Imprints of Gravitational Millilensing on the Light Curve of GRBs

Abstract

In this work, we search for signatures of gravitational millilensing in Gamma-ray bursts (GRB) in which the source-lens-observer geometry produces two images that manifest in the GRB light curve as superimposed peaks with identical temporal variability (or echoes), separated by the time delay between the two images. According to the sensitivity of our detection method, we consider millilensing events due to point mass lenses in the range of $10^5-10^7{M}_{\odot }$ at lens redshift about half that of the GRB, with a time delay in the order of $10$ seconds. Current GRB observatories are capable of resolving and constraining this lensing scenario if the above conditions are met. We investigated the Fermi/GBM GRB archive from the year 2008 to 2020 using the autocorrelation technique and we found one millilensed GRB candidate out of 2137 GRBs searched, which we use to estimate the optical depth of millilensed GRBs by performing a Monte-Carlo simulation to find the efficiency of our detection method. Considering a point-mass model for the gravitational lens, where the lens is a supermassive black hole, we show that the density parameter of black holes (${\Omega }_{BH}$) with mass $\approx 10^6{M}_{\odot }$ is about $0.007\pm 0.004$. Our result is one order of magnitude larger compared to consist with previous work in a lower mass range ($10^2-10^3{M}_{\odot }$), which gave a density parameter ${\Omega }_{BH}\approx 5\times 10^{-4}$, and recent work in the mass range of $10^2-10^7{M}_{\odot }$ that reported ${\Omega }_{BH}\approx 4.6\times 10^{-4}$. The mass fraction of black holes in this mass range to the total mass of the universe would be $f\approx {\Omega }_{BH}/{\Omega }_M=0.027\pm 0.016$.

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Cited by in corpus (10)

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• Fermi-GBM Observation of GRB 090717034: ${\chi }^2$ Test Confirms Evidence of Gravitational Lensing by a Supermassive Black Hole with Million Solar Mass
• Detection of GeV emission from an ultra-long gamma-ray burst with the Fermi Large Area Telescope
• A Multi-Wavelength Survey of Transient Lensing Opportunities for Primordial Black Hole Searches
• The radio afterglow of the ultra-long GRB 220627A
• Machine Learning Identification of Gravitationally Microlensed Gamma-Ray Bursts