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
Yurchenko S
(2020)
ExoMol molecular line lists - XXXVII. Spectra of acetylene
in Monthly Notices of the Royal Astronomical Society
Davies CTH
(2020)
Lattice QCD Matrix Elements for the B_{s}^{0}-B[over ¯]_{s}^{0} Width Difference beyond Leading Order.
in Physical review letters
Cuesta-Lazaro C
(2020)
Towards a non-Gaussian model of redshift space distortions
in Monthly Notices of the Royal Astronomical Society
Eager-Nash J
(2020)
Implications of different stellar spectra for the climate of tidally locked Earth-like exoplanets
in Astronomy & Astrophysics
Rosca-Mead R
(2020)
Structure of Neutron Stars in Massive Scalar-Tensor Gravity
in Symmetry
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
Pakmor R
(2020)
The orbital phase space of contracted dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Campargue A
(2020)
Observation of electric-quadrupole infrared transitions in water vapor
in Physical Review Research
Clarke C
(2020)
Forbidden line diagnostics of photoevaporative disc winds
in Monthly Notices of the Royal Astronomical Society
Vidal J
(2020)
Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
in Monthly Notices of the Royal Astronomical Society
Aurrekoetxea J
(2020)
The effects of potential shape on inhomogeneous inflation
in Journal of Cosmology and Astroparticle Physics
Collins GS
(2020)
A steeply-inclined trajectory for the Chicxulub impact.
in Nature communications
Cooper R
(2020)
Subcritical dynamos in rapidly rotating planar convection
in Physical Review Fluids
Vandenbroucke B
(2020)
Infrared luminosity functions and dust mass functions in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2020)
Do model emission line galaxies live in filaments at z ~ 1?
in Monthly Notices of the Royal Astronomical Society
Wu X
(2020)
Photometric properties of reionization-epoch galaxies in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Richardson M
(2020)
Simulating gas kinematic studies of high-redshift galaxies with the HARMONI integral field spectrograph
in Monthly Notices of the Royal Astronomical Society
Currie L
(2020)
Convection with misaligned gravity and rotation: simulations and rotating mixing length theory
in Monthly Notices of the Royal Astronomical Society
Haehnelt M
(2020)
Probing delayed-end reionization histories with the 21-cm LAE cross-power spectrum
in Monthly Notices of the Royal Astronomical Society
Yoo T
(2020)
On the origin of low escape fractions of ionizing radiation from massive star-forming galaxies at high redshift
in Monthly Notices of the Royal Astronomical Society
Navarro J
(2020)
The edge of the Galaxy
in Monthly Notices of the Royal Astronomical Society
Sykes C
(2020)
Determining the primordial helium abundance and UV background using fluorescent emission in star-free dark matter haloes
in Monthly Notices of the Royal Astronomical Society
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
Barausse E
(2020)
Prospects for fundamental physics with LISA
in General Relativity and Gravitation
Howson T
(2020)
Phase mixing and wave heating in a complex coronal plasma
in Astronomy & Astrophysics
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
Henriques B
(2020)
L-GALAXIES 2020: Spatially resolved cold gas phases, star formation, and chemical enrichment in galactic discs
in Monthly Notices of the Royal Astronomical Society
Clark V
(2020)
The high-temperature rotation-vibration spectrum and rotational clustering of silylene (SiH2)
in Journal of Quantitative Spectroscopy and Radiative Transfer
Cooper L
(2020)
B c ? B s ( d ) form factors from lattice QCD
in Physical Review D
Adamek J
(2020)
Numerical solutions to Einstein's equations in a shearing-dust universe: a code comparison
in Classical and Quantum Gravity
Lovell M
(2020)
Local group star formation in warm and self-interacting dark matter cosmologies
in Monthly Notices of the Royal Astronomical Society
Bastian N
(2020)
The globular cluster system mass-halo mass relation in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Ilee J
(2020)
Observing protoplanetary discs with the Square Kilometre Array - I. Characterizing pebble substructure caused by forming planets
in Monthly Notices of the Royal Astronomical Society
Beraldo e Silva L
(2020)
Geometric properties of galactic discs with clumpy episodes
in Monthly Notices of the Royal Astronomical Society
Panic O
(2020)
TW Hya: an old protoplanetary disc revived by its planet
in Monthly Notices of the Royal Astronomical Society
Xu W
(2020)
Galaxy properties in the cosmic web of EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Can K
(2020)
Lattice QCD evaluation of the Compton amplitude employing the Feynman-Hellmann theorem
in Physical Review D
Bate M
(2020)
Photoionizing feedback in spiral arm molecular clouds
in Monthly Notices of the Royal Astronomical Society
Edwards B
(2020)
ARES I: WASP-76 b, A Tale of Two HST Spectra*
in The Astronomical Journal
Bower R
(2020)
Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Aoyama T
(2020)
The anomalous magnetic moment of the muon in the Standard Model
in Physics Reports
Arthuis P
(2020)
Ab Initio Computation of Charge Densities for Sn and Xe Isotopes.
in Physical review letters
Yurchenko S
(2020)
ExoMol line lists - XXXIX. Ro-vibrational molecular line list for CO2
in Monthly Notices of the Royal Astronomical Society
Pagano P
(2020)
Hydrogen non-equilibrium ionisation effects in coronal mass ejections
in Astronomy & Astrophysics
Robertson A
(2020)
Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
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
Hassan S
(2020)
Testing galaxy formation simulations with damped Lyman-a abundance and metallicity evolution
in Monthly Notices of the Royal Astronomical Society