Detection of Partial Coherence due to Multipath Propagation for FRB 20220413B with CHIME/FRB
arXiv:2512.11969 · doi:10.1103/f2nh-hktz
Abstract
Fast radio bursts (FRBs) are a millisecond-long transient phenomenon that propagate across extragalactic distances and are effectively a point source. Radio wave propagation through inhomogeneous distributions of plasma can act as a lens, generating multiple images of the emitted electric field. A lens can produce images of a point source where the phase of the electric field between images remains coherent when observed by a radio telescope. FRB 20220413B shows a complicated pulse structure with time separated components that may be image copies of the main components due to plasma lensing. We perform several analyses to determine if FRB 20220413B is consistent with expectations of a plasma lensed FRB. We analyze and fit the morphology of the burst to a plasma lens model and find consistency in the spectro-temporal profile but not the observed flux. Using the complex-valued channelized voltage data from the CHIME telescope, we perform a time-lag correlation analysis and report correlation signatures present in the electric field of FRB 20220413B. We find that there exists an excess correlation signature only in absolute power and not in phase. We perform a frequency-lag correlation analysis on the spectra of all subcomponents of the burst and find a consistent scintillation bandwidth across all components. We find the scintillation bandwidth is consistent with expectations of scattering due to the Milky Way. We interpret this as all burst components propagating through the same scintillation screen located in the Milky Way, which would generate the excess variance signature observed, even in the absence of phase coherence between burst components. We find that while the burst morphology can be modeled by a plasma lens, the coherent signature present in the time-lag correlation is consistent with the expectations of a common scattering screen, but not coherent plasma lensing.
arXiv comment20 pages, 12 figures
References in corpus (30)
- A bright millisecond radio burst of extragalactic origin
- A Population of Fast Radio Bursts at Cosmological Distances
- A fast radio burst associated with a Galactic magnetar
- 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
- An extreme magneto-ionic environment associated with the fast radio burst source FRB 121102
- Dense magnetized plasma associated with a fast radio burst
- The CHIME Fast Radio Burst Project: System Overview
- Lensing of Fast Radio Bursts as a Probe of Compact Dark Matter
- Lensing of Fast Radio Bursts by Plasma Structures in Host Galaxies
- FRB microstructure revealed by the real-time detection of FRB170827
- The Gaussian Plasma Lens in Astrophysics. Refraction
- The spectral properties of the bright FRB population
- Extremely band-limited repetition from a fast radio burst source
- Pulsar emission amplified and resolved by plasma lensing in an eclipsing binary
- An analysis pipeline for CHIME/FRB full-array baseband data
- A Plasma Prism Model for an Anomalous Dispersion Event in the Crab Pulsar
- Extreme Scattering Events Towards Two Young Pulsars
- Wave effects in the microlensing of pulsars and FRBs by point masses
- Looking for MACHOs in the Spectra of Fast Radio Bursts
- An analysis of the time-frequency structure of several bursts from FRB121102 detected with MeerKAT
- Descattering of Giant Pulses in PSR B1957+20
- Stellar prospects for FRB gravitational lensing
- A fast radio burst localized at detection to an edge-on galaxy using very-long-baseline interferometry
- Nanolensed fast Radio Bursts
- NE2001p: A Native Python Implementation of the NE2001 Galactic Electron Density Model
- Scintillation Arc from FRB 20220912A
- Constraining the FRB mechanism from scintillation in the host galaxy
- Simulating FRB Morphologies and Coherent Phase Correlation Signatures from Multi-Plane Astrophysical Lensing
- Scintillometry of Fast Radio Bursts: Resolution effects in two-screen models