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| Evolutionary tracks of massive stars with different rotation and metallicity in neutrino H-R diagram | |
Wang, Hao1,2; Zhu, Chunhua1 ; Liu, Helei1; Guo, Sufen1; Lu, Guoliang1,2
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| 2023-10-10 | |
| Source Publication | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| ISSN | 0035-8711 |
| Volume | 526Issue:3Pages:4335-4344 |
| Contribution Rank | 2 |
| Abstract | Neutrino losses play a crucial role in the evolution of massive stars. We study the neutrino luminosity of stars ranging from 20 to 90 M-circle dot from Zero Age Main Sequence to Fe Core Collapse (FeCC) with different rotation and metallicity in a neutrino Hertzsprung-Russell diagram. In our simulations, we consider omega/omega(crit )= 0 and 0.7 to represent non-rotation and high rotation, respectively, and set the metallicities to 0.014, 0.001, and 0.0001. During hydrogen burning stages, neutrino luminosity primarily originates from CNO cycle, and increases with higher stellar mass while decreasing with increasing metallicity. For the high metallicity models (Z = 0.014) during the helium burning stage, the reduction of the hydrogen envelope caused by a larger mass loss rate leads to a gradual decrease in neutrino luminosity. The rapid rotation results in extra mixing inside massive stars, which increases the neutrino luminosity during main sequence, while decreases the neutrino luminosity during helium burning phase. Simultaneously, the rapid rotation also increases CO core mass, which enhances the neutrino luminosity during C and O burning phase. We also investigate the effect of neutrino magnetic moment (NMM) on the massive stars. We find that the energy loss caused by the NMM does not have effects on the evolutionary destiny of massive stars, and it does not significant change the compactness at the time of FeCC. |
| Keyword | neutrinos stars: evolution Hertzsprung-Russell and colour-magnitude diagrams stars: massive stars: rotation |
| DOI | 10.1093/mnras/stad3071 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | WEAK INTERACTION RATES ; WOLF-RAYET STARS ; MAGNETIC-MOMENT ; PRESUPERNOVA EVOLUTION ; HOMOGENEOUS EVOLUTION ; STELLAR EVOLUTION ; MAGELLANIC-CLOUD ; MODULES ; NUCLEI ; MODELS |
| Funding Project | This work received the generous support of the National Natural Science Foundation of China, project no. U2031204, 12163005, 12288102, and 12263006, the science research grants from the China Manned Space Project with no. CMS-CSST-2021-A10, the Natural Sci[U2031204] ; This work received the generous support of the National Natural Science Foundation of China, project no. U2031204, 12163005, 12288102, and 12263006, the science research grants from the China Manned Space Project with no. CMS-CSST-2021-A10, the Natural Sci[12163005] ; This work received the generous support of the National Natural Science Foundation of China, project no. U2031204, 12163005, 12288102, and 12263006, the science research grants from the China Manned Space Project with no. CMS-CSST-2021-A10, the Natural Sci[12288102] ; This work received the generous support of the National Natural Science Foundation of China, project no. U2031204, 12163005, 12288102, and 12263006, the science research grants from the China Manned Space Project with no. CMS-CSST-2021-A10, the Natural Sci[12263006] ; National Natural Science Foundation of China[CMS-CSST-2021-A10] ; China Manned Space Project[2021D01C075] ; China Manned Space Project[2022D01D85] ; China Manned Space Project[2022TSYCLJ0006] ; Natural Science Foundation of Xinjiang |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001097539800005 |
| Publisher | OXFORD UNIV PRESS |
| Funding Organization | This work received the generous support of the National Natural Science Foundation of China, project no. U2031204, 12163005, 12288102, and 12263006, the science research grants from the China Manned Space Project with no. CMS-CSST-2021-A10, the Natural Sci ; National Natural Science Foundation of China ; China Manned Space Project ; Natural Science Foundation of Xinjiang |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5614 |
| Collection | 射电天文研究室_理论天体物理研究团组 |
| Corresponding Author | Zhu, Chunhua; Lu, Guoliang |
| Affiliation | 1.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830017, Peoples R China 2.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1-St, Urumqi 830011, Peoples R China |
| Recommended Citation GB/T 7714 | Wang, Hao,Zhu, Chunhua,Liu, Helei,et al. Evolutionary tracks of massive stars with different rotation and metallicity in neutrino H-R diagram[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,526(3):4335-4344. |
| APA | Wang, Hao,Zhu, Chunhua,Liu, Helei,Guo, Sufen,&Lu, Guoliang.(2023).Evolutionary tracks of massive stars with different rotation and metallicity in neutrino H-R diagram.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,526(3),4335-4344. |
| MLA | Wang, Hao,et al."Evolutionary tracks of massive stars with different rotation and metallicity in neutrino H-R diagram".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 526.3(2023):4335-4344. |
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| File Name/Size | DocType | Version | Access | License | ||
| Wang-2023-Evolutiona（4810KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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