@article{HoelterLemkeWeinzierletal.2025, author = {H{\"o}lter, Arne and Lemke, Mathias and Weinzierl, Stefan and Stein, Lewin}, title = {Non-Reflecting Characteristic Boundary Conditions for Adjoint Time-Domain Acoustic Simulations}, journal = {Journal of Theoretical and Computational Acoustics}, year = {2025}, abstract = {Accurate acoustic simulations in the free field require non-reflective boundary conditions to suppress spurious reflections at the computational domain boundaries. Although several characteristic-based formulations for direct (forward) simulations have been proposed in recent decades, the adjoint formulations of such characteristic-based boundary conditions (CBCs) have received limited atten- tion in the literature and lack a comprehensive analysis. This paper presents the derivation and evaluation of adjoint CBCs complementing the existing direct CBCs. Both the forward and adjoint CBCs are applied to the (nonlinear) Euler equations and linear acoustic equations in time-domain simulations. In this manner, the CBCs are investigated and subsequently compared to assess their respective accuracy and consistency. The CBCs were implemented using both a single-point and a zonal approach, with the former optionally combined with a sponge layer. Both approaches yielded comparable results in direct and adjoint simulations, while the zonal CBC exhibited improved ac- curacy at lower frequencies. Across the evaluated frequency range of approximately 350 - 5600 Hz, spurious reflections were attenuated by up to -70dB in both forward and adjoint cases, demon- strating the effectiveness and consistency of the proposed boundary treatment.}, language = {en} } @article{RaharinirinaSunkaravonKleistetal.2024, author = {Raharinirina, Nomenjanahary Alexia and Sunkara, Vikram and von Kleist, Max and Fackeldey, Konstantin and Weber, Marcus}, title = {Multi-Input data ASsembly for joint Analysis (MIASA): A framework for the joint analysis of disjoint sets of variables}, volume = {19}, journal = {PLOS ONE}, number = {5}, publisher = {Public Library of Science}, doi = {10.1371/journal.pone.0302425}, pages = {26}, year = {2024}, language = {en} } @article{RodriguesPelaDraxl2024, author = {Rodrigues Pel{\´a}, Ronaldo and Draxl, Claudia}, title = {Speeding up all-electron real-time TDDFT demonstrated by the exciting package}, volume = {304}, journal = {Comput. Phys. Commun.}, arxiv = {http://arxiv.org/abs/https://arxiv.org/abs/2403.04351}, doi = {10.1016/j.cpc.2024.109292}, pages = {109292}, year = {2024}, language = {en} } @article{HoeflingStraube2025, author = {H{\"o}fling, Felix and Straube, Arthur}, title = {Langevin equations and a geometric integration scheme for the overdamped limit of rotational Brownian motion of axisymmetric particles}, volume = {7}, journal = {Physical Review Research}, arxiv = {http://arxiv.org/abs/2403.04501}, doi = {10.1103/wzdn-29p4}, pages = {043034}, year = {2025}, abstract = {The translational motion of anisotropic or self-propelled colloidal particles is closely linked with the particle's orientation and its rotational Brownian motion. In the overdamped limit, the stochastic evolution of the orientation vector follows a diffusion process on the unit sphere and is characterized by an orientation-dependent ("multiplicative") noise. As a consequence, the corresponding Langevin equation attains different forms depending on whether Itō's or Stratonovich's stochastic calculus is used. We clarify that both forms are equivalent and derive them in a top-down approach from a geometric construction of Brownian motion on the unit sphere, based on infinitesimal random rotations. Our approach suggests further a geometric integration scheme for rotational Brownian motion, which preserves the normalization constraint of the orientation vector exactly. We show that a simple implementation of the scheme, using Gaussian random rotations, converges weakly at order 1 of the integration time step, and we outline an advanced variant of the scheme that is weakly exact for an arbitrarily large time step. Due to a favorable prefactor of the discretization error, already the Gaussian scheme allows for integration time steps that are one order of magnitude larger compared to a commonly used algorithm for rotational Brownian dynamics simulations based on projection on the constraining manifold. For torques originating from constant external fields, we prove by virtue of the Fokker-Planck equation that the constructed diffusion process satisfies detailed balance and converges to the correct equilibrium distribution. The analysis is restricted to time-homogeneous rotational Brownian motion (i.e., a single rotational diffusion constant), which is relevant for axisymmetric particles and also chemically anisotropic spheres, such as self-propelled Janus particles.}, language = {en} } @misc{SchintkeGrevedeCuveland2024, author = {Schintke, Florian and Greve, Nico and de Cuveland, Jan}, title = {Recent Flesnet developments and work in progress}, journal = {CBM Progress Report 2023}, editor = {Friese, Volker and Gasik, Piotr and Selyuzhenkov, Ilya}, publisher = {GSI Helmholtzzentrum f{\"u}r Schwerionenforschung GmbH}, doi = {10.15120/GSI-2024-00765}, pages = {132}, year = {2024}, language = {en} } @inproceedings{WitzkeLoesserBountrisetal.2024, author = {Witzke, Joel and L{\"o}ßer, Ansgar and Bountris, Vasilis and Schintke, Florian and Scheuermann, Bj{\"o}rn}, title = {I/O of Scientific Workflows Monitored in Detail}, booktitle = {20th IEEE International Conference on e-Science, e-Science 2024, Osaka, Japan, September 16-20, 2024}, doi = {10.1109/E-SCIENCE62913.2024.10678728}, pages = {1 -- 2}, year = {2024}, language = {en} } @article{WitzkeLoesserBountrisetal.2024, author = {Witzke, Joel and L{\"o}ßer, Ansgar and Bountris, Vasilis and Schintke, Florian and Scheuermann, Bj{\"o}rn}, title = {Low-level I/O Monitoring for Scientific Workflows}, volume = {abs/2408.00411}, journal = {CoRR}, arxiv = {http://arxiv.org/abs/2408.00411}, doi = {10.48550/ARXIV.2408.00411}, pages = {1 -- 10}, year = {2024}, language = {en} } @article{FritschSchorr2024, author = {Fritsch, Daniel and Schorr, Susan}, title = {Disorder induced band gap lowering in kesterite type Cu2ZnSnSe4 and Ag2ZnSnSe4: a first-principles and special quasirandom structures investigation}, volume = {36}, journal = {Journal of Physics: Condensed Matter}, number = {37}, publisher = {IOP Publishing}, issn = {0953-8984}, doi = {10.1088/1361-648X/ad52de}, year = {2024}, abstract = {Abstract Quaternary chalcogenides, i.e. Cu2ZnSnS4, crystallising in the kesterite crystal structure have already been demonstrated as potential building blocks of thin film solar cells, containing only abundant elements and exhibiting power conversion efficiencies of about 14.9\% so far. However, due to the potential presence of several structurally similar polymorphs, the unequivocal identification of their ground state crystal structures required the application of more elaborate neutron diffraction experiments. One particular complication arose from the later identified Cu-Zn disorder, present in virtually all thin film samples. Subsequently, it has been shown experimentally that this unavoidable Cu-Zn disorder leads to a band gap lowering in the respective samples. Additional theoretical investigations, mostly based on Monte-Carlo methods, tried to understand the atomistic origin of this disorder induced band gap lowering. Here, we present theoretical results from first-principles calculations based on density functional theory for the disorder induced band gap lowering in kesterite Cu2ZnSnSe4 and Ag2ZnSnSe4, where the Cu-Zn and Ag-Zn disorder is modelled via a supercell approach and special quasirandom structures. Results of subsequent analyses of structural, electronic, and optical properties are discussed with respect to available experimental results, and will provide additional insight and knowledge towards the atomistic origin of the observed disorder induced band gap lowering in kesterite type materials.}, language = {en} } @inproceedings{KramerLaeuter2024, author = {Kramer, Tobias and L{\"a}uter, Matthias}, title = {Benchmarking the rotating jet model of cometary activity with the trajectory of comet 67P/Churyumov-Gerasimenko}, volume = {17}, booktitle = {EPSC Abstracts}, doi = {10.5194/epsc2024-207}, year = {2024}, abstract = {An important tool to assess the composition and the spatial origin of cometary material is the analysis of its trajectory reflecting gravitational acceleration due to solar system bodies complemented by non-gravitational accelerations (NGA).}, language = {en} } @article{AttreeGutierrezGroussinetal.2024, author = {Attree, Nicholas and Guti{\´e}rrez, Pedro and Groussin, Olivier and B{\"u}rger, Johanna and Keller, Horst Uwe and Kramer, Tobias and LASAGNI MANGHI, RICCARDO and L{\"a}uter, Matthias and Lemos, Pablo and Markkanen, Johannes and Marschall, Raphael and Schuckart, Christian}, title = {Varying water activity and momentum transfer on comet 67P/Churyumov-Gerasimenko from its non-gravitational forces and torques}, volume = {690}, journal = {Astronomy and Astrophysics}, arxiv = {http://arxiv.org/abs/2408.10877}, doi = {10.1051/0004-6361/202450728}, pages = {A82}, year = {2024}, abstract = {Aims. We investigate the ability of a simultaneous fitting of comet 67P/Churyumov-Gerasimenko's non-gravitational forces, torques, and total water-outgassing rate, as observed by Rosetta, to constrain complex thermophysical models of cometary material. Methods. We extend the previous work of fitting geographically defined surface outgassing models to the Rosetta observations by testing the effects of a more detailed geomorphological mapping, the resolution of the shape-model used, self-heating by neighbouring facets on the shape-model, thermal inertia in the outgassing solution, and the variation in the momentum coupling between the gas and the nucleus. We also directly compare the non-gravitational acceleration curves available in the literature. Results. We correct an error in the calculation of pole-orientation in the previous paper. We find that, under the assumptions of the model, non-gravitational forces and torques are driven by water sublimation from the nucleus, thermal inertia and self-heating have only minor effects, spatially uniform activity cannot explain 67P's non-gravitational dynamics, spatially uniform momentum transfer cannot explain 67P's non-gravitational dynamics, and different terrain types have different instantaneous responses to insolation. Conclusions. Consolidated terrain facing south on 67P/Churyumov-Gerasimenko has a high outgassing flux, a steep response to insolation, and a large gas momentum transfer coefficient. Instead, that facing north behaves differently, producing little to no water outgassing, and with a lower momentum transfer efficiency. Dusty terrain also has a lower outgassing rate and momentum transfer efficiency, and either depletes its volatile component or is buried in fall-back as the comet approaches the Sun. Momentum transfer appears correlated with insolation, likely due to an increased enhancement in the gas temperature as the dust it flows through is heated.}, language = {en} } @inproceedings{AttreeGutierrezGroussinetal.2024, author = {Attree, Nicholas and Guti{\´e}rrez, Pedro and Groussin, Olivier and B{\"u}rger, Johanna and Keller, Horst Uwe and Kramer, Tobias and Lasagni Manghi, Riccardo and L{\"a}uter, Matthias and Lemos, Pablo and Markkanen, Johannes and Marschall, Raphael and Schuckart, Christian}, title = {The Results of ISSI Team \#547: Understanding the Activity of Comets Through 67P's Dynamics}, volume = {17}, booktitle = {EPSC Abstracts}, doi = {10.5194/epsc2024-82}, year = {2024}, abstract = {Understanding cometary activity gives us an insight into the materials properties, and therefore formation and evolution processes of these relatively pristine protoplanetary objects. We will present the results of an International Space Science Institute project to investigate the phenomenon through the effects of the outgassing activity on the orbit and spin-state of comet 67P/Churymov-Gerasimenko, e.g. its non-gravitational dynamics. This International Team gathered experts in orbital dynamics and trajectory reconstruction together with thermophysical modellers and comet observationalists, in order to compare the available extractions of 67P's non-gravitational acceleration (NGA) from its trajectory. The team then fitted a combination of the NGA, the non-gravitational torque (NGT), and the total water-outgassing rate with a thermophysical activity model. The results of this model will be presented. In particular, it was found that: non-gravitational forces and torques are driven by water sublimation from the nucleus; thermal inertia and self-heating have only minor effects; spatially uniform activity cannot explain 67P's non-gravitational dynamics; spatially uniform momentum transfer cannot explain 67P's non-gravitational dynamics; and different terrain types have different instantaneous responses to insolation. The implications of these findings for the modelling of cometary material and the variety of surface types seen on 67P will be discussed.}, language = {en} } @article{RoyHoefling2024, author = {Roy, Sutapa and H{\"o}fling, Felix}, title = {Critical surface adsorption of confined binary liquids with locally conserved mass and composition}, volume = {122}, journal = {Molecular Physics}, number = {21-22}, doi = {10.1080/00268976.2024.2391998}, pages = {e2391998}, year = {2024}, abstract = {Close to a solid surface, the properties of a fluid deviate significantly from their bulk values. In this context, we study the surface adsorption profiles of a symmetric binary liquid confined to a slit pore by means of molecular dynamics simulations; the latter naturally entails that mass and concentration are locally conserved. Near a bulk consolute point, where the liquid exhibits a demixing transition with the local concentration as the order parameter, we determine the order parameter profiles and characterise the relevant critical scaling behaviour, in the regime of strong surface attraction, for a range of pore widths and temperatures. The obtained order parameter profiles decay monotonically near the surfaces, also in the presence of a pronounced layering in the number density. Overall, our results agree qualitatively with recent theoretical predictions from a mesoscopic field-theoretical approach for the canonical ensemble.}, language = {en} } @phdthesis{Jami2024, author = {Jami, Masoud}, title = {Optimizing Checkpoint/Restart and Input/Output for Large Scale Applications}, publisher = {Humboldt-Universit{\"a}t zu Belin}, doi = {10.18452/29985}, pages = {162}, year = {2024}, language = {en} } @article{MarcelliBottinelliMontandonEbrahimiViandetal.2025, author = {Marcelli, Giorgia and Bottinelli Montandon, Tecla and Ebrahimi Viand, Roya and H{\"o}fling, Felix}, title = {Fluid flow inside slit-shaped nanopores: the role of surface morphology at the molecular scale}, volume = {162}, journal = {The Journal of Chemical Physics}, arxiv = {http://arxiv.org/abs/2411.04882}, doi = {10.1063/5.0246573}, pages = {104101}, year = {2025}, abstract = {Non-equilibrium molecular dynamics (NEMD) simulations of fluid flow have highlighted the peculiarities of nanoscale flows compared to classical fluid mechanics; in particular, boundary conditions can deviate from the no-slip behavior at macroscopic scales. For fluid flow in slit-shaped nanopores, we demonstrate that surface morphology provides an efficient control on the slip length, which approaches zero when matching the molecular structures of the pore wall and the fluid. Using boundary-driven, energy-conserving NEMD simulations with a pump-like driving mechanism, we examine two types of pore walls—mimicking a crystalline and an amorphous material—that exhibit markedly different surface resistances to flow. The resulting flow velocity profiles are consistent with Poiseuille theory for incompressible, Newtonian fluids when adjusted for surface slip. For the two pores, we observe partial slip and no-slip behavior, respectively. The hydrodynamic permeability corroborates that the simulated flows are in the Darcy regime. However, the confinement of the fluid gives rise to an effective viscosity below its bulk value; wide pores exhibit a crossover between boundary and bulk-like flows. In addition, the thermal isolation of the flow causes a linear increase in fluid temperature along the flow, which we relate to strong viscous dissipation and heat convection, utilizing conservation laws of fluid mechanics. Noting that the investigated fluid model does not form droplets, our findings challenge the universality of previously reported correlations between slippage, solvophobicity, and a depletion zone. Furthermore, they underscore the need for molecular-scale modeling to accurately capture the fluid dynamics near boundaries and in nanoporous materials, where macroscopic models may not be applicable.}, language = {en} } @article{ZhongHoeflingJohn2025, author = {Zhong, Xin and H{\"o}fling, Felix and John, Timm}, title = {Hydrogen diffusion in garnet: insights from atomistic simulations}, volume = {26}, journal = {Geochemistry Geophysics Geosystems}, arxiv = {http://arxiv.org/abs/2410.07724}, doi = {10.1029/2024GC011951}, pages = {e2024GC011951}, year = {2025}, abstract = {Garnet has been widely used to decipher the pressure-temperature-time history of rocks, but its physical properties such as elasticity and diffusion are strongly affected by trace amounts of hydrogen. Experimental measurements of H diffusion in garnet are limited to room pressure. We use atomistic simulations to study H diffusion in perfect and defective garnet lattices, focusing on protonation defects at the Si and Mg sites, which are shown to be energetically favored. Transient trapping of H renders ab-initio simulations of H diffusion computationally challenging, which is overcome with machine learning techniques by training a deep neural network that encodes the interatomic potential. Our results from such deep potential molecular dynamics (DeePMD) simulations show high mobility of hydrogen in defect-free garnet lattices, whereas H diffusivity is significantly diminished in defective lattices. Tracer simulations focusing on H alone highlight the vital role of atomic vibrations of heavier atoms like Mg on the release of H atoms. Two regimes of H diffusion are identified: a diffuser-dominated regime at high hydrogen content with low activation energies due to saturation of vacancies by hydrogen, and a vacancy-dominated regime at low hydrogen content with high activation energies due to trapping of H atoms at vacancy sites. These regimes account for experimental observations, such as a H-concentration dependent diffusivity and the discrepancy in activation energy between deprotonation and D-H exchange experiments. This study underpins the crucial role of vacancies in H diffusion and demonstrates the utility of machine-learned interatomic potentials in studying kinetic processes in the Earth's interior.}, language = {en} } @article{CarusoSentefAttaccaliteetal.2026, author = {Caruso, Fabio and Sentef, Michael and Attaccalite, Claudio and Bonitz, Michael and Draxl, Claudia and De Giovannini, Umberto and Eckstein, Martin and Ernstorfer, Ralph and Fechner, Michael and Gr{\"u}ning, Myrta and H{\"u}bener, Hannes and Joost, Jan-Philip and Juraschek, Dominik and Karrasch, Christoph and Marvin Kennes, Dante and Latini, Simone and Lu, I-Te and Neufeld, Ofer and Perfetto, Enrico and Rettig, Laurenz and Rodrigues Pel{\´a}, Ronaldo and Rubio, Angel and Rudzinski, Joseph and Ruggenthaler, Michael and Sangalli, Davide and Sch{\"u}ler, Michael and Shallcross, Samuel and Sharma, Sangeeta and Stefanucci, Gianluca and Werner, Philipp}, title = {The 2025 Roadmap to Ultrafast Dynamics: Frontiers of Theoretical and Computational Modelling}, volume = {9}, journal = {J. Phys. Mater.}, number = {1}, arxiv = {http://arxiv.org/abs/2501.06752}, doi = {10.1088/2515-7639/ae1165}, year = {2026}, language = {en} } @misc{RagyanszkiJiFournier2024, author = {Ragyanszki, Anita and Ji, Hongchen and Fournier, Rene}, title = {Understanding the Origins of Life - A Machine learning approach to estimate reaction mechanisms of biotic precursors}, journal = {Perspectives and challenges of future HPC installations for atomistic and molecular simulations}, year = {2024}, abstract = {Life as we know it is the result of billions of years of evolution; yet, understanding how the very first organisms came into existence is a challenge that has yet to be solved. One theory states that components of the first biotic molecules may not have formed on Earth. Rather, they may have initially formed in the interstellar medium (ISM) and been transported to Earth, as supported by recorded instances of organic molecules detected in space. The ISM, with its low temperatures and specific collision processes, allows for molecular stability and the formation of biotic precursors that would otherwise be unlikely in Earth's prebiotic conditions. Understanding how these molecules formed in the ISM may be the key to determining how life began. The goal of this research is to develop a new model for solving astrobiophysical problems by studying the formation mechanisms of biomolecules found in the ISM. Although such pathways have been studied individually, there has not yet been a comprehensive method to understand all the formation reactions that can occur in ISM. Several quantum chemical and numerical methods are available for finding transition states (TS) and energy barriers (E) of chemical reactions but are time-consuming and can hardly be applied to systems with more than a few atoms. Our main interest is to develop a a machine learning approach to approximate TS, and E, requiring as input only estimates of geometry and energies of reactants and products. Using a complete dataset 300 reaction features are computed, and an estimate of E is obtained by fitting a Kernel Ridge Regression (KRR) model with Laplacian kernel, and a fully connected Artificial Neural Network (ANN) to estimate reaction energy barriers.}, language = {en} } @misc{RagyanszkiJiFournier2024, author = {Ragyanszki, Anita and Ji, Hongchen and Fournier, Rene}, title = {Understanding the Origins of Life - A Machine learning approach to estimate reaction mechanisms of biotic precursors}, journal = {SIMPLAIX}, year = {2024}, abstract = {Understanding the Origins of Life - A Machine learning approach to estimate reaction mechanisms of biotic precursors. Life as we know it is the result of billions of years of evolution; however, understanding how the very first organisms came into existence is a challenge that has yet to be solved. One theory states that components of these molecules may have formed in the interstellar medium (ISM) and been transported to Earth. The ISM, with its specific conditions, allows for molecular stability and the formation of biotic precursors that would otherwise be unlikely in Earth's prebiotic conditions. Understanding how these molecules formed in the ISM may be the key to determining how life began. The goal of this research is to develop a model for solving astrobiophysical problems by studying the formation mechanisms of biomolecules found in the ISM. Although such pathways have been studied individually, there has not yet been a comprehensive method to understand the complete reactions mechanisms. Several QM methods are available for finding transition states (TS) and energy barriers (E) of chemical reactions but are time-consuming and can hardly be applied to more complex systems. Our interest is to develop a machine learning approach to approximate TS, and E, requiring as input only estimates of geometry and energies of reactants and products.}, language = {en} } @inproceedings{ChristgauDylanLuebkeetal.2025, author = {Christgau, Steffen and Dylan, Everingham and L{\"u}bke, Max and De Lucia, Marco and Puhan, Danny and Schelten, Niklas and Schnor, Bettina and Signer, Hannes and Spazier, Johannes and Stabernack, Benno and Steinert, Fritjof and Yahdzhyiev, Serhii}, title = {On the Usability and Energy Efficiency of High-Level Synthesis for FPGA-based Network-Attached Accelerators}, booktitle = {2025 IEEE International Parallel and Distributed Processing Symposium Workshops (IPDPSW)}, doi = {10.1109/IPDPSW66978.2025.00139}, pages = {886 -- 895}, year = {2025}, abstract = {Heterogeneity in high performance computing systems is one of the most promising approaches towards more energy-efficient computing on one hand and satisfying the raising demand of global computation capacity on the other hand. Besides the well-known key components like CPUs and GPGPUs are domain-specific accelerators like TPUs, FPGAs well known for their energy efficiency. This is especially true for highly specialized use cases. Network-attached accelerators promise more scalability and flexibility for FPGA usage in HPC environments. Easy and efficient programming of those accelerators is, however, still an open issue. Based on a framework for such accelerators which enables decoupling of FPGAs from their host system, we present a workflow using High-Level Synthesis (HLS) to offload application kernels to them. We evaluate this approach against a conventional Hardware Description Language (HDL) based workflow. In addition, we introduce the energy measurement tool EMA and assess the energy efficiency of both HLS and HDL design.}, language = {en} } @article{LaeuterKramer2025, author = {L{\"a}uter, Matthias and Kramer, Tobias}, title = {Rotation dynamics and torque efficiency of cometary nuclei}, volume = {699}, journal = {Astronomy \& Astrophysics}, arxiv = {http://arxiv.org/abs/2507.06036}, doi = {10.1051/0004-6361/202553845}, pages = {A75}, year = {2025}, abstract = {The dynamics of a rigid cometary nucleus is described by the evolutions of its center-of-mass and of its rotation state. Solar irradiation that reaches the surface of a cometary nucleus causes the sublimation of volatiles that form the coma around the nucleus. The sublimation process transfers linear momentum and rotational angular momentum from the nucleus to the surrounding space, and thus affects the dynamics via nongravitational forces and nongravitational torques. With the exception of close approaches to planets, these torques exert the dominant influence on the rotation states of cometary nuclei. The Rosetta mission 2014-2016 accompanying comet 67P/Churyumov-Gerasimenko provides the longest continuous observational data to track its rotation state. In particular, the data set encompasses the direction of the angular velocity, denoted by ω, and the angular frequency |ω|over a time period of approximately 700 days. The observed change of the rotation state is not explained by a low heat conductivity thermophysical model in combination with a homogeneous surface ice coverage of comet 67P. Spatially and/or temporally varying weights for effective active fraction with respect to a prescribed set of surface regions provide a potential solution to this problem. Here, we present a methodology for classifying the surface based on vectorial efficiency of the torque. On any cometary surface without geometric symmetry, the methodology highlights the decomposition into eight characteristic regions that encode the signs of torque efficiency with respect to all vector components. This decomposition is divided into two subsets of four regions each of which is located in one of both hemispheric regions. We analyze in detail rotation states close to lowest energy and different thermophysical models, and we discuss how the uncertainties of observations affect the model parameters. We study the occurrence of these regions for an oblate ellipsoid, a nearprolate ellipsoid, a bilobed shape, and a shape model analogous to that of comet 67P. The sensitivity analysis for comet 67P indicates that the observations constrain only one of the eight weights uniquely. The other directions are poorly constrained and show the limitation of the rotational data to determine the regional activity on comet 67P.}, language = {en} } @misc{elBahnasawy2025, type = {Master Thesis}, author = {el Bahnasawy, Henry}, title = {Konzeption und Entwicklung einer Plattform zur geographisch verteilten Bereitstellung von latenzkritischen Anwendungen}, pages = {102}, year = {2025}, language = {de} } @article{RossiQiaoDykstraetal.2025, author = {Rossi, Thomas and Qiao, Lu and Dykstra, Conner P. and Rodrigues Pel{\´a}, Ronaldo and Gnewkow, Richard and Wallick, Rachel F. and Burke, John H. and Nicholas, Erin and March, Anne-Marie and Doumy, Gilles and Buchholz, D. Bruce and Deparis, Christiane and Zu{\~n}iga-P{\´e}rez, Jesus and Weise, Michael and Ellmer, Klaus and Fondell, Mattis and Draxl, Claudia and van der Veen, Renske}, title = {Dynamic control of X-ray core-exciton resonances by Coulomb screening in photoexcited semiconductors}, volume = {6}, journal = {Communications Materials}, arxiv = {http://arxiv.org/abs/2412.01945}, doi = {10.1038/s43246-025-00909-w}, pages = {191}, year = {2025}, language = {en} }