FRB cosmology with the RM-PRS Luminosity Correlation

Abstract

Fast Radio Bursts (FRBs) have emerged as a powerful tool for cosmological studies, particularly through the dispersion measure-redshift ($\mathrm{DM}-z$) relation. This work proposes a novel calibration method for FRBs using the Yang-Li-Zhang (YLZ) empirical relation, which links the rotation measure (RM) of FRBs to the luminosity of their associated persistent radio sources (PRS). We demonstrate that this approach provides independent constraints on cosmological parameters, bypassing limitations inherent to traditional $\mathrm{DM}-z$ method. Utilizing the current sample of four YLZ-calibrated FRBs, we derive a Hubble constant measurement of $H_0=86.18_{-14.99}^{+18.03}\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$ (68\% CL). Monte Carlo simulations indicate that a future catalog of 400 FRB-PSR systems could reduce the relative uncertainty of $H_0$ to 4.5\%. Combining YLZ-calibrated FRBs with $\mathrm{DM}-z$ sample reveals critical synergies: joint analysis of equalized samples ($N=100$ for both methods) reduces the relative uncertainty of $H_0$ to 2.9\%, mainly because the incorporation of PRS observations substantially mitigates the degeneracy between the parameters such as IGM baryon mass fraction ($f_{\mathrm{IGM}}$) and other cosmological parameters inherent to the $\mathrm{DM}-z$ relation.

8 pages, 5 figures;

References in corpus (46)

• A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
• A bright millisecond radio burst of extragalactic origin
• The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
• A New Electron Density Model for Estimation of Pulsar and FRB Distances
• First results from the IllustrisTNG simulations: radio haloes and magnetic fields
• A Population of Fast Radio Bursts at Cosmological Distances
• The direct localization of a fast radio burst and its host
• The Host Galaxy and Redshift of the Repeating Fast Radio Burst FRB 121102
• A census of baryons in the Universe from localized fast radio bursts
• Fast Radio Burst Discovered in the Arecibo Pulsar ALFA Survey
• An extreme magneto-ionic environment associated with the fast radio burst source FRB 121102
• Fast Radio Bursts: An Extragalactic Enigma
• The Repeating Fast Radio Burst FRB 121102 as Seen on Milliarcsecond Angular Scales
• Millisecond Magnetar Birth Connects FRB 121102 to Superluminous Supernovae and Long Duration Gamma-ray Bursts
• Locating the "missing" baryons with extragalactic dispersion measure estimates
• A repeating fast radio burst associated with a persistent radio source
• Five new Fast Radio Bursts from the HTRU high latitude survey: first evidence for two-component bursts
• Cosmological implications of Fast Radio Burst / Gamma-Ray Burst Associations
• A Burst in a Wind Bubble and the Impact on Baryonic Ejecta: High-Energy Gamma-Ray Flashes and Afterglows from Fast Radio Bursts and Pulsar-Driven Supernova Remnants
• The Physics of Fast Radio Bursts
• A concordance picture of FRB 121102 as a flaring magnetar embedded in a magnetized ion-electron wind nebula
• A fast radio burst source at a complex magnetised site in a barred galaxy
• Fast radio bursts as a cosmic probe?
• The Physics of Fast Radio Bursts
• Fast Radio Burst/Gamma-Ray Burst Cosmography
• A measurement of Hubble's Constant using Fast Radio Bursts
• Magnetic field reversal in the turbulent environment around a repeating fast radio burst
• Probing the Intergalactic Medium with Fast Radio Bursts
• An 8\% Determination of the Hubble Constant from localized Fast Radio Bursts
• Future Cosmological Constraints from Fast Radio Bursts
• Intergalactic medium dispersion measures of fast radio bursts estimated from IllustrisTNG simulation and their cosmological applications
• The Large Dispersion and Scattering of FRB 20190520B are Dominated by the Host Galaxy
• Radio Emission from Pulsar Wind Nebulae without Surrounding Supernova Ejecta: Application to FRB 121102
• Temporal Scattering, Depolarization, and Persistent Radio Emission from Magnetized Inhomogeneous Environments Near Repeating Fast Radio Burst Sources
• Synchrotron heating by a fast radio burst in a self-absorbed synchrotron nebula and its observational signature
• Constraining the era of helium reionization using fast radio bursts
• Exploring the epoch of hydrogen reionization using FRBs
• On the Use of Fast Radio Burst Dispersion Measures as Distance Measures
• The FRB20190520B Sightline Intersects Foreground Galaxy Clusters
• Are persistent emission luminosity and rotation measure of fast radio bursts related?
• Deep Synoptic Array science: Two fast radio burst sources in massive galaxy clusters
• Measuring Hubble constant using localized and unlocalized fast radio bursts
• Discovery of a PRS associated with FRB 20240114A
• Probing Cosmology with 92 Localized Fast Radio Bursts and DESI BAO
• Fast Radio Bursts as probes of the late-time universe: a new insight on the Hubble tension
• Cosmological Parameter Estimate from Persistent Radio Sources of Fast Radio Bursts

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