Unusual Intraburst Variations of Polarization States in FRB 20210912A and FRB 20230708A: Effects of Plasma Birefringence?

Fast radio bursts (FRBs) are highly energetic events of short-duration intense radio emission, the origin of which remains elusive. Polarization of the FRB signals carries information about the emission source as well as the magnetoionic media the signal passes through before reaching terrestrial ra...

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Main Authors: Apurba Bera, Clancy W. James, Mark M. McKinnon, Ronald D. Ekers, Tyson Dial, Adam T. Deller, Keith W. Bannister, Marcin Glowacki, Ryan M. Shannon
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adba59
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author Apurba Bera
Clancy W. James
Mark M. McKinnon
Ronald D. Ekers
Tyson Dial
Adam T. Deller
Keith W. Bannister
Marcin Glowacki
Ryan M. Shannon
author_facet Apurba Bera
Clancy W. James
Mark M. McKinnon
Ronald D. Ekers
Tyson Dial
Adam T. Deller
Keith W. Bannister
Marcin Glowacki
Ryan M. Shannon
author_sort Apurba Bera
collection DOAJ
description Fast radio bursts (FRBs) are highly energetic events of short-duration intense radio emission, the origin of which remains elusive. Polarization of the FRB signals carries information about the emission source as well as the magnetoionic media the signal passes through before reaching terrestrial radio telescopes. Currently known FRBs show a diverse range of polarization, sometimes with complex features, making it challenging to describe them in a unified model. FRB 20230708A and FRB 20210912A are two bright and highly polarized (apparently) one-off FRBs detected in the Commensal Real-time ASKAP Fast Transients survey with the Australian Square Kilometre Array Pathfinder (ASKAP) that exhibit time-dependent conversion between linear and circular polarizations as well as intraburst (apparent) variation of the Faraday rotation measure. We investigate the intraburst temporal evolution of the polarization state of radio emission in these two events using the Poincaré sphere representation and find that the trajectories of the polarization state are well described by great circles on the Poincaré sphere. These polarization features may be signatures of a transition between two partially coherent orthogonal polarization modes or propagation through a birefringent medium. We find that the observed variations of the polarization states of these two FRBs are qualitatively consistent with a magnetospheric origin of the bursts and the effects of propagation through a birefringent medium with linearly polarized modes located close to the emission source—likely in the outer magnetosphere or near-wind region of a neutron star.
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spelling doaj-art-232de5b105fb4f3bab38a2c08c1f0dbe2025-08-20T03:40:02ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01982211910.3847/1538-4357/adba59Unusual Intraburst Variations of Polarization States in FRB 20210912A and FRB 20230708A: Effects of Plasma Birefringence?Apurba Bera0https://orcid.org/0000-0002-2864-4110Clancy W. James1https://orcid.org/0000-0002-6437-6176Mark M. McKinnon2https://orcid.org/0009-0009-7038-1295Ronald D. Ekers3https://orcid.org/0000-0002-3532-9928Tyson Dial4https://orcid.org/0009-0004-1205-8805Adam T. Deller5https://orcid.org/0000-0001-9434-3837Keith W. Bannister6https://orcid.org/0000-0003-2149-0363Marcin Glowacki7https://orcid.org/0000-0002-5067-8894Ryan M. Shannon8https://orcid.org/0000-0002-7285-6348International Centre for Radio Astronomy Research, Curtin University , Bentley, WA 6102, Australia ; apurba.bera@curtin.edu.au, clancy.james@curtin.edu.auInternational Centre for Radio Astronomy Research, Curtin University , Bentley, WA 6102, Australia ; apurba.bera@curtin.edu.au, clancy.james@curtin.edu.auNational Radio Astronomy Observatory , Socorro, NM 87801, USA ; mmckinno@nrao.eduInternational Centre for Radio Astronomy Research, Curtin University , Bentley, WA 6102, Australia ; apurba.bera@curtin.edu.au, clancy.james@curtin.edu.au; Australia Telescope National Facility , CSIRO, Space and Astronomy, PO Box 76, Epping, NSW 1710, AustraliaCentre for Astrophysics and Supercomputing, Swinburne University of Technology , Hawthorn, VIC 3122, AustraliaCentre for Astrophysics and Supercomputing, Swinburne University of Technology , Hawthorn, VIC 3122, Australia; OzGrav , the ARC Centre of Excellence for Gravitational Wave Discovery, AustraliaAustralia Telescope National Facility , CSIRO, Space and Astronomy, PO Box 76, Epping, NSW 1710, Australia; Sydney Institute for Astronomy, School of Physics, The University of Sydney , NSW 2006, AustraliaInternational Centre for Radio Astronomy Research, Curtin University , Bentley, WA 6102, Australia ; apurba.bera@curtin.edu.au, clancy.james@curtin.edu.auCentre for Astrophysics and Supercomputing, Swinburne University of Technology , Hawthorn, VIC 3122, AustraliaFast radio bursts (FRBs) are highly energetic events of short-duration intense radio emission, the origin of which remains elusive. Polarization of the FRB signals carries information about the emission source as well as the magnetoionic media the signal passes through before reaching terrestrial radio telescopes. Currently known FRBs show a diverse range of polarization, sometimes with complex features, making it challenging to describe them in a unified model. FRB 20230708A and FRB 20210912A are two bright and highly polarized (apparently) one-off FRBs detected in the Commensal Real-time ASKAP Fast Transients survey with the Australian Square Kilometre Array Pathfinder (ASKAP) that exhibit time-dependent conversion between linear and circular polarizations as well as intraburst (apparent) variation of the Faraday rotation measure. We investigate the intraburst temporal evolution of the polarization state of radio emission in these two events using the Poincaré sphere representation and find that the trajectories of the polarization state are well described by great circles on the Poincaré sphere. These polarization features may be signatures of a transition between two partially coherent orthogonal polarization modes or propagation through a birefringent medium. We find that the observed variations of the polarization states of these two FRBs are qualitatively consistent with a magnetospheric origin of the bursts and the effects of propagation through a birefringent medium with linearly polarized modes located close to the emission source—likely in the outer magnetosphere or near-wind region of a neutron star.https://doi.org/10.3847/1538-4357/adba59Time domain astronomyRadio transient sourcesRadio bursts
spellingShingle Apurba Bera
Clancy W. James
Mark M. McKinnon
Ronald D. Ekers
Tyson Dial
Adam T. Deller
Keith W. Bannister
Marcin Glowacki
Ryan M. Shannon
Unusual Intraburst Variations of Polarization States in FRB 20210912A and FRB 20230708A: Effects of Plasma Birefringence?
The Astrophysical Journal
Time domain astronomy
Radio transient sources
Radio bursts
title Unusual Intraburst Variations of Polarization States in FRB 20210912A and FRB 20230708A: Effects of Plasma Birefringence?
title_full Unusual Intraburst Variations of Polarization States in FRB 20210912A and FRB 20230708A: Effects of Plasma Birefringence?
title_fullStr Unusual Intraburst Variations of Polarization States in FRB 20210912A and FRB 20230708A: Effects of Plasma Birefringence?
title_full_unstemmed Unusual Intraburst Variations of Polarization States in FRB 20210912A and FRB 20230708A: Effects of Plasma Birefringence?
title_short Unusual Intraburst Variations of Polarization States in FRB 20210912A and FRB 20230708A: Effects of Plasma Birefringence?
title_sort unusual intraburst variations of polarization states in frb 20210912a and frb 20230708a effects of plasma birefringence
topic Time domain astronomy
Radio transient sources
Radio bursts
url https://doi.org/10.3847/1538-4357/adba59
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