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Coverage dependent H2 desorption energy: a quantitative explanation based on encounter desorption mechanism
Meng, Qingkuan1; Chang, Qiang1; Zhao, Gang1; Quan, Donghui2,3; Tsuge, Masashi4; Zhang, Xia3; Zhang, Yong5; Li, Xiao-Hu3
2023-09-29
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume526Issue:2Pages:2394-2399
Contribution Rank3
AbstractRecent experiments show that the desorption energy of H-2 on a diamond-like carbon surface depends on the H-2 coverage of the surface. We aim to quantitatively explain the coverage dependent H-2 desorption energy measured by the experiments. We derive a math formula to calculate an effective H-2 desorption energy based on the encounter desorption mechanism. The effective H-2 desorption energy depends on two key parameters, the desorption energy of H-2 on H-2 substrate and the ratio of H-2 diffusion barrier to its desorption energy. The calculated effective H-2 desorption energy qualitatively agrees with the coverage dependent H-2 desorption energy measured by the experiments if the values of these two parameters in literature are used in the calculations. We argue that the difference between the effective H-2 desorption energy and the experimental results is due to the lack of knowledge about these two parameters. So, we recalculate these two parameters based on experimental data. Good agreement between theoretical and experimental results can be achieved if these two updated parameters are used in the calculations.
Keywordastrochemistry ISM: abundances ISM: molecules
DOI10.1093/mnras/stad2905
Indexed BySCI
Language英语
WOS KeywordMOLECULAR-HYDROGEN FORMATION ; SURFACE H-2 ; INTERSTELLAR ; ICE ; SIMULATION ; ABUNDANCE ; CHEMISTRY ; ATOMS
Funding ProjectNational Natural Science Foundation of China[12173023] ; National Natural Science Foundation of China[11973075] ; National Natural Science Foundation of China[11973099] ; National Natural Science Foundation of China[12203091] ; National Natural Science Foundation of China
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001159221300036
PublisherOXFORD UNIV PRESS
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5898
Collection中国科学院新疆天文台
Corresponding AuthorChang, Qiang
Affiliation1.Shandong Univ Technol, Sch Phys & Optoeletron Engn, Zibo 255000, Peoples R China
2.Zhejiang Lab, Res Ctr Intelligent Comp Platforms, Hangzhou 311100, Peoples R China
3.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
4.Hokkaido Univ, Inst Low Temp Sci, Kita 19,Nishi 8,Kita Ku, Sapporo 0600819, Japan
5.Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519082, Peoples R China
Recommended Citation
GB/T 7714
Meng, Qingkuan,Chang, Qiang,Zhao, Gang,et al. Coverage dependent H2 desorption energy: a quantitative explanation based on encounter desorption mechanism[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,526(2):2394-2399.
APA Meng, Qingkuan.,Chang, Qiang.,Zhao, Gang.,Quan, Donghui.,Tsuge, Masashi.,...&Li, Xiao-Hu.(2023).Coverage dependent H2 desorption energy: a quantitative explanation based on encounter desorption mechanism.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,526(2),2394-2399.
MLA Meng, Qingkuan,et al."Coverage dependent H2 desorption energy: a quantitative explanation based on encounter desorption mechanism".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 526.2(2023):2394-2399.
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