Power Spectra for Cold Dark Matter and its Variants

Abstract

The bulk of recent cosmological research has focused on the adiabatic cold dark matter model and its simple extensions. Here we present an accurate fitting formula that describes the matter transfer functions of all common variants, including mixed dark matter models. The result is a function of wavenumber, time, and six cosmological parameters: the massive neutrino density, number of neutrino species degenerate in mass, baryon density, Hubble constant, cosmological constant, and spatial curvature. We show how observational constraints---e.g. the shape of the power spectrum, the abundance of clusters and damped Lyman-alpha systems, and the properties of the Lyman-alpha forest--- can be extended to a wide range of cosmologies, including variations in the neutrino and baryon fractions in both high-density and low-density universes.

20 pages, LaTeX, 4 figures. Submitted to ApJ. Electronic versions of the fitting formula, as well as simple codes to output cosmological quantities (e.g. sigma_8) as a function of parameters and illustrative animations of parameter dependence, are available at http://www.sns.ias.edu/~whu/transfer/transfer.html

References in corpus (14)

• Baryonic Features in the Matter Transfer Function
• Recovery of the Power Spectrum of Mass Fluctuations from Observations of the Lyman-alpha Forest
• Microwave Background Constraints on Cosmological Parameters
• The Intracluster Gas Fraction in X-ray Clusters : Constraints on the Clustered Mass Density
• A Lower Bound on the Cosmic Baryon Density
• Redshift Evolution of Galaxy Cluster Densities
• Physical Properties of the Lyman Alpha Forest in a Cold Dark Matter Cosmology
• Small Scale Perturbations in a General MDM Cosmology
• Determining the Amplitude of Mass Fluctuations in the Universe
• Testing Cosmological Models Against the Abundance of Damped Lyman-Alpha Absorbers
• Probing the universe with the Lyman-alpha forest: II. The column density distribution
• Evolution of Small Scale Cosmological Baryon Perturbations and Matter Transfer Functions
• Cosmological Constraints from High-Redshift Damped Lyman-Alpha Systems
• Tensor Anisotropies in an Open Universe

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• Painting halos from cosmic density fields of dark matter with physically motivated neural networks
• Constraints on Light WIMP candidates from the Isotropic Diffuse Gamma-Ray Emission
• ASOHF: a new adaptive spherical overdensity halo finder
• Population III Star Formation in a Lambda WDM Universe
• Separating out the Alcock-Paczynski Effect on 21cm Fluctuations
• Accelerating Large-Scale-Structure data analyses by emulating Boltzmann solvers and Lagrangian Perturbation Theory
• Integrated Sachs-Wolfe Effect for Gravitational Radiation
• Fingerprinting Dark Energy II: weak lensing and galaxy clustering tests
• Angular correlations in the cosmic gamma-ray background from dark matter annihilation around intermediate-mass black holes
• Polarization as an indicator of intrinsic alignment in radio weak lensing
• The Emergence of the First Star-free Atomic Cooling Haloes in the Universe
• Measuring AGN Feedback with the Sunyaev-Zel'dovich Effect
• Clustering of X-Ray-Selected AGN
• Galaxy cluster mergers
• CosmicNet II: Emulating extended cosmologies with efficient and accurate neural networks
• Fingerprinting Dark Energy III: distinctive marks of viscosity
• Acoustic peaks and dips in the CMB power spectrum: observational data and cosmological constraints
• A Statistical Analysis of Intergalactic Medium Transmission Approaching Reionization
• Cosmological Constraints from the Large Scale Weak Lensing of SDSS MaxBCG Clusters
• Non-Gaussianity in Large Scale Structure and Minkowski Functionals
• Strong gravitational lensing and galactic bulges
• Thermal constraints on the reionisation of hydrogen by population-II stellar sources
• Testing the accuracy of the Hydro-PM approximation in numerical simulations of the Lyman-alpha forest
• Inferring high redshift large-scale structure dynamics from the Lyman-alpha forest
• Cosmological Simulations of the Preheating Scenario for Galaxy Cluster Formation: Comparison to Analytic Models and Observations
• Using Weak Lensing to find Halo Masses
• Did Massive Primordial Stars Preenrich the Lyman Alpha Forest?
• Forming supermassive black holes by accreting dark and baryon matter
• Cosmology with Superluminous Supernovae
• Early structure formation from primordial density fluctuations with a blue-tilted power spectrum
• The Impact of Wrong Assumptions in BAO Reconstruction
• A cosmological view of extreme mass-ratio inspirals in nuclear star clusters
• Fully-Coupled Simulation of Cosmic Reionization. I: Numerical Methods and Tests
• Impacts of the physical data model on the forward inference of initial conditions from biased tracers
• A closer look at CMB constraints on WIMP dark matter
• Matrix-free Large Scale Bayesian inference in cosmology
• Quintessential $\alpha$-attractor inflation: forecasts for Stage IV galaxy surveys
• Information Gains from Cosmological Probes
• Adaptive mesh refinement simulations of a galaxy cluster merger - I. Resolving and modelling the turbulent flow in the cluster outskirts
• Cosmology with clusters of galaxies
• Comparisons of Cosmological MHD Galaxy Cluster Simulations to Radio Observations
• Convergence of Galaxy Properties with Merger Tree Temporal Resolution
• Measuring large-scale structure with quasars in narrow-band filter surveys
• The Minimum Halo Mass for Star Formation at z = 6 - 8
• Reionization and the large-scale 21 cm-cosmic microwave background cross correlation
• Non-Gravitational Contributions to the Clustering of Ly-alpha Selected Galaxies: Implications for Cosmological Surveys
• Statistical uncertainties and systematic errors in weak lensing mass estimates of galaxy clusters
• Power Spectrum of Cosmic Momentum Field Measured from the SFI Galaxy Sample
• Distribution of the very first PopIII stars and their relation to bright z~6 quasars
• Neutrino Halos in Clusters of Galaxies and their Weak Lensing Signature
• Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum
• Gravitational Lensing by a Compound Population of Halos: Standard Models
• Feedback from Clustered Sources During Reionization
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• Constraints on the Inner Cluster Mass Profile and the Power Spectrum Normalization from Strong Lensing Statistics
• Surveys of Galaxy Clusters with the Sunyaev Zel'dovich Effect
• Light gravitino dark matter: LHC searches and Hubble tension
• The Most Massive Black Holes in the Universe: Effects of Mergers in Massive Galaxy Clusters
• Constraints on massive vector dark energy models from integrated Sachs-Wolfe-galaxy cross-correlations
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• Radio Point Sources and the Thermal SZ Power Spectrum
• Weak Lensing by Line-of-sight Halos as the Origin of Flux-ratio Anomalies in Quadruply Lensed QSOs
• Multi-messenger constraints on the annihilating dark matter interpretation of the positron excess
• Composition of Low Redshift Halo Gas
• Strong gravitational lensing: why no central black holes?
• Constraints on black hole duty cycles and the black hole-halo relation from SDSS quasar clustering
• Cosmological shock waves: clues to the formation history of haloes
• Exploring Large-scale Structure with Billions of Galaxies
• A Snapshot Survey for Gravitational Lenses Among z>=4.0 Quasars: II. Constraints on the 4.0<z<4.5 Quasar Population
• Weak lensing and dark energy: the impact of dark energy on nonlinear dark matter clustering
• Non-Gaussianity in the Weak Lensing Correlation Function Likelihood -- Implications for Cosmological Parameter Biases
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• What Can the Distribution of Intergalactic Metals Tell us About the History of Cosmological Enrichment?
• The evolution of the Lyman-alpha forest effective optical depth following HeII reionisation
• History of Hydrogen Reionization in the Cold Dark Matter Model
• The Cosmological Constant Problem, an Inspiration for New Physics
• Neural physical engines for inferring the halo mass distribution function
• Probing the Curious Case of a Galaxy Cluster Merger in Abell 115 with High Fidelity Chandra X-ray Temperature and Radio Maps
• The locations of halo formation and the peaks formalism
• Turbulence driven by structure formation in the circum-galactic medium
• MHD Turbulence and Cosmic Ray Reacceleration in Galaxy Clusters
• Going Nonlinear with Dark Energy Cosmologies
• Flux-limited strong gravitational lensing and dark energy
• Understanding the PSCz Galaxy Power Spectrum with N-body Simulations
• Dark energy effects on the Lyman-alpha forest
• Constraints on Cosmological Parameters from the Lyman-alpha Forest Power Spectrum and COBE-DMR
• Measuring Unified Dark Matter with 3D Cosmic Shear
• An optimal survey geometry of weak lensing survey: minimizing super-sample covariance
• DM haloes in the fifth-force cosmology
• A roadmap to cosmological parameter analysis with third-order shear statistics I: Modelling and validation
• PT challenge: Validation of ShapeFit on large-volume, high-resolution mocks
• Measuring Coherent Motions in the Universe
• Primordial Non-Gaussianity Estimation using 21 cm Tomography from the Epoch of Reionization
• Cluster Mergers and the Origin of the ARCADE-2 Excess
• Oscillating nonlinear large scale structure in growing neutrino quintessence
• Joint modeling of the probability distribution and power spectrum of the Lya forest: comparison with observations at z=3
• Anthropic predictions for vacuum energy and neutrino masses
• Constraints on Inflation
• Tests of Neutrino and Dark Radiation Models from Galaxy and CMB surveys
• Effects of Velocity-Dependent Dark Matter Annihilation on the Energy Spectrum of the Extragalactic Gamma-ray Background
• Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
• Gravitational Lensing by Dark Matter Halos with Non-universal Density Profiles
• Probing the Cosmic X-ray and MeV Gamma-ray Background Radiation through the Anisotropy
• Will Multiple Probes of Dark Energy find Modified Gravity?
• syren-halofit: A fast, interpretable, high-precision formula for the $\Lambda$CDM nonlinear matter power spectrum
• A Systematic Search for Galaxy Proto-Cluster Cores at $z\sim 2$
• A new model for the full shape of the large-scale power spectrum
• Explicit Bayesian treatment of unknown foreground contaminations in galaxy surveys
• The median density of the Universe
• The statistics of voids as a tool to constrain cosmological parameters: sigma_8 and Omega_m h
• Redshift requirements for cosmic shear with intrinsic alignment
• Weak lensing: Dark Matter, Dark Energy and Dark Gravity
• Radiative Feedback in Relic HII Regions at High-Redshift
• Smallest Remnants of Early Matter Domination
• Can decaying particle explain cosmic infrared background excess?
• Constraints on Primordial Power Spectrum from Galaxy Luminosity Functions
• A hierarchical field-level inference approach to reconstruction from sparse Lyman-$\alpha$ forest data
• The Effect of Large-Scale Power on Simulated Spectra of the Lya forest
• A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• Building robust AGN mock catalogs to unveil black hole evolution and for survey planning
• How Much Can We Learn From A Merging Cold Front Cluster? : Insights From X-ray Temperature and Radio Maps of Abell 3667
• Dark sectors of the Universe: A Euclid survey approach
• Dark-matter halo mergers as a fertile environment for low-mass Population III star formation
• Imprints of deviations from the gravitational inverse-square law on the power spectrum of mass fluctuations
• Can We Detect the Anisotropic Shapes of Quasar HII Regions During Reionization Through The Small-Scale Redshifted 21cm Power Spectrum?
• The power spectrum of the CfA/SSRS UZC galaxy redshift survey
• Integrated Sachs-Wolfe-galaxy cross-correlation bounds on the two branches of the minimal theory of massive gravity
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Intermittent Features of the QSO Ly$\alpha$ Transmitted Flux: Results from Hydrodynamic Cosmological Simulations
• A precise symbolic emulator of the linear matter power spectrum
• Diffuse gamma-ray background and cosmic-ray positrons from annihilating dark matter
• Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
• Estimating the weak-lensing rotation signal in radio cosmic shear surveys
• Growth index of matter perturbations in the light of Dark Energy Survey
• Weak Lensing of the CMB: Power Spectrum Covariance
• Color Tomography
• The dominant origin of diffuse Ly$\alpha$ halos around LAEs explored by SED fitting and clustering analysis
• Probing the large scale structure using gravitational-wave observations of binary black holes
• Structure and Turbulence in Simulated Galaxy Clusters and the Implications for the Formation of Radio Halos
• Impacts of biasing schemes in the one-loop integrated perturbation theory
• Nonlinear Evolution of Anisotropic Cosmological Power
• The scale-dependent signature of primordial non-Gaussianity in the large-scale structure of cosmic reionization
• Impact of magnetic fields on Population III star formation
• Cluster Lensing of QSOs as a Probe of LCDM and Dark Energy Cosmologies
• Halo models of HI selected galaxies
• Measuring weak lensing correlations of Type Ia Supernovae
• The First Compact Objects in the $\Lambda$-dominated Universe
• Detecting the Baryons in Matter Power Spectra
• On The Road To More Realistic Galaxy Cluster Simulations: The Effects of Radiative Cooling and Thermal Feedback Prescriptions on the Observational Properties of Simulated Galaxy Clusters
• The Santa Fe Light Cone Simulation Project: II. The Prospects for Direct Detection of the WHIM with SZE Surveys
• Cosmological parameter forecasts by a joint 2D tomographic approach to CMB and galaxy clustering
• Extremely-Metal Poor Stars in the Milky Way: A Second Generation Formed after Reionization
• Weak Lensing by Intergalactic Mini-Structures in Quadruple Lens Systems: Simulation and Detection
• The Complementarity of Redshift-space Distortions and the Integrated Sachs-Wolfe Effect: A 3D Spherical Analysis
• Infrared Properties of z=7 Galaxies from Cosmological Simulations
• Data Compression and Inference in Cosmology with Self-Supervised Machine Learning
• Time-Varying Dark Energy Constraints From the Latest SN Ia, BAO and SGL
• Cosmological Simulations of Isotropic Conduction in Galaxy Clusters
• Modification of the 21-cm power spectrum by X-rays during the epoch of reionisation
• Constraining fast radio burst progenitors with gravitational lensing
• Triggering the Formation of Halo Globular Clusters with Galaxy Outflows
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• Bayesian power-spectrum inference with foreground and target contamination treatment
• Comparison of observing modes for statistical estimation of the 21cm signal from the Epoch of Reionisation
• Breaking Cosmological Degeneracies in Galaxy Cluster Surveys with a Physical Model of Cluster Structure
• The nonlinear evolution of baryonic overdensities in the early universe: Initial conditions of numerical simulations
• Beyond the growth rate of cosmic structure: Testing modified gravity models with an extra degree of freedom
• Evolution of dark matter velocity dispersion
• Cosmologically probing ultra-light particle dark matter using 21 cm signals
• Predictions of Quasar Clustering: Redshift, Luminosity and Selection Dependence
• Validating the Fisher approach for stage IV spectroscopic surveys
• Effects of neutrino mass and asymmetry on cosmological structure formation
• Halo statistics in non-Gaussian cosmologies: the collapsed fraction, conditional mass function, and halo bias from the path-integral excursion set method
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• Stacking weak lensing signals of SZ clusters to constrain cluster physics
• A Simple Analytic Treatment of Linear Growth of Structure with Baryon Acoustic Oscillations
• Modification of the 21-cm power spectrum by quasars during the epoch of reionisation
• On Mitigation of the Uncertainty in Nonlinear Matter Clustering for Cosmic Shear Tomography
• Neutrino footprint in Large Scale Structure
• Cosmological parameters from complementary observations of the Universe
• syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Role of the Hubble Scale in the Weak Lensing vs. CMB Tension
• Constraining f(R) gravity with cross-correlation of galaxies and cosmic microwave background lensing
• Decaying warm dark matter and structure formation
• A Halo Occupation Interpretation Of Quasars At $z\sim 1.5$ Using Very Small Scale Clustering Information
• Using machine learning to compress the matter transfer function $T(k)$
• Describing variations of the Fisher-matrix across parameter space
• The effects of primordial non-Gaussianity on giant-arc statistics
• Field-Based Physical Inference From Peculiar Velocity Tracers
• Anisotropy in the matter distribution beyond the baryonic acoustic oscillation scale
• Cross-correlating the Thermal Sunyaev-Zel'dovich Effect and the Distribution of Galaxy Clusters
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• A group-galaxy cross-correlation function analysis in zCOSMOS
• The Lyman-alpha forest at redshifts 0.1 -- 1.6: good agreement between a large hydrodynamic simulation and HST spectra
• Perfectly parallel cosmological simulations using spatial comoving Lagrangian acceleration
• The Statistical Discrepancy between the IGM and Dark Matter Fields: One-Point Statistics
• Suppressing variance in 21-cm signal simulations during reionization
• The Anisotropy of the Extragalactic Radio Background from Dark Matter Annihilation
• Euclid preparation. Modelling spectroscopic clustering on mildly nonlinear scales in beyond-$\Lambda$CDM models
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• Little Red Dots as Direct-collapse Black Hole Nurseries
• Suppression of Dwarf Galaxy Formation by Cosmic Shocks
• Constraining the neutrino mass using a multi-tracer combination of two galaxy surveys and CMB lensing
• The XMM-Newton Wide Field Survey in the COSMOS Field: Clustering Dependence of X-ray Selected AGN on Host Galaxy Properties
• Far-Infrared Properties of Lyman Break Galaxies from Cosmological Simulations
• Clustering of CODEX clusters
• Effects of P-wave Annihilation on the Angular Power Spectrum of Extragalactic Gamma-rays from Dark Matter Annihilation
• Probing reionization using quasar near-zones at redshift z ~ 6
• Noise Estimates for Measurements of Weak Lensing from the Lyman-alpha Forest
• Nonsingular density profiles of dark matter halos and Strong gravitational lensing
• Feedback Processes in Early-Type Galaxies
• The Properties of X-ray Cold Fronts in a Statistical Sample of Simulated Galaxy Clusters
• Detecting baryon acoustic oscillations by 3d weak lensing
• LimberJack.jl: auto-differentiable methods for angular power spectra analyses
• Quintessential early dark energy
• Using large scale structure data and a halo model to constrain Generalised Dark Matter
• Combining Weak Lensing Tomography with Halo Clustering to Probe Dark Energy
• Extragalactic and galactic gamma-rays and neutrinos from annihilating dark matter
• Note on the Robustness of the Neutrino Mass Bounds from Cosmology
• Connecting the Dots: Tracking Galaxy Evolution Using Constant Cumulative Number Density at 3<z<7
• Weighing neutrinos using high redshift galaxy luminosity functions
• The biasing phenomenon
• Dark-energy dependent test of general relativity at cosmological scales
• Testing the scale-dependent hemispherical asymmetry with the 21-cm power spectrum from the epoch of reionization
• Testing a Phenomenologically Extended DGP Model with Upcoming Weak Lensing Surveys
• Light Dark Matter: A Common Solution to the Lithium and $H_0$ Problems
• Improving precision and accuracy in cosmology with model-independent spectrum and bispectrum
• Abundance matching for low mass galaxies in the CDM and FDM models
• Cosmological implications of tracker scalar fields: Testing the evidence for dynamical dark energy with recent data
• An Introduction into the Theory of Cosmological Structure Formation
• Constraining Neutrino mass using the large scale HI distribution in the Post-reionization epoch
• Prospects of probing quintessence with HI 21-cm intensity mapping survey
• Uncertainties in the S-Z selected cluster angular power spectrum
• High-redshift microlensing and the spatial distribution of dark matter in the form of MACHOs
• The Impact of Secondary non-Gaussianities in the CMB on Cosmological Parameter Estimation
• Manufacturing cosmic rays in the evolving dynamical states of galaxy clusters
• Too hot to handle? Analytic solutions for massive neutrino or warm dark matter cosmologies
• The CMB neutrino mass / vacuum energy degeneracy: a simple derivation of the degeneracy slopes
• Anisotropic Halo Model
• Probing Neutrinos from Planck and Forthcoming Galaxy Redshift Surveys
• First and second order cosmological perturbations in light mass Galileon models
• Machine learning unveils the linear matter power spectrum of modified gravity
• Skewness as a probe of Baryon Acoustic Oscillations
• Constraints on structure formation models from Sunyaev-Zel'dovich Effect
• Flavon Magneto-Baryogenesis
• An Eulerian Perturbation Approach to Large Scale Structures: Extending the Adhesion Approximation
• Radio-relic and the diffuse emission trail discovered in a low mass galaxy cluster Abell 1697
• Constraining Dark Energy From Splitting Angle Statistic of Strong Gravitational Lenses
• The extragalactic $\gamma$-ray background: imprints from the physical properties and evolution of star-forming galaxy populations
• Prospects for Observing High-redshift Radio-loud Quasars in the SKA Era: Paving the Way for 21-cm Forest Observations
• Predictions for the Counts of Faint, High-Redshift Galaxies in the Mid-Infrared
• Cross-Correlation Studies with CMB Polarization Maps
• Statistical features of 21-cm emission from the epoch between reionization and Gunn-Peterson transparency
• Optimising tomography for weak gravitational lensing surveys
• Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies
• Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos
• Turbulence-induced deviation between baryonic field and dark matter field in the spatial distribution of the Universe
• Gravitational corrections to light propagation in a perturbed FLRW-universe and corresponding weak lensing spectra
• Endowing $\mathbf{\Lambda }$ with a dynamic nature: constraints in a spatially curved Universe
• The Effect of Interplanetary Scintillation on Epoch of Reionisation Power Spectra
• Field-level multiprobe analysis of the CMB, integrated Sachs-Wolfe effect, and the galaxy density maps
• Simulated Predictions for HI at $z=3.35$ with the Ooty Wide Field Array (OWFA) -- II: Foreground Avoidance
• Condition for dust evacuation from the first galaxies
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Evidence for Non-Linear Growth of Structure from an X-ray Selected Cluster Survey using a Novel Joint Analysis of the Chandra and XMM-Newton Archives
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• Probing the large-scale structure of the universe through gravitational-wave observations
• On the $2^{\text{nd}}$ feature of the matter two-point function
• Revisiting coupled CDM-massive neutrino perturbations in diverse cosmological backgrounds
• Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• High-Significance Detection of Correlation Between the Unresolved Gamma-Ray Background and the Large Scale Cosmic Structure
• Differentiable Cosmological Hydrodynamics for Field-Level Inference and High Dimensional Parameter Constraints
• Efficient implementation of the Time Renormalization Group
• Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
• Strong Lensing Probabilities in a Cosmological Model with a Running Primordial Power Spectrum
• Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models
• Complexity Phenomena and ROMA of the Magnetospheric Cusp, Hydrodynamic Turbulence, and the Cosmic Web
• Hybrid summary statistics: neural weak lensing inference beyond the power spectrum
• Systematic error due to isotropic inhomogeneities
• Weak lensing forecasts for dark energy, neutrinos and initial conditions
• Peaks in the cosmological density field: parameter constraints from 2dF Galaxy Redshift Survey data
• Neutrino Masses, Dark Energy and the Gravitational Lensing of Pregalactic HI
• Extending evolution mapping to massive neutrinos with COMET
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Interpretable and physics-informed emulator for the linear matter power spectrum from machine learning
• Neutrinos in Astrophysics and Cosmology: Theoretical Advanced Study Institute (TASI) 2020 Lectures
• Bayesian inference methodology for Primordial Power Spectrum reconstructions from Large Scale Structure
• Mean maps for cosmic web structures in cosmological initial conditions
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• Neutrino physics from future weak lensing surveys
• Global 21 cm signal: a promising probe of primordial features
• Towards a multi-tracer neutrino mass measurement with line-intensity mapping
• The linear bias of radio galaxies at z~0.3 via cosmic microwave background lensing
• Models for the Clustering of Far-Infrared and Sub-millimetre selected Galaxies
• An Order Statistics Approach to the Halo Model for Galaxies
• The Reionization History in the Lognormal Model
• Combined $13\times 2$-point analysis of the Cosmic Microwave Background and Large-Scale Structure: implications for the $S_8$-tension and neutrino mass constraints
• Dark halo densities, substructure, and the initial power spectrum
• Weighing Neutrinos with Large-Scale Structure
• Cosmological parameters from observational data on the large scale structure of the Universe
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Toward a Measurement of the Transverse Peculiar Velocity of Galaxy Pairs
• Particle production during inflation: constraints expected from redshifted 21 cm observations from the epoch of reionization
• Merging Rates of the First Objects and the Formation of First Mini-Filaments in Models with Massive Neutrinos
• Massive neutrinos and interacting dark matter look alike through the lens of lensing
• Empirical formulae to describe some physical properties of small groups of protogalaxies with multiplicity
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• A new gravitational N-body simulation algorithm for investigation of cosmological chaotic advection
• Redshift Drift fluctuations from N-body simulations
• The Diversity of Core Halo Structure in the Fuzzy Dark Matter Model
• The gravitational wave background induced by nonlinear interactions between isotropic inhomogeneities and anisotropic inhomogeneous density perturbations
• Numerical approaches to star formation and SuperNovae energy feedback in simulations of galaxy clusters
• Cosmology with the Roman Space Telescope -- Synergies with CMB lensing
• Constraining Quintessence Models with ISW-tSZ Cross-Correlations: A Comparative Analysis of Thawing, Tracker, and Scaling-Freezing Dynamics
• Slow neutrinos: non-linearity and momentum-space emulation
• Baryon Acoustic Oscillations in tomographic Angular Density and Redshift Fluctuations
• Redshift effects implications on revised models of Stephan's quintet
• Massive Neutrinos Promote the Size Growth of Early-Type Galaxies
• The Mass Function of Dark Matter Haloes in a Cosmological Model with a Running Primordial Power Spectrum