Strong gravitational lensing and microlensing of supernovae
Sherry H. Suyu, Ariel Goobar, Thomas Collett, Anupreeta More, Giorgos, Vernardos

TL;DR
Gravitational lensing and microlensing of supernovae offer new methods for cosmological measurements and astrophysical insights, with upcoming surveys expected to significantly increase discoveries and scientific opportunities.
Contribution
This paper provides an overview of the emerging field of lensed supernovae, highlighting new methods, upcoming survey prospects, and scientific applications.
Findings
Lensed SNe can constrain the Hubble constant via time delays.
Upcoming surveys like LSST will discover many lensed SNe.
Lensed SNe can probe SN progenitors, sizes, and dust properties.
Abstract
Strong gravitational lensing and microlensing of supernovae (SNe) are emerging as a new probe of cosmology and astrophysics in recent years. We provide an overview of this nascent research field, starting with a summary of the first discoveries of strongly lensed SNe. We describe the use of the time delays between multiple SN images as a way to measure cosmological distances and thus constrain cosmological parameters, particularly the Hubble constant, whose value is currently under heated debates. New methods for measuring the time delays in lensed SNe have been developed, and the sample of lensed SNe from the upcoming Rubin Observatory Legacy Survey of Space and Time (LSST) is expected to provide competitive cosmological constraints. Lensed SNe are also powerful astrophysical probes. We review the usage of lensed SNe to constrain SN progenitors, acquire high-z SN spectra through…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies
