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@ARTICLE{Reinwardt:588803,
author = {Reinwardt, Simon and Baev, Ivan and Cieslik, Patrick and
Baev, Karolin and Buhr, Ticia and Perry-Sassmannshausen,
Alexander and Schippers, Stefan and Mueller, Alfred and
Trinter, Florian and Viefhaus, Jens and Martins, Michael},
title = {{S}oft {X}-{R}ay-induced {D}imerization of {M}ethane},
journal = {The astrophysical journal / 1},
volume = {952},
number = {1},
issn = {0004-637X},
address = {London},
publisher = {Institute of Physics Publ.},
reportid = {PUBDB-2023-04960},
pages = {39},
year = {2023},
note = {Open Access},
abstract = {Carbon 1s excitation of methane, CH4, has been studied in
the gas phase using the ion trap integrated with the
photon–ion instrument at PETRA III/DESY and soft X-rays
from the beamline P04. The created photoions are stored
within the ion trap so that in further steps the photoions
can undergo reactions with neutral methane molecules. The
ionic photoproducts as well as reaction products created
thereby are mass-over-charge analyzed by an ion
time-of-flight spectrometer. Besides the photoions, product
ions with up to three carbon atoms are found. In contrast to
experiments using vacuum ultraviolet radiation, especially
highly reactive product ions with a small number of hydrogen
atoms such as ${{\rm{C}}}_{2}{{\rm{H}}}_{2}^{+}$ and
${{\rm{C}}}_{2}{{\rm{H}}}_{3}^{+}$ are found, which are
important precursors for larger hydrocarbons such as C6H6.
Possible production routes of the product ions are analyzed
on the basis of a model that considers the probabilities for
photofragmentation and the first subsequent chemical
reaction step. The model indicates that the high degree of
fragmentation by photons with energies around 280 eV is
favoring these products. The results of the measurements
show that the products like
${{\rm{C}}}_{2}{{\rm{H}}}_{2}^{+}$ and
${{\rm{C}}}_{2}{{\rm{H}}}_{3}^{+}$ can be generated by a
single collision of the ionization product with neutral
methane. The results suggest that soft X-rays might be
important for chemical reactions in planetary atmospheres,
which has usually not been taken into account. However, due
to the high degree of fragmentation and large cross sections
involved, they can have a large influence even when the
corresponding photon flux is rather small.},
cin = {DOOR ; HAS-User / UNI/EXP / FS-PETRA-S},
ddc = {520},
cid = {I:(DE-H253)HAS-User-20120731 /
$I:(DE-H253)UNI_EXP-20120731$ /
I:(DE-H253)FS-PETRA-S-20210408},
pnm = {631 - Matter – Dynamics, Mechanisms and Control
(POF4-631) / 6G3 - PETRA III (DESY) (POF4-6G3) / DFG project
170620586 - SFB 925: Licht-induzierte Dynamik und Kontrolle
korrelierter Quantensysteme (170620586) / DFG project
245652604 - Photo-induzierte Prozesse endohedraler
Fulleren-Ionen: Experiment (245652604) / DFG project
389115454 - K-Schalen-Photoionisation negativ geladener
atomarer Ionen (389115454) / DFG project 510114039 -
Dissoziationsdynamik von rumpfniveauangeregten ionischen,
molekularen Radikalen (510114039)},
pid = {G:(DE-HGF)POF4-631 / G:(DE-HGF)POF4-6G3 /
G:(GEPRIS)170620586 / G:(GEPRIS)245652604 /
G:(GEPRIS)389115454 / G:(GEPRIS)510114039},
experiment = {EXP:(DE-H253)P-P04-20150101},
typ = {PUB:(DE-HGF)16},
UT = {WOS:001031344400001},
doi = {10.3847/1538-4357/acd937},
url = {https://bib-pubdb1.desy.de/record/588803},
}