@article{GerlachMonningerSchleieretal.2021, author = {Gerlach, Marius and Monninger, Sophie and Schleier, Domenik and Hemberger, Patrick and Goettel, James T. and Braunschweig, Holger and Fischer, Ingo}, title = {Photoelectron Photoion Coincidence Spectroscopy of NCl\(_{3}\) and NCl\(_{2}\)}, series = {ChemPhysChem}, volume = {22}, journal = {ChemPhysChem}, number = {21}, doi = {10.1002/cphc.202100537}, url = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-257322}, pages = {2164-2167}, year = {2021}, abstract = {We investigate NCl\(_{3}\) and the NCl\(_{2}\) radical by photoelectron-photoion coincidence spectroscopy using synchrotron radiation. The mass selected threshold photoelectron spectrum (ms-TPES) of NCl\(_{3}\) is broad and unstructured due to the large geometry change. An ionization energy of 9.7±0.1 eV is estimated from the spectrum and supported by computations. NCl2 is generated by photolysis at 213 nm from NCl\(_{3}\) and its ms-TPES shows an extended vibrational progression with a 90 meV spacing that is assigned to the symmetric N-Cl stretching mode in the cation. An adiabatic ionization energy of 9.94 ± 0.02 eV is determined.}, language = {en} } @article{ReuschHolzmeierGerlachetal.2019, author = {Reusch, Engelbert and Holzmeier, Fabian and Gerlach, Marius and Fischer, Ingo and Hemberger, Patrick}, title = {Decomposition of Picolyl Radicals at High Temperature: A Mass Selective Threshold Photoelectron Spectroscopy Study}, series = {Chemistry - A European Journal}, volume = {25}, journal = {Chemistry - A European Journal}, number = {72}, doi = {10.1002/chem.201903937}, url = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-208132}, pages = {16652-16659}, year = {2019}, abstract = {The reaction products of the picolyl radicals at high temperature were characterized by mass-selective threshold photoelectron spectroscopy in the gas phase. Aminomethylpyridines were pyrolyzed to initially produce picolyl radicals (m /z =92). At higher temperatures further thermal reaction products are generated in the pyrolysis reactor. All compounds were identified by mass-selected threshold photoelectron spectroscopy and several hitherto unexplored reactive molecules were characterized. The mechanism for several dissociation pathways was outlined in computations. The spectrum of m /z =91, resulting from hydrogen loss of picolyl, shows four isomers, two ethynyl pyrroles with adiabatic ionization energies (IE\(_{ad}\)) of 7.99 eV (2-ethynyl-1H -pyrrole) and 8.12 eV (3-ethynyl-1H -pyrrole), and two cyclopentadiene carbonitriles with IE′s of 9.14 eV (cyclopenta-1,3-diene-1-carbonitrile) and 9.25 eV (cyclopenta-1,4-diene-1-carbonitrile). A second consecutive hydrogen loss forms the cyanocyclopentadienyl radical with IE′s of 9.07 eV (T\(_0\)) and 9.21 eV (S\(_1\)). This compound dissociates further to acetylene and the cyanopropynyl radical (IE=9.35 eV). Furthermore, the cyclopentadienyl radical, penta-1,3-diyne, cyclopentadiene and propargyl were identified in the spectra. Computations indicate that dissociation of picolyl proceeds initially via a resonance-stabilized seven-membered ring.}, language = {en} } @article{SchleierGerlachPratimMukhopadhyayetal.2022, author = {Schleier, Domenik and Gerlach, Marius and Pratim Mukhopadhyay, Deb and Karaev, Emil and Schaffner, Dorothee and Hemberger, Patrick and Fischer, Ingo}, title = {Ammonia Borane, NH\(_{3}\)BH\(_{3}\): A Threshold Photoelectron-Photoion Coincidence Study of a Potential Hydrogen-Storage Material}, series = {Chemistry-A European Journal}, volume = {28}, journal = {Chemistry-A European Journal}, number = {42}, doi = {10.1002/chem.202201378}, url = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-318895}, year = {2022}, abstract = {We have investigated the photoionization of ammonia borane (AB) and determined adiabatic ionization energy to be 9.26±0.03 eV for the X\(^{+}\) \(^{2}\)E←X \(^{1}\)A\(_{1}\) transition. Although the threshold photoelectron spectrum appears at first glance to be similar to the one of the isosteric ethane, the electronic situation differs markedly, due to different orbital energies. In addition, an appearance energy AE\(_{0K}\)-(NH\(_{3}\)BH\(_{3}\), NH\(_{3}\)BH\(_{2}\)\(^{+}\))= 10.00±0.03 eV has been determined, corresponding to the loss of a hydrogen atom at the BH\(_{3}\)-site. From the data, a 0 K bond dissociation energy for the B-H bond in the cation of 71.5±3 kJ mol\(^{-1}\) was derived, whereas the one in the neutral compound has been estimated to be 419±10 kJ mol\(^{-1}\).}, language = {en} } @phdthesis{Gerlach2023, author = {Gerlach, Marius David}, title = {Spectroscopy of fulminic acid HCNO with VUV- and soft X-ray radiation}, doi = {10.25972/OPUS-32972}, url = {http://nbn-resolving.de/urn:nbn:de:bvb:20-opus-329722}, school = {Universit{\"a}t W{\"u}rzburg}, year = {2023}, abstract = {Die Fulmins{\"a}ure HCNO wurde zum ersten Mal im Jahre 1800 synthetisiert und wurde seitdem immer wieder verwendet, um neue chemische Konzepte und Theorien zu entwickeln. Durch die erstmalige Entdeckung der Fulmins{\"a}ure im Weltall im Jahr 2009 ist die Fulmins{\"a}ure heutzutage vor allem im Bereich der Astrochemie interessant. In dieser Doktorarbeit haben wir die Interaktion von Fulmins{\"a}ure mit interstellar Strahlung, genauer mit VUV- sowie weicher R{\"o}ntgenstrahlung untersucht. In Zuge der Messung mit VUV-Strahlung konnten wir das Photoelektronenspektrum von HCNO mit hoher Aufl{\"o}sung aufnehmen und den Renner-Teller verzerrten Grundzustand des Kations mit Hilfe von Wellenpaketdynamiksimulationen beschreiben. Außerdem konnten wir den Mechanismus der dissoziativen Photoionisation bis zu einer Bindungsenergie von 15.3 eV aufkl{\"a}ren. Mit weicher R{\"o}ntgenstrahlung ist es m{\"o}glich die 1s Elektronen des HCNO zu ionisieren oder anzuregen. Der erzeugte Zustand zerf{\"a}llt anschließend durch einen Auger-Meitner Prozess, bei dem ein Auger-Elektron erzeugt wird. Im Zuge der Auger-Elektronenspektroskopie haben wir die kinetische Energie dieser Elektronen gemessen und konnten mittels quantenchemischer Rechnung die beobachten Signale analysieren. Wir untersuchten außerdem, wie das durch den Auger-Meitner Prozess erzeugte Ion zerf{\"a}llt. Hier konnten wir eine Selektivit{\"a}t des Zerfalls beobachten, je nachdem welches der 1s Elektronen im ersten Schritt angeregt oder ionisiert wurde. Diese Beobachtung konnten wir durch ein einfaches thermodynamisches Argument erkl{\"a}ren. Diese Arbeit gibt also ein vollst{\"a}ndiges Bild {\"u}ber die Interaktion von HCNO mit ionisierender Strahlung. Die erhaltenen Daten k{\"o}nnten f{\"u}r die Beschreibung von HCNO im interstellaren Raum Bedeutung haben.}, subject = {Chemie}, language = {en} }