Michael Gatchell, Raka Paul, MingChao Ji, Stefan Rosén, Richard D. Thomas, Henrik Cederquist, Henning T. Schmidt, Åsa Larson, Henning Zettergren
{"title":"C$_{60}^+$ 和 C$_{60}^-$ 离子的相互中和:激发能量和状态选择性速率系数","authors":"Michael Gatchell, Raka Paul, MingChao Ji, Stefan Rosén, Richard D. Thomas, Henrik Cederquist, Henning T. Schmidt, Åsa Larson, Henning Zettergren","doi":"arxiv-2409.11851","DOIUrl":null,"url":null,"abstract":"Context: Mutual neutralization between cations and anions play an important\nrole in determining the charge-balance in certain astrophysical environments.\nHowever, empirical data for such reactions involving complex molecular species\nhas been lacking due to challenges in performing experimental studies, leaving\nthe astronomical community to rely on decades old models with large\nuncertainties for describing these processes in the interstellar medium. Aims:\nTo investigate the mutual neutralization (MN) reaction, C$_{60}^+$ + C$_{60}^-$\n$\\rightarrow$ C$_{60}^*$ + C$_{60}$, for collisions at interstellar-like\nconditions. Methods: The mutual neutralization reaction between C$_{60}^+$ and\nC$_{60}^-$ at collision energies of 100\\,meV was studied using the Double\nElectroStatic Ion Ring ExpEriment, DESIREE, and its merged-beam capabilities.\nTo aid in the interpretation of the experimental results, semi-classical\nmodeling based on the Landau-Zener approach was performed for the studied\nreaction. Results: We experimentally identify a narrow range of kinetic\nenergies for the neutral reaction products. Modeling was used to calculate the\nquantum state-selective reaction probabilities, absolute cross sections, and\nrate coefficients of these MN reactions, using the experimental results as a\nbenchmark. The MN cross sections are compared with model results for electron\nattachment to C$_{60}$ and electron recombination with C$_{60}^+$. Conclusions:\nThe present results show that it is crucial to take mutual polarization\neffects, the finite sizes, and the final quantum states of both molecular ions\ninto account for reliable predictions of MN rates expected to strongly\ninfluence the charge-balance and chemistry in, e.g., dense molecular clouds.","PeriodicalId":501304,"journal":{"name":"arXiv - PHYS - Chemical Physics","volume":"17 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Mutual neutralization of C$_{60}^+$ and C$_{60}^-$ ions: Excitation energies and state-selective rate coefficients\",\"authors\":\"Michael Gatchell, Raka Paul, MingChao Ji, Stefan Rosén, Richard D. Thomas, Henrik Cederquist, Henning T. Schmidt, Åsa Larson, Henning Zettergren\",\"doi\":\"arxiv-2409.11851\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Context: Mutual neutralization between cations and anions play an important\\nrole in determining the charge-balance in certain astrophysical environments.\\nHowever, empirical data for such reactions involving complex molecular species\\nhas been lacking due to challenges in performing experimental studies, leaving\\nthe astronomical community to rely on decades old models with large\\nuncertainties for describing these processes in the interstellar medium. Aims:\\nTo investigate the mutual neutralization (MN) reaction, C$_{60}^+$ + C$_{60}^-$\\n$\\\\rightarrow$ C$_{60}^*$ + C$_{60}$, for collisions at interstellar-like\\nconditions. Methods: The mutual neutralization reaction between C$_{60}^+$ and\\nC$_{60}^-$ at collision energies of 100\\\\,meV was studied using the Double\\nElectroStatic Ion Ring ExpEriment, DESIREE, and its merged-beam capabilities.\\nTo aid in the interpretation of the experimental results, semi-classical\\nmodeling based on the Landau-Zener approach was performed for the studied\\nreaction. Results: We experimentally identify a narrow range of kinetic\\nenergies for the neutral reaction products. Modeling was used to calculate the\\nquantum state-selective reaction probabilities, absolute cross sections, and\\nrate coefficients of these MN reactions, using the experimental results as a\\nbenchmark. The MN cross sections are compared with model results for electron\\nattachment to C$_{60}$ and electron recombination with C$_{60}^+$. Conclusions:\\nThe present results show that it is crucial to take mutual polarization\\neffects, the finite sizes, and the final quantum states of both molecular ions\\ninto account for reliable predictions of MN rates expected to strongly\\ninfluence the charge-balance and chemistry in, e.g., dense molecular clouds.\",\"PeriodicalId\":501304,\"journal\":{\"name\":\"arXiv - PHYS - Chemical Physics\",\"volume\":\"17 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-18\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Chemical Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.11851\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Chemical Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.11851","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Mutual neutralization of C$_{60}^+$ and C$_{60}^-$ ions: Excitation energies and state-selective rate coefficients
Context: Mutual neutralization between cations and anions play an important
role in determining the charge-balance in certain astrophysical environments.
However, empirical data for such reactions involving complex molecular species
has been lacking due to challenges in performing experimental studies, leaving
the astronomical community to rely on decades old models with large
uncertainties for describing these processes in the interstellar medium. Aims:
To investigate the mutual neutralization (MN) reaction, C$_{60}^+$ + C$_{60}^-$
$\rightarrow$ C$_{60}^*$ + C$_{60}$, for collisions at interstellar-like
conditions. Methods: The mutual neutralization reaction between C$_{60}^+$ and
C$_{60}^-$ at collision energies of 100\,meV was studied using the Double
ElectroStatic Ion Ring ExpEriment, DESIREE, and its merged-beam capabilities.
To aid in the interpretation of the experimental results, semi-classical
modeling based on the Landau-Zener approach was performed for the studied
reaction. Results: We experimentally identify a narrow range of kinetic
energies for the neutral reaction products. Modeling was used to calculate the
quantum state-selective reaction probabilities, absolute cross sections, and
rate coefficients of these MN reactions, using the experimental results as a
benchmark. The MN cross sections are compared with model results for electron
attachment to C$_{60}$ and electron recombination with C$_{60}^+$. Conclusions:
The present results show that it is crucial to take mutual polarization
effects, the finite sizes, and the final quantum states of both molecular ions
into account for reliable predictions of MN rates expected to strongly
influence the charge-balance and chemistry in, e.g., dense molecular clouds.