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
Kordov Z
(2020)
Electromagnetic contribution to S - ? mixing using lattice QCD + QED
in Physical Review D
Kordov Z
(2021)
State mixing and masses of the p 0 , ? and ? ' mesons from n f = 1 + 1 + 1 lattice QCD + QED
in Physical Review D
Koponen J
(2022)
Properties of low-lying charmonia and bottomonia from lattice QCD + QED
in Suplemento de la Revista Mexicana de Física
Kong S
(2022)
Filament formation via collision-induced magnetic reconnection - formation of a star cluster
in Monthly Notices of the Royal Astronomical Society
Koiwai T
(2022)
A first glimpse at the shell structure beyond 54Ca: Spectroscopy of 55K, 55Ca, and 57Ca
in Physics Letters B
Kobayashi C
(2020)
New Type Ia Supernova Yields and the Manganese and Nickel Problems in the Milky Way and Dwarf Spheroidal Galaxies
in The Astrophysical Journal
Kobayashi C
(2020)
Stellar migrations and metal flows - Chemical evolution of the thin disc of a simulated Milky Way analogous galaxy
in Monthly Notices of the Royal Astronomical Society
Kobayashi C
(2020)
The Origin of Elements from Carbon to Uranium
in The Astrophysical Journal
Kirchschlager F
(2023)
Dust survival rates in clumps passing through the Cas A reverse shock - II. The impact of magnetic fields
in Monthly Notices of the Royal Astronomical Society
Kirchschlager F
(2020)
Silicate Grain Growth due to Ion Trapping in Oxygen-rich Supernova Remnants like Cassiopeia A
in The Astrophysical Journal
Kimm T
(2022)
A Systematic Study of the Escape of LyC and Lya Photons from Star-forming, Magnetized Turbulent Clouds
in The Astrophysical Journal Supplement Series
Khachaturyants T
(2022)
Bending waves excited by irregular gas inflow along warps
in Monthly Notices of the Royal Astronomical Society
Khachaturyants T
(2022)
The pattern speeds of vertical breathing waves
in Monthly Notices of the Royal Astronomical Society: Letters
Khachaturyants T
(2021)
How stars formed in warps settle into (and contaminate) thick discs
in Monthly Notices of the Royal Astronomical Society
Kewley L
(2020)
Oxygen loss from simulated galaxies and the metal flow main sequence: predicting the dependence on mass and environment
in Monthly Notices of the Royal Astronomical Society
Kelly A
(2022)
Apostle-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Kelly A
(2021)
The origin of X-ray coronae around simulated disc galaxies
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
Kegerreis J
(2020)
Atmospheric Erosion by Giant Impacts onto Terrestrial Planets: A Scaling Law for any Speed, Angle, Mass, and Density
in The Astrophysical Journal
Kegerreis J
(2020)
Atmospheric Erosion by Giant Impacts onto Terrestrial Planets
in The Astrophysical Journal
Keating L
(2020)
Long troughs in the Lyman-a forest below redshift 6 due to islands of neutral hydrogen
in Monthly Notices of the Royal Astronomical Society
Keating L
(2020)
Constraining the second half of reionization with the Ly ß forest
in Monthly Notices of the Royal Astronomical Society
Kay S
(2020)
The intracluster light as a tracer of the total matter density distribution: a view from simulations
in Monthly Notices of the Royal Astronomical Society
Katz H
(2023)
The challenges of identifying Population III stars in the early Universe
in Monthly Notices of the Royal Astronomical Society
Katz H
(2020)
New methods for identifying Lyman continuum leakers and reionization-epoch analogues
in Monthly Notices of the Royal Astronomical Society
Katz H
(2022)
RAMSES-RTZ: non-equilibrium metal chemistry and cooling coupled to on-the-fly radiation hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Katz H
(2023)
The SPHINX Public Data Release: Forward Modelling High-Redshift JWST Observations with Cosmological Radiation Hydrodynamics Simulations
in The Open Journal of Astrophysics
Katz H
(2023)
Two modes of LyC escape from bursty star formation: implications for [C ii ] deficits and the sources of reionization
in Monthly Notices of the Royal Astronomical Society
Katsianis A
(2020)
The high-redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: towards addressing the tension between observations and simulations
in Monthly Notices of the Royal Astronomical Society
Katsianis A
(2021)
The specific star formation rate function at different mass scales and quenching: a comparison between cosmological models and SDSS
in Monthly Notices of the Royal Astronomical Society
Karunakaran A
(2021)
Satellites around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations versus Simulations
in The Astrophysical Journal Letters
Kannan R
(2023)
The MillenniumTNG project: the galaxy population at z = 8
in Monthly Notices of the Royal Astronomical Society
Kalaghatgi C
(2021)
Investigating the effect of in-plane spin directions for precessing binary black hole systems
in Physical Review D
Joudaki S
(2020)
KiDS+VIKING-450 and DES-Y1 combined: Cosmology with cosmic shear
in Astronomy & Astrophysics
Joswig F
(2023)
Exploring distillation at the SU(3) flavour symmetric point
Jones C
(2021)
Fully developed anelastic convection with no-slip boundaries
in Journal of Fluid Mechanics
Johnston C
(2021)
A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method
in Astronomy & Astrophysics
Johnson C
(2021)
Excited J - - meson resonances at the SU(3) flavor point from lattice QCD
in Physical Review D
Ježo T
(2023)
Resonance-aware NLOPS matching for off-shell $$ t\overline{t} $$ + tW production with semileptonic decays
in Journal of High Energy Physics
Jennings F
(2023)
Shattering and growth of cold clouds in galaxy clusters: the role of radiative cooling, magnetic fields, and thermal conduction
in Monthly Notices of the Royal Astronomical Society
Jennings F
(2023)
Halo scaling relations and hydrostatic mass bias in the simba simulation from realistic mock X-ray catalogues
in Monthly Notices of the Royal Astronomical Society
Jahns-Schindler J
(2023)
How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
in Monthly Notices of the Royal Astronomical Society
Jackson T
(2020)
The star formation properties of the observed and simulated AGN Universe: BAT versus EAGLE
in Monthly Notices of the Royal Astronomical Society
Jackson R
(2021)
The origin of low-surface-brightness galaxies in the dwarf regime
in Monthly Notices of the Royal Astronomical Society
Jackson R
(2021)
Dark matter-deficient dwarf galaxies form via tidal stripping of dark matter in interactions with massive companions
in Monthly Notices of the Royal Astronomical Society
Izquierdo A
(2021)
The Disc Miner I. A statistical framework to detect and quantify kinematical perturbations driven by young planets in discs
in Astronomy & Astrophysics
Izquierdo A
(2021)
The Cloud Factory II: gravoturbulent kinematics of resolved molecular clouds in a galactic potential
in Monthly Notices of the Royal Astronomical Society
Iyer K
(2020)
The diversity and variability of star formation histories in models of galaxy evolution
in Monthly Notices of the Royal Astronomical Society
Irodotou D
(2022)
The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Irodotou D
(2021)
Using angular momentum maps to detect kinematically distinct galactic components
in Monthly Notices of the Royal Astronomical Society