Chin. Phys. Lett.  2017, Vol. 34 Issue (4): 049701    DOI: 10.1088/0256-307X/34/4/049701
GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS |
Nucleosynthesis in Advection-Dominated Accretion Flow onto a Black Hole
Jiang Zhang1,2**, Ren-Yi Ma3**, Hong-Jie Li4, Bo Zhang5
1Department of Mathematics and Science, Hebei GEO University, Shijiazhuang 050016
2Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011
3Department of Astronomy, Xiamen University, Xiamen 361005
4School of Sciences, Hebei University of Science and Technology, Shijiazhuang 050016
5Department of Physics, Hebei Normal University, Shijiazhuang 050016
Cite this article:   
Jiang Zhang, Ren-Yi Ma, Hong-Jie Li et al  2017 Chin. Phys. Lett. 34 049701
Download: PDF(3091KB)   PDF(mobile)(3059KB)   HTML
Export: BibTeX | EndNote | Reference Manager | ProCite | RefWorks
Abstract Nucleosynthesis in advection-dominated accretion flow (ADAF) onto a black hole is proposed to be an important role in chemical evolution around compact stars. We investigate the nucleosynthesis in ADAF relevant for a black hole of low mass, different from that of the self-similar solution. In particular, the presence of supersolar metal mass fractions of some isotopes seems to be associated with the known black hole nucleosynthesis in ADAF, which offers further evidence of diversity of the chemical enrichment.
Received: 15 December 2016      Published: 21 March 2017
PACS:  97.10.Cv (Stellar structure, interiors, evolution, nucleosynthesis, ages)  
  26.40.+r (Cosmic ray nucleosynthesis)  
  97.10.Tk (Abundances, chemical composition)  
Fund: Supported by the National Natural Science Foundation of China under Grant Nos 11547041, 11403007, 11673007, 11643007, 11333004, U1531130, 11673059, 11390374 and 11521303, and the Chinese Academy of Sciences under Grant Nos KJZD-EW-M06-01 and QYZDB-SSW-SYS001.
TRENDMD:   
URL:  
http://cpl.iphy.ac.cn/10.1088/0256-307X/34/4/049701       OR      http://cpl.iphy.ac.cn/Y2017/V34/I4/049701
Service
E-mail this article
E-mail Alert
RSS
Articles by authors
Jiang Zhang
Ren-Yi Ma
Hong-Jie Li
Bo Zhang
[1]Burbidge M, Burbidge G R, Fowler W and Hoyle F 1957 Rev. Mod. Phys. 29 547
[2]Busso M, Gallino R and Wasserburg G J 1999 Annu. Rev. Astron. Astrophys. 37 239
[3]Arnould M, Goriely S and Takahashi K 2007 Phys. Rep. 450 97
[4]Han Z and Podsiadlowski Ph 2004 Mon. Not. R. Astron. Soc. 350 1301
[5]Wang B and Han Z 2012 New Astron. Rev. 56 122
[6]Shakura N I and Sunyaev R A 1973 Astron. Astrophys. 24 337
[7]Narayan R and Yi I 1994 Astrophys. J. 428 L13
[8]Narayan R, Kato S and Honma F 1997 Astrophys. J. 476 49
[9]Banerjee I and Mukhopadhyay B 2013 Astrophys. J. 778 8
[10]Mukhopadhyay B and Chakrabarti S K 2000 Astron. Astrophys. 353 1029
[11]Surman R McLaughlin G C and Sabbatino N 2011 Astrophys. J. 743 155
[12]Hu T and Peng Q H 2008 Astrophys. J. 681 96
[13]Yuan F, Quataert E and Narayan R 2003 Astrophys. J. 598 301
[14]Timmes F X 1999 Astrophys. J. Suppl. Ser. 124 241
[15]Timmes F X, Hoffman R D and Woosley S E 2000 Astrophys. J. Suppl. Ser. 129 377
[16]Savaglio S, Rau A, Greiner J et al 2012 Mon. Not. R. Astron. Soc. 420 627
[17]Xu Y D and Cao X 2010 Astrophys. J. 716 1423
[18]Zhang H, Wang Y, Yuan F, Ding F, Luo X and Peng Q H 2009 Astron. Astrophys. 502 419
[19]Zhang J, Wang B, Zhang B and Han Z 2012 Chin. Phys. Lett. 29 019701
[20]Wang J T and Song H F 2016 Chin. Phys. Lett. 33 099702
Related articles from Frontiers Journals
[1] Zhi Li, Han-Feng Song, Wei-Guo Peng. Effect of Tidal Torques on Rotational Mixing in Close Binaries[J]. Chin. Phys. Lett., 2018, 35(7): 049701
[2] Jiang-Tao Wang, Han-Feng Song. The Pulsation Induced by Mass Transfer in Critically Rotating Stars[J]. Chin. Phys. Lett., 2016, 33(09): 049701
[3] ZHANG Jiang, **, WANG Bo, ZHANG Bo, HAN Zhan-Wen,. Reanalysis of the Isotopic Mixture of Neutron-Capture Elements in the Metal-Poor Star HD 175305[J]. Chin. Phys. Lett., 2012, 29(1): 049701
[4] CUI Dong-Nuan, GENG Yuan-Yuan, CUI Wen-Yuan, ZHANG Bo. Mass Fraction of 13C-Pocket in Metal-Poor AGB Stars and the Primary Nature of Neutron Source[J]. Chin. Phys. Lett., 2009, 26(3): 049701
[5] CUI Wen-Yuan, , CUI Dong-Nuan, DU Yun-Shuang, ZHANG Bo,. Neutron-Capture Elements in the Double-Enhanced Star HE 1305-0007: a New s- and r-Process Paradigm[J]. Chin. Phys. Lett., 2007, 24(5): 049701
[6] ZHANG Feng-Hui, HAN Zhan-Wen, LI Li-Fang. Effect of the Initial Mass Function of Primaries on Binary Stellar Populations[J]. Chin. Phys. Lett., 2005, 22(4): 049701
[7] SONG Han-Feng, ZHANG Bo, ZHANG Jiang, WU Hai-Bin, PENG Qiu-He. R-Process Nucleosynthesis and Galactic Chemical Evolution of the Ba Peak Elements[J]. Chin. Phys. Lett., 2003, 20(11): 049701
[8] WANG Fei-Lu, ZHAO Gang, YUAN Jian-Min,. Density Dependence of the Detailed Spectral Line Effects on the Opacity of Astrophysical Abundant Elements: Oxygen[J]. Chin. Phys. Lett., 2003, 20(10): 049701
[9] ZHANG Miao-Jing, , ZHANG Bo, , LI Guang-Lie,. Abundance Distribution of Slow-Process Main Heavy Elements in AGB Stars[J]. Chin. Phys. Lett., 2003, 20(6): 049701
[10] ZHANG Feng-Hui, HAN Zhan-Wen, LI Li-Fang, Jarrod R. Hurley. Evolutionary Population Synthesis for Single Stellar Populations[J]. Chin. Phys. Lett., 2002, 19(11): 049701
[11] PENG Qiuhe. Are Massive Main Sequence Stars and Wolf-Rayet Stars Detectable Sources of the Intersteller Medium 26A1? [J]. Chin. Phys. Lett., 1994, 11(8): 049701
Viewed
Full text


Abstract