From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology | Paper Citation Record

Observation 5370be5f-4635-457f-9265-d71d58b64087 · outbound

This paper cites The corresponding electromagnetic and thermodynamic scalings are described in Refs.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology The corresponding electromagnetic and thermodynamic scalings are described in Refs

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Unresolved cited work

Reference 2

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Unresolved cited work

Reference 3

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This paper cites Restoration is obtained by inverting Eq.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Restoration is obtained by inverting Eq

Reference 4

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Unresolved cited work

Reference 5

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Unresolved cited work

Reference 6

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Observation 381bb72a-c899-453f-9f0e-b4e32698d2ca · outbound

This paper cites denote intrinsic coordinates on the shell hypersurface Σ, whereas hatted indices ˆa,ˆb,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology denote intrinsic coordinates on the shell hypersurface Σ, whereas hatted indices ˆa,ˆb,

Reference 7

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This paper cites On the ordinary branch ϵ+ = ϵ− = +1 and in the static limit ˙R = 0, it reduces directly to Eq.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology On the ordinary branch ϵ+ = ϵ− = +1 and in the static limit ˙R = 0, it reduces directly to Eq

Reference 8

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Unresolved cited work

Reference 9

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Unresolved cited work

Reference 10

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Unresolved cited work

Reference 11

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This paper cites The spatial geometry and extrinsic curvature must satisfy the Hamiltonian and momentum constraints.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology The spatial geometry and extrinsic curvature must satisfy the Hamiltonian and momentum constraints

Reference 12

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This paper cites The conformal geometry, extrinsic curvature, and matter sources must approach together the values induced by the homogeneous Space II-A FLRW exterior.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology The conformal geometry, extrinsic curvature, and matter sources must approach together the values induced by the homogeneous Space II-A FLRW exterior

Reference 13

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Unresolved cited work

Reference 14

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Observation 945ea03b-9dd4-48a9-ad9f-d1485e8b88d5 · outbound

This paper cites In particular, ∆ ME integrates the Eulerian energy contrast with the proper-volume element of the chosen ADM slice.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology In particular, ∆ ME integrates the Eulerian energy contrast with the proper-volume element of the chosen ADM slice

Reference 15

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Observation 23a2c94c-2505-43dd-8cfc-84d594cafb90 · outbound

This paper cites A prescribed positive compensated matter-source family supplies the Eulerian energy and momentum sources together with the rest-frame energy density and pressure.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology A prescribed positive compensated matter-source family supplies the Eulerian energy and momentum sources together with the rest-frame energy density and pressure

Reference 16

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Observation e78ba3c8-c6c3-474c-8cbb-e2e74753a5bc · outbound

This paper cites Singular hypersurfaces and thin shells in general relativity,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Singular hypersurfaces and thin shells in general relativity,

Reference 17

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This paper cites The influence of the expansion of space on the gravitation fields surrounding the individual stars,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology The influence of the expansion of space on the gravitation fields surrounding the individual stars,

Reference 18

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Observation 8d318c9c-4a56-4d77-9aa4-659a1f4db35c · outbound

This paper cites Influence of global cosmological expansion on local dynamics and kinematics.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Influence of global cosmological expansion on local dynamics and kinematics

Reference 19

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This paper cites Generalized Swiss-Cheese Cosmologies II: Spherical Dust.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Generalized Swiss-Cheese Cosmologies II: Spherical Dust

Reference 20

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This paper cites Kinematics and Dynamics of General Relativity,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Kinematics and Dynamics of General Relativity,

Reference 21

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Observation 749bbeb3-093d-4553-b950-36e206a81b56 · outbound

This paper cites Initial Data in General Relativity Described by Expansion, Conformal Deformation and Drift.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Initial Data in General Relativity Described by Expansion, Conformal Deformation and Drift

Reference 22

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Observation 279f8235-0bad-4dd2-94ff-941ca9f108f9 · outbound

This paper cites Killing vector fields and a homogeneous isotropic universe.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Killing vector fields and a homogeneous isotropic universe

Reference 23

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Observation 0cd52d10-5cae-4fcf-b113-44013bbf23cb · outbound

This paper cites An Introduction to mathematical cosmology,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology An Introduction to mathematical cosmology,

Reference 24

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Unresolved cited work

Reference 25

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This paper cites Revisiting varying speed of light in cosmology: Insights from the Friedmann-Lemaˆ ıtre-Robertson-Walker Metric,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Revisiting varying speed of light in cosmology: Insights from the Friedmann-Lemaˆ ıtre-Robertson-Walker Metric,

Reference 26

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This paper cites Geometric Matching of Local Static Regions in Cosmological Spacetimes with an Evolving Lapse.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Geometric Matching of Local Static Regions in Cosmological Spacetimes with an Evolving Lapse

Reference 27

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Observation a369391b-6216-4f84-9fa8-b21482f2dfd6 · outbound

This paper cites Constraint on the minimally extended varying speed of light using time dilations in type Ia supernovae.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Constraint on the minimally extended varying speed of light using time dilations in type Ia supernovae

Reference 28

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Observation b3834603-c46e-481d-b387-ad2ca602b12b · outbound

This paper cites The significance of measuring cosmological time dilation in the Dark Energy Survey Supernova Program,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology The significance of measuring cosmological time dilation in the Dark Energy Survey Supernova Program,

Reference 29

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Observation 7f2f263b-18c8-4ed9-bf94-35937d7d7c4b · outbound

This paper cites A unified interpretation of supernova, GRB, and QSO time dilation signals in a generalized cosmological time framework,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology A unified interpretation of supernova, GRB, and QSO time dilation signals in a generalized cosmological time framework,

Reference 30

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Observation 09f26a82-9f6c-45a8-8b3c-efbc0ab459e0 · outbound

This paper cites To the problem of nonvanishing gravitation mass,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology To the problem of nonvanishing gravitation mass,

Reference 31

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Observation 5a25b2f9-c4ca-4310-a8e0-66f3e1f1b36d · outbound

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

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space

Reference 32

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From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Chameleon Cosmology

Reference 33

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This paper cites Dynamical effects of the cosmological constant,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Dynamical effects of the cosmological constant,

Reference 34

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Observation fe607ef9-8ddf-4e3b-9f6f-3cb3bbdaca8c · outbound

This paper cites Spherical collapse model with and without curvature.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Spherical collapse model with and without curvature

Reference 35

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Observation 048ed73e-ab3a-47f6-a17b-83e9839a7f0a · outbound

This paper cites Spherical collapse model with non-clustering dark energy.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Spherical collapse model with non-clustering dark energy

Reference 36

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Observation c9bbd877-0e86-4284-9772-0382ba0a65ce · outbound

This paper cites Singular hypersurfaces and thin shells in cosmology,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Singular hypersurfaces and thin shells in cosmology,

Reference 37

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Observation b6e88cdc-2c2e-4f16-8ff8-ef91581a5c93 · outbound

This paper cites The minimally extended Varying Speed of Light (meVSL).

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology The minimally extended Varying Speed of Light (meVSL)

Reference 38

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This paper cites A viable varying speed of light model in the RW metric.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology A viable varying speed of light model in the RW metric

Reference 39

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This paper cites The cosmological evolution condition of the Planck constant in the varying speed of light models through adiabatic expansion,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology The cosmological evolution condition of the Planck constant in the varying speed of light models through adiabatic expansion,

Reference 40

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This paper cites 3+1 formalism of the minimally extended varying speed of light model.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology 3+1 formalism of the minimally extended varying speed of light model

Reference 41

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This paper cites Classical Mechanics.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Classical Mechanics

Reference 42

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Observation cd445449-66f3-40a0-be79-535a1f0ca1b1 · outbound

This paper cites The Large Scale Structure of Space-Time,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology The Large Scale Structure of Space-Time,

Reference 43

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Observation 27a05991-036b-42ec-b9e0-a5ce04d17831 · outbound

This paper cites Relativistic equations for adiabatic, spherically symmetric gravitational collapse,.

From a Sharp Thin-Shell Obstruction to a Smooth Positive-Density Initial-Data Embedding of a Virialized Halo in Lambda-FLRW Cosmology Relativistic equations for adiabatic, spherically symmetric gravitational collapse,

Reference 44

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