# Latest Projects (Overview)

Find out about the latest simulation projects run on the GCS supercomputers. For the complete overview of projects, sorted by research fields, please choose from the list in the left column.

## CARo – Computational Aeroacoustics of Rotors

Using state-of-the-art simulation technology for highly resolved computational fluid dynamics (CFD) solutions, the helicopter and aeroacoustics group at the Institute of Aerodynamics and Gasdynamics at the University of Stuttgart has simulated the complex aerodynamics, aeromechanics, and aeroacoustics of rotorcraft for years. By advancing the established flow solver FLOWer, which now integrates higher order accuracy and systematic concentration of spatial resolution in targeted regions, the IAG-based group was able to obtain results for complete helicopters at certification-relevant flight states within the variance of individual flight tests for the aerodynamic noise.

**Principal Investigator:** Manuel Keßler, Institut für Aerodynamik und Gasdynamik, Universität Stuttgart (Germany)

**HPC Platform:** Hazel Hen (HLRS) -** Date published: **July 2018* (CARo)*

**More: CARo – Computational Aeroacoustics of Rotors …**

## Numerical Simulation of Rotary Wing Aerodynamics, Aeroelasticity and Aeroacoustics (HELISIM)

Researchers of the Insitute of Aerdynamics and Gasdynamics at the University of Stuttgart leverage high-performance computing to analyse the behaviour of helicopters during various states of flight. Investigations range from deep analyses of fundamental aerodynamic phenomena like dynamic stall on the retreating blade to surveys over a broad spectrum of flight states over the full flight envelope of new configurations, to reduce flight mechanical risks. Recently, the group was able to simulate the first robust representation of the so-called tail-shake phenomenon—an interference between the aerodynamic wake of the rotor and upper fuselage and the tail boom with its elastic behaviour.

**Principal Investigator:** Manuel Keßler, Institut für Aerodynamik und Gasdynamik, Universität Stuttgart (Germany)

**HPC Platform:** Hazel Hen (HLRS) -** Date published: **July 2018* (HELISIM)*

**More: Numerical Simulation of Rotary Wing Aerodynamics, Aeroelasticity and Aeroacoustics (HELISIM) …**

## Studying *Structure* to Understand *Function* in Phases of the Elements

“If you want to understand function, study structure” (F. Crick). In the case of carbon, the very different properties of graphite, diamond, and carbon nanotubes can then be traced to different atomic arrangements. The elements provide a fruitful field of study in general. There are fewer than 100 stable elements, and trends can be identified more readily than in alloys with infinitely many compositions. He we describe cluster, amorphous, and liquid phases of the group 15 elements bismuth and antimony using molecular dynamics simulations based on density functional theory.

**Principal Investigator:** Robert O. Jones, Forschungszentrum Jülich (Germany)

**HPC Platform:** JUQUEEN (JSC) - **Date published:** July 2018* **(hpg00)*

**More: Studying Structure to Understand Function in Phases of the Elements …**

## Planet Formation Through the Gravitational Collapse of Solids and Gas

Planetesimals are kilometre-sized planetary building blocks in the early solar system. Scientists pioneered a scenario in which turbulent concentrations of the icy and dusty material leads to sufficiently large densities in which self-gravity dominates over gas shear and tidal forces of the star. As a consequence, the material collapses spontaneously under its own weight into planetesimals. Therefore, the motion of many millions of particles in magneto-hydro-dynamically and particle driven turbulence and include the gravity among gas and particles are all simulated in one huge simulation. The goal is to link the observations of dust around young stars in a quantified way to an initial mass distribution of planetesimals.

**Principal Investigator: **Hubert Klahr, Max-Planck-Institut für Astronomie, Heidelberg (Germany)

**HPC Platform:** JUQUEEN of JSC - **Date published:** July 2018 *(hhd19)*

**More: Planet Formation Through the Gravitational Collapse of Solids and Gas …**

## Linear-Scaling Transport Approach for Innovative Electronic Materials

Researchers elucidate the molecular doping of prototypical representatives for the class of molecular semiconductors. As n-type dopants, molecular radicals, closed-shell molecules and metal-organic species are compared. By using the HPC system SuperMUC, they simulate doping-induced states and compare the simulations with ultraviolet photoemission and inverse photoemission spectra. One challenge in the simulations is the necessary accuracy of the computation of the involved energies in the doping process, which requires ab initio approaches. In addition, the disordered material blends include many complex molecules whose charging states and charging energies need to be simulated by taking into account the blend’s dielectric properties and microscopic molecular arrangement.

**Principal Investigator:** Frank Ortmann, Technische Universität Dresden (Germany)

**HPC Platform:** SuperMUC (LRZ) - **Date published:** June 2018* **(pr84po)*

**More: Linear-Scaling Transport Approach for Innovative Electronic Materials …**

## Towards Exascale Simulations of Plasma Fusion Devices

The generation of clean, sustainable energy from plasma fusion reactors is currently limited by the presence of microinstabilities that arise during the fusion process, despite international efforts such as the ITER experiment, currently under construction in southern France. Numerical simulations are crucial to understand, predict, and control plasma turbulence with the help of large-scale computations. Due to the high dimensionality of the underlying equations, the fully resolved simulation of the numerical ITER is out of scope with classical discretization schemes, even for the next generation of exascale computers. With five research groups from mathematics, physics, and computer science, the SPPEXA project EXAHD has proposed to use a hierarchical discretization scheme, so-called Sparse Grids, to overcome the current computational limits (number of discretization points per dimension and memory requirements). This way, it will be possible to enable high-resolution simulations, to ensure scalability of the simulations to future exascale computers and beyond, and even to be able to cope with faults and failures which will be more frequent for the next generation of supercomputers.

**Principal Investigator:** Dirk Pflüger, Institute for Parallel and Distributed Systems, University of Stuttgart (Germany)

**HPC Platform:** Hazel Hen (HLRS) -** Date published: **June 2018* (exaHD)*

**More: Towards Exascale Simulations of Plasma Fusion Devices …**

## First Principles Multiscale Kinetic Modelling of Catalytic Reactions

Researchers at the Technical University of Munich study surface catalytic processes at a variety of scales, combining several different theoretical methods. They take into account the molecular scale of chemical reactions by first principles calculations of thermodynamic adsorption energies and kinetic reaction barriers. These calculations serve as input for mesoscopic models, which include the statistical interplay between the various chemical reactions and allow to predict macroscopic reaction rates and product selectivities. The work provides new insight into the mechanisms of catalytic reactions and gives important leads how to design improved catalyst materials.

**Principal Investigator:** Karsten Reuter, Lehrstuhl für Theoretische Chemie, Technische Universität München (Germany)

**HPC Platform:** SuperMUC (LRZ) - **Date published:** June 2018* **(pr94sa)*

**More: First Principles Multiscale Kinetic Modelling of Catalytic Reactions …**

## Direct Numerical Simulation of Turbulent Heat Transfer with a Supercritical Fluid

In the quest for efficiency enhancement in energy conversion, supercritical carbon dioxide (sCO2) is an attractive alternative working fluid. However, the heat transfer to sCO2 is much different in the supercritical region than the subcritical region due to the strong variation of thermophysical properties which bring the effects of flow acceleration and buoyancy. The peculiarity in heat transfer and flow characteristics cannot be predicted accurately by using conventional correlations or Reynolds-Averaged Naiver-Stokes (RANS) simulations based on the turbulence models. Therefore, direct numerical simulation (DNS) is used in this ongoing project. In DNS, the Naiver-Stokes equations are numerically solved without any turbulence models. For this accurate and reliable approach, one needs to resolve very fine spatial and temporal scales, which ultimately results in the requirement of high-performance computing.

**Principal Investigator:** Eckart Laurien, Institute of Nuclear Energy and Energy Systems (IKE), University of Stuttgart (Germany)

**HPC Platform:** Hazel Hen (HLRS) -** Date published: **May 2018* (DNSTHTS)*

**More: Direct Numerical Simulation of Turbulent Heat Transfer with a Supercritical Fluid …**

## Petascale Computations for Atomic and Molecular Collisions: PAMOP and PAMOP2

An international group of scientists leverages high-performance computing to support current and future measurements of atomic photoionization cross-sections at various synchrotron radiation facilities, ion-atom collision experiments, together with plasma, fusion and astrophysical applications. In their work they solve the Schrödinger or Dirac equation using the *R-*matrix or *R-*matrix with pseudo-states approach from first principles. Cross-sections and rates for radiative charge transfer, radiative association, and photodissociation collision processes between atoms and ions of interest for several astrophysical applications are presented.

**Principal Investigator: **Alfred Müller, Institut für Atom- und Molekülphysik, Universität Giessen (Germany)

**HPC Platform:** Hazel Hen/HLRS - **Date published:** May 2018 *(PAMOP/PAMOP2)*

**More: Petascale Computations for Atomic and Molecular Collisions: PAMOP and PAMOP2 …**

## Simulating the Universe: Predictive Galaxy Formation towards the Smallest Scales

Modern simulations of galaxy formation, which simultaneously follow the co-evolution of dark matter, cosmic gas, stars, and supermassive black holes, enable us to directly calculate the observable signatures that arise from the complex process of cosmic structure formation. TNG50 is an unprecedented ‘next generation’ cosmological, magneto-hydrodynamical simulation -- the third and final volume of the IllustrisTNG project. It captures spatial scales as small as ~100 parsecs, resolving the interior structure of galaxies, and incorporates a comprehensive model for galaxy formation physics.

**Principal Investigator: **Dylan Nelson, MPA Garching, and Annalisa Pillepich, MPIA Heidelberg (Germany)

**HPC Platform:** Hazel Hen/HLRS - **Date published:** May 2018 *(GCS-dwar)*

**More: Simulating the Universe: Predictive Galaxy Formation towards the Smallest Scales …**

## Multiscale Simulations of Fluid-Structure-Acoustic Interaction

This project was part of the ExaFSA project that investigates the possibility to exploit high-performance computing systems for integrated simulations of all parts contributing to noise generation in flows around obstacles. Such computations are challenging, as they involve the interaction of various physical effects on different scales. In this context, the compute time on SuperMUC granted for this project was used to particularly investigate the coupling of the flow within a large acoustic domain with individual discretization methods.

**Principal Investigator:** Sabine Roller, University of Siegen, Institute of Simulation Techniques and Scientific Computing (Germany)

**HPC Platform:** SuperMUC (LRZ) -** Date published: **April 2018* (pr84xu)*

**More: Multiscale Simulations of Fluid-Structure-Acoustic Interaction …**

## The Emergence of Structures in the Next Generation of Hydrodynamical Cosmological Simulations

Hydrodynamical simulations of galaxy formation have now reached sufficient physical fidelity to allow detailed predictions for their formation and evolution over cosmic time. The aim of this project is to carry out a new generation of structure formation simulations, IllustrisTNG, that reach sufficient volume to make accurate predictions for clustering on cosmologically relevant scales, while at the same time being able to compute detailed galaxy morphologies, the enrichment of diffuse gas with metals, and the amplification of magnetic fields during structure growth.

**Principal Investigator: **Volker Springel, Heidelberg Institute for Theoretical Studies, Heidelberg University, and Max-Planck Institute for Astrophysics (Germany)

**HPC Platform:** Hazel Hen/HLRS - **Date published:** April 2018 *(GCS-ILLU)*

**More: The Emergence of Structures in the Next Generation of Hydrodynamical Cosmological Simulations …**

## Thermodynamics with Overlap Fermions

The Universe soon after the Big Bang was hot and full of massless particles, so called fermions and bosons. As it expanded and cooled down particles become massive. They acquired mass from several kinds of mechanisms, which are investigated in detail in heavy-ion collision experiments, and also in theory. Ab-initio theoretical calculations require simulating massless particles on a supercomputer. This is a difficult problem, fortunately with an existing solution, the so-called overlap discretization of fermions. Here we make simulations with overlap fermions using supercomputing power.

**Principal Investigator:** Balint Toth, Bergische Universität Wuppertal (Germany)

**HPC Platform:** JUQUEEN (JSC) - **Date published: **April 2018 *(hwu26)*

**More: Thermodynamics with Overlap Fermions …**

## Exploring the QCD Phase Diagram Using the Complex Langevin Equation

The simulation of nuclear matter at nonzero baryon density presents a notoriously hard problem in lattice QCD. The usual simulation strategies depend on the exploration of the configuration space by interpreting the weight of each configuration in an average as a probability, which is however not valid here as the weight is non positive. This is called the ‘sign problem’ of nonzero density QCD. In this project, the researchers use a method based on the Complex Langevin equation evading the sign problem to map out the phase diagram of nuclear matter.

**Principal Investigator:** Dénes Sexty, Bergische Universität Wuppertal (Germany)

**HPC Platform:** JUQUEEN (JSC) - **Date published: **March 2018 *(hwu22)*

**More: Exploring the QCD Phase Diagram Using the Complex Langevin Equation …**

## Hadronic Corrections to the Muon Anomalous Magnetic Moment

Supercomputing resources are used to investigate a long standing discrepancy between theoretical calculation and experiment in the case of an elementary particle called muon. This muon magnetic moment puzzle is considered by many as a smoking gun for new physics, ie. something that cannot t into the current framework of particle physics.

**Principal Investigator:** Kálmán Szabó, Forschungszentrum Jülich GmbH (Germany)

**HPC Platform:** JUQUEEN (JSC) - **Date published: **March 2018 *(hfz00)*

**More: Hadronic Corrections to the Muon Anomalous Magnetic Moment …**

## Numerical Investigation of Convective Patterns in the Solar Near-Surface Shear Layer

The characteristic patterns seen on the solar surface, on gas giants, in Earth's atmosphere and oceans, and many other geo- and astrophysical settings originate from turbulent convection dynamics flows driven by a density difference caused by, for instance, a temperature gradient. Convection in itself is inherently complex, but often it is the interaction with other forces, such as the Coriolis and Lorentz force due to rotation and magnetic fields, that determines the actual shape and behaviour of the flow structures. Understanding these convective patterns is often essentially tantamount to understanding the underlying physics at play. In this project, surveys through the huge parameter space are conducted, to not only categorise flow morphologies, but also to derive theoretical relations, in particular, for the heat and momentum transport.

**Principal Investigator:** Olga Shishkina, Max Planck Institute for Dynamics and Self-Organization, Göttingen (Germany)

**HPC Platform:** SuperMUC (LRZ) - **Date published:** March 2018* **(pr94na)*

**More: Numerical Investigation of Convective Patterns in the Solar Near-Surface Shear Layer …**

## Model Development for Fluid Flow Applications

The dynamic behaviour of fluid motion is driven by processes on a wide range of spatial and temporal scales. In a project run by Heidelberg University scientists, parts of model systems that describe fluid dynamics and temperature evolution were investigated. The models are formulated in terms of velocity, temperature, pressure, and density. The researchers employ a hierarchy of different physical models with an increasing degree of complexity. Additionally, uncertain input parameters are taken into account.

**Principal Investigator:** Philipp Gerstner, Engineering Mathematics and Computing Lab (EMCL), Ruprecht-Karls-Universität Heidelberg (Germany)

**HPC Platform:** JUQUEEN (JSC) -** Date published: **March 2018* (hka14)*

**More: Model Development for Fluid Flow Applications …**

## Study of Strong Decays and Resonances at the Physical Pion Mass in Lattice QCD

In the quark model mesons are made up of a quark and an antiquark and baryons of three quarks. The theory of the strong interactions, QCD, however, suggests that more complicated structures are possible. New experimental results strongly point at the possibility of tetraquarks, close to strong decay thresholds into two mesons. To understand these structures, simulations are necessary that include these scattering states. For the first time such as study was performed in Lattice QCD, with nearly physical quark masses. First the well-known ρ-resonance was investigated and then the Tetraquark candidate states D*_{s0}(2317) and D_{s1}(2460).

**Principal Investigator:** Gunnar Bali, Institut für Theoretische Physik, Universität Regensburg (Germany)

**HPC Platform:** SuperMUC (LRZ) - **Date published: **March 2018 *(pr94ni)*

**More: Study of Strong Decays and Resonances at the Physical Pion Mass in Lattice QCD …**

## Investigation of Green Propellants in Rocket Combustion Chambers

Researchers at the Chair of Turbomachinery and Flight Propulsion (LTF) at the Technical University Munich numerically investigate flow and combustion in rocket engines using “green” propellants. The current focus involves researching methane/oxygen as a propellant combination, promising to be a good replacement for the commonly used hydrazine, offering good performance, storability, and handling qualities, while also being significantly less toxic. The goal of the project is an improved understanding of the relevant physical processes and a reliable prediction of thermal loads on the combustor.

**Principal Investigator:** Prof. Dr.- Ing. Oskar J. Haidn, TUM Department of Mechanical Engineering, Technical University of Munich (Germany)

**HPC Platform:** SuperMUC (LRZ) -** Date published: **March 2018* (pr83bi)*

**More: Investigation of Green Propellants in Rocket Combustion Chambers …**

## Theoretical Heterogeneous Catalysis from Advanced Ab Initio Molecular Dynamics Simulations

The work horse of chemical industry is heterogeneous catalysis meaning that complex solid materials (catalysts) are used to facilitate chemical reactions, thus reducing production costs. To improve such catalysts in a systematic manner, knowledge of the ongoing reactions is most desirable. One of the key reactions industry performs at large scales is methanol (“wood alcohol”, H_{3}COH) synthesis from syngas being a mixture of gaseous CO_{2}, CO, and H_{2}. Scientists investigated the methanol production which is catalyzed using copper nanoparticles on a zinc oxide support. Based on sophisticated molecular dynamics sampling techniques in conjunction with the large-scale parallel platform SuperMUC at LRZ, they discovered a hitherto unknown complex reaction network with many parallel paths as well as dead ends that ultimately leads to the reaction of syngas to methanol.

**Principal Investigator:** Dominik Marx, Lehrstuhl für Theoretische Chemie, Ruhr-Universität Bochum, Bochum (Germany)

**HPC Platform:** SuperMUC (LRZ) - **Date published:** March 2018* **(pr63ce)*

**More: Theoretical Heterogeneous Catalysis from Advanced Ab Initio Molecular Dynamics Simulations …**

## Hadron Scattering and Resonance Properties from Lattice QCD

It is a long lasting dream in nuclear physics to study nuclei like, for instance, carbon directly from Quantum Chromodynamics (QCD), the underlying fundamental theory of strong interactions. Such an endeavor is very challenging both, methodically and numerically. Towards this goal physicists from the European Twisted Mass Collaboration and in particular the University of Bonn have started to investigate two hadron systems using the approach of Lattice QCD.

**Principal Investigator:** Carsten Urbach, Helmholtz Institut für Strahlen und Kernphysik (Theorie), Rheinische Friedrich-Wilhelms-Universität Bonn (Germany)

**HPC Platform:** JUQUEEN/JSC and Hazel Hen/HLRS

**Date published: **February 2018 *(hbn28/GCS_hsrp)*

**More: Hadron Scattering and Resonance Properties from Lattice QCD …**

## Turbulent Convection at Very Low Prandtl Numbers

In many turbulent convection flows in nature and technology the thermal diffusivity is much higher than the kinematic viscosity which means that the Prandtl number is very low. Applications of this regime reach from deep solar convection, via convection in the liquid metal core of the Earth to liquid metal batteries for grid energy storage and nuclear engineering technology. Laboratory experiments in low-Prandtl-number convection for Pr < 0.1 have to be conducted in liquid metals which are inaccessible for laser imaging techniques and require analysis by ultrasound or X-rays. Direct numerical simulations of this regime of turbulent convection at high Rayleigh numbers are the only way to reveal the full three-dimensional structure of temperature and velocity fields.

**Principal Investigator:** Jörg Schumacher, Technische Universität Ilmenau (Germany)

**HPC Platform:** JUQUEEN (JSC) -** Date published: **February 2018* (hil09)*

**More: Turbulent Convection at Very Low Prandtl Numbers …**

## Fathoming the Processes inside Rocket Combustion Chambers

At the Institute of Combustion Technology for Aerospace Engineering (IVLR) of the University of Stuttgart a team of scientists numerically investigates reacting flows at conditions typical for modern space transportation systems. The goal of the project is the better understanding of the ongoing processes in the combustion chambers and an improvement of the thermal load predictions. The research is integrated into the program "Technological Foundations for the Design of Thermally and Mechanically Highly Loaded Components of Future Space Transportation Systems" funded by the DFG.

**Principal Investigator:** Peter Gerlinger, IVLR, Universität Stuttgart (Germany)

**HPC Platform:** Hazel Hen (HLRS) -** Date published: **February 2018* (scrcomb)*

**More: Fathoming the Processes inside Rocket Combustion Chambers …**

## Numerical Analysis of Space Launcher Wake Flows

A research group from the Institute of Aerodynamics (AIA) of the RWTH Aachen University utilized the computing power of Hazel Hen for large-scale simulations to analyze the intricate wake flow phenomena of space launchers. The objective of the project is the fundamental understanding of the origin of so called buffet loads acting on the nozzle which can lead to critical structural damage and to develop flow control devices to increase the efficiency and reliability of orbital transportation systems necessary for the steadily increasing demand for communication and navigation satellites.

**Principal Investigator:** Wolfgang Schröder, Institute of Aerodynamics, RWTH Aachen University (Germany)

**HPC Platform:** Hazel Hen (HLRS) -** Date published: **February 2018* (gcs_jean)*

**More: Numerical Analysis of Space Launcher Wake Flows …**

## Influence of Velocity Changes During Directional Solidification Using Large-Scale Phase-Field Simulations

Simulations have long been an integral part to supplement experiment and theory and became a powerful method to improve the understanding of physical phenomena. Leveraging the phase-field method - an established means for the investigation of the diffusion and phase-transformation-included microstructure evolution during solidification processes in 3D - materials scientists use high-performance computing to study representative volume elements resolving the multiphase microstructure which can be compared with experimental micrographs. Massive-parallel and highly optimized solvers are applied to increase the efficiencies of the simulations in the scientists' pursuit to investigate the directional solidification of binary and ternary eutectic reactions in large-scale domains.

**Principal Investigator:** Britta Nestler, Karlsruhe Institute of Technology, Karlsruhe (Germany)

**HPC Platform:** Hazel Hen (HLRS) - **Date published:** February 2018** ***(pace3d)*

**More: Influence of Velocity Changes During Directional Solidification Using Large-Scale Phase-Field Simulations …**

## Improved Characterization of Fluxes Across Compartmental Interfaces

Data Assimilation is an integral tool to enable precise forecasts and becomes increasingly important to derive the values of uncertain parameters due to lack of observations. Numerical models of Earth system compartments are coupled in order to simulate physically consistent water and energy fluxes in the subsurface-landsurface-atmosphere system. Such model systems become increasingly important to analyze and understand the complex processes at boundaries of terrestrial compartments and interdependencies of states across these boundaries. As such, data assimilation for these coupled systems needs to be developed.

**Principal Investigator:** Clemens Simmer, Meteorological Institute, University of Bonn (Germany)

**HPC Platform:** JUQUEEN/JURECA (JSC) - **Date published:** February 2018* (hbn29)*

**More: Improved Characterization of Fluxes Across Compartmental Interfaces …**

## Unravelling the interior Evolution of Rocky Planets Through Large-Scale Numerical Simulations

The large amount of data returned by several space missions to the terrestrial planets has greatly improved our understanding of the similarities and differences between the innermost planets of our Solar System. Nevertheless, their interior remains poorly known since most of the data is related to surface processes. In the absence of direct data of the interior evolution of terrestrial planets, numerical simulations of mantle convection are an important mean to reconstruct the thermal and chemical history of the interior of the Earth, Moon, Mercury, Venus and Mars. In this project, run on Hornet of HLRS, researchers used the mantle convection code Gaia to model the thermal evolution of terrestrial planets and in particular the early stage of their history.

**Principal Investigator: **Ana-Catalina Plesa, German Aerospace Center/DLR, Berlin (Germany)

**HPC Platform:** Hornet/HLRS - **Date published:** January 2018* (MATHECO)*

**More: Unravelling the interior Evolution of Rocky Planets Through Large-Scale Numerical Simulations …**