Jets and spectral states with three-components of accretion flow around a black hole

[2105.06172] Jets and spectral states with three-components of accretion flow around a black hole Skip to main content Search Submit Donate Log in Search arXiv Press Enter to search · Advanced search Astrophysics > High Energy Astrophysical Phenomena arXiv:2105.06172 (astro-ph) This paper has been withdrawn by Rajiv Kumar [Submitted on 13 May 2021 ( v1 ), last revised 13 Apr 2026 (this version, v2)] Title: Jets and spectral states with three-components of accretion flow around a black hole Authors: Rajiv Kumar , Ye-Fei Yuan View a PDF of the paper titled Jets and spectral states with three-components of accretion flow around a black hole, by Rajiv Kumar and 1 other authors No PDF available, click to view other formats Abstract: It is generally believed that high energy radiation (power-law components) can be mostly produced by a hot corona gas in the accreting black holes. There is a very popular hybrid disk radial coupling model that the inner part of cool Keplerian disk (or Shakura-Sunyaev disk) can produce advection-dominated accretion flow or corona-like structure, which can also generate outflows/jets. Here we argue that this simple coupling model cannot explain the whole hardness-intensity diagram of the spectral states and their transitions, and associated jets of a $X-$ray binary. Based on recent theoretical works on advective disk structures around a black hole, as well as many observational behaviors of a source, we conclude that there should be a third component of hot accretion flow with the radial coupling model, which can successfully explain all the spectral states and transitions. Interestingly, this model also provides a new scenario for the jet generation, launching, and evolution during the states with help of created barrier of the inner flow. We have also find out the jet kinetic power expression with our new jet generation scenario. Comments: This arXiv:2105.06172 article substantially matches the arXiv:2210.00683 article. Therefore, I would like to withdraw this arXiv:2105.06172 article. Thank you for your time and consideration Subjects: High Energy Astrophysical Phenomena (astro-ph.HE) Cite as: arXiv:2105.06172 [astro-ph.HE] (or arXiv:2105.06172v2 [astro-ph.HE] for this version) https://doi.org/10.48550/arXiv.2105.06172 Focus to learn more arXiv-issued DOI via DataCite Submission history From: Rajiv Kumar [ view email ] [v1] Thu, 13 May 2021 10:03:23 UTC (297 KB) [v2] Mon, 13 Apr 2026 21:34:03 UTC (1 KB) (withdrawn) Full-text links: Access Paper: View a PDF of the paper titled Jets and spectral states with three-components of accretion flow around a black hole, by Rajiv Kumar and 1 other authors Withdrawn No license for this version due to withdrawn Current browse context: astro-ph.HE < prev | next > new | recent | 2021-05 Change to browse by: astro-ph References & Citations INSPIRE HEP NASA ADS Google Scholar Semantic Scholar export BibTeX citation Loading... BibTeX formatted citation × loading... Data provided by: Bookmark Bibliographic Tools Bibliographic and Citation Tools Bibliographic Explorer Toggle Bibliographic Explorer ( What is the Explorer? ) Connected Papers Toggle Connected Papers ( What is Connected Papers? ) Litmaps Toggle Litmaps ( What is Litmaps? ) scite.ai Toggle scite Smart Citations ( What are Smart Citations? ) Code, Data, Media Code, Data and Media Associated with this Article alphaXiv Toggle alphaXiv ( What is alphaXiv? ) Links to Code Toggle CatalyzeX Code Finder for Papers ( What is CatalyzeX? ) DagsHub Toggle DagsHub ( What is DagsHub? ) GotitPub Toggle Gotit.pub ( What is GotitPub? ) Huggingface Toggle Hugging Face ( What is Huggingface? ) ScienceCast Toggle ScienceCast ( What is ScienceCast? ) Demos Demos Replicate Toggle Replicate ( What is Replicate? ) Spaces Toggle Hugging Face Spaces ( What is Spaces? ) Spaces Toggle TXYZ.AI ( What is TXYZ.AI? ) Related Papers Recommenders and Search Tools Link to Influence Flower Influence Flower ( What are Influence Flowers? ) Core recommender toggle CORE Recommender ( What is CORE? ) IArxiv recommender toggle IArxiv Recommender ( What is IArxiv? ) Author Venue Institution Topic About arXivLabs arXivLabs: experimental projects with community collaborators arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs . Which authors of this paper are endorsers? | Disable MathJax ( What is MathJax? ) We gratefully acknowledge support from our major funders , member institutions , , and all contributors. About · Help · Contact · Subscribe · Copyright · Privacy · Accessibility · Operational Status (opens in new tab) Major funding support from

Related documents

• Thermodynamic topology of black holes and an invariant of spacetime#927186
• Scalar particle in the Kiselev-anti-de-Sitter black hole background#1064534
• Spherical Accretion onto Konoplya Zhidenko Black Holes: Sonic Point Analysis and Fluid Dynamics#784816
• Spherical Accretion onto Konoplya Zhidenko Black Holes: Sonic Point Analysis and Fluid Dynamics#783226
• Mass inflation or scalaron rigidity: Cauchy horizons in metric f(R)#1064433