TY - JOUR A1 - Gerlach, Marius A1 - Monninger, Sophie A1 - Schleier, Domenik A1 - Hemberger, Patrick A1 - Goettel, James T. A1 - Braunschweig, Holger A1 - Fischer, Ingo T1 - Photoelectron Photoion Coincidence Spectroscopy of NCl\(_{3}\) and NCl\(_{2}\) JF - ChemPhysChem N2 - 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. KW - radicals KW - photoelectron spectroscopy KW - synchrotron radiation KW - nitrogen trichloride KW - photolysis Y1 - 2021 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-257322 VL - 22 IS - 21 ER - TY - JOUR A1 - Reusch, Engelbert A1 - Holzmeier, Fabian A1 - Gerlach, Marius A1 - Fischer, Ingo A1 - Hemberger, Patrick T1 - Decomposition of Picolyl Radicals at High Temperature: A Mass Selective Threshold Photoelectron Spectroscopy Study JF - Chemistry - A European Journal N2 - 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. KW - ionization energy KW - photoelectron spectroscopy KW - pyrolysis KW - radicals KW - synchrotron radiation Y1 - 2019 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-208132 VL - 25 IS - 72 ER - TY - JOUR A1 - Schleier, Domenik A1 - Gerlach, Marius A1 - Pratim Mukhopadhyay, Deb A1 - Karaev, Emil A1 - Schaffner, Dorothee A1 - Hemberger, Patrick A1 - Fischer, Ingo T1 - Ammonia Borane, NH\(_{3}\)BH\(_{3}\): A Threshold Photoelectron-Photoion Coincidence Study of a Potential Hydrogen-Storage Material JF - Chemistry-A European Journal N2 - 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\(^{-1}\). KW - ammonia borane KW - photoelectron spectroscopy KW - molecular orbitals KW - hydrogen storage KW - Jahn–Teller effect Y1 - 2022 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-318895 VL - 28 IS - 42 ER - TY - THES A1 - Gerlach, Marius David T1 - Spectroscopy of fulminic acid HCNO with VUV- and soft X-ray radiation T1 - Spektroskopie der Fulminsäure HCNO mit VUV- und weicher Röntgenstrahlung N2 - Die Fulminsäure 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 Fulminsäure im Weltall im Jahr 2009 ist die Fulminsäure heutzutage vor allem im Bereich der Astrochemie interessant. In dieser Doktorarbeit haben wir die Interaktion von Fulminsäure mit interstellar Strahlung, genauer mit VUV- sowie weicher Röntgenstrahlung untersucht. In Zuge der Messung mit VUV-Strahlung konnten wir das Photoelektronenspektrum von HCNO mit hoher Auflösung 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 aufklären. Mit weicher Röntgenstrahlung ist es möglich die 1s Elektronen des HCNO zu ionisieren oder anzuregen. Der erzeugte Zustand zerfällt 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 zerfällt. Hier konnten wir eine Selektivität 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 erklären. Diese Arbeit gibt also ein vollständiges Bild über die Interaktion von HCNO mit ionisierender Strahlung. Die erhaltenen Daten könnten für die Beschreibung von HCNO im interstellaren Raum Bedeutung haben. N2 - Fulminic acid, HCNO, was first synthesized in the year 1800 and has since then been used numerous times to develop new chemical theories and concepts. Nowadays, research on HCNO is mainly motivated due to its detection in interstellar space in the year 2009. In this thesis, we investigated the interaction of fulminic acid with VUV- and soft X-ray radiation, i.e., radiation that is also present in the interstellar medium. In our study using VUV radiation, we were able to record the photoelectron spectrum of HCNO with high resolution and we were able to simulate the Renner-Teller distorted ground state of the cation using simulation of wavepacket dynamics. We also elucidated the mechanism of the dissociative photoionisation up to 15.3 eV binding energy. Using soft X-ray radiation enables us to ionise or excite the 1s electrons of HCNO. The created state can decay via an Auger-Meitner process, which produces an Auger electron. We measured the kinetic energy of these auger electron and were able to analyse the observed signals using quantum chemical calculations. We also investigated how the ion fragments after the Auger-Meitner process. We observed a site-selectivity, where the initial ionisation/excitation site influenced the product distribution. We were able to explain this observation with a simple thermodynamic argument. This thesis provides a comprehensive description of the interaction of HCNO with ionising radiation. The obtained data may be valuable for the description of the behaviour of HCNO in interstellar space. KW - Chemie KW - Auger-Spektroskopie KW - Photoelektronenspektroskopie KW - Fulminsäure KW - Astrochemie KW - Kosmochemie Y1 - 2023 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-329722 ER -