@article{VogelEbelSchuermannetal.2019, author = {Vogel, Stefanie and Ebel, Kenny and Sch{\"u}rmann, Robin Mathis and Heck, Christian and Meiling, Till and Milosavljevic, Aleksandar R. and Giuliani, Alexandre and Bald, Ilko}, title = {Vacuum-UV and Low-Energy Electron-Induced DNA Strand Breaks}, series = {ChemPhysChem : a European journal of chemical physics and physical chemistry}, volume = {20}, journal = {ChemPhysChem : a European journal of chemical physics and physical chemistry}, number = {6}, publisher = {Wiley-VCH}, address = {Weinheim}, issn = {1439-4235}, doi = {10.1002/cphc.201801152}, pages = {823 -- 830}, year = {2019}, abstract = {DNA is effectively damaged by radiation, which can on the one hand lead to cancer and is on the other hand directly exploited in the treatment of tumor tissue. DNA strand breaks are already induced by photons having an energy below the ionization energy of DNA. At high photon energies, most of the DNA strand breaks are induced by low-energy secondary electrons. In the present study we quantified photon and electron induced DNA strand breaks in four different 12mer oligonucleotides. They are irradiated directly with 8.44 eV vacuum ultraviolet (VUV) photons and 8.8 eV low energy electrons (LEE). By using Si instead of VUV transparent CaF2 as a substrate the VUV exposure leads to an additional release of LEEs, which have a maximum energy of 3.6 eV and can significantly enhance strand break cross sections. Atomic force microscopy is used to visualize strand breaks on DNA origami platforms and to determine absolute values for the strand break cross sections. Upon irradiation with 8.44 eV photons all the investigated sequences show very similar strand break cross sections in the range of 1.7-2.3x10(-16) cm(2). The strand break cross sections for LEE irradiation at 8.8 eV are one to two orders of magnitude larger than the ones for VUV photons, and a slight sequence dependence is observed. The sequence dependence is even more pronounced for LEEs with energies <3.6 eV. The present results help to assess DNA damage by photons and electrons close to the ionization threshold.}, language = {en} } @article{SchuermannVogelEbeletal.2018, author = {Sch{\"u}rmann, Robin Mathis and Vogel, Stefanie and Ebel, Kenny and Bald, Ilko}, title = {The physico-chemical basis of DNA radiosensitization}, series = {Chemistry - a European journal}, volume = {24}, journal = {Chemistry - a European journal}, number = {41}, publisher = {Wiley-VCH}, address = {Weinheim}, issn = {0947-6539}, doi = {10.1002/chem.201800804}, pages = {10271 -- 10279}, year = {2018}, abstract = {High-energy radiation is used in combination with radiosensitizing therapeutics to treat cancer. The most common radiosensitizers are halogenated nucleosides and cisplatin derivatives, and recently also metal nanoparticles have been suggested as potential radiosensitizing agents. The radiosensitizing action of these compounds can at least partly be ascribed to an enhanced reactivity towards secondary low-energy electrons generated along the radiation track of the high-energy primary radiation, or to an additional emission of secondary reactive electrons close to the tumor tissue. This is referred to as physico-chemical radiosensitization. In this Concept article we present current experimental methods used to study fundamental processes of physico-chemical radiosensitization and discuss the most relevant classes of radiosensitizers. Open questions in the current discussions are identified and future directions outlined, which can lead to optimized treatment protocols or even novel therapeutic concepts.}, language = {en} }