• 文献检索
  • 文档翻译
  • 深度研究
  • 学术资讯
  • Suppr Zotero 插件Zotero 插件
  • 邀请有礼
  • 套餐&价格
  • 历史记录
应用&插件
Suppr Zotero 插件Zotero 插件浏览器插件Mac 客户端Windows 客户端微信小程序
定价
高级版会员购买积分包购买API积分包
服务
文献检索文档翻译深度研究API 文档MCP 服务
关于我们
关于 Suppr公司介绍联系我们用户协议隐私条款
关注我们

Suppr 超能文献

核心技术专利:CN118964589B侵权必究
粤ICP备2023148730 号-1Suppr @ 2026

文献检索

告别复杂PubMed语法,用中文像聊天一样搜索,搜遍4000万医学文献。AI智能推荐,让科研检索更轻松。

立即免费搜索

文件翻译

保留排版,准确专业,支持PDF/Word/PPT等文件格式,支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述,25分钟生成高质量综述,智能提取关键信息,辅助科研写作。

立即免费体验

星际碳质颗粒上氢形成过程中的能量分配。分子动力学模拟的见解。

Energy partitioning in H formation on interstellar carbonaceous grains. Insights from molecular dynamics simulations.

作者信息

Jubert Léana, Martínez-Bachs Berta, Pareras Gerard, Rimola Albert

机构信息

Departament de Química, Universitat Autònoma de Barcelona, Bellaterra 08193, Catalonia, Spain.

Accademia delle Scienze di Torino, Via Maria Vittoria, 3, 10123 Torino, Italy.

出版信息

Phys Chem Chem Phys. 2025 Jul 7. doi: 10.1039/d5cp01585e.

DOI:10.1039/d5cp01585e
PMID:40620133
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC12230782/
Abstract

Molecular hydrogen (H) stands as the most abundant molecule within the interstellar medium (ISM), primarily originating from the coupling of two H atoms on the surfaces of dust grains. The role of dust grains during the H formation is of third bodies, dissipating the nascent reaction energy and thereby stabilizing the newly formed molecule and preventing it from dissociating back. Whether the formed H remains adsorbed or not on the surface (in this latter case undergoing chemical desorption, CD) largely depends on the type of grain and its capability to absorb the reaction energy excess. In diffuse interstellar clouds, dust grains are typically bare and are composed primarily of silicates or carbonaceous materials, while in denser regions they are covered in ices mostly of water. While water-ice-covered grains have been elucidated to be efficient third bodies, the behavior of carbonaceous grains is still unknown. In this study, molecular dynamics (AIMD) simulations are employed to analyze how the reaction energy is distributed between the newly formed H and a large graphene slab, as a model of carbonaceous grains in diffuse clouds, and assess the feasibility of CD. The results indicate that only a fraction of the reaction energy is absorbed by the surface, leaving the newly formed H with sufficient internal energy for CD to occur.

摘要

分子氢(H₂)是星际介质(ISM)中最丰富的分子,主要源于尘埃颗粒表面两个氢原子的耦合。尘埃颗粒在H₂形成过程中起到第三体的作用,消散新生反应能量,从而稳定新形成的分子并防止其解离回去。形成的H₂是否仍吸附在表面(在后一种情况下会发生化学解吸,CD)很大程度上取决于颗粒的类型及其吸收多余反应能量的能力。在弥漫星际云中,尘埃颗粒通常是裸露的,主要由硅酸盐或碳质材料组成,而在密度较大的区域,它们被 mostly of water 冰覆盖。虽然已阐明被水冰覆盖的颗粒是有效的第三体,但碳质颗粒的行为仍然未知。在本研究中,采用分子动力学(AIMD)模拟来分析反应能量如何在新形成的H₂和作为弥漫云中碳质颗粒模型的大石墨烯平板之间分布,并评估化学解吸的可行性。结果表明,只有一部分反应能量被表面吸收,使新形成的H₂具有足够的内能以发生化学解吸。 注:原文中“ices mostly of water”表述有误,推测可能是“ices mostly of water ice”,翻译时按推测内容翻译为“被水冰覆盖”。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/eb958ec1c218/d5cp01585e-f5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/01c772c9a3bd/d5cp01585e-f1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/b4ff31797ed6/d5cp01585e-f2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/c899f692f386/d5cp01585e-f3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/158e4d179503/d5cp01585e-f4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/eb958ec1c218/d5cp01585e-f5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/01c772c9a3bd/d5cp01585e-f1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/b4ff31797ed6/d5cp01585e-f2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/c899f692f386/d5cp01585e-f3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/158e4d179503/d5cp01585e-f4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d07e/12230782/eb958ec1c218/d5cp01585e-f5.jpg

相似文献

1
Energy partitioning in H formation on interstellar carbonaceous grains. Insights from molecular dynamics simulations.星际碳质颗粒上氢形成过程中的能量分配。分子动力学模拟的见解。
Phys Chem Chem Phys. 2025 Jul 7. doi: 10.1039/d5cp01585e.
2
IR-Induced CO Photodesorption from Pure CO Ice and CO on Amorphous Solid Water.红外诱导的纯一氧化碳冰及无定形固态水中一氧化碳的光解吸
ACS Earth Space Chem. 2025 May 22;9(6):1607-1621. doi: 10.1021/acsearthspacechem.5c00040. eCollection 2025 Jun 19.
3
The Black Book of Psychotropic Dosing and Monitoring.《精神药物剂量与监测黑皮书》
Psychopharmacol Bull. 2024 Jul 8;54(3):8-59.
4
Sexual Harassment and Prevention Training性骚扰与预防培训
5
Short-Term Memory Impairment短期记忆障碍
6
Idiopathic (Genetic) Generalized Epilepsy特发性(遗传性)全身性癫痫
7
Signs and symptoms to determine if a patient presenting in primary care or hospital outpatient settings has COVID-19.在基层医疗机构或医院门诊环境中,如果患者出现以下症状和体征,可判断其是否患有 COVID-19。
Cochrane Database Syst Rev. 2022 May 20;5(5):CD013665. doi: 10.1002/14651858.CD013665.pub3.
8
Autistic Students' Experiences of Employment and Employability Support while Studying at a UK University.自闭症学生在英国大学学习期间的就业经历及就业支持情况
Autism Adulthood. 2025 Apr 3;7(2):212-222. doi: 10.1089/aut.2024.0112. eCollection 2025 Apr.
9
"In a State of Flow": A Qualitative Examination of Autistic Adults' Phenomenological Experiences of Task Immersion.“心流状态”:对自闭症成年人任务沉浸现象学体验的质性研究
Autism Adulthood. 2024 Sep 16;6(3):362-373. doi: 10.1089/aut.2023.0032. eCollection 2024 Sep.
10
Management of urinary stones by experts in stone disease (ESD 2025).结石病专家对尿路结石的管理(2025年结石病专家共识)
Arch Ital Urol Androl. 2025 Jun 30;97(2):14085. doi: 10.4081/aiua.2025.14085.

本文引用的文献

1
Ab-initio dynamic study of mechanisms for dust-mediated molecular hydrogen formation in space.空间中尘埃介导分子氢形成机制的从头算动力学研究。
Commun Chem. 2025 Apr 1;8(1):97. doi: 10.1038/s42004-025-01489-z.
2
Formation of Methanol via Fischer-Tropsch Catalysis by Cosmic Iron Sulphide.通过宇宙硫化铁的费托催化作用形成甲醇。
Chemphyschem. 2024 Sep 2;25(17):e202400272. doi: 10.1002/cphc.202400272. Epub 2024 Jul 12.
3
Quantum Tunnelling Driven H Formation on Graphene.量子隧穿驱动石墨烯上氢的形成。
J Phys Chem Lett. 2022 Apr 14;13(14):3173-3181. doi: 10.1021/acs.jpclett.2c00520. Epub 2022 Apr 1.
4
Non-energetic Formation of Ethanol via CCH Reaction with Interstellar HO Ices. A Computational Chemistry Study.通过星际HO冰与CCH反应非能量驱动形成乙醇。一项计算化学研究。
ACS Earth Space Chem. 2022 Mar 17;6(3):496-511. doi: 10.1021/acsearthspacechem.1c00369. Epub 2022 Mar 7.
5
CP2K: An electronic structure and molecular dynamics software package - Quickstep: Efficient and accurate electronic structure calculations.CP2K:一个电子结构与分子动力学软件包 - Quickstep:高效且精确的电子结构计算
J Chem Phys. 2020 May 21;152(19):194103. doi: 10.1063/5.0007045.
6
Quantification of the Role of Chemical Desorption in Molecular Clouds.分子云中化学解吸作用的量化
Acc Chem Res. 2021 Feb 16;54(4):745-753. doi: 10.1021/acs.accounts.0c00636. Epub 2021 Jan 27.
7
TRAVIS-A free analyzer for trajectories from molecular simulation.TRAVIS - 一款用于分子模拟轨迹的免费分析工具。
J Chem Phys. 2020 Apr 30;152(16):164105. doi: 10.1063/5.0005078.
8
Influence of surface coverage on the chemical desorption process.表面覆盖率对化学解吸过程的影响。
J Chem Phys. 2014 Jul 7;141(1):014304. doi: 10.1063/1.4885847.
9
Diffusion, adsorption, and desorption of molecular hydrogen on graphene and in graphite.分子氢在石墨烯和石墨上的扩散、吸附和脱附。
J Chem Phys. 2013 Jul 28;139(4):044706. doi: 10.1063/1.4813919.
10
Insights into H2 formation in space from ab initio molecular dynamics.从从头算分子动力学角度看空间中 H2 的形成。
Proc Natl Acad Sci U S A. 2013 Apr 23;110(17):6674-7. doi: 10.1073/pnas.1301433110. Epub 2013 Apr 9.