Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на этот ресурс: http://elar.urfu.ru/handle/10995/130804
Полная запись метаданных
Поле DCЗначениеЯзык
dc.contributor.authorBulak, M.en
dc.contributor.authorPaardekooper, D. M.en
dc.contributor.authorFedoseev, G.en
dc.contributor.authorSamarth, P.en
dc.contributor.authorLinnartz, H.en
dc.date.accessioned2024-04-05T16:33:07Z-
dc.date.available2024-04-05T16:33:07Z-
dc.date.issued2023-
dc.identifier.citationBulak, M, Paardekooper, D, Fedoseev, G, Samarth, P & Linnartz, H 2023, 'Disentangling UV photodesorption and photoconversion rates of H2O ice at 20 K: Measured with laser desorption post ionization mass spectrometry', Astronomy and Astrophysics, Том. 677, A99. https://doi.org/10.1051/0004-6361/202245273harvard_pure
dc.identifier.citationBulak, M., Paardekooper, D., Fedoseev, G., Samarth, P., & Linnartz, H. (2023). Disentangling UV photodesorption and photoconversion rates of H2O ice at 20 K: Measured with laser desorption post ionization mass spectrometry. Astronomy and Astrophysics, 677, [A99]. https://doi.org/10.1051/0004-6361/202245273apa_pure
dc.identifier.issn0004-6361-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Hybrid Gold3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85172410960&doi=10.1051%2f0004-6361%2f202245273&partnerID=40&md5=81224430a8676a94a060b9b54ae987611
dc.identifier.otherhttps://www.aanda.org/articles/aa/pdf/forth/aa45273-22.pdfpdf
dc.identifier.urihttp://elar.urfu.ru/handle/10995/130804-
dc.description.abstractContext. The nondissociative ultraviolet photodesorption of water ice is a nonthermal desorption mechanism required to account for detected abundances of gas-phase water toward cold regions within the interstellar medium. Previous experimental and theoretical studies provide a range of photodesorption rates for H2O ice and point to a convoluted competition with other molecular processes following the absorption of a UV photon in the ice. Ultraviolet irradiation also induces photodissociation, resulting in the formation of radicals that may directly desorb triggering gas-phase reactions or recombine in surface reactions. Aims. In this work, we aim to quantify the effects of photodesorption and investigate photoconversion upon UV photolysis of an H2O ice. Methods. We irradiated a porous amorphous H2O ice at 20 K with UV photons in the 7-10.2 eV range and compared the measurements to a nearly identical experiment that included a layer of argon coating on top of the water ice. The purpose of the argon coating is to quench any type of photon-triggered desorption. To trace ice composition and thickness, laser desorption post ionization time-of-flight mass spectrometry was utilized. This method is independent of the (non)dissociative character of a process and provides a diagnostic tool different from earlier studies that allows an independent check. Results. The total photodesorption rate for a porous amorphous H2O ice at 20 K we derive is (1.0 ± 0.2) × 10-3 per incident UV photon (7-10.2 eV), which is in agreement with the available literature. This rate is based on the elemental balance of oxygen-bearing species. As a result, we placed an upper limit on the intact (H2O) and dissociative (OH) desorption rates equal to 1.0 × 10-3 per incident UV photon, while for the reactive desorption (O2), this limit is equal to 0.5 × 10-3 per incident UV photon. Photoconversion depletes the H2O ice at a rate of (2.3 ± 0.2) × 10-3 per incident UV photon. At low UV fluence (9.0 × 1017 photons cm-2), the loss of H2O is balanced by photoproduct formation (O2 and H2O2). At high UV fluence (4.5 × 1018 photons cm-2), about 50% of the initial H2O molecules are depleted. This amount is not matched by the registered O-bearing products, which points to an additional, unaccounted loss channel of H2O. © The Authors 2023.en
dc.description.sponsorshipH2020 Marie Skłodowska-Curie Actions, MSCA: 722346; European Commission, EC; Horizon 2020; Ministry of Science and Higher Education of the Russian Federation: FEUZ-2020-0038en
dc.description.sponsorshipM.B. and H.L. acknowledge the European Union (EU) and Horizon 2020 funding awarded under the Marie Skłodowska-Curie action to the EUROPAH consortium (grant number 722346) as well as NOVA 5 funding. Additional funding has been realized through a NWO-VICI grant. G.F. acknowledges financial support from the Russian Ministry of Science and Higher Education via the State Assignment Contract FEUZ-2020-0038. The authors acknowledge Andreas Riedo for initial experiments for this project and A.G.G.M. Tielens as well as M. Bertin for helpful discussions and feedback.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.rightscc-byother
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/unpaywall
dc.sourceAstronomy & Astrophysics2
dc.sourceAstronomy and Astrophysicsen
dc.subjectASTROCHEMISTRYen
dc.subjectISM: MOLECULESen
dc.subjectMETHODS: LABORATORY: SOLID STATEen
dc.subjectMOLECULAR PROCESSESen
dc.subjectPROTOPLANETARY DISKSen
dc.subjectULTRAVIOLET: ISMen
dc.subjectCOATINGSen
dc.subjectGASESen
dc.subjectICEen
dc.subjectIONIZATION OF GASESen
dc.subjectIRRADIATIONen
dc.subjectMASS SPECTROMETRYen
dc.subjectMOLECULESen
dc.subjectPHASE INTERFACESen
dc.subjectPHOTODISSOCIATIONen
dc.subjectPHOTOIONIZATIONen
dc.subjectPHOTOLYSISen
dc.subjectPHOTONSen
dc.subjectSURFACE REACTIONSen
dc.subjectASTROCHEMISTRYen
dc.subjectISM:MOLECULESen
dc.subjectMETHOD: LABORATORY: SOLID STATEen
dc.subjectMETHODS:LABORATORYen
dc.subjectMOLECULAR PROCESSen
dc.subjectPHOTO-DESORPTIONen
dc.subjectPHOTOCONVERSIONen
dc.subjectPROTOPLANETARY DISKSen
dc.subjectULTRAVIOLET: ISMen
dc.subjectUV PHOTONSen
dc.subjectDESORPTIONen
dc.titleDisentangling UV photodesorption and photoconversion rates of H2O ice at 20 K: Measured with laser desorption post ionization mass spectrometryen
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.type|info:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1051/0004-6361/202245273-
dc.identifier.scopus85172410960-
local.contributor.employeeBulak, M., Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, Leiden, 2300 RA, Netherlandsen
local.contributor.employeePaardekooper, D.M., Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, Leiden, 2300 RA, Netherlandsen
local.contributor.employeeFedoseev, G., Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, Leiden, 2300 RA, Netherlands, Research Laboratory for Astrochemistry, Ural Federal University, Kuibysheva St. 48, Ekaterinburg, 620026, Russian Federationen
local.contributor.employeeSamarth, P., Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, Leiden, 2300 RA, Netherlandsen
local.contributor.employeeLinnartz, H., Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, Leiden, 2300 RA, Netherlandsen
local.volume677-
dc.identifier.wos001067113700007-
local.contributor.departmentLaboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, Leiden, 2300 RA, Netherlandsen
local.contributor.departmentResearch Laboratory for Astrochemistry, Ural Federal University, Kuibysheva St. 48, Ekaterinburg, 620026, Russian Federationen
local.identifier.pure45995335-
local.description.orderA99-
local.identifier.eid2-s2.0-85172410960-
local.identifier.wosWOS:001067113700007-
Располагается в коллекциях:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

Файлы этого ресурса:
Файл Описание РазмерФормат 
2-s2.0-85172410960.pdf915,9 kBAdobe PDFПросмотреть/Открыть


Лицензия на ресурс: Лицензия Creative Commons Creative Commons