2025ApJ...981..133W


Query : 2025ApJ...981..133W

2025ApJ...981..133W - Astrophys. J., 981, 133 (2025/March-2)

Effect of Deviations from General Relativity on Searches for Gravitational-wave Microlensing and Type II Strong Lensing.

WRIGHT M., JANQUART J. and JOHNSON-MCDANIEL N.K.

Abstract (from CDS):

As the gravitational-wave (GW) detector network is upgraded and the sensitivity of the detectors improves, novel scientific avenues open for exploration. For example, tests of general relativity (GR) will become more accurate as smaller deviations can be probed. Additionally, the detection of lensed GWs becomes more likely. However, these new avenues could also interact with each other, and a GW event presenting deviations from GR could be mistaken for a lensed one. Here, we explore how phenomenological deviations from GR or binaries of exotic compact objects could impact those lensing searches focusing on a single event. We consider strong lensing, millilensing, and microlensing, and find that certain phenomenological deviations from GR may be mistaken for all of these types of lensing. Therefore, our study shows that future candidate lensing events would need to be carefully examined to avoid a false claim of lensing where instead a deviation from GR has been seen.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Gravitational lensing - Gravitational microlensing - Gravitational waves - General relativity

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 GrW 190521 GWE ~ ~           ~ 409 0

Query : 2025ApJ...981..133W

Basic data :
GrW 190521 -- Gravitational Wave Event
Other object types:
otypes_help
GWE (GrW)
ICRS coord. (ep=J2000) :
No Coord.

Identifiers (2) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

GrW 190521 030229 GrW 190521

References (409 between 1850 and 2026) (Total 409)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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