2 0 + β2 m2 Pl B2ρ0 is the mass squared of the cosmological field

Reference 8

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Observation 0d18d3c5-a672-4428-875c-af5344b0c563 · outbound

This paper cites this large coupling between scalar and matter is the raison d’ˆ etre of screening and should be screened to avoid large effects of modified gravity.

Matter influence on large-scale scalar dynamics this large coupling between scalar and matter is the raison d’ˆ etre of screening and should be screened to avoid large effects of modified gravity

Reference 9

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Matter influence on large-scale scalar dynamics Unresolved cited work

Reference 10

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Observation fa6f73ac-084b-40c7-b972-bc7859956514 · outbound

This paper cites This is the screening criterion guaranteeing that all substructures are screened.

Matter influence on large-scale scalar dynamics This is the screening criterion guaranteeing that all substructures are screened

Reference 11

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Observation 38f04d9c-23ad-4384-8e61-facf61ef612a · outbound

This paper cites At this order we can then use the equivalence between Gaussian noises ξ(x)≡ β mPl B1(¯ϕ(t))j>(x) (121) relating the noise to the short distance random source.

Matter influence on large-scale scalar dynamics At this order we can then use the equivalence between Gaussian noises ξ(x)≡ β mPl B1(¯ϕ(t))j>(x) (121) relating the noise to the short distance random source

Reference 12

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Observation 33a1dc06-3333-4679-af0d-b6e8998958c7 · outbound

This paper cites In (110) the noise contribution is potentially larger than the source coming from the large scale fluctuationsδj < contrary to the unscreened case.

Matter influence on large-scale scalar dynamics In (110) the noise contribution is potentially larger than the source coming from the large scale fluctuationsδj < contrary to the unscreened case

Reference 13

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Observation d29460b4-eb79-4d78-ab87-70fe2dbdbc4a · outbound

This paper cites Dynamics of dark energy.

Matter influence on large-scale scalar dynamics Dynamics of dark energy

Reference 14

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Observation 3762848f-d8fe-4845-b446-00499e0c0ee4 · outbound

This paper cites Beyond the Cosmological Standard Model.

Matter influence on large-scale scalar dynamics Beyond the Cosmological Standard Model

Reference 15

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Observation d049c8ee-dc84-49b7-b1c2-1c3d9f4e7353 · outbound

This paper cites Brax, Rept.

Matter influence on large-scale scalar dynamics Brax, Rept

Reference 16

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Observation ab484f32-4798-44fa-ba52-e18cbd987b05 · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Matter influence on large-scale scalar dynamics DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 17

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Observation ede164f2-6af1-4a41-bc2b-9d827b85037b · outbound

This paper cites Extended Dark Energy analysis using DESI DR2 BAO measurements.

Matter influence on large-scale scalar dynamics Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 18

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Observation 2bbfb832-e285-40f9-9b86-ef89d0423443 · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Matter influence on large-scale scalar dynamics DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 19

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Observation 7e1a4bb0-ef33-4484-81a8-66659f665463 · outbound

This paper cites Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey.

Matter influence on large-scale scalar dynamics Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey

Reference 20

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Observation c48b46d4-7222-4a34-adf6-299cee5c851b · outbound

This paper cites Coupled Quintessence.

Matter influence on large-scale scalar dynamics Coupled Quintessence

Reference 21

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This paper cites Weinberg's theorem, phantom crossing and screening.

Matter influence on large-scale scalar dynamics Weinberg's theorem, phantom crossing and screening

Reference 22

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Observation 272dc21b-f2c9-485b-baa7-2450ae9231c5 · outbound

This paper cites Bertotti, L.

Matter influence on large-scale scalar dynamics Bertotti, L

Reference 23

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This paper cites Archidiacono, E.

Matter influence on large-scale scalar dynamics Archidiacono, E

Reference 24

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Observation 55be61bd-1f4c-4bca-bfea-2e17141dd450 · outbound

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

Matter influence on large-scale scalar dynamics Update on Coupled Dark Energy and the $H_0$ tension

Reference 25

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Observation aa33d0d6-9040-4afb-acb1-9d3300b9649a · outbound

This paper cites Super-acceleration as Signature of Dark Sector Interaction.

Matter influence on large-scale scalar dynamics Super-acceleration as Signature of Dark Sector Interaction

Reference 26

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Observation 9c64d75f-2132-43f4-8134-ef4cefe4d341 · outbound

This paper cites Matching current observational constraints with nonminimally coupled dark energy.

Matter influence on large-scale scalar dynamics Matching current observational constraints with nonminimally coupled dark energy

Reference 27

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Observation 95de6968-8e21-47e8-93f3-a41c26762d1d · outbound

This paper cites Khoury, M.-X.

Matter influence on large-scale scalar dynamics Khoury, M.-X

Reference 28

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This paper cites Testing for w<-1 in the Solar System.

Matter influence on large-scale scalar dynamics Testing for w<-1 in the Solar System

Reference 29

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This paper cites Testing Screened Modified Gravity.

Matter influence on large-scale scalar dynamics Testing Screened Modified Gravity

Reference 30

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Matter influence on large-scale scalar dynamics Tests of Chameleon Gravity

Reference 31

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

Matter influence on large-scale scalar dynamics Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space

Reference 32

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Matter influence on large-scale scalar dynamics Chameleon Cosmology

Reference 33

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Observation e59e3bba-ec16-49f8-a848-db02c22868e9 · outbound

This paper cites Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration.

Matter influence on large-scale scalar dynamics Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration

Reference 34

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This paper cites The Dilaton and Modified Gravity.

Matter influence on large-scale scalar dynamics The Dilaton and Modified Gravity

Reference 35

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Observation cda17d5d-13d5-44ce-87bb-327db77eef45 · outbound

This paper cites Strongly Coupled Chameleon Fields: New Horizons in Scalar Field Theory.

Matter influence on large-scale scalar dynamics Strongly Coupled Chameleon Fields: New Horizons in Scalar Field Theory

Reference 36

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Matter influence on large-scale scalar dynamics Unresolved cited work

Reference 37

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Observation a16f90d2-f15f-4c10-9a73-7ed6056676cb · outbound

This paper cites Growth of Cosmic Structure.

Matter influence on large-scale scalar dynamics Growth of Cosmic Structure

Reference 38

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Matter influence on large-scale scalar dynamics Unresolved cited work

Reference 39

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Matter influence on large-scale scalar dynamics Unresolved cited work

Reference 40

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Observation 2b487a9a-d993-4a0f-89ac-3a3e3b234b5f · outbound

This paper cites Colas, Z.

Matter influence on large-scale scalar dynamics Colas, Z

Reference 41

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Matter influence on large-scale scalar dynamics Unresolved cited work

Reference 42

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Observation e4499e5f-0245-444d-a8ba-ea6d37022ee0 · outbound

This paper cites Screening maps of the local Universe I -- Methodology.

Matter influence on large-scale scalar dynamics Screening maps of the local Universe I -- Methodology

Reference 43

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Matter influence on large-scale scalar dynamics Unresolved cited work

Reference 44

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Observation c99e9c76-5872-4c96-b6f9-86932b06dc06 · outbound

This paper cites The halo model for cosmology: a pedagogical review.

Matter influence on large-scale scalar dynamics The halo model for cosmology: a pedagogical review

Reference 45

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Observation d1004da7-1a6b-4c13-b5a6-533e7ee64e91 · outbound

This paper cites Ansari, A.

Matter influence on large-scale scalar dynamics Ansari, A

Reference 46

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Observation a9a8c6f1-735b-472d-b578-bc75b09f50ef · outbound

This paper cites Direct signatures of the formation time of galaxies.

Matter influence on large-scale scalar dynamics Direct signatures of the formation time of galaxies

Reference 47

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Observation 1e4b4554-33fa-4c14-83fb-181c43ecd9b9 · outbound

This paper cites Nonlinear Gravitational Radiation Reaction: Failed Tail, Memories & Squares.

Matter influence on large-scale scalar dynamics Nonlinear Gravitational Radiation Reaction: Failed Tail, Memories & Squares

Reference 48

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Observation e917f904-bcc6-4d71-aeba-a656256f94be · outbound

This paper cites Tail effects of self-interacting scalar fields.

Matter influence on large-scale scalar dynamics Tail effects of self-interacting scalar fields

Reference 49

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Observation eb296316-d5f3-4ddf-b0e3-e5b84c725005 · outbound

This paper cites Gauging Open EFTs from the top down.

Matter influence on large-scale scalar dynamics Gauging Open EFTs from the top down

Reference 50

Resolution: verified exact; local_arxiv, observed 2026-07-01T20:16:10.971794Z

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Observation 7b3f91d6-81c6-4ffb-9208-597ed1276988 · outbound

This paper cites Schwinger-Keldysh Path Integral for Gauge theories.

Matter influence on large-scale scalar dynamics Schwinger-Keldysh Path Integral for Gauge theories

Reference 51

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Observation fc2ad9b0-595a-400c-9c1d-ac62ff73e4c5 · outbound

This paper cites Stochastic inflation from a non-equilibrium renormalization group.

Matter influence on large-scale scalar dynamics Stochastic inflation from a non-equilibrium renormalization group

Reference 52

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Observation cc75e184-fd8b-4fa5-8446-eafb4d89e81c · outbound

This paper cites Gravitational-wave lensing beyond rays: a disordered-system approach.

Matter influence on large-scale scalar dynamics Gravitational-wave lensing beyond rays: a disordered-system approach

Reference 53

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Observation 691545ff-bd99-4773-9c5a-ad4acde5985c · outbound

This paper cites The In-Out Formalism for In-In Correlators.

Matter influence on large-scale scalar dynamics The In-Out Formalism for In-In Correlators

Reference 54

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Observation ea17160d-7539-4aef-b268-932b62d61ff3 · outbound

This paper cites Screened Axio-dilaton Cosmology: Novel Forms of Early Dark Energy.

Matter influence on large-scale scalar dynamics Screened Axio-dilaton Cosmology: Novel Forms of Early Dark Energy

Reference 55

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Observation 93f5efd1-ec26-4d99-b544-d3fddec7a43c · outbound

This paper cites Detecting Dark Energy in Orbit -- the Cosmological Chameleon.

Matter influence on large-scale scalar dynamics Detecting Dark Energy in Orbit -- the Cosmological Chameleon

Reference 56

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This paper cites Kittel,Introduction to Solid State Physics(Wiley, 2004).

Matter influence on large-scale scalar dynamics Kittel,Introduction to Solid State Physics(Wiley, 2004)

Reference 57

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