Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures

Abstract

For future surveys of fast radio bursts (FRBs), we clarify information available from cosmic dispersion measures (DMs) through cross-correlation analyses of foreground dark matter haloes (hosting galaxies and galaxy clusters) with their known redshifts. With a halo-model approach, we predict that the cross-correlation with cluster-sized haloes is less affected by the details of gastrophysics, providing robust cosmological information. For less massive haloes, the cross-correlation at angular scales of $<10\mathrm{arcmin}$ is sensitive to gas expelled from the halo centre due to galactic feedback. Assuming $20000$ FRBs over $20000{\mathrm{deg}}^2$ with a localisation error being 3 arcmin, we expect that the cross-correlation signal at halo masses of $10^{12}-10^{14}{M}_{\odot }$ can be measured with a level of $\sim 1\%$ precision in a redshift range of $0<z<1$. Such precise measurements enable one to put a 1.5\% level constraint on ${\sigma }_8({\Omega }_{\mathrm{M}}/0.3{)}^{0.5}$ and a 3\% level constraint on $({\Omega }_{\mathrm{b}}/0.049)(h/0.67)(f_{\mathrm{e}}/0.95)$ (${\sigma }_8$, ${\Omega }_{\mathrm{M}}$, ${\Omega }_{\mathrm{b}}$, $h$ and $f_{\mathrm{e}}$ are the linear mass variance smoothed at $8h^{-1}\mathrm{Mpc}$, mean mass density, mean baryon density, the present-day Hubble parameter and fraction of free electrons in cosmic baryons today), whereas the gas-to-halo mass relation in galaxies and clusters can be constrained with a level of $10\%-20\%$. Furthermore the cross-correlation analyses can break the degeneracy among ${\Omega }_{\mathrm{b}}$, $h$ and $f_{\mathrm{e}}$, inherent in the DM-redshift relation. Our proposal opens new possibilities for FRB cosmology, while it requires extensive galaxy redshift catalogues and further improvement of the halo model.

arXiv comment21 pages, 9 figures, 4 tables. Accepted for publication in MNRAS

References in corpus (144)

• Planck 2015 results. XIII. Cosmological parameters
• The Structure of Cold Dark Matter Halos
• The Seventh Data Release of the Sloan Digital Sky Survey
• Efficient Computation of CMB anisotropies in closed FRW models
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Large scale bias and the peak background split
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
• Baryonic Features in the Matter Transfer Function
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• The Baryon Oscillation Spectroscopic Survey of SDSS-III
• Halo Models of Large Scale Structure
• First results from the IllustrisTNG simulations: matter and galaxy clustering
• Toward a halo mass function for precision cosmology: the limits of universality
• First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
• First results from the IllustrisTNG simulations: the galaxy color bimodality
• An analytic model for the spatial clustering of dark matter haloes
• Observational Probes of Cosmic Acceleration
• First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium
• UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10
• The Cosmic Baryon Budget
• The Circumgalactic Medium
• A New Electron Density Model for Estimation of Pulsar and FRB Distances
• First results from the IllustrisTNG simulations: radio haloes and magnetic fields
• The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures
• Where are the Baryons?
• The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests
• A Repeating Fast Radio Burst
• Dancing in the dark: galactic properties trace spin swings along the cosmic web
• The direct localization of a fast radio burst and its host
• The Connection between Galaxies and their Dark Matter Halos
• redMaPPer I: Algorithm and SDSS DR8 Catalog
• KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
• Cosmic Growth History and Expansion History
• The Fifth Data Release of the Sloan Digital Sky Survey
• The Host Galaxy and Redshift of the Repeating Fast Radio Burst FRB 121102
• Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)
• A census of baryons in the Universe from localized fast radio bursts
• The Cosmic Energy Inventory
• One percent determination of the primordial deuterium abundance
• Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
• Cosmology with cosmic shear observations: a review
• The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology
• Fast Radio Bursts: An Extragalactic Enigma
• The Expansion of the Universe is Faster than Expected
• A repeating fast radio burst source localised to a nearby spiral galaxy
• A single fast radio burst localized to a massive galaxy at cosmological distance
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty
• The Halo Occupation Distribution and the Physics of Galaxy Formation
• Weak lensing for precision cosmology
• Periodic activity from a fast radio burst source
• Towards a realistic population of simulated galaxy groups and clusters
• The CHIME Fast Radio Burst Project: System Overview
• A universal model for halo concentrations
• The Evolution of the Intergalactic Medium
• The Search for the Missing Baryons at Low Redshift
• A fast radio burst localised to a massive galaxy
• Cosmological Model Predictions for Weak Lensing: Linear and Nonlinear Regimes
• The Cosmic Baryon and Metal Cycles
• Locating the "missing" baryons with extragalactic dispersion measure estimates
• Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
• Observations of the MIssing Baryons in the warm-hot intergalactic medium
• The low density and magnetization of a massive galaxy halo exposed by a fast radio burst
• A Weak Lensing Study of X-ray Groups in the COSMOS survey: Form and Evolution of the Mass-Luminosity Relation
• Power Spectrum Super-Sample Covariance
• The Mass-Concentration-Redshift Relation of Cold Dark Matter Halos
• Cosmic Dispersion Measure from Gamma-Ray Burst Afterglows: Probing the Reionization History and the Burst Environment
• Cosmological implications of Fast Radio Burst / Gamma-Ray Burst Associations
• Evidence of Galaxy Cluster Motions with the Kinematic Sunyaev-Zel'dovich Effect
• Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology
• Lensing of Fast Radio Bursts as a Probe of Compact Dark Matter
• Probing the Cosmic Reionization History and Local Environment of Gamma-Ray Bursts through Radio Dispersion
• Host Galaxy Properties and Offset Distributions of Fast Radio Bursts: Implications for their Progenitors
• A nearby repeating fast radio burst in the direction of M81
• A new method to quantify the effects of baryons on the matter power spectrum
• The SPTpol Extended Cluster Survey
• Self-Calibration of Cluster Dark Energy Studies: Observable-Mass Distribution
• The Growth of Cool Cores and Evolution of Cooling Properties in a Sample of 83 Galaxy Clusters at 0.3 < z < 1.2 Selected from the SPT-SZ Survey
• Mapping stellar content to dark matter halos using galaxy clustering and galaxy-galaxy lensing in the SDSS DR7
• Impact of baryon physics on dark matter structures: a detailed simulation study of halo density profiles
• Simulations of Wide-Field Weak Lensing Surveys I: Basic Statistics and Non-Gaussian Effects
• An optically-selected cluster catalog at redshift 0.1<z<1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data
• Modelling baryonic feedback for survey cosmology
• The Atacama Cosmology Telescope: The Two-Season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog
• Properties of gas in and around galaxy haloes
• The host galaxies and progenitors of Fast Radio Bursts localized with the Australian Square Kilometre Array Pathfinder
• Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
• Gas Clumping in the Outskirts of Lambda-CDM Clusters
• The Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos
• Unifying X-ray Scaling Relations from Galaxies to Clusters
• FRB 121102 is coincident with a star forming region in its host galaxy
• Evidence for the kinematic Sunyaev-Zeľdovich effect with ACTPol and velocity reconstruction from BOSS
• Constraints on Hydrodynamical Subgrid Models from Quasar Absorption Line Studies of the Simulated Circumgalactic Medium
• Scaling relations for galaxy clusters: properties and evolution
• The clustering of galaxies at z~0.5 in the SDSS-III Data Release 9 BOSS-CMASS sample: a test for the LCDM cosmology
• The effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulation
• The gas fractions of dark matter haloes hosting simulated $\sim L^{\star }$ galaxies are governed by the feedback history of their black holes
• Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
• Constraints on the mass-richness relation from the abundance and weak lensing of SDSS clusters
• Properties of gas clumps and gas clumping factor in the intra cluster medium
• A Distant Fast Radio Burst Associated to its Host Galaxy with the Very Large Array
• LRP 2020 Whitepaper: The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD)
• The Stacked Thermal SZ Signal of Locally Brightest Galaxies in Planck Full Mission Data: Evidence for Galaxy Feedback?
• Baryon Cycling in the Low-Redshift Circumgalactic Medium: A Comparison of Simulations to the COS-Halos Survey
• Constraints on the missing baryons from the kinetic Sunyaev-Zeldovich effect in Planck data
• Cosmology with kSZ: breaking the optical depth degeneracy with Fast Radio Bursts
• Dissecting the Local Environment of FRB 190608 in the Spiral Arm of its Host Galaxy
• A Measurement of the Galaxy Group-Thermal Sunyaev-Zel'dovich Effect Cross-Correlation Function
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• CHIME/FRB Catalog 1 results: statistical cross-correlations with large-scale structure
• The Two-Halo Term in Stacked Thermal Sunyaev-Zel'dovich Measurements: Implications for Self-Similarity
• X-ray scaling relations of early-type galaxies
• Modeling Fast Radio Burst Dispersion and Scattering Properties in the First CHIME/FRB Catalog
• Redshift Estimation and Constraints on Intergalactic and Interstellar Media from Dispersion and Scattering of Fast Radio Bursts
• Cosmology-insensitive estimate of IGM baryon mass fraction from five localized fast radio bursts
• Radio Pulsars in the Magellanic Clouds
• The impact of stellar feedback on hot gas in galaxy haloes: the Sunyaev-Zel'dovich effect and soft X-ray emission
• Disentangling the Cosmic Web Towards FRB 190608
• Limits on precursor and afterglow radio emission from a fast radio burst in a star-forming galaxy
• Measuring the circum- and inter-galactic baryon contents with fast radio bursts
• The WiggleZ Dark Energy Survey: Final Data Release and the Metallicity of UV-Luminous Galaxies
• Sample variance in photometric redshift calibration: cosmological biases and survey requirements
• Including beyond-linear halo bias in halo models
• Fast radio bursts to be detected with the Square Kilometre Array
• Constraints on the FRB rate at 700-900 MHz
• A possible Chandra and Hubble Space Telescope detection of extragalactic WHIM towards PG 1116+215
• Statistical modelling of the cosmological dispersion measure
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• H$\alpha$ intensity map of the repeating fast radio burst FRB 121102 host galaxy from Subaru/Kyoto 3DII AO-assisted optical integral-field spectroscopy
• X-ray and SZ constraints on the properties of hot CGM
• On the Cluster Physics of Sunyaev-Zel'dovich and X-ray Surveys IV: Characterizing Density and Pressure Clumping due to Infalling Substructures
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• Large-scale clustering as a probe of the origin and the host environment of fast radio bursts
• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• Characterizing fast radio bursts through statistical cross-correlations
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• Scatter in Sunyaev--Zel'dovich effect scaling relations explained by inter-cluster variance in mass accretion histories
• Cosmology from weak lensing alone and implications for the Hubble tension
• Effect of Redshift Distributions of Fast Radio Bursts on Cosmological Constraints
• VOEvent Standard for Fast Radio Bursts
• Probing WHIM around Galaxy Clusters with Fast Radio Bursts and the Sunyaev-Zel'dovich effect
• Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
• Constraints on circum-galactic media from Sunyaev-Zel'dovich effects and X-ray data
• Revealing the Warm and Hot Halo Baryons via Thomson Scattering of Quasar Light

Cited by in corpus (4)

• The Physics of Fast Radio Bursts
• Probing the interaction between dark energy and dark matter with future fast radio burst observations
• Expanding Fireball in Magnetar Bursts and Fast Radio Bursts
• Improvement of cosmological constraints with the cross correlation between line-of-sight optical galaxy and FRB dispersion measure