High-time resolution search for compact objects using fast radio burst gravitational lens interferometry with CHIME/FRB

The gravitational field of compact objects, such as primordial black holes, can create multiple images of background sources. For transients such as fast radio bursts (FRBs), these multiple images can be resolved in the time domain. Under certain circumstances, these images not only have similar burst morphologies but are also phase-coherent at the electric field level. With a novel dechannelization algorithm and a matched filtering technique, we search for repeated copies of the same electric field waveform in observations of FRBs detected by the FRB backend of the Canadian Hydrogen Mapping Intensity Experiment (CHIME). An interference fringe from a coherent gravitational lensing signal will appear in the time-lag domain as a statistically-significant peak in the time-lag autocorrelation function. We calibrate our statistical significance using telescope data containing no FRB signal. Our dataset consists of ∼ 100-ms long recordings of voltage data from 172 FRB events, dechannelized to 1.25-ns time resolution. This coherent search algorithm allows us to search for gravitational lensing signatures from compact objects in the mass range of 10 − 4 − 10 4 M (cid:12) . After ruling out an anomalous candidate due to diffractive scintillation, we find no significant detections of gravitational lensing in the 172 FRB events that have been analyzed. In a companion work [1], we interpret the constraints on dark matter from this search.

[1]  D. Michilli,et al.  Scintillation Timescales of Bright FRBs Detected by CHIME/FRB , 2021, Research Notes of the AAS.

[2]  K. Liao,et al.  Search for Lensing Signatures from the Latest Fast Radio Burst Observations and Constraints on the Abundance of Primordial Black Holes , 2021, The Astrophysical Journal.

[3]  Kendrick M. Smith,et al.  The First CHIME/FRB Fast Radio Burst Catalog , 2021, The Astrophysical Journal Supplement Series.

[4]  E. Thrane,et al.  Evidence for an intermediate-mass black hole from a gravitationally lensed gamma-ray burst , 2021, Nature Astronomy.

[5]  M. Dobbs,et al.  An Analysis Pipeline for CHIME/FRB Full-array Baseband Data , 2020, The Astrophysical Journal.

[6]  Davor Cubranic,et al.  A Synoptic VLBI Technique for Localizing Nonrepeating Fast Radio Bursts with CHIME/FRB , 2020, 2008.11738.

[7]  M. Halpern,et al.  The CHIME Pulsar Project: System Overview , 2020, The Astrophysical Journal Supplement Series.

[8]  A. Green,et al.  Primordial black holes as a dark matter candidate , 2020, Journal of Physics G: Nuclear and Particle Physics.

[9]  B. Carr,et al.  Primordial Black Holes as Dark Matter: Recent Developments , 2020, 2006.02838.

[10]  J. Prochaska,et al.  A census of baryons in the Universe from localized fast radio bursts , 2020, Nature.

[11]  O. Wucknitz,et al.  Cosmology with gravitationally lensed repeating fast radio bursts , 2020, Astronomy & Astrophysics.

[12]  K. Liao,et al.  Constraints on Compact Dark Matter with Fast Radio Burst Observations , 2020, The Astrophysical Journal.

[13]  J. Prochaska,et al.  Spectropolarimetric Analysis of FRB 181112 at Microsecond Resolution: Implications for Fast Radio Burst Emission Mechanism , 2020, The Astrophysical Journal.

[14]  J. Prochaska,et al.  First Constraints on Compact Dark Matter from Fast Radio Burst Microstructure , 2020, The Astrophysical Journal.

[15]  S. Foreman,et al.  Wave effects in the microlensing of pulsars and FRBs by point masses , 2020, 2002.01570.

[16]  A. Katz,et al.  Looking for MACHOs in the spectra of fast radio bursts , 2019, Monthly Notices of the Royal Astronomical Society.

[17]  M. Oguri Strong gravitational lensing of explosive transients , 2019, Reports on progress in physics. Physical Society.

[18]  S. Djorgovski,et al.  A fast radio burst localized to a massive galaxy , 2019, Nature.

[19]  Shami Chatterjee,et al.  Fast Radio Bursts: An Extragalactic Enigma , 2019, Annual Review of Astronomy and Astrophysics.

[20]  M. Lower,et al.  Five new real-time detections of fast radio bursts with UTMOST , 2019, Monthly Notices of the Royal Astronomical Society.

[21]  C. W. James,et al.  The Spectral Properties of the Bright Fast Radio Burst Population , 2018, The Astrophysical Journal.

[22]  A. Katz,et al.  Femtolensing by dark matter revisited , 2018, Journal of Cosmology and Astroparticle Physics.

[23]  D. V. Wiebe,et al.  The CHIME Fast Radio Burst Project: System Overview , 2018, The Astrophysical Journal.

[24]  D. Eichler Nanolensed Fast Radio Bursts , 2017, 1711.04764.

[25]  Bing Zhang,et al.  Strongly lensed repeating fast radio bursts as precision probes of the universe , 2017, Nature Communications.

[26]  Wenbin Lu,et al.  Probing Motion of Fast Radio Burst Sources by Timing Strongly Lensed Repeaters , 2017, 1706.06103.

[27]  R. S. Wharton,et al.  Lensing of Fast Radio Bursts by Plasma Structures in Host Galaxies , 2017, 1703.06580.

[28]  A. Keimpema,et al.  A direct localization of a fast radio burst and its host , 2017, Nature.

[29]  A. Ganguly,et al.  Dense magnetized plasma associated with a fast radio burst , 2015, Nature.

[30]  R. Poleski,et al.  The OGLE view of microlensing towards the Magellanic Clouds – IV. OGLE-III SMC data and final conclusions on MACHOs , 2011, 1106.2925.

[31]  M. Khlopov Primordial black holes , 2007, 0801.0116.

[32]  J. Beaulieu,et al.  Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds , 2006, astro-ph/0607207.

[33]  A. J. Drake,et al.  The MACHO Project: Microlensing Results from 5.7 Years of Large Magellanic Cloud Observations , 2000, astro-ph/0001272.

[34]  Sabine Fenstermacher Handbook Of Pulsar Astronomy , 2016 .

[35]  B. Alder,et al.  Methods in computational physics: advances in research and applications. Vol._14: Radio astronomy. , 1975 .