Generating Moving Field Initial Conditions with Spatially Varying Boost | Paper Citation Record

Observation 89455c81-1403-48ac-88c4-bf84b7c2fb1d · outbound

This paper cites Efstathiou, M.

Generating Moving Field Initial Conditions with Spatially Varying Boost Efstathiou, M

Reference 1

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Observation 76a50842-5627-4335-8966-60376076d360 · outbound

This paper cites Matarrese, O.

Generating Moving Field Initial Conditions with Spatially Varying Boost Matarrese, O

Reference 2

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Observation b08d065c-3ad4-4831-9130-52cf59b1c938 · outbound

This paper cites Transients from Initial Conditions: A Perturbative Analysis.

Generating Moving Field Initial Conditions with Spatially Varying Boost Transients from Initial Conditions: A Perturbative Analysis

Reference 3

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Observation 4a52662e-9e3e-4bbc-a543-408875db6aa1 · outbound

This paper cites Valageas, Transients from zel’dovich initial condi- 6 tions, Astron.

Generating Moving Field Initial Conditions with Spatially Varying Boost Valageas, Transients from zel’dovich initial condi- 6 tions, Astron

Reference 4

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Observation aa43dc36-f61f-44a0-88e5-fe905d1205db · outbound

This paper cites The Evolution of Baryon Density Fluctuations in Multi-Component Cosmological Simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost The Evolution of Baryon Density Fluctuations in Multi-Component Cosmological Simulations

Reference 5

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Observation c51c221b-e7d0-4b45-8f39-1cbfc2337323 · outbound

This paper cites Initial conditions to cosmological N-body simulations, or how to run an ensemble of simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Initial conditions to cosmological N-body simulations, or how to run an ensemble of simulations

Reference 6

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Observation a63bba47-fa7b-4336-82f9-f1d42cc11b05 · outbound

This paper cites Transients from Initial Conditions in Cosmological Simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Transients from Initial Conditions in Cosmological Simulations

Reference 7

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Observation 474dd850-6299-4bf8-9ae4-56d76f3996de · outbound

This paper cites Transients from initial conditions based on Lagrangian perturbation theory in N-body simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Transients from initial conditions based on Lagrangian perturbation theory in N-body simulations

Reference 8

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Observation 9298dabe-6ac1-41dd-89d2-c48926dc2ef8 · outbound

This paper cites Multi-scale initial conditions for cosmological simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Multi-scale initial conditions for cosmological simulations

Reference 9

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Observation 70209456-e032-4925-bf01-7614cb63081c · outbound

This paper cites Effects of the initial conditions on cosmological $N$-body simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Effects of the initial conditions on cosmological $N$-body simulations

Reference 10

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Observation bcbe6a04-c563-46c9-ada6-94f415efd354 · outbound

This paper cites The Properties of Cosmic Velocity Fields.

Generating Moving Field Initial Conditions with Spatially Varying Boost The Properties of Cosmic Velocity Fields

Reference 11

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Observation 379c8f80-a736-4c4c-a450-59cef85f4b32 · outbound

This paper cites General relativistic corrections to $N$-body simulations and the Zel'dovich approximation.

Generating Moving Field Initial Conditions with Spatially Varying Boost General relativistic corrections to $N$-body simulations and the Zel'dovich approximation

Reference 12

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Observation c0123e83-6b48-4faa-ae21-0c8398ef0fe9 · outbound

This paper cites General relativity and cosmic structure formation.

Generating Moving Field Initial Conditions with Spatially Varying Boost General relativity and cosmic structure formation

Reference 13

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Observation 73d0248e-b01e-4786-b692-508d09bf2dac · outbound

This paper cites gevolution: a cosmological N-body code based on General Relativity.

Generating Moving Field Initial Conditions with Spatially Varying Boost gevolution: a cosmological N-body code based on General Relativity

Reference 14

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Observation a1b68a3d-dbca-4e44-8cd4-1821afbf8af2 · outbound

This paper cites Initial Conditions for Accurate N-Body Simulations of Massive Neutrino Cosmologies.

Generating Moving Field Initial Conditions with Spatially Varying Boost Initial Conditions for Accurate N-Body Simulations of Massive Neutrino Cosmologies

Reference 15

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Observation 80ca7004-b04b-442d-8b22-eb90f5bbb77a · outbound

This paper cites Improving Initial Conditions for Cosmological $N$-Body Simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Improving Initial Conditions for Cosmological $N$-Body Simulations

Reference 16

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Observation 56cbc56d-4804-48f3-b00b-902faeae387f · outbound

This paper cites Transients from Initial Conditions Based on Lagrangian Perturbation Theory in $N$-body Simulations III: The Case of GADGET-2 Code.

Generating Moving Field Initial Conditions with Spatially Varying Boost Transients from Initial Conditions Based on Lagrangian Perturbation Theory in $N$-body Simulations III: The Case of GADGET-2 Code

Reference 17

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Observation 7900d628-fcf7-499c-adb1-ea3dcba69702 · outbound

This paper cites Simulating cosmic structure formation with the GADGET-4 code.

Generating Moving Field Initial Conditions with Spatially Varying Boost Simulating cosmic structure formation with the GADGET-4 code

Reference 18

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Observation a304066b-4c99-4257-b82a-506c56a2570c · outbound

This paper cites Higher-order initial conditions for mixed baryon-CDM simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Higher-order initial conditions for mixed baryon-CDM simulations

Reference 19

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Observation b3e2ce0e-cadb-4fd6-9f94-af0a2d6a9d12 · outbound

This paper cites Accurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errors.

Generating Moving Field Initial Conditions with Spatially Varying Boost Accurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errors

Reference 20

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Observation 3eb37db5-d210-42ee-8c01-c1e29913f436 · outbound

This paper cites GRAMSES: a new route to general relativistic $N$-body simulations in cosmology. Part II. Initial conditions.

Generating Moving Field Initial Conditions with Spatially Varying Boost GRAMSES: a new route to general relativistic $N$-body simulations in cosmology. Part II. Initial conditions

Reference 21

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Observation a1eb5721-4524-496e-a943-88aab0989d8a · outbound

This paper cites Large-scale dark matter simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Large-scale dark matter simulations

Reference 22

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Observation cc3ba4cf-b9a3-4c54-991f-aca6694b3b2e · outbound

This paper cites Starting Cosmological Simulations from the Big Bang.

Generating Moving Field Initial Conditions with Spatially Varying Boost Starting Cosmological Simulations from the Big Bang

Reference 23

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Observation ce98b985-27ba-40af-ae4f-4e21dbfb8ae4 · outbound

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Generating Moving Field Initial Conditions with Spatially Varying Boost Unresolved cited work

Reference 24

Resolution: verified exact; raw_fallback, observed 2026-08-06T22:01:33.334335Z

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Observation b2e2e4fc-906f-4284-b5d8-54f4e590e70b · outbound

This paper cites 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal.

Generating Moving Field Initial Conditions with Spatially Varying Boost 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal

Reference 25

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Observation 5e0e086f-1664-413d-8755-4521c7cf09a1 · outbound

This paper cites Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe.

Generating Moving Field Initial Conditions with Spatially Varying Boost Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe

Reference 26

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Observation 235f7b17-a8e0-48a5-a02d-eafb7b9c6d84 · outbound

This paper cites ARTIST: Fast radiative transfer for large-scale simulations of the epoch of reionisation.

Generating Moving Field Initial Conditions with Spatially Varying Boost ARTIST: Fast radiative transfer for large-scale simulations of the epoch of reionisation

Reference 27

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:33.247064Z

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Observation 0aa70351-fa59-4d8a-a526-c1b3dba9e724 · outbound

This paper cites Probing the thermal history during reionization using a semi-numerical photon-conserving code SCRIPT.

Generating Moving Field Initial Conditions with Spatially Varying Boost Probing the thermal history during reionization using a semi-numerical photon-conserving code SCRIPT

Reference 28

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Observation 008e1151-352e-4fac-ae50-cc0ffb107365 · outbound

This paper cites AMBER: A Semi-numerical Abundance Matching Box for the Epoch of Reionization.

Generating Moving Field Initial Conditions with Spatially Varying Boost AMBER: A Semi-numerical Abundance Matching Box for the Epoch of Reionization

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:31.984045Z

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Observation 7c91a5db-b852-4773-897a-01a7307420a1 · outbound

This paper cites Patchy Kinetic Sunyaev-Zel'dovich Effect with Controlled Reionization History and Morphology.

Generating Moving Field Initial Conditions with Spatially Varying Boost Patchy Kinetic Sunyaev-Zel'dovich Effect with Controlled Reionization History and Morphology

Reference 30

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Observation 75940d02-afac-4934-a503-2d909c17e433 · outbound

This paper cites Modeling Cosmic Reionization.

Generating Moving Field Initial Conditions with Spatially Varying Boost Modeling Cosmic Reionization

Reference 31

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Observation d9546c06-321d-45da-9e86-94449cb85deb · outbound

This paper cites Sugiyama, KINK - ANTIKINK COLLISIONS IN THE TWO-DIMENSIONAL PHI**4 MODEL, Prog.

Generating Moving Field Initial Conditions with Spatially Varying Boost Sugiyama, KINK - ANTIKINK COLLISIONS IN THE TWO-DIMENSIONAL PHI**4 MODEL, Prog

Reference 32

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Observation 1b245e5e-8c88-48c1-a92d-ace3d29d242c · outbound

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Generating Moving Field Initial Conditions with Spatially Varying Boost Unresolved cited work

Reference 33

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Observation 8269fbe1-0de0-4306-9f58-5d1c333e2d59 · outbound

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Generating Moving Field Initial Conditions with Spatially Varying Boost Unresolved cited work

Reference 34

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Observation 9db1e30c-4405-4d90-9395-44e8b8d5ccc4 · outbound

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Generating Moving Field Initial Conditions with Spatially Varying Boost Unresolved cited work

Reference 35

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Observation a77ba8f1-5e3f-4f21-be37-0d3ac164227a · outbound

This paper cites Vachaspati, Kinks and Domain Walls : An Introduc- tion to Classical and Quantum Solitons(Oxford Univer- sity Press, 2007).

Generating Moving Field Initial Conditions with Spatially Varying Boost Vachaspati, Kinks and Domain Walls : An Introduc- tion to Classical and Quantum Solitons(Oxford Univer- sity Press, 2007)

Reference 36

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Observation a9e5ebf7-ff04-4ae9-88a6-75eeeea74f5c · outbound

This paper cites Achucarro and R.

Generating Moving Field Initial Conditions with Spatially Varying Boost Achucarro and R

Reference 37

Resolution: verified exact; raw_fallback, observed 2026-08-06T22:01:33.198588Z

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Observation 25b890b5-733a-44cd-810c-639e9b1006b7 · outbound

This paper cites Kink-antikink collisions in the phi^6 model.

Generating Moving Field Initial Conditions with Spatially Varying Boost Kink-antikink collisions in the phi^6 model

Reference 38

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Observation beee806d-9ad7-40de-b9f2-3ea13e29cd68 · outbound

This paper cites Kink interactions in the (1+1)-dimensional $\varphi^6$ model.

Generating Moving Field Initial Conditions with Spatially Varying Boost Kink interactions in the (1+1)-dimensional $\varphi^6$ model

Reference 39

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:33.113591Z

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Observation 5bd1bbcf-2d2a-41e8-8810-e50883c4fc72 · outbound

This paper cites Ultra-relativistic oscillon collisions.

Generating Moving Field Initial Conditions with Spatially Varying Boost Ultra-relativistic oscillon collisions

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:33.101620Z

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Observation e8c02e67-16b9-44f7-8f5c-af8a72064d48 · outbound

This paper cites A Clash of Kinks: Phase shifts in colliding non-integrable solitons.

Generating Moving Field Initial Conditions with Spatially Varying Boost A Clash of Kinks: Phase shifts in colliding non-integrable solitons

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:33.090527Z

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Observation 13be1b1d-b6d9-4c4f-9afa-9f9bd647a5d4 · outbound

This paper cites A scattering theory of ultrarelativistic solitons.

Generating Moving Field Initial Conditions with Spatially Varying Boost A scattering theory of ultrarelativistic solitons

Reference 42

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:33.078652Z

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Observation 1c43e2d4-4ff6-4550-b878-8b473c92d5fd · outbound

This paper cites Relativistic head-on collisions of $U(1)$ gauged Q-balls.

Generating Moving Field Initial Conditions with Spatially Varying Boost Relativistic head-on collisions of $U(1)$ gauged Q-balls

Reference 43

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:33.065492Z

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Observation 9b18c014-20ab-440d-9070-9a3805daa0b6 · outbound

This paper cites Dynamics of $U(1)$ gauged Q-balls in three spatial dimensions.

Generating Moving Field Initial Conditions with Spatially Varying Boost Dynamics of $U(1)$ gauged Q-balls in three spatial dimensions

Reference 44

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:33.052783Z

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Observation 372933fa-bb8d-4164-9d9d-5bb4a64f4c55 · outbound

This paper cites Universal Flow in the First fm/c at RHIC.

Generating Moving Field Initial Conditions with Spatially Varying Boost Universal Flow in the First fm/c at RHIC

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:33.040403Z

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Observation 89051cc0-ef3f-4f13-8831-bd8a9d22d530 · outbound

This paper cites Fluctuating Glasma initial conditions and flow in heavy ion collisions.

Generating Moving Field Initial Conditions with Spatially Varying Boost Fluctuating Glasma initial conditions and flow in heavy ion collisions

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.043336Z

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Observation c0c03b66-c6e8-416b-aaa2-ac68f1ac32d5 · outbound

This paper cites Hydrodynamic Modeling of Heavy-Ion Collisions.

Generating Moving Field Initial Conditions with Spatially Varying Boost Hydrodynamic Modeling of Heavy-Ion Collisions

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.046838Z

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Observation 3c849c53-5376-4525-8ce0-b13b079dbc8a · outbound

This paper cites Collective flow and viscosity in relativistic heavy-ion collisions.

Generating Moving Field Initial Conditions with Spatially Varying Boost Collective flow and viscosity in relativistic heavy-ion collisions

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.051131Z

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Observation 152d54cd-3d88-4d48-a56f-ebc9b002e312 · outbound

This paper cites Alternative ansatz to wounded nucleon and binary collision scaling in high-energy nuclear collisions.

Generating Moving Field Initial Conditions with Spatially Varying Boost Alternative ansatz to wounded nucleon and binary collision scaling in high-energy nuclear collisions

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.055793Z

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Observation 86294650-c4d3-410a-a6ff-3493ac88734f · outbound

This paper cites The energy-momentum tensor at the earliest stage of relativistic heavy ion collisions.

Generating Moving Field Initial Conditions with Spatially Varying Boost The energy-momentum tensor at the earliest stage of relativistic heavy ion collisions

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.059995Z

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Observation e35a2538-b2f5-49a8-aa82-f9b373569db3 · outbound

This paper cites A method of generating initial conditions for cosmological N body simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost A method of generating initial conditions for cosmological N body simulations

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:32.982081Z

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Observation 0acc2bd7-d3a7-4471-a49e-d686089d2ad3 · outbound

This paper cites an unresolved cited work.

Generating Moving Field Initial Conditions with Spatially Varying Boost Unresolved cited work

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.067501Z

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Observation 1b48e4e6-65d2-490b-86f0-ba112dff567a · outbound

This paper cites Madelung, Quantentheorie in hydrodynamischer Form, Z.

Generating Moving Field Initial Conditions with Spatially Varying Boost Madelung, Quantentheorie in hydrodynamischer Form, Z

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.070147Z

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Observation 2db76ced-3312-4552-b99a-39986b3577b1 · outbound

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Generating Moving Field Initial Conditions with Spatially Varying Boost Unresolved cited work

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.073251Z

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Observation 466ea3da-b076-4d2d-9947-65c655fede52 · outbound

This paper cites Formation and structure of ultralight bosonic dark matter halos.

Generating Moving Field Initial Conditions with Spatially Varying Boost Formation and structure of ultralight bosonic dark matter halos

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.076042Z

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Observation 432c4667-a825-455a-bb71-53d8b6e951c3 · outbound

This paper cites The art of simulating the early Universe -- Part I.

Generating Moving Field Initial Conditions with Spatially Varying Boost The art of simulating the early Universe -- Part I

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.078791Z

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Observation 8d6741a7-134a-4fa7-961a-6ea73bd40a10 · outbound

This paper cites The halo mass function and filaments in full cosmological simulations with fuzzy dark matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost The halo mass function and filaments in full cosmological simulations with fuzzy dark matter

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.081821Z

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Observation 252a3cb0-fe3b-4f13-8058-d20ebb21f341 · outbound

This paper cites Free Streaming in Warm Wave Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Free Streaming in Warm Wave Dark Matter

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.085054Z

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Observation eac4562d-b7af-4045-8371-4802cda315c8 · outbound

This paper cites Barone, F.

Generating Moving Field Initial Conditions with Spatially Varying Boost Barone, F

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.088797Z

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Unavailable: canonical work link unavailable.

Observation 96dfaa3f-b4ef-4b03-aead-04424fed89d3 · outbound

This paper cites an unresolved cited work.

Generating Moving Field Initial Conditions with Spatially Varying Boost Unresolved cited work

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.091667Z

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Observation 440e41ca-af45-4d8b-8c52-9ce2152dd652 · outbound

This paper cites Mandelstam, Soliton Operators for the Quantized Sine-Gordon Equation, Phys.

Generating Moving Field Initial Conditions with Spatially Varying Boost Mandelstam, Soliton Operators for the Quantized Sine-Gordon Equation, Phys

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Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.094899Z

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Observation 01d5ecec-f94f-4635-9af7-5644076eb983 · outbound

This paper cites an unresolved cited work.

Generating Moving Field Initial Conditions with Spatially Varying Boost Unresolved cited work

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.097853Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7dd87c1b-1509-4962-ba97-3f06a6fb0d69 · outbound

This paper cites an unresolved cited work.

Generating Moving Field Initial Conditions with Spatially Varying Boost Unresolved cited work

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.100826Z

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Observation 9c5d927d-374c-4f0b-8741-de85492d284b · outbound

This paper cites Gravitational Wave Emission from Collisions of Compact Scalar Solitons.

Generating Moving Field Initial Conditions with Spatially Varying Boost Gravitational Wave Emission from Collisions of Compact Scalar Solitons

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.103757Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82f77680-33e2-4d15-9186-b1c0eccf5d01 · outbound

This paper cites Collisions of Dark Matter Axion Stars with Astrophysical Sources.

Generating Moving Field Initial Conditions with Spatially Varying Boost Collisions of Dark Matter Axion Stars with Astrophysical Sources

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.106904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 76622f55-3ae9-441f-84da-ab00af3786ae · outbound

This paper cites Black hole formation in relativistic Oscillaton collisions.

Generating Moving Field Initial Conditions with Spatially Varying Boost Black hole formation in relativistic Oscillaton collisions

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.110224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f0d120d2-624d-4fd1-b56e-6b98d5d517ef · outbound

This paper cites Formation, Gravitational Clustering and Interactions of Non-relativistic Solitons in an Expanding Universe.

Generating Moving Field Initial Conditions with Spatially Varying Boost Formation, Gravitational Clustering and Interactions of Non-relativistic Solitons in an Expanding Universe

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.113639Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb1cd3be-27ca-4b34-a2b1-211c62dc7a6e · outbound

This paper cites Vector Dark Matter from Inflationary Fluctuations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Vector Dark Matter from Inflationary Fluctuations

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.117390Z

Source-reported events for the cited work

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Observation 0ad49dd1-ebe7-4768-acb1-b36c2e2a4384 · outbound

This paper cites Ahmed, B.

Generating Moving Field Initial Conditions with Spatially Varying Boost Ahmed, B

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.120634Z

Source-reported events for the cited work

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Observation b5907ec8-1231-4fa3-bb87-9031756993ae · outbound

This paper cites Production of Purely Gravitational Dark Matter: The Case of Fermion and Vector Boson.

Generating Moving Field Initial Conditions with Spatially Varying Boost Production of Purely Gravitational Dark Matter: The Case of Fermion and Vector Boson

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.123317Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1521d8b2-facf-4381-8327-4ec4548b1670 · outbound

This paper cites Gravitational production of vector dark matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Gravitational production of vector dark matter

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.126832Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd5ad475-fa50-47ec-9ff4-226c0ddfe712 · outbound

This paper cites Completely Dark Photons from Gravitational Particle Production During Inflation.

Generating Moving Field Initial Conditions with Spatially Varying Boost Completely Dark Photons from Gravitational Particle Production During Inflation

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.130008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 89cd6237-8732-43f2-bf53-5611280c2e63 · outbound

This paper cites Strongly self-interacting vector dark matter via freeze-in.

Generating Moving Field Initial Conditions with Spatially Varying Boost Strongly self-interacting vector dark matter via freeze-in

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.133457Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 96959f86-e03a-4904-8625-eed8613ecae8 · outbound

This paper cites Feebly coupled vector boson dark matter in effective theory.

Generating Moving Field Initial Conditions with Spatially Varying Boost Feebly coupled vector boson dark matter in effective theory

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:32.771406Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 177c8df9-eb08-410b-aaa8-24f13619c7e2 · outbound

This paper cites Non-minimally Coupled Vector Boson Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Non-minimally Coupled Vector Boson Dark Matter

Reference 75

Resolution: verified exact; local_arxiv, observed 2026-08-06T22:01:32.758479Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c5f08178-30b1-4bd3-8130-56516ee7aab0 · outbound

This paper cites Opening up the QCD axion window.

Generating Moving Field Initial Conditions with Spatially Varying Boost Opening up the QCD axion window

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.143734Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ded2d70b-c712-477c-ae88-b280988c4a2f · outbound

This paper cites Relic Abundance of Dark Photon Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Relic Abundance of Dark Photon Dark Matter

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.146899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c3634c4-ebd3-43bb-840b-f13c577ff31d · outbound

This paper cites Parametric Resonance Production of Ultralight Vector Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Parametric Resonance Production of Ultralight Vector Dark Matter

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.149881Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b4d66e4a-66c2-4ec0-95c9-6e5655ebf34c · outbound

This paper cites Dark Photon Dark Matter Produced by Axion Oscillations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Dark Photon Dark Matter Produced by Axion Oscillations

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.153213Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dd2fd8ad-051e-4d6a-a1c5-65a825219141 · outbound

This paper cites Vector dark matter production at the end of inflation.

Generating Moving Field Initial Conditions with Spatially Varying Boost Vector dark matter production at the end of inflation

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.156187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f1ab9c89-f834-44e4-8f87-7765876a9f76 · outbound

This paper cites Vector dark matter production from inflation with symmetry breaking.

Generating Moving Field Initial Conditions with Spatially Varying Boost Vector dark matter production from inflation with symmetry breaking

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.159070Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b855cc5c-cd3e-4a04-beaf-3364319d9483 · outbound

This paper cites Dark Light, Dark Matter and the Misalignment Mechanism.

Generating Moving Field Initial Conditions with Spatially Varying Boost Dark Light, Dark Matter and the Misalignment Mechanism

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.162079Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 333a9c9e-634f-4dd5-b3d8-5a4aa6b22029 · outbound

This paper cites WISPy Cold Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost WISPy Cold Dark Matter

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.165289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f1840cd-e107-446c-bfb1-2734d353d627 · outbound

This paper cites Vector Coherent Oscillation Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Vector Coherent Oscillation Dark Matter

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.168284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b3089e05-f45e-4559-8e28-7bcad6dc3969 · outbound

This paper cites Viable Vector Coherent Oscillation Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Viable Vector Coherent Oscillation Dark Matter

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.171382Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9524a682-8307-4313-b92b-c945f187b419 · outbound

This paper cites Ultralight scalars as cosmological dark matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Ultralight scalars as cosmological dark matter

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.174161Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f5c70531-98a3-4e6c-b984-ede3e7828b7b · outbound

This paper cites Cold and Fuzzy Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Cold and Fuzzy Dark Matter

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.177535Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1892b484-4986-4db7-8911-18433246e1f0 · outbound

This paper cites Ultra-Light Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Ultra-Light Dark Matter

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.180797Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 276a9b3e-3f86-42ee-b78b-084c8b5b6630 · outbound

This paper cites Wave Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Wave Dark Matter

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.183880Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9792234-80c0-425e-94e4-3280540af7ab · outbound

This paper cites Beyond Schr\"{o}dinger-Poisson: Nonrelativistic Effective Field Theory for Scalar Dark Matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Beyond Schr\"{o}dinger-Poisson: Nonrelativistic Effective Field Theory for Scalar Dark Matter

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.187077Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 36113286-dc22-444e-813d-4c0a5d95b785 · outbound

This paper cites Effective theories for a nonrelativistic field in an expanding universe: Induced self-interaction, pressure, sound speed, and viscosity.

Generating Moving Field Initial Conditions with Spatially Varying Boost Effective theories for a nonrelativistic field in an expanding universe: Induced self-interaction, pressure, sound speed, and viscosity

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.190354Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 116eccb7-0900-48af-8447-263aef079310 · outbound

This paper cites Relativistic Corrections to Nonrelativistic Effective Field Theories.

Generating Moving Field Initial Conditions with Spatially Varying Boost Relativistic Corrections to Nonrelativistic Effective Field Theories

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.193677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 93656e6b-4c5c-413e-91f7-b6b3a8e6145f · outbound

This paper cites Classical Nonrelativistic Effective Field Theories for a Real Scalar Field.

Generating Moving Field Initial Conditions with Spatially Varying Boost Classical Nonrelativistic Effective Field Theories for a Real Scalar Field

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.197589Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 208b1fc1-bba2-43f1-8d66-0589b83daf2e · outbound

This paper cites Cosmic Structure as the Quantum Interference of a Coherent Dark Wave.

Generating Moving Field Initial Conditions with Spatially Varying Boost Cosmic Structure as the Quantum Interference of a Coherent Dark Wave

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.200717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 33be314e-502c-4e97-ad59-377ab77cbe43 · outbound

This paper cites Understanding the Core-Halo Relation of Quantum Wave Dark Matter, $\psi$DM, from 3D Simulations.

Generating Moving Field Initial Conditions with Spatially Varying Boost Understanding the Core-Halo Relation of Quantum Wave Dark Matter, $\psi$DM, from 3D Simulations

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.204434Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d32fc90b-1029-47fc-863d-64d89e60fbee · outbound

This paper cites Cosmological particle-in-cell simulations with ultralight axion dark matter.

Generating Moving Field Initial Conditions with Spatially Varying Boost Cosmological particle-in-cell simulations with ultralight axion dark matter

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.207715Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ab143f9-7bb6-48ff-a4ae-e1ee6ba681a7 · outbound

This paper cites PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics.

Generating Moving Field Initial Conditions with Spatially Varying Boost PyUltraLight: A Pseudo-Spectral Solver for Ultralight Dark Matter Dynamics

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.210846Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f86a6e39-0e29-4cd0-8775-bdf3229e30de · outbound

This paper cites Numerical and Perturbative Computations of the Fuzzy Dark Matter Model.

Generating Moving Field Initial Conditions with Spatially Varying Boost Numerical and Perturbative Computations of the Fuzzy Dark Matter Model

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.214194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4aa93828-d757-4e46-904f-0d67a37bd39b · outbound

This paper cites Galactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation.

Generating Moving Field Initial Conditions with Spatially Varying Boost Galactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.217839Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6eccff8-2c60-462f-b2f4-d4d0a9b2b724 · outbound

This paper cites Oscillations and Random Walk of the Soliton Core in a Fuzzy Dark Matter Halo.

Generating Moving Field Initial Conditions with Spatially Varying Boost Oscillations and Random Walk of the Soliton Core in a Fuzzy Dark Matter Halo

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-06T22:01:32.220921Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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