DIRAC-3 Operations 2019-22 - UCL
Lead Research Organisation:
University College London
Department Name: 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:
1) 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.
2) 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.
3) Development and delivery of co-design projects with industry partners to improve future generations of hardware and software.
4) 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.
5) 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.
6) 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:
1) 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.
2) 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.
3) Development and delivery of co-design projects with industry partners to improve future generations of hardware and software.
4) 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.
5) 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.
6) 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
Aviles A
(2020)
Marked correlation functions in perturbation theory
in Journal of Cosmology and Astroparticle Physics
Badger S
(2023)
Isolated photon production in association with a jet pair through next-to-next-to-leading order in QCD
in Journal of High Energy Physics
Baek G
(2020)
Radiative Transfer Modeling of EC 53: An Episodically Accreting Class I Young Stellar Object
in The Astrophysical Journal
Bahé Y
(2022)
The importance of black hole repositioning for galaxy formation simulations
in Monthly Notices of the Royal Astronomical Society
Bahé Y
(2021)
Strongly lensed cluster substructures are not in tension with ?CDM
in Monthly Notices of the Royal Astronomical Society
Ballabio G
(2023)
[O i ] 6300 Å emission as a probe of external photoevaporation of protoplanetary discs
in Monthly Notices of the Royal Astronomical Society
Ballabio G
(2021)
HD 143006: circumbinary planet or misaligned disc?
in Monthly Notices of the Royal Astronomical Society
Bamber J
(2021)
Growth of accretion driven scalar hair around Kerr black holes
in Physical Review D
Bamber J
(2021)
Quasinormal modes of growing dirty black holes
in Physical Review D
Bamber J
(2023)
Black hole merger simulations in wave dark matter environments
in Physical Review D
Bantilan H
(2021)
Cauchy evolution of asymptotically global AdS spacetimes with no symmetries
in Physical Review D
Bantilan H
(2020)
Real-Time Dynamics of Plasma Balls from Holography
in Physical Review Letters
Baraffe I
(2022)
Local heating due to convective overshooting and the solar modelling problem
in Astronomy & Astrophysics
Baraffe I
(2023)
A study of convective core overshooting as a function of stellar mass based on two-dimensional hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Baraffe I
(2021)
Two-dimensional simulations of solar-like models with artificially enhanced luminosity I. Impact on convective penetration
in Astronomy & Astrophysics
Barausse E
(2020)
Prospects for fundamental physics with LISA
in General Relativity and Gravitation
Barber C
(2019)
Calibrated, cosmological hydrodynamical simulations with variable IMFs III: spatially resolved properties and evolution
in Monthly Notices of the Royal Astronomical Society
Barbieri C
(2019)
Lepton scattering from Ar 40 and Ti 48 in the quasielastic peak region
in Physical Review C
Barker A
(2019)
Angular momentum transport by the GSF instability: non-linear simulations at the equator
in Monthly Notices of the Royal Astronomical Society
Barnes D
(2021)
Characterizing hydrostatic mass bias with mock-X
in Monthly Notices of the Royal Astronomical Society
Barone A
(2023)
Approaches to inclusive semileptonic B(s)-meson decays from Lattice QCD
in Journal of High Energy Physics
Barrera M
(2023)
The MillenniumTNG Project: semi-analytic galaxy formation models on the past lightcone
in Monthly Notices of the Royal Astronomical Society
Barrera-Hinojosa C
(2020)
GRAMSES: a new route to general relativistic N -body simulations in cosmology. Part II. Initial conditions
in Journal of Cosmology and Astroparticle Physics
Barrera-Hinojosa C
(2021)
Vector modes in ?CDM: the gravitomagnetic potential in dark matter haloes from relativistic N -body simulations
in Monthly Notices of the Royal Astronomical Society
Barrera-Hinojosa C
(2022)
Looking for a twist: probing the cosmological gravitomagnetic effect via weak lensing-kSZ cross-correlations
in Monthly Notices of the Royal Astronomical Society
Barrera-Hinojosa C
(2020)
GRAMSES: a new route to general relativistic N -body simulations in cosmology. Part I. Methodology and code description
in Journal of Cosmology and Astroparticle Physics
Bartlett D
(2021)
Spatially offset black holes in the Horizon-AGN simulation and comparison to observations
in Monthly Notices of the Royal Astronomical Society
Bartlett D
(2021)
Constraints on Galileons from the positions of supermassive black holes
in Physical Review D
Bartlett D
(2021)
Calibrating galaxy formation effects in galactic tests of fundamental physics
in Physical Review D
Bastian N
(2020)
The globular cluster system mass-halo mass relation in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Bate M
(2023)
The statistical properties of stars at redshift, z = 5, compared with the present epoch
in Monthly Notices of the Royal Astronomical Society
Bate M
(2020)
Photoionizing feedback in spiral arm molecular clouds
in Monthly Notices of the Royal Astronomical Society
Batelaan M
(2023)
Feynman-Hellmann approach to transition matrix elements and quasidegenerate energy states
in Physical Review D
Batelaan M
(2023)
Moments and power corrections of longitudinal and transverse proton structure functions from lattice QCD
in Physical Review D
Battino U
(2019)
NuGrid stellar data set - III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z= 0.01, Z = 0.02, and Z = 0.03
in Monthly Notices of the Royal Astronomical Society
Baugh C
(2022)
Modelling emission lines in star-forming galaxies
in Monthly Notices of the Royal Astronomical Society
Baugh C
(2020)
Sensitivity analysis of a galaxy formation model
in Monthly Notices of the Royal Astronomical Society
Baugh C
(2019)
Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter haloes
in Monthly Notices of the Royal Astronomical Society
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
Bazavov A
(2023)
Light-quark connected intermediate-window contributions to the muon g - 2 hadronic vacuum polarization from lattice QCD
in Physical Review D
Beane S
(2021)
Charged multihadron systems in lattice QCD + QED
in Physical Review D
Becker C
(2020)
Proca-stinated cosmology. Part I. A N -body code for the vector Galileon
in Journal of Cosmology and Astroparticle Physics
Becker G
(2021)
The mean free path of ionizing photons at 5 < z < 6: evidence for rapid evolution near reionization
in Monthly Notices of the Royal Astronomical Society
Beckett A
(2021)
The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet
in Monthly Notices of the Royal Astronomical Society
Beg R
(2022)
Evolution, Structure, and Topology of Self-generated Turbulent Reconnection Layers
in The Astrophysical Journal
Belokurov V
(2023)
Energy wrinkles and phase-space folds of the last major merger
in Monthly Notices of the Royal Astronomical Society
Bena I
(2019)
Holographic dual of hot Polchinski-Strassler quark-gluon plasma
in Journal of High Energy Physics
Bending T
(2022)
Supernovae and photoionizing feedback in spiral arm molecular clouds
in Monthly Notices of the Royal Astronomical Society
Benitez-Llambay A
(2021)
The Tail of Late-forming Dwarf Galaxies in ?CDM
in The Astrophysical Journal Letters
Benitez-Llambay A
(2020)
The detailed structure and the onset of galaxy formation in low-mass gaseous dark matter haloes
in Monthly Notices of the Royal Astronomical Society