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
Cardoso V
(2023)
Curvature and dynamical spacetimes: can we peer into the quantum regime?
in Classical and Quantum Gravity
Cataldi P
(2022)
Fingerprints of modified gravity on galaxies in voids
in Monthly Notices of the Royal Astronomical Society
Cataneo M
(2022)
The matter density PDF for modified gravity and dark energy with Large Deviations Theory
in Monthly Notices of the Royal Astronomical Society
Cayuso R
(2023)
Self-Consistent Modeling of Gravitational Theories beyond General Relativity
in Physical Review Letters
Ceuster F
(2022)
3D Line Radiative Transfer & Synthetic Observations with Magritte
in Journal of Open Source Software
Chaikin E
(2023)
A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
in Monthly Notices of the Royal Astronomical Society
Chaikin E
(2022)
The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
in Monthly Notices of the Royal Astronomical Society
Chakraborty B
(2021)
Improved V c s determination using precise lattice QCD form factors for D ? K l ?
in Physical Review D
Chan K
(2022)
Single fluid versus multifluid: comparison between single-fluid and multifluid dust models for disc-planet interactions
in Monthly Notices of the Royal Astronomical Society
Chan T
(2021)
Smoothed particle radiation hydrodynamics: two-moment method with local Eddington tensor closure
in Monthly Notices of the Royal Astronomical Society
Chang C
(2023)
Publisher Erratum to: Global fits of simplified models for dark matter with GAMBIT II. Vector dark matter with an s-channel vector mediator
in The European Physical Journal C
Chang C
(2023)
Global fits of simplified models for dark matter with GAMBIT I. Scalar and fermionic models with s-channel vector mediators
in The European Physical Journal C
Chang C
(2023)
Global fits of simplified models for dark matter with GAMBIT II. Vector dark matter with an s-channel vector mediator
in The European Physical Journal C
Changeat Q
(2021)
An Exploration of Model Degeneracies with a Unified Phase Curve Retrieval Analysis: The Light and Dark Sides of WASP-43 b
in The Astrophysical Journal
Changeat Q
(2020)
KELT-11 b: Abundances of Water and Constraints on Carbon-bearing Molecules from the Hubble Transmission Spectrum
in The Astronomical Journal
Changeat Q
(2020)
TauREx3 PhaseCurve: A 1.5D Model for Phase-curve Description
in The Astrophysical Journal
Changeat Q
(2024)
Is the Atmosphere of the Ultra-hot Jupiter WASP-121 b Variable?
in The Astrophysical Journal Supplement Series
Changeat Q
(2023)
ESA-Ariel Data Challenge NeurIPS 2022: introduction to exo-atmospheric studies and presentation of the Atmospheric Big Challenge (ABC) Database
in RAS Techniques and Instruments
Changeat Q
(2022)
Disentangling atmospheric compositions of K2-18 b with next generation facilities.
in Experimental astronomy
Changeat Q
(2022)
On Spectroscopic Phase-curve Retrievals: H 2 Dissociation and Thermal Inversion in the Atmosphere of the Ultrahot Jupiter WASP-103 b
in The Astronomical Journal
Changeat Q
(2022)
Five Key Exoplanet Questions Answered via the Analysis of 25 Hot-Jupiter Atmospheres in Eclipse
in The Astrophysical Journal Supplement Series
Changeat Q
(2021)
The Hubble WFC3 Emission Spectrum of the Extremely Hot Jupiter KELT-9b
in The Astrophysical Journal Letters
Chawdhry H
(2021)
NNLO QCD corrections to diphoton production with an additional jet at the LHC
in Journal of High Energy Physics
Chawdhry H
(2021)
Two-loop leading-colour QCD helicity amplitudes for two-photon plus jet production at the LHC
in Journal of High Energy Physics
Chawdhry H
(2021)
Two-loop leading-color helicity amplitudes for three-photon production at the LHC
in Journal of High Energy Physics
Chen C
(2023)
Can a binary star host three giant circumbinary planets?
in Monthly Notices of the Royal Astronomical Society
Cheng A
(2023)
Momentum transfer from the DART mission kinetic impact on asteroid Dimorphos
in Nature
Cheung G
(2021)
DK I = 0, $$ D\overline{K} $$ I = 0, 1 scattering and the $$ {D}_{s0}^{\ast } $$(2317) from lattice QCD
in Journal of High Energy Physics
Christiansen J
(2020)
Jet feedback and the photon underproduction crisis in simba
in Monthly Notices of the Royal Astronomical Society
Christie D
(2021)
The impact of mixing treatments on cloud modelling in 3D simulations of hot Jupiters
in Monthly Notices of the Royal Astronomical Society
Christie D
(2022)
The impact of phase equilibrium cloud models on GCM simulations of GJ 1214b
in Monthly Notices of the Royal Astronomical Society
Christie D
(2022)
CAMEMBERT: A Mini-Neptunes General Circulation Model Intercomparison, Protocol Version 1.0.A CUISINES Model Intercomparison Project
in The Planetary Science Journal
Chubb K
(2021)
The ExoMolOP database: Cross sections and k -tables for molecules of interest in high-temperature exoplanet atmospheres
in Astronomy & Astrophysics
Clark V
(2020)
The high-temperature rotation-vibration spectrum and rotational clustering of silylene (SiH2)
in Journal of Quantitative Spectroscopy and Radiative Transfer
Clark VHJ
(2021)
Modelling the non-local thermodynamic equilibrium spectra of silylene (SiH2).
in Physical chemistry chemical physics : PCCP
Clarke C
(2020)
Forbidden line diagnostics of photoevaporative disc winds
in Monthly Notices of the Royal Astronomical Society
Clarke P
(2021)
Probing inflation with precision bispectra
in Journal of Cosmology and Astroparticle Physics
Clough K
(2021)
Continuity equations for general matter: applications in numerical relativity
in Classical and Quantum Gravity
Clough K
(2022)
Ghost Instabilities in Self-Interacting Vector Fields: The Problem with Proca Fields
in Physical Review Letters
Coates L
(2021)
Observing relativistic features in large-scale structure surveys - II. Doppler magnification in an ensemble of relativistic simulations
in Monthly Notices of the Royal Astronomical Society
Coleman G
(2022)
Dusty circumbinary discs: inner cavity structures and stopping locations of migrating planets
in Monthly Notices of the Royal Astronomical Society
Collins C
(2023)
Helium as a signature of the double detonation in Type Ia supernovae
in Monthly Notices of the Royal Astronomical Society
Collins C
(2022)
Double detonations: variations in Type Ia supernovae due to different core and He shell masses - II. Synthetic observables
in Monthly Notices of the Royal Astronomical Society
Collins C
(2023)
3D radiative transfer kilonova modelling for binary neutron star merger simulations
in Monthly Notices of the Royal Astronomical Society
Collins GS
(2020)
A steeply-inclined trajectory for the Chicxulub impact.
in Nature communications
Colquhoun B
(2023)
Precise determination of decay rates for ? c ? ? ? , J / ? ? ? ? c , and J / ? ? ? c e + e - from lattice QCD
in Physical Review D
Colò G
(2020)
Isoscalar monopole and quadrupole modes in Mo isotopes: Microscopic analysis
in Physics Letters B
Conaboy L
(2023)
Relative baryon-dark matter velocities in cosmological zoom simulations
in Monthly Notices of the Royal Astronomical Society
Constantino T
(2021)
Suppression of lithium depletion in young low-mass stars from fast rotation
in Astronomy & Astrophysics