Testing a Galactic Lensing Hypothesis with the Prompt Emission of GRB 221009A
Research Notes of the AAS(2024)
摘要
Even at modest amplification, the optical depth to gravitational lensing
through the Galaxy is <10^-5. However, the large apparent
isotropic-equivalent energy of GRB 221009A coupled with a path through low
Galactic latitude suggests that the conditional probability that this
particular GRB was lensed is greater than the very low a priori expectation.
With the extreme brightness of the prompt emission, this Galactic lensing
hypothesis can be constrained by autocorrelation analysis of Fermi photons on
0.1-1000 ms timescales. In relating lensing mass, magnification, and
autocorrelation timescale, I show that a lensed-induced autocorrelation
signature by stellar lenses falls below the minimal variability timescale (MVT)
expected from a black hole central engine. However, lensing by Galactic dark
matter MACHOs (M_l > 10-1000 M_⊙) could be confirmed with this approach.
Regardless, at a peak γ-ray photon rate of >30 ms^-1, GRB 221009A
represents a prime opportunity to measure the smallest MVTs of GRBs.
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关键词
galactic lensing hypothesis,grb 221009a,prompt emission
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