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
Orkney M
(2023)
EDGE: the shape of dark matter haloes in the faintest galaxies
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2022)
EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
in Monthly Notices of the Royal Astronomical Society
Owen J
(2020)
Testing exoplanet evaporation with multitransiting systems
in Monthly Notices of the Royal Astronomical Society
Owen J
(2020)
Massive discs around low-mass stars
in Monthly Notices of the Royal Astronomical Society
Owens A
(2024)
ExoMol line lists - LI. Molecular line lists for lithium hydroxide (LiOH)
in Monthly Notices of the Royal Astronomical Society
Owens A
(2021)
Theoretical rovibronic spectroscopy of the calcium monohydroxide radical (CaOH).
in The Journal of chemical physics
Owens A
(2024)
ExoMol line lists - LVIII. High-temperature molecular line list of carbonyl sulphide (OCS)
in Monthly Notices of the Royal Astronomical Society
Owens A
(2022)
ExoMol line lists - XLVII. Rovibronic molecular line list of the calcium monohydroxide radical (CaOH)
in Monthly Notices of the Royal Astronomical Society
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
Pagano P
(2020)
Effect of coronal loop structure on wave heating through phase mixing
in Astronomy & Astrophysics
Pagano P
(2020)
Hydrogen non-equilibrium ionisation effects in coronal mass ejections
in Astronomy & Astrophysics
Pakmor R
(2024)
Magnetic field amplification in cosmological zoom simulations from dwarf galaxies to galaxy groups
in Monthly Notices of the Royal Astronomical Society
Pakmor R
(2020)
The orbital phase space of contracted dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Pakmor R
(2023)
The MillenniumTNG Project: the hydrodynamical full physics simulation and a first look at its galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Pallero D
(2024)
Galaxy evolution in modified gravity simulations: using galaxy properties to constrain our gravitational model
in Monthly Notices of the Royal Astronomical Society
Pandya A
(2022)
Dynamics of a nonminimally coupled scalar field in asymptotically AdS 4 spacetime
in Classical and Quantum Gravity
Panic O
(2020)
TW Hya: an old protoplanetary disc revived by its planet
in Monthly Notices of the Royal Astronomical Society
Pariat E
(2023)
Comparison of magnetic energy and helicity in coronal jet simulations
in Astronomy & Astrophysics
Parrott W
(2023)
Standard Model predictions for B ? K l + l - , B ? K l 1 - l 2 + and B ? K ? ? ¯ using form factors from N f = 2 + 1 + 1 lattice QCD
in Physical Review D
Parrott W
(2021)
Toward accurate form factors for B -to-light meson decay from lattice QCD
in Physical Review D
Parrott W
(2023)
B ? K and D ? K form factors from fully relativistic lattice QCD
in Physical Review D
Parrott W
(2022)
$V_{cs}$ determination from $D \to{}K \ell \nu$
Pastorek A
(2022)
New physical insights: Formamide discharge decomposition and the role of fragments in the formation of large biomolecules.
in Spectrochimica acta. Part A, Molecular and biomolecular spectroscopy
Pastorek A
(2022)
Time-resolved fourier transform infrared emission spectroscopy of NH radical in the X3S- ground state
in Journal of Quantitative Spectroscopy and Radiative Transfer
Patsourakos S
(2020)
Decoding the Pre-Eruptive Magnetic Field Configurations of Coronal Mass Ejections
in Space Science Reviews
Pearce F
(2021)
Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
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
Pedersen C
(2020)
Massive neutrinos and degeneracies in Lyman-alpha forest simulations
in Journal of Cosmology and Astroparticle Physics
Pedersen C
(2021)
An emulator for the Lyman-a forest in beyond-?CDM cosmologies
in Journal of Cosmology and Astroparticle Physics
Pellen M
(2022)
Angular coefficients in $$\hbox {W}+\hbox {j}$$ production at the LHC with high precision
in The European Physical Journal C
Penzlin A
(2024)
Viscous circumbinary protoplanetary discs - I. Structure of the inner cavity
in Monthly Notices of the Royal Astronomical Society
Pereira-Wilson M
(2023)
The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Petrovic H
(2024)
Material transport in protoplanetary discs with massive embedded planets
in Monthly Notices of the Royal Astronomical Society
Pettini M
(2020)
A bound on the 12C/13C ratio in near-pristine gas with ESPRESSO
in Monthly Notices of the Royal Astronomical Society
Pezzella M
(2021)
A method for calculating temperature-dependent photodissociation cross sections and rates.
in Physical chemistry chemical physics : PCCP
Pfeffer J
(2022)
Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2020)
Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2023)
Globular cluster metallicity distributions in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2024)
Origin of the correlation between stellar kinematics and globular cluster system richness in ultradiffuse galaxies
in Monthly Notices of the Royal Astronomical Society
Pfeifer S
(2020)
The BAHAMAS project: effects of dynamical dark energy on large-scale structure
in Monthly Notices of the Royal Astronomical Society
Phillips M
(2020)
A new set of atmosphere and evolution models for cool T-Y brown dwarfs and giant exoplanets
in Astronomy & Astrophysics
Pichon C
(2020)
And yet it flips: connecting galactic spin and the cosmic web
in Monthly Notices of the Royal Astronomical Society
Pichon C
(2020)
Why do extremely massive disc galaxies exist today?
in Monthly Notices of the Royal Astronomical Society
Pierens A
(2023)
Three-dimensional evolution of radiative circumbinary discs: The size and shape of the inner cavity
in Astronomy & Astrophysics
Pimpanuwat B
(2020)
Maser flares driven by variations in pumping and background radiation
in Monthly Notices of the Royal Astronomical Society
Pizzati E
(2024)
Revisiting the extreme clustering of z ˜ 4 quasars with large volume cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Pizzati E
(2024)
A unified model for the clustering of quasars and galaxies at z ˜ 6
in Monthly Notices of the Royal Astronomical Society
Ploeckinger S
(2020)
Radiative cooling rates, ion fractions, molecule abundances, and line emissivities including self-shielding and both local and metagalactic radiation fields
in Monthly Notices of the Royal Astronomical Society
Ploeckinger S
(2024)
Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multiphase interstellar medium
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 |