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| Format: | Preprint |
| Published: |
2026
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| Online Access: | https://arxiv.org/abs/2603.28666 |
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| _version_ | 1866916017427447808 |
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| author | Xu, Chun |
| author_facet | Xu, Chun |
| contents | We propose that changing-look AGN transitions arise from variations in the size of the inner ADAF disk. The AGN accretion disk consists of an outer thin disk and an inner thick ADAF component, whose size is intrinsically unstable and evolves over time. The size variations of the ADAF are governed by a parameter η, which represents the turbulence strength within the accretion flow. ηalso determines the accretion rate onto the central black hole and controls jet formation and outflow rate, with the latter regulating the line-of-sight absorption. From the perspective of a variable ADAF, changing-state and changing-observation AGN are two sides of the same coin. We further discuss gigahertz-peaked and compact steep-spectrum radio sources as possible manifestations of intermediate-to-large scale ADAFs. Finally, we propose that AGN unification models should include both orientation and ADAF size as key parameters. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2603_28666 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Variable ADAF disk as the origin of Changing-Look AGN Xu, Chun High Energy Astrophysical Phenomena We propose that changing-look AGN transitions arise from variations in the size of the inner ADAF disk. The AGN accretion disk consists of an outer thin disk and an inner thick ADAF component, whose size is intrinsically unstable and evolves over time. The size variations of the ADAF are governed by a parameter η, which represents the turbulence strength within the accretion flow. ηalso determines the accretion rate onto the central black hole and controls jet formation and outflow rate, with the latter regulating the line-of-sight absorption. From the perspective of a variable ADAF, changing-state and changing-observation AGN are two sides of the same coin. We further discuss gigahertz-peaked and compact steep-spectrum radio sources as possible manifestations of intermediate-to-large scale ADAFs. Finally, we propose that AGN unification models should include both orientation and ADAF size as key parameters. |
| title | Variable ADAF disk as the origin of Changing-Look AGN |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2603.28666 |