Observational signatures of microlensing in gravitational waves at LIGO/Virgo frequencies

J. M. DIego, O. A. Hannuksela, P. L. Kelly, G. Pagano, T. Broadhurst, K. Kim, T. G.F. Li, G. F. Smoot

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6 Scopus citations

Abstract

Microlenses with typical stellar masses (a few M) have traditionally been disregarded as potential sources of gravitational lensing effects at LIGO/Virgo frequencies, since the time delays are often much smaller than the inverse of the frequencies probed by LIGO/Virgo, resulting in negligible interference effects at LIGO/Virgo frequencies. While this is true for isolated microlenses in this mass regime, we show how, under certain circumstances and for realistic scenarios, a population of microlenses (for instance stars and remnants from a galaxy halo or from the intracluster medium) embedded in a macromodel potential (galaxy or cluster) can conspire together to produce time delays of order one millisecond, which would produce significant interference distortions in the observed strains. At sufficiently large magnification factors (of several hundred), microlensing effects should be common in gravitationally lensed gravitational waves. We explored the regime where the predicted signal falls in the frequency range probed by LIGO/Virgo. We find that stellar mass microlenses, permeating the lens plane, and near critical curves, can introduce interference distortions in strongly lensed gravitational waves. Lensed events with negative parity, or saddle points (which have never before been studied in the context of gravitational waves), and that take place near caustics of macromodels, are more likely to produce measurable interference effects at LIGO/Virgo frequencies. This is the first study that explores the effect of a realistic population of microlenses, including a macromodel, on strongly lensed gravitational waves.

Original languageEnglish (US)
Article numberA130
JournalAstronomy and Astrophysics
Volume627
DOIs
StatePublished - Jul 1 2019

Bibliographical note

Funding Information:
Acknowledgements. J.M.D. acknowledges the support of projects AYA2015-64508-P (MINECO/FEDER, UE), funded by the Ministerio de Economia y Competitividad. J.M.D. acknowledges the hospitality of the Physics Department at the University of Pennsylvania for hosting him during the preparation of this work. The authors thank Mark Trodden for useful comments. O.A.H. is supported by the Hong Kong Ph.D. Fellowship Scheme (HKPFS) issued by the Research Grants Council (RGC) of Hong Kong. The work of O.A.H., K.K., and T.G.F.L. was partially supported by grants from the Research Grants Council of the Hong Kong (Project No. CUHK14310816, CUHK24304317 and/or CUHK 14306218) and the Direct Grant for Research from the Research Committee of the Chinese University of Hong Kong.

Keywords

  • Gravitational lensing: strong
  • Gravitational waves

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