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
Davies C
(2021)
Constraining cosmology with weak lensing voids
in Monthly Notices of the Royal Astronomical Society
Silva HO
(2021)
Dynamical Descalarization in Binary Black Hole Mergers.
in Physical review letters
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
Rogers J
(2021)
Photoevaporation versus core-powered mass-loss: model comparison with the 3D radius gap
in Monthly Notices of the Royal Astronomical Society
Grand R
(2021)
Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
in Monthly Notices of the Royal Astronomical Society
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
Glowacki M
(2021)
The redshift evolution of the baryonic Tully-Fisher relation in SIMBA
in Monthly Notices of the Royal Astronomical Society
Threlfall J
(2021)
Can Multi-threaded Flux Tubes in Coronal Arcades Support a Magnetohydrodynamic Avalanche?
in Solar physics
Wareing C
(2021)
Striations, integrals, hourglasses, and collapse - thermal instability driven magnetic simulations of molecular clouds
in Monthly Notices of the Royal Astronomical Society
Grisdale K
(2021)
Physical properties and scaling relations of molecular clouds: the impact of star formation
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
A general framework to test gravity using galaxy clusters - V. A self-consistent pipeline for unbiased constraints of f ( R ) gravity
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
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
Cui W
(2021)
The origin of galaxy colour bimodality in the scatter of the stellar-to-halo mass relation
in Nature Astronomy
Manzoni G
(2021)
Modelling the quenching of star formation activity from the evolution of the colour-magnitude relation in VIPERS
in New Astronomy
Schirra A
(2021)
Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Zarrouk P
(2021)
Baryon acoustic oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
in Monthly Notices of the Royal Astronomical Society
Traykova D
(2021)
Dynamical friction from scalar dark matter in the relativistic regime
in Physical Review D
Bennett E
(2021)
Glueballs and strings in S p ( 2 N ) Yang-Mills theories
in Physical Review D
Al-Refaie A
(2021)
TauREx 3: A Fast, Dynamic, and Extendable Framework for Retrievals
in The Astrophysical Journal
Del Debbio L
(2021)
Renormalization of the energy-momentum tensor in three-dimensional scalar SU(N) theories using the Wilson flow
in Physical Review D
Halim S
(2021)
Assessing the survivability of biomarkers within terrestrial material impacting the lunar surface
in Icarus
Deason A
(2021)
The mass of the Milky Way out to 100 kpc using halo stars
in Monthly Notices of the Royal Astronomical Society
Ruiz-Macias O
(2021)
Characterizing the target selection pipeline for the Dark Energy Spectroscopic Instrument Bright Galaxy Survey
in Monthly Notices of the Royal Astronomical Society
Elbers W
(2021)
An optimal non-linear method for simulating relic neutrinos
in Monthly Notices of the Royal Astronomical Society
Igoshev A
(2021)
3D Magnetothermal Simulations of Tangled Crustal Magnetic Field in Central Compact Objects
in The Astrophysical Journal
Srinivasan S
(2021)
Cosmological gravity on all scales. Part II. Model independent modified gravity N-body simulations
in Journal of Cosmology and Astroparticle Physics
Hamilton E
(2021)
Model of gravitational waves from precessing black-hole binaries through merger and ringdown
in Physical Review D
Chawdhry H
(2021)
Two-loop leading-color helicity amplitudes for three-photon production at the LHC
in Journal of High Energy Physics
Baxter E
(2021)
The correlation of high-redshift galaxies with the thermal Sunyaev-Zel'dovich effect traces reionization
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
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
Semenov M
(2021)
Rovibronic spectroscopy of PN from first principles.
in Physical chemistry chemical physics : PCCP
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
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
Shao S
(2021)
The survival of globular clusters in a cuspy Fornax
in Monthly Notices of the Royal Astronomical Society
Lovell C
(2021)
Reproducing submillimetre galaxy number counts with cosmological hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Nazari Z
(2021)
Oscillon collapse to black holes
in Journal of Cosmology and Astroparticle Physics
Hou J
(2021)
How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
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
DeGraf C
(2021)
Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
in Monthly Notices of the Royal Astronomical Society
Linh B
(2021)
Investigation of the ground-state spin inversion in the neutron-rich Cl 47 , 49 isotopes
in Physical Review C
BeraldoĀ eĀ Silva L
(2021)
Co-formation of the thin and thick discs revealed by APOGEE-DR16 and Gaia -DR2
in Monthly Notices of the Royal Astronomical Society
Steele T
(2021)
Precise calibration of the one-loop bispectrum in the effective field theory of large scale structure
in Physical Review D
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
Buividovich P
(2021)
Numerical study of the chiral separation effect in two-color QCD at finite density
in Physical Review D
Stafford S
(2021)
Testing extensions to ?CDM on small scales with forthcoming cosmic shear surveys
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
Alioli S
(2021)
Four-lepton production in gluon fusion at NLO matched to parton showers
in The European Physical Journal C
| 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 |
| 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 |