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
Clough K
(2021)
Continuity equations for general matter: applications in numerical relativity
in Classical and Quantum Gravity
Buividovich P
(2021)
Static magnetic susceptibility in finite-density $$SU\left( 2\right) $$ lattice gauge theory
in The European Physical Journal A
Upadhyay A
(2021)
Star formation histories of Coma cluster galaxies matched to simulated orbits hint at quenching around first pericenter
in Astronomy & Astrophysics
Appleby S
(2021)
The low-redshift circumgalactic medium in simba
in Monthly Notices of the Royal Astronomical Society
Yip K
(2021)
Peeking inside the Black Box: Interpreting Deep-learning Models for Exoplanet Atmospheric Retrievals
in The Astronomical Journal
Czakon M
(2021)
NNLO QCD corrections to leptonic observables in top-quark pair production and decay
in Journal of High Energy Physics
Ragusa E
(2021)
Circumbinary and circumstellar discs around the eccentric binary IRAS 04158+2805 - a testbed for binary-disc interaction
in Monthly Notices of the Royal Astronomical Society
Davies C
(2021)
Optimal void finders in weak lensing maps
in Monthly Notices of the Royal Astronomical Society
Ramsøy M
(2021)
Rivers of gas - I. Unveiling the properties of high redshift filaments
in Monthly Notices of the Royal Astronomical Society
Nightingale J
(2021)
PyAutoLens: Open-Source Strong Gravitational Lensing
in Journal of Open Source Software
Ahad S
(2021)
The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at 0 < z < 1.5
in Monthly Notices of the Royal Astronomical Society
Becker G
(2021)
The mean free path of ionizing photons at 5 < z < 6: evidence for rapid evolution near reionization
in Monthly Notices of the Royal Astronomical Society
Ballabio G
(2021)
HD 143006: circumbinary planet or misaligned disc?
in Monthly Notices of the Royal Astronomical Society
Constantino T
(2021)
Suppression of lithium depletion in young low-mass stars from fast rotation
in Astronomy & Astrophysics
Nixon C
(2021)
Accretion discs with non-zero central torque
in New Astronomy
Fossati M
(2021)
MUSE analysis of gas around galaxies (MAGG) - III. The gas and galaxy environment of z = 3-4.5 quasars
in Monthly Notices of the Royal Astronomical Society
Hughes M
(2021)
What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Cheung G
(2021)
DK I = 0, $$ D\overline{K} $$ I = 0, 1 scattering and the $$ {D}_{s0}^{\ast } $$(2317) from lattice QCD
in Journal of High Energy Physics
Aumann T
(2021)
Quenching of single-particle strength from direct reactions with stable and rare-isotope beams
in Progress in Particle and Nuclear Physics
Witstok J
(2021)
Prospects for observing the low-density cosmic web in Lyman- a emission
in Astronomy & Astrophysics
Agudelo Rueda J
(2021)
Three-dimensional magnetic reconnection in particle-in-cell simulations of anisotropic plasma turbulence
in Journal of Plasma Physics
Elliott E
(2021)
Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
in Monthly Notices of the Royal Astronomical Society
Manzoni G
(2021)
Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS
in New Astronomy
Foster C
(2021)
The MAGPI survey: Science goals, design, observing strategy, early results and theoretical framework
in Publications of the Astronomical Society of Australia
Vandenbroucke B
(2021)
Polarised emission from aligned dust grains in nearby galaxies: Predictions from the Auriga simulations
in Astronomy & Astrophysics
Owens A
(2021)
ExoMol line lists - XLI. High-temperature molecular line lists for the alkali metal hydroxides KOH and NaOH
in Monthly Notices of the Royal Astronomical Society
Lega E
(2021)
Migration of Jupiter-mass planets in low-viscosity discs
in Astronomy & Astrophysics
Camps P
(2021)
Effects of Spatial Discretization in Lya Line Radiation Transfer Simulations
in The Astrophysical Journal
Clark V
(2021)
Modelling the non-local thermodynamic equilibrium spectra of silylene (SiH 2 )
in Physical Chemistry Chemical Physics
Habouzit M
(2021)
Supermassive black holes in cosmological simulations I: M BH - M ? relation and black hole mass function
in Monthly Notices of the Royal Astronomical Society
Wurster J
(2021)
The impact of non-ideal magnetohydrodynamic processes on discs, outflows, counter-rotation, and magnetic walls during the early stages of star formation
in Monthly Notices of the Royal Astronomical Society
Bourne M
(2021)
AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
in Monthly Notices of the Royal Astronomical Society
Czakon M
(2021)
B-hadron production in NNLO QCD: application to LHC t$$ \overline{t} $$ events with leptonic decays
in Journal of High Energy Physics
Guandalin C
(2021)
Observing relativistic features in large-scale structure surveys - I. Multipoles of the power spectrum
in Monthly Notices of the Royal Astronomical Society
Ryan S
(2021)
Excited and exotic bottomonium spectroscopy from lattice QCD
in Journal of High Energy Physics
Mitchell M
(2021)
The impact of modified gravity on the Sunyaev-Zeldovich effect
in Monthly Notices of the Royal Astronomical Society
Smith A
(2021)
Reducing the variance of redshift space distortion measurements from mock galaxy catalogues with different lines of sight
in Monthly Notices of the Royal Astronomical Society
Nazari Z
(2021)
Oscillon collapse to black holes
in Journal of Cosmology and Astroparticle Physics
Lee E
(2022)
A multisimulation study of relativistic SZ temperature scalings in galaxy clusters and groups
in Monthly Notices of the Royal Astronomical Society
Qiao L
(2022)
The evolution of protoplanetary discs in star formation and feedback simulations
in Monthly Notices of the Royal Astronomical Society
Bolton JS
(2022)
Comparison of Low-Redshift Lyman-a Forest Observations to Hydrodynamical Simulations with Dark Photon Dark Matter.
in Physical review letters
Sawala T
(2022)
The SIBELIUS Project: E Pluribus Unum
in Monthly Notices of the Royal Astronomical Society
Drew A
(2022)
Radiation from global topological strings using adaptive mesh refinement: Methodology and massless modes
in Physical Review D
Wakita S
(2022)
Effect of Impact Velocity and Angle on Deformational Heating and Postimpact Temperature
in Journal of Geophysical Research: Planets
Wright S
(2022)
Non-local thermal equilibrium spectra of atmospheric molecules for exoplanets
in Monthly Notices of the Royal Astronomical Society
Christie D
(2022)
CAMEMBERT: A Mini-Neptunes General Circulation Model Intercomparison, Protocol Version 1.0.A CUISINES Model Intercomparison Project
in The Planetary Science Journal
Borukhovetskaya A
(2022)
The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
in Monthly Notices of the Royal Astronomical Society
Nobels F
(2022)
The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Dobbs C
(2022)
The formation of massive stellar clusters in converging galactic flows with photoionization
in Monthly Notices of the Royal Astronomical Society
Zhang H
(2022)
Spherical accretion of collisional gas in modified gravity I: self-similar solutions and a new cosmological hydrodynamical code
in Monthly Notices of the Royal Astronomical Society
| 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 |