Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation | Paper Citation Record

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation G” (Gaussian), “SF

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This paper cites Baumann,Cosmology(Cambridge University Press, 2022).

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Baumann,Cosmology(Cambridge University Press, 2022)

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This paper cites First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters

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This paper cites Cosmological parameters from SDSS and WMAP.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Cosmological parameters from SDSS and WMAP

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

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Planck 2018 results. VI. Cosmological parameters

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This paper cites Sato, Mon.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Sato, Mon

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This paper cites Albrecht and P.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Albrecht and P

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This paper cites Results from the Wilkinson Microwave Anisotropy Probe.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Results from the Wilkinson Microwave Anisotropy Probe

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Observation 5beb8f1c-12ff-4788-9f74-67d4b9330baf · outbound

This paper cites Non-Gaussianity from Inflation: Theory and Observations.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Non-Gaussianity from Inflation: Theory and Observations

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Observation 702dfcad-9d67-4784-a005-030c25b6e3b8 · outbound

This paper cites Primordial Non-Gaussianities from Inflation Models.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Primordial Non-Gaussianities from Inflation Models

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Observation 732294eb-b461-46de-8e57-6a7e51da9b60 · outbound

This paper cites Primordial non-Gaussianity from the large scale structure.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Primordial non-Gaussianity from the large scale structure

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Observation 86b2f47f-2317-4a71-9e35-e34ae479e7b3 · outbound

This paper cites Hunting for Primordial Non-Gaussianity in the Cosmic Microwave Background.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Hunting for Primordial Non-Gaussianity in the Cosmic Microwave Background

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This paper cites Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Abdurashidovaet al.(HERA), Astrophys

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This paper cites An Effective Bias Expansion for 21 cm Cosmology in Redshift Space.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation An Effective Bias Expansion for 21 cm Cosmology in Redshift Space

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Observation 5076cf1b-ef43-40f8-a345-c6fba6b962d6 · outbound

This paper cites Bayesian field-level inference of primordial non-Gaussianity using next-generation galaxy surveys.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Bayesian field-level inference of primordial non-Gaussianity using next-generation galaxy surveys

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This paper cites How much information can be extracted from galaxy clustering at the field level?.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation How much information can be extracted from galaxy clustering at the field level?

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This paper cites Andrewset al., arXiv e-Prints (2026), arXiv:2603.20855 [astro-ph.CO].

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Andrewset al., arXiv e-Prints (2026), arXiv:2603.20855 [astro-ph.CO]

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Naturally inflating on steep potentials through electromagnetic dissipation

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Gauge Fields and Inflation

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation A review of Axion Inflation in the era of Planck

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Lattice Simulations of Axion-U(1) Inflation

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation The strong backreaction regime in axion inflation

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Lattice simulations of axion-U(1) inflation: gravitational waves, magnetic fields, and scalar statistics

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Schwinger effect in axion inflation on a lattice

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Jamieson, A

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Quijote-PNG: Simulations of primordial non-Gaussianity and the information content of the matter field power spectrum and bispectrum

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Adiabatic Modes in Cosmology

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Large Nongaussianity in Axion Inflation

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Non-Gaussianities and chiral gravitational waves in natural steep inflation

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Gauge-field production during axion inflation in the gradient expansion formalism

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Instability in axion inflation with strong backreaction from gauge modes

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Barbon, N

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Accurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errors

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Simulating cosmic structure formation with the GADGET-4 code

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Superconformal Inflationary $\alpha$-Attractors

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Planck 2018 results. IX. Constraints on primordial non-Gaussianity

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation The Non-Gaussian Halo Mass Function with fNL, gNL and tauNL

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Toward a halo mass function for precision cosmology: the limits of universality

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Lucchin and S

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation The abundance of high-redshift objects as a probe of non-Gaussian initial conditions

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Unresolved cited work

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation A population of red candidate massive galaxies ~600 Myr after the Big Bang

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Stress Testing $\Lambda$CDM with High-redshift Galaxy Candidates

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Observation 533eeee4-b73f-4a66-bf12-7d3fdf8a9aa3 · outbound

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Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings

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This paper cites Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys

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This paper cites UNCOVER spectroscopy confirms a surprising ubiquity of AGN in red galaxies at $z>5$.

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation UNCOVER spectroscopy confirms a surprising ubiquity of AGN in red galaxies at $z>5$

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