Revisiting High-energy Polarization from Leptonic and Hadronic Blazar Scenarios
| dc.contributor.author | Zhang, Haocheng | en.ZA |
| dc.contributor.author | Böttcher, Markus | en.ZA |
| dc.contributor.author | Liodakis, Ioannis | en.ZA |
| dc.date.accessioned | 2025-10-24T07:06:41Z | en.ZA |
| dc.date.issued | 2024 | en.ZA |
| dc.description | Journal Article, Faculty of Natural and Agricultural Sciences, Centre for Space Research (CSR)-- Potchefstroom Campus | en.ZA |
| dc.description.abstract | X-ray and MeV polarization can be powerful diagnostics for leptonic and hadronic blazar models. Previous strongly favor a multizone framework. Thus, the leptonic and hadronic polarization predictions need to be revisited. Here we identify two generic radiation transfer effects, namely, double depolarization and energy stratification, that can have an impact on the leptonic and hadronic polarization. We show how they are generalized from previously known multizone effects of the primary electron synchrotron radiation. Under our generic multizone model, the leptonic polarization degree is expected to be much lower than the one-zone prediction, unlikely detectable in most cases. The hadronic polarization degree can reach a value as high as the primary electron synchrotron polarization during simultaneous multiwavelength flares, consistent with the one-zone prediction. Therefore, IXPE and future X-ray and MeV polarimeters such as eXTP, COSI, and AMEGO-X, have good chances to detect hadronic polarization during flares. However, the hadronic polarization cannot be well constrained during the quiescent state. Nonetheless, if some blazar jets possess relatively stable large-scale magnetic structures, as suggested by radio observations, a nontrivial polarization degree may show up for the hadronic model after a very long exposure time (1 yr). | en.ZA |
| dc.description.sponsorship | Acknowledgments We thank the anonymous referee for very constructive comments. H.Z. was supported by NASA under award No. 80GSFC21M0002. H.Z. is supported by Fermi GI Program Cycle 16, award No. 22-FERMI22-0015. I.L. was supported by the NASA Postdoctoral Program at the Marshall Space Flight Center, administered by Oak Ridge Associated Universities under contract with NASA. The work of M.B. is supported in part by the Department of Science and Innovation and the National Research Foundation of South Africa through a grant in support of the South African Gamma-Ray Astronomy Programme (SA-GAMMA). | en.ZA |
| dc.identifier.citation | Böttcher, Markus. et al. 2024. Revisiting High-energy Polarization from Leptonic and Hadronic Blazar Scenarios. Astrophysical Journal, (2024), 967:93 (8pp), [https://iopscience.iop.org/article/10.3847/1538-4357/ad77a7/pdf] | en.ZA |
| dc.identifier.uri | https://iopscience.iop.org/article/10.3847/1538-4357/ad77a7/pdf | en.ZA |
| dc.identifier.uri | http://hdl.handle.net/10394/43737 | en.ZA |
| dc.language.iso | en | en.ZA |
| dc.publisher | Astrophysical Journal | en.ZA |
| dc.subject | Blazars (164) | en.ZA |
| dc.subject | High Energy Astrophysics (739) | en.ZA |
| dc.subject | Polarimetry (1278) | en.ZA |
| dc.subject | Relativistic Jets (1390) | en.ZA |
| dc.title | Revisiting High-energy Polarization from Leptonic and Hadronic Blazar Scenarios | en.ZA |
| dc.type | Article | en.ZA |
