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
Slyz A
(2020)
How to quench a dwarf galaxy: The impact of inhomogeneous reionization on dwarf galaxies and cosmic filaments
in Monthly Notices of the Royal Astronomical Society
Evans T
(2020)
How unusual is the Milky Way's assembly history?
in Monthly Notices of the Royal Astronomical Society
Lower S
(2020)
How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting
in The Astrophysical Journal
Hou J
(2021)
How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
in Monthly Notices of the Royal Astronomical Society
Edwards B
(2020)
Hubble WFC3 Spectroscopy of the Habitable-zone Super-Earth LHS 1140 b
in The Astronomical Journal
Moews B
(2021)
Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Ziampras A
(2023)
Hydrodynamic turbulence in disks with embedded planets
in Astronomy & Astrophysics
Sirks E
(2024)
Hydrodynamical simulations of merging galaxy clusters: giant dark matter particle colliders, powered by gravity
in Monthly Notices of the Royal Astronomical Society
Pagano P
(2020)
Hydrogen non-equilibrium ionisation effects in coronal mass ejections
in Astronomy & Astrophysics
Bosman S
(2022)
Hydrogen reionization ends by z = 5.3: Lyman-a optical depth measured by the XQR-30 sample
in Monthly Notices of the Royal Astronomical Society
Pearce F
(2020)
Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
in Monthly Notices of the Royal Astronomical Society
Kegerreis J
(2022)
Immediate Origin of the Moon as a Post-impact Satellite
in The Astrophysical Journal Letters
Dai K
(2024)
Impact Momentum Transfer-Insights from Numerical Simulation of Impacts on Large Boulders of Asteroids
in The Planetary Science Journal
Hutchinson A
(2023)
Impact of corotation on gradual solar energetic particle event intensity profiles
in Astronomy & Astrophysics
Vlaykov D
(2022)
Impact of radial truncation on global 2D hydrodynamic simulations for a Sun-like model
in Monthly Notices of the Royal Astronomical Society
Han D
(2022)
Impact of Radiation Feedback on the Formation of Globular Cluster Candidates during Cloud-Cloud Collisions
in The Astrophysical Journal
Eager-Nash J
(2020)
Implications of different stellar spectra for the climate of tidally locked Earth-like exoplanets
in Astronomy & Astrophysics
Raste J
(2021)
Implications of the z > 5 Lyman-a forest for the 21-cm power spectrum from the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
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
Chakraborty B
(2021)
Improved V c s determination using precise lattice QCD form factors for D ? K l ?
in Physical Review D
Donevski D
(2020)
In pursuit of giants I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies
in Astronomy & Astrophysics
Trujillo-Gomez S
(2023)
In situ or accreted? Using deep learning to infer the origin of extragalactic globular clusters from observables
in Monthly Notices of the Royal Astronomical Society
Callan F
(2024)
Including a luminous central remnant in radiative transfer simulations for Type Iax supernovae
in Monthly Notices of the Royal Astronomical Society
Borrow J
(2021)
Inconsistencies arising from the coupling of galaxy formation sub-grid models to pressure-smoothed particle hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Dome T
(2025)
Increased burstiness at high redshift in multiphysics models combining supernova feedback, radiative transfer, and cosmic rays
in Monthly Notices of the Royal Astronomical Society
Falck B
(2021)
Indra: a public computationally accessible suite of cosmological N -body simulations
in Monthly Notices of the Royal Astronomical Society
Towler I
(2024)
Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulations
in Monthly Notices of the Royal Astronomical Society
Poole-McKenzie R
(2020)
Informing dark matter direct detection limits with the ARTEMIS simulations
in Journal of Cosmology and Astroparticle Physics
Vandenbroucke B
(2020)
Infrared luminosity functions and dust mass functions in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Civiš S
(2023)
Infrared Spectra of Small Radicals for Exoplanetary Spectroscopy: OH, NH, CN and CH: The State of Current Knowledge.
in Molecules (Basel, Switzerland)
Czakon M
(2023)
Infrared-safe flavoured anti-kT jets
in Journal of High Energy Physics
Kupilas M
(2021)
Interactions of a shock with a molecular cloud at various stages of its evolution due to thermal instability and gravity
in Monthly Notices of the Royal Astronomical Society
Ratnasingam R
(2023)
Internal gravity waves in massive stars II. Frequency analysis across stellar mass
in Astronomy & Astrophysics
Stevenson P
(2020)
Internuclear potentials from the Sky3D code
in IOP SciNotes
Buie E
(2020)
Interpreting Observations of Absorption Lines in the Circumgalactic Medium with a Turbulent Medium
in The Astrophysical Journal
Hill A
(2022)
Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Robinson A
(2024)
Introducing cuDisc : a 2D code for protoplanetary disc structure and evolution calculations
in Monthly Notices of the Royal Astronomical Society
Young A
(2024)
Introducing two improved methods for approximating radiative cooling in hydrodynamical simulations of accretion discs
in Monthly Notices of the Royal Astronomical Society
Vizgan D
(2022)
Investigating the [C ii]-to-H i Conversion Factor and the H i Gas Budget of Galaxies at z ˜ 6 with Hydrodynamic Simulations
in The Astrophysical Journal Letters
Householder A
(2024)
Investigating the Atmospheric Mass Loss of the Kepler-105 Planets Straddling the Radius Gap
in The Astronomical Journal
Kalaghatgi C
(2021)
Investigating the effect of in-plane spin directions for precessing binary black hole systems
in Physical Review D
Linh B
(2021)
Investigation of the ground-state spin inversion in the neutron-rich Cl 47 , 49 isotopes
in Physical Review C
Scardoni C
(2022)
Inward and outward migration of massive planets: moving towards a stalling radius
in Monthly Notices of the Royal Astronomical Society
Hellinger P
(2022)
Ion-scale Transition of Plasma Turbulence: Pressure-Strain Effect
in The Astrophysical Journal
Dickey C
(2021)
IQ Collaboratory. II. The Quiescent Fraction of Isolated, Low-mass Galaxies across Simulations and Observations
in The Astrophysical Journal
Trotta D
(2023)
Irregular Proton Injection to High Energies at Interplanetary Shocks
in The Astrophysical Journal Letters
Changeat Q
(2024)
Is the Atmosphere of the Ultra-hot Jupiter WASP-121 b Variable?
in The Astrophysical Journal Supplement Series
Whitworth D
(2022)
Is the molecular KS relationship universal down to low metallicities?
in Monthly Notices of the Royal Astronomical Society
Badger S
(2023)
Isolated photon production in association with a jet pair through next-to-next-to-leading order in QCD
in Journal of High Energy Physics
Colò G
(2020)
Isoscalar monopole and quadrupole modes in Mo isotopes: Microscopic analysis
in Physics Letters B
| 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 |