What is the nature of GW230529? An exploration of the gravitational lensing hypothesis
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2024
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| author | Janquart, Justin Keitel, David Lo, Rico K. L. Chan, Juno C. L. Ezquiaga, Jose Marìa Hannuksela, Otto A. Li, Alvin K. Y. More, Anupreeta Phurailatpam, Hemantakumar Singh, Neha Uronen, Laura E. Wright, Mick Adhikari, Naresh Biscoveanu, Sylvia Bulik, Tomasz Farah, Amanda M. Heffernan, Anna Joshi, Prathamesh Juste, Vincent Kedia, Atul Nichols, Shania A. Pratten, Geraint Rawcliffe, C. Roy, Soumen Sänger, Elise M. Tong, Hui Trevor, M. Vujeva, Luka Zevin, Michael |
| author_facet | Janquart, Justin Keitel, David Lo, Rico K. L. Chan, Juno C. L. Ezquiaga, Jose Marìa Hannuksela, Otto A. Li, Alvin K. Y. More, Anupreeta Phurailatpam, Hemantakumar Singh, Neha Uronen, Laura E. Wright, Mick Adhikari, Naresh Biscoveanu, Sylvia Bulik, Tomasz Farah, Amanda M. Heffernan, Anna Joshi, Prathamesh Juste, Vincent Kedia, Atul Nichols, Shania A. Pratten, Geraint Rawcliffe, C. Roy, Soumen Sänger, Elise M. Tong, Hui Trevor, M. Vujeva, Luka Zevin, Michael |
| contents | On the 29th of May 2023, the LIGO-Virgo-KAGRA Collaboration observed a compact binary coalescence event consistent with a neutron star-black hole merger, though the heavier object of mass 2.5-4.5 $M_\odot$ would fall into the purported lower mass gap. An alternative explanation for apparent observations of events in this mass range has been suggested as strongly gravitationally lensed binary neutron stars. In this scenario, magnification would lead to the source appearing closer and heavier than it really is. Here, we investigate the chances and possible consequences for the GW230529 event to be gravitationally lensed. We find this would require high magnifications and we obtain low rates for observing such an event, with a relative fraction of lensed versus unlensed observed events of $2 \times 10^{-3}$ at most. When comparing the lensed and unlensed hypotheses accounting for the latest rates and population model, we find a 1/58 chance of lensing, disfavoring this option. Moreover, when the magnification is assumed to be strong enough to bring the mass of the heavier binary component below the standard limits on neutron star masses, we find high probability for the lighter object to have a sub-solar mass, making the binary even more exotic than a mass-gap neutron star-black hole system. Even when the secondary is not sub-solar, its tidal deformability would likely be measurable, which is not the case for GW230529. Finally, we do not find evidence for extra lensing signatures such as the arrival of additional lensed images, type-II image dephasing, or microlensing. Therefore, we conclude it is unlikely for GW230529 to be a strongly gravitationally lensed binary neutron star signal. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2409_07298 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | What is the nature of GW230529? An exploration of the gravitational lensing hypothesis Janquart, Justin Keitel, David Lo, Rico K. L. Chan, Juno C. L. Ezquiaga, Jose Marìa Hannuksela, Otto A. Li, Alvin K. Y. More, Anupreeta Phurailatpam, Hemantakumar Singh, Neha Uronen, Laura E. Wright, Mick Adhikari, Naresh Biscoveanu, Sylvia Bulik, Tomasz Farah, Amanda M. Heffernan, Anna Joshi, Prathamesh Juste, Vincent Kedia, Atul Nichols, Shania A. Pratten, Geraint Rawcliffe, C. Roy, Soumen Sänger, Elise M. Tong, Hui Trevor, M. Vujeva, Luka Zevin, Michael General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena On the 29th of May 2023, the LIGO-Virgo-KAGRA Collaboration observed a compact binary coalescence event consistent with a neutron star-black hole merger, though the heavier object of mass 2.5-4.5 $M_\odot$ would fall into the purported lower mass gap. An alternative explanation for apparent observations of events in this mass range has been suggested as strongly gravitationally lensed binary neutron stars. In this scenario, magnification would lead to the source appearing closer and heavier than it really is. Here, we investigate the chances and possible consequences for the GW230529 event to be gravitationally lensed. We find this would require high magnifications and we obtain low rates for observing such an event, with a relative fraction of lensed versus unlensed observed events of $2 \times 10^{-3}$ at most. When comparing the lensed and unlensed hypotheses accounting for the latest rates and population model, we find a 1/58 chance of lensing, disfavoring this option. Moreover, when the magnification is assumed to be strong enough to bring the mass of the heavier binary component below the standard limits on neutron star masses, we find high probability for the lighter object to have a sub-solar mass, making the binary even more exotic than a mass-gap neutron star-black hole system. Even when the secondary is not sub-solar, its tidal deformability would likely be measurable, which is not the case for GW230529. Finally, we do not find evidence for extra lensing signatures such as the arrival of additional lensed images, type-II image dephasing, or microlensing. Therefore, we conclude it is unlikely for GW230529 to be a strongly gravitationally lensed binary neutron star signal. |
| title | What is the nature of GW230529? An exploration of the gravitational lensing hypothesis |
| topic | General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2409.07298 |