DiRAC-3 Operations 2019-2022 - Edinburgh
Lead Research Organisation:
University of Edinburgh
Department Name: Sch of Physics and Astronomy
Abstract
Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.
Planned Impact
The DiRAC-3 Facility strategy for impact and innovation delivery is well-aligned with the UK government Industrial Strategy. As such, much of our societal and economic impact will continue to be driven by our engagements with industry. Each DiRAC-3 service provider has a local industrial strategy to deliver continued high levels of industrial engagement and to explore avenues to increase innovation and industrial returns over the next three years. Progress towards the industrial strategy goals will be monitored by the Service Management Boards and the DiRAC Technical Manager and reported to STFC via the DiRAC Oversight Committee.
The "Pathways to Impact" document attached to the lead JeS form for this proposal describes the overall DiRAC-3 industrial strategy, including our strategic goals and key performance indicators.
Examples of the expected impact of DiRAC-3 include:
Dissemination of best practice in High Performance Computing software engineering throughout the theoretical Particle Physics, Astronomy and Nuclear physics communities in the UK as well as to industry partners.
Training of the next generation of research scientists to tackle problems effectively on state-of-the- art of High Performance Computing facilities. Such skills are much in demand from high-tech industry and the cadre of highly-skilled, computationally literate individuals nurtured by DiRAC-3 will have influence beyond academia and will help to maintain the UK's scientific and economic leadership.
Development and delivery of co-design projects with industry partners to improve future generations of hardware and software.
Development of new techniques in the area of High Performance Data Analytics which will benefit industry partners and researchers in other fields such as biomedicine, biology, engineering, economics and social science, and the natural environment who can use these developments to improve research outcomes in their areas.
Sharing of best practice on the design and operation of distributed HPC facilities with UK National e-Infrastructure partners and providing leadership towards an integrated UKRI National e-Infrastructure. By supporting the uptake of emerging technologies by the DiRAC research communities, we will enable other research communities, both in academia and industry, to explore the value of using leading-edge technology to support their research workflows.
Engagement with the general public to promote interest in science, and to explain how our ability to solve complex problems using the latest computer technology leads to new scientific capabilities/insights. Engagement of this kind also naturally encourages the uptake of STEM subjects in schools.
The "Pathways to Impact" document attached to the lead JeS form for this proposal describes the overall DiRAC-3 industrial strategy, including our strategic goals and key performance indicators.
Examples of the expected impact of DiRAC-3 include:
Dissemination of best practice in High Performance Computing software engineering throughout the theoretical Particle Physics, Astronomy and Nuclear physics communities in the UK as well as to industry partners.
Training of the next generation of research scientists to tackle problems effectively on state-of-the- art of High Performance Computing facilities. Such skills are much in demand from high-tech industry and the cadre of highly-skilled, computationally literate individuals nurtured by DiRAC-3 will have influence beyond academia and will help to maintain the UK's scientific and economic leadership.
Development and delivery of co-design projects with industry partners to improve future generations of hardware and software.
Development of new techniques in the area of High Performance Data Analytics which will benefit industry partners and researchers in other fields such as biomedicine, biology, engineering, economics and social science, and the natural environment who can use these developments to improve research outcomes in their areas.
Sharing of best practice on the design and operation of distributed HPC facilities with UK National e-Infrastructure partners and providing leadership towards an integrated UKRI National e-Infrastructure. By supporting the uptake of emerging technologies by the DiRAC research communities, we will enable other research communities, both in academia and industry, to explore the value of using leading-edge technology to support their research workflows.
Engagement with the general public to promote interest in science, and to explain how our ability to solve complex problems using the latest computer technology leads to new scientific capabilities/insights. Engagement of this kind also naturally encourages the uptake of STEM subjects in schools.
Organisations
Publications
Reid J
(2020)
Coronal energy release by MHD avalanches: Heating mechanisms
in Astronomy & Astrophysics
Hildebrandt H
(2020)
KiDS+VIKING-450: Cosmic shear tomography with optical and infrared data
in Astronomy & Astrophysics
Blondin S
(2022)
StaNdaRT: a repository of standardised test models and outputs for supernova radiative transfer
in Astronomy & Astrophysics
Hutchinson A
(2023)
Impact of corotation on gradual solar energetic particle event intensity profiles
in Astronomy & Astrophysics
Sifón C
(2024)
The history and mass content of cluster galaxies in the EAGLE simulation
in Astronomy & Astrophysics
Drummond B
(2020)
Implications of three-dimensional chemical transport in hot Jupiter atmospheres: Results from a consistently coupled chemistry-radiation-hydrodynamics model
in Astronomy & Astrophysics
Fenton A
(2024)
The 3D structure of disc-instability protoplanets
in Astronomy & Astrophysics
Nowak M
(2024)
The orbit of HD 142527 B is too compact to explain many of the disc features
in Astronomy & Astrophysics
Upadhyay A
(2021)
Star formation histories of Coma cluster galaxies matched to simulated orbits hint at quenching around first pericenter
in Astronomy & Astrophysics
Montargès M
(2023)
The VLT/SPHERE view of the ATOMIUM cool evolved star sample I. Overview: Sample characterization through polarization analysis
in Astronomy & Astrophysics
Constantino T
(2021)
Suppression of lithium depletion in young low-mass stars from fast rotation
in Astronomy & Astrophysics
Dutta R
(2024)
Metal line emission around z < 1 galaxies
in Astronomy & Astrophysics
Rouillard A
(2020)
Models and data analysis tools for the Solar Orbiter mission
in Astronomy & Astrophysics
Witstok J
(2021)
Prospects for observing the low-density cosmic web in Lyman- a emission
in Astronomy & Astrophysics
Nelson R
(2023)
Gas accretion onto Jupiter mass planets in discs with laminar accretion flows
in Astronomy & Astrophysics
Vandenbroucke B
(2021)
Polarised emission from aligned dust grains in nearby galaxies: Predictions from the Auriga simulations
in Astronomy & Astrophysics
Lega E
(2021)
Migration of Jupiter-mass planets in low-viscosity discs
in Astronomy & Astrophysics
Reissl S
(2020)
Synthetic observations of spiral arm tracers of a simulated Milky Way analog
in Astronomy & Astrophysics
Ratnasingam R
(2023)
Internal gravity waves in massive stars II. Frequency analysis across stellar mass
in Astronomy & Astrophysics
Evstafyeva T
(2023)
Unequal-mass boson-star binaries: initial data and merger dynamics
in Classical and Quantum Gravity
Figueras P
(2020)
Gravitational collapse in cubic Horndeski theories
in Classical and Quantum Gravity
Helfer T
(2022)
Malaise and remedy of binary boson-star initial data
in Classical and Quantum Gravity
Adamek J
(2020)
Numerical solutions to Einstein's equations in a shearing-dust universe: a code comparison
in Classical and Quantum Gravity
Pandya A
(2022)
Dynamics of a nonminimally coupled scalar field in asymptotically AdS 4 spacetime
in Classical and Quantum Gravity
Cardoso V
(2023)
Curvature and dynamical spacetimes: can we peer into the quantum regime?
in Classical and Quantum Gravity
Radia M
(2022)
Lessons for adaptive mesh refinement in numerical relativity
in Classical and Quantum Gravity
Hoy C
(2024)
A rapid multi-modal parameter estimation technique for LISA
in Classical and Quantum Gravity
Gerosa D
(2022)
The irreducible mass and the horizon area of LIGO's black holes
in Classical and Quantum Gravity
Croft R
(2023)
The gravitational afterglow of boson stars
in Classical and Quantum Gravity
Sedda M
(2020)
The missing link in gravitational-wave astronomy: discoveries waiting in the decihertz range
in Classical and Quantum Gravity
Clough K
(2021)
Continuity equations for general matter: applications in numerical relativity
in Classical and Quantum Gravity
Ripley J
(2022)
Computing the quasinormal modes and eigenfunctions for the Teukolsky equation using horizon penetrating, hyperboloidally compactified coordinates
in Classical and Quantum Gravity
Aurrekoetxea J
(2020)
Coherent gravitational waveforms and memory from cosmic string loops
in Classical and Quantum Gravity
Barone T
(2024)
Gravitational lensing reveals cool gas within 10-20 kpc around a quiescent galaxy
in Communications Physics
Abhishek
(2024)
The TDHF code Sky3D version 1.2
in Computer Physics Communications
Tsang Y
(2020)
Characterising Jupiter's dynamo radius using its magnetic energy spectrum
in Earth and Planetary Science Letters
Skullerud J
(2022)
Hadrons at high temperature: An update from the FASTSUM collaboration
in EPJ Web of Conferences
Lawlor D
(2022)
Thermal Transitions in Dense Two-Colour QCD
in EPJ Web of Conferences
Spriggs T
(2022)
A comparison of spectral reconstruction methods applied to non-zero temperature NRQCD meson correlation functions
in EPJ Web of Conferences
Attanasio F
(2022)
Equation of state from complex Langevin simulations
in EPJ Web of Conferences
Di Carlo M
(2022)
Electromagnetic finite-size effects beyond the point-like approximation
in EPJ Web of Conferences
Changeat Q
(2022)
Disentangling atmospheric compositions of K2-18 b with next generation facilities.
in Experimental astronomy
Trotta D
(2022)
Single-spacecraft techniques for shock parameters estimation: A systematic approach
in Frontiers in Astronomy and Space Sciences
Tinoco-Arenas A
(2022)
Parametric Study of Magnetosheath Jets in 2D Local Hybrid Simulations
in Frontiers in Astronomy and Space Sciences
Matteini L
(2020)
Magnetic Field Turbulence in the Solar Wind at Sub-ion Scales: In Situ Observations and Numerical Simulations
in Frontiers in Astronomy and Space Sciences
Stevenson P
(2022)
Mean-field simulations of Es-254 + Ca-48 heavy-ion reactions
in Frontiers in Physics
Rizzuti F
(2024)
Stellar Evolution and Convection in 3D Hydrodynamic Simulations of a Complete Burning Phase
in Galaxies
Barausse E
(2020)
Prospects for fundamental physics with LISA
in General Relativity and Gravitation
Gupta P
(2022)
A study of global magnetic helicity in self-consistent spherical dynamos
in Geophysical & Astrophysical Fluid Dynamics
Mason S
(2022)
Magnetoconvection in a rotating spherical shell in the presence of a uniform axial magnetic field
in Geophysical & Astrophysical Fluid Dynamics
| Title | Supplemental data for the report "Optimisation of lattice simulations energy efficiency" |
| Description | Supplemental data for the report "Optimisation of lattice simulations energy efficiency". Also available as a git repository. It contains: Full copy of benchmark run directories Power monitoring scripts Power monitoring raw measurements Power monitoring data analysis and results used in the report For a more complete description, please see the README.md file. |
| Type Of Material | Database/Collection of data |
| Year Produced | 2022 |
| Provided To Others? | Yes |
| URL | https://zenodo.org/record/7057645 |
| Title | Supplemental data for the report "Optimisation of lattice simulations energy efficiency" |
| Description | Supplemental data for the report "Optimisation of lattice simulations energy efficiency". Also available as a git repository. It contains: Full copy of benchmark run directories Power monitoring scripts Power monitoring raw measurements Power monitoring data analysis and results used in the report For a more complete description, please see the README.md file. |
| Type Of Material | Database/Collection of data |
| Year Produced | 2022 |
| Provided To Others? | Yes |
| URL | https://zenodo.org/record/7057644 |