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Radiation damage following the ionising radiation of tissue has different scenarios and mechanisms depending on the projectiles or radiation modality. We investigate the radiation damage effects due to shock waves produced by ions. We analyse the strength of the shock wave capable of directly producing DNA strand breaks and, depending on the ion's linear energy transfer, estimate the radius from the ion's path, within which DNA damage by the shock wave mechanism is dominant. At much smaller values of linear energy transfer, the shock waves turn out to be instrumental in propagating reactive species formed close to the ion's path to large distances, successfully competing with diffusion.
Capturing intermolecular interactions accurately is essential for describing, e.g., morphology of molecular matter on the nanoscale. When it reveals characteristics which are not directly accessible through experiments or ab initio theories, a model here becomes eminently beneficial. In laboratory astrochemistry, the intense study of ices has led i.a. to the exploration of the spontelectric state of nanofilms. Despite its success in biophysics or biochemistry and despite its predictive power, molecular modeling has however not yet been widely deployed for solid-state astrochemistry. In this article, therefore a pertinent hitherto unaddressed problem is tackled by means of the classical molecular-dynamics method, namely the unknown distribution of relative dipole orientations in spontelectric cis-methyl formate (MF). In doing so, from ab initio data, a molecular model is derived which confirms for the first time the anomalous temperature-dependent polarization of MF. These insights thus represent a further step toward understanding spontelectric behavior. Moreover, unprecedented first-principles predictions are reported regarding the ground-state geometry of the MF trimer and tetramer. In conjunction with the study of the binding to carbonaceous substrates, these additional findings can help to exemplarily elucidate molecular ice formation in astrochemical settings.
We have investigated the channeling process of charged particles in a bent crystal. Invoking simple assumptions we derive a criterion, which determines whether channeling occurs or not. We obtain the same criterion using the Dirac equation. It is shown that the centrifugal force acting on the particle in the bent crystal significantly alters the effective transverse potential. The cases of axial and planar channeling are considered. The channeling probability and the dechanneling probability due to tunneling of the particle under the barrier in the effective transverse potential are estimated. These probabilities depend on the specific scaling parameter characterizing the process. Using the quasiclassical theory of synchrotron radiation we have calculated the contribution to the radiation spectrum, which arises due to the curvature of the channel. This contribution becomes significant to TeV electrons or positrons. Some practical consequences of our results are briefly discussed.
