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
Mitchell M
(2021)
A general framework to test gravity using galaxy clusters IV: cluster and halo properties in DGP gravity
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
A general framework to test gravity using galaxy clusters III: observable-mass scaling relations in f ( R ) gravity
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
The impact of modified gravity on the Sunyaev-Zeldovich effect
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2020)
Galactic outflow rates in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2022)
How gas flows shape the stellar-halo mass relation in the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2022)
Baryonic mass budgets for haloes in the eagle simulation, including ejected and prevented gas
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2020)
Galactic inflow and wind recycling rates in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Mocz P
(2023)
Cosmological structure formation and soliton phase transition in fuzzy dark matter with axion self-interactions
in Monthly Notices of the Royal Astronomical Society
Moews B
(2021)
Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Molaro M
(2022)
The effect of inhomogeneous reionization on the Lyman a forest power spectrum at redshift z > 4: implications for thermal parameter recovery
in Monthly Notices of the Royal Astronomical Society
Molaro M
(2023)
Possible evidence for a large-scale enhancement in the Lyman-a forest power spectrum at redshift z = 4
in Monthly Notices of the Royal Astronomical Society
Monaco P
(2020)
The accuracy of weak lensing simulations
in Monthly Notices of the Royal Astronomical Society
Montargès M
(2023)
The VLT/SPHERE view of the ATOMIUM cool evolved star sample I. Overview: Sample characterization through polarization analysis
in Astronomy & Astrophysics
Morello G
(2023)
Spitzer thermal phase curve of WASP-121 b
in Astronomy & Astrophysics
Morison A
(2024)
Effects of stratification on overshooting and waves atop the convective core of M? main-sequence stars
in Monthly Notices of the Royal Astronomical Society
Mosbech M
(2023)
Gravitational-wave event rates as a new probe for dark matter microphysics
in Physical Review D
Mou Z
(2021)
Simulations of a bubble wall interacting with an electroweak plasma
in Journal of High Energy Physics
Mougeot M
(2020)
Examining the N = 28 shell closure through high-precision mass measurements of Ar 46 - 48
in Physical Review C
Mukherjee S
(2021)
SEAGLE - II. Constraints on feedback models in galaxy formation from massive early-type strong-lens galaxies
in Monthly Notices of the Royal Astronomical Society
Murtas G
(2024)
Kink Instability of Flux Ropes in Partially Ionized Plasmas
in The Astrophysical Journal
Murtas G
(2022)
Collisional ionization and recombination effects on coalescence instability in chromospheric partially ionized plasmas
in Physics of Plasmas
Nasir F
(2024)
Deep learning the intergalactic medium using Lyman-alpha forest at 4 = z = 5
in Monthly Notices of the Royal Astronomical Society
Navarro J
(2020)
The edge of the Galaxy
in Monthly Notices of the Royal Astronomical Society
Nazari Z
(2021)
Oscillon collapse to black holes
in Journal of Cosmology and Astroparticle Physics
Nealon R
(2020)
Rocking shadows in broken circumbinary discs
in Monthly Notices of the Royal Astronomical Society: Letters
Nealon R
(2020)
Spirals, shadows & precession in HD 100453 - II. The hidden companion
in Monthly Notices of the Royal Astronomical Society
Nealon R
(2019)
Flyby-induced misalignments in planet-hosting discs
in Monthly Notices of the Royal Astronomical Society
Negri A
(2022)
The luminosity of cluster galaxies in the Cluster-EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Nelson R
(2023)
Gas accretion onto Jupiter mass planets in discs with laminar accretion flows
in Astronomy & Astrophysics
Nicholson B
(2024)
HD152843 b & c: the masses and orbital periods of a sub-Neptune and a superpuff Neptune
in Monthly Notices of the Royal Astronomical Society
Nightingale J
(2023)
Abell 1201: detection of an ultramassive black hole in a strong gravitational lens
in Monthly Notices of the Royal Astronomical Society
Nightingale J
(2021)
PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
in Journal of Open Source Software
Nightingale J
(2021)
PyAutoLens: Open-Source Strong Gravitational Lensing
in Journal of Open Source Software
Nightingale J
(2024)
Scanning for dark matter subhaloes in Hubble Space Telescope imaging of 54 strong lenses
in Monthly Notices of the Royal Astronomical Society
Nikolaev A
(2020)
Mesonic correlators at non-zero baryon chemical potential
Nixon C
(2021)
Partial, Zombie, and Full Tidal Disruption of Stars by Supermassive Black Holes
in The Astrophysical Journal
Nixon C
(2022)
Stellar Revival and Repeated Flares in Deeply Plunging Tidal Disruption Events
in The Astrophysical Journal Letters
Nixon C
(2021)
Accretion discs with non-zero central torque
in New Astronomy
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
Nobels F
(2024)
Tests of subgrid models for star formation using simulations of isolated disc galaxies
in Monthly Notices of the Royal Astronomical Society
Norman S
(2021)
Stars Crushed by Black Holes. I. On the Energy Distribution of Stellar Debris in Tidal Disruption Events
in The Astrophysical Journal
Nowak M
(2024)
The orbit of HD 142527 B is too compact to explain many of the disc features
in Astronomy & Astrophysics
Oestreicher A
(2024)
Backreaction in Numerical Relativity: Averaging on Newtonian gauge-like hypersurfaces in Einstein Toolkit cosmological simulations
in The Open Journal of Astrophysics
Offler S
(2020)
News from bottomonium spectral functions in thermal QCD
Oleskiewicz P
(2020)
Sensitivity analysis of a galaxy formation model
in Monthly Notices of the Royal Astronomical Society
Olsen K
(2021)
sígame v3: Gas Fragmentation in Postprocessing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
in The Astrophysical Journal
Oman K
(2024)
A warm dark matter cosmogony may yield more low-mass galaxy detections in 21-cm surveys than a cold dark matter one
in Monthly Notices of the Royal Astronomical Society
Oppenheimer B
(2020)
Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2023)
Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2021)
EDGE: two routes to dark matter core formation in ultra-faint dwarfs
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 |