Phase-transition-induced Collapse of Proto-compact Stars and Its Implication for Supernova Explosions

doi:10.3847/1538-4357/ada146

YNAO OpenIR > 大样本恒星演化研究组

	Phase-transition-induced Collapse of Proto-compact Stars and Its Implication for Supernova Explosions
	Huang, Xu-Run 1; Cha S(查帅)2,3 ; Chu, Ming-chung 1; O'Connor, Evan P.4; Chen, Lie-Wen 5
发表期刊	ASTROPHYSICAL JOURNAL
	2025-02-01
卷号	979 期号:2
DOI	10.3847/1538-4357/ada146
产权排序	第2完成单位
收录类别	SCI
摘要	A hadron-quark phase transition (PT) may trigger supernova explosions during stellar core collapse. However, both success and failure have occurred in previous attempts to explode dying stars via this mechanism. We systematically explore the outcomes of the PT-induced collapse of mock proto-compact stars (PCSs) with a constant entropy and lepton fraction, with spherically symmetric general relativistic hydrodynamic simulations and a controlled series of hybrid equations of state. Our results reveal the qualitative dependence of successful and failed explosions on the PT and quark matter characteristics. A small portion (similar to 0.04%-1%) of the released binding energy Delta EB transforms into the diagnostic explosion energy Eexp,diag, which saturates at similar to 6 x 1051 erg near the black hole formation. Note that our Eexp,diag represents an upper limit of the final explosion energies in realistic supernova simulations. We draw the phase diagrams indicative of the possible fates of supernova explosions driven by hadron-quark PTs, where the control parameters are the onset density, the energy gap of the PT, and the quark matter speed of sound. Our findings can guide further self-consistent investigations on PT-driven core-collapse supernovae and help identify hadron-quark PT-induced PCS collapse from future observations.
资助项目	Research Grants Council, University Grants Committee ((sic)(sic)(sic)(sic)(sic))https://doi.org/10.13039/501100002920; Shanghai Jiao Tong University via the Fellowship of Outstanding PhD Graduates[14300320]; Shanghai Jiao Tong University via the Fellowship of Outstanding PhD Graduates[14304322]; Research Grant Council of the Hong Kong Special Administrative Region, China[12288102]; Research Grant Council of the Hong Kong Special Administrative Region, China[12473031]; Research Grant Council of the Hong Kong Special Administrative Region, China[12393811]; National Natural Science Foundation of China (NSFC)[202201BC070003]; Natural Science Foundation of Yunnan Province[202401BC070007]; Yunnan Fundamental Research Project[2020-00452]; Swedish Research Council[12235010]; National Natural Science Foundation of China[2020SKA0120300]; National SKA Program of China[23JC1402700]; Science and Technology Commission of Shanghai Municipality
项目资助者	Research Grants Council, University Grants Committee ((sic)(sic)(sic)(sic)(sic))https://doi.org/10.13039/501100002920 ; Shanghai Jiao Tong University via the Fellowship of Outstanding PhD Graduates[14300320, 14304322] ; Research Grant Council of the Hong Kong Special Administrative Region, China[12288102, 12473031, 12393811] ; National Natural Science Foundation of China (NSFC)[202201BC070003] ; Natural Science Foundation of Yunnan Province[202401BC070007] ; Yunnan Fundamental Research Project[2020-00452] ; Swedish Research Council[12235010] ; National Natural Science Foundation of China[2020SKA0120300] ; National SKA Program of China[23JC1402700] ; Science and Technology Commission of Shanghai Municipality
语种	英语
学科领域	天文学 ; 恒星与银河系
文章类型	Article
出版者	IOP Publishing Ltd
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN	0004-637X
URL	查看原文
WOS记录号	WOS:001403371500001
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	STRONGLY INTERACTING MATTER ; CORE-COLLAPSE ; QUARK MATTER ; PROGENITOR DEPENDENCE ; STATE ; SIMULATIONS ; EQUATIONS ; REVIVAL ; SIGNAL ; SHOCK
引用统计
文献类型	期刊论文
版本	出版稿
条目标识符	http://ir.ynao.ac.cn/handle/114a53/28065
专题	大样本恒星演化研究组
作者单位	1.Department of Physics, the Chinese University of Hong Kong, Hong Kong S. A. R., People's Republic of China; 2.Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming 650216, People's Republic of China; [email protected]; 3.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China; 4.The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden; 5.School of Physics and Astronomy, Shanghai Key Laboratory for Particle Physics and Cosmology, and Key Laboratory for Particle Astrophysics and Cosmology (MOE), Shanghai Jiao Tong University, Shanghai 200240, People's Republic of China
推荐引用方式 GB/T 7714	Huang, Xu-Run,Cha S,Chu, Ming-chung,et al. Phase-transition-induced Collapse of Proto-compact Stars and Its Implication for Supernova Explosions[J]. ASTROPHYSICAL JOURNAL,2025,979(2).
APA	Huang, Xu-Run,查帅,Chu, Ming-chung,O'Connor, Evan P.,&Chen, Lie-Wen.(2025).Phase-transition-induced Collapse of Proto-compact Stars and Its Implication for Supernova Explosions.ASTROPHYSICAL JOURNAL,979(2).
MLA	Huang, Xu-Run,et al."Phase-transition-induced Collapse of Proto-compact Stars and Its Implication for Supernova Explosions".ASTROPHYSICAL JOURNAL 979.2(2025).

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