DiRAC-2.5 - the pathway to DiRAC Phase 3
Lead Research Organisation:
Durham University
Department Name: Physics
Abstract
We request funding to relocate the Blue Wonder HPC cluster and associated storage, currently at the Hartree Centre at Daresbury, to Durham, together with installation and hardware maintenance costs. This move would enable DiRAC to expand the current DiRAC-2 Data centric service, managed by Durham, by a factor of two in both computing power and data storage capacity. The new service would be called the DiRAC-2.5 Data Centric service.
Planned Impact
DiRAC would seek to continue to engage with industry at various levels, from the
provision of computing cycles for industrial applications to the
exchange of technical knowledge and shared training programmes. The
facility will serve to train young scientists in the most advanced
techniques for supercomputing. These have extensive applications beyond
academia, for example in industry and finance. Finally, output from Dirac-based
projects will be used for science outreach activities.
provision of computing cycles for industrial applications to the
exchange of technical knowledge and shared training programmes. The
facility will serve to train young scientists in the most advanced
techniques for supercomputing. These have extensive applications beyond
academia, for example in industry and finance. Finally, output from Dirac-based
projects will be used for science outreach activities.
Organisations
Publications
Rizzuti F
(2022)
Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
in Monthly Notices of the Royal Astronomical Society
Bantilan H
(2020)
Real-Time Dynamics of Plasma Balls from Holography.
in Physical review letters
Zheng Y
(2022)
Rapidly quenched galaxies in the Simba cosmological simulation and observations
in Monthly Notices of the Royal Astronomical Society
Kulier A
(2023)
Ram pressure stripping in the EAGLE simulation
Kulier A
(2023)
Ram Pressure Stripping in the EAGLE Simulation
in The Astrophysical Journal
De Ceuster F
(2023)
Radiative transfer as a Bayesian linear regression problem
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
Reina-Campos M
(2022)
Radial distributions of globular clusters trace their host dark matter halo: insights from the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Quera-Bofarull A
(2021)
Qwind3: UV line-driven accretion disc wind models for AGN feedback
Quera-Bofarull A
(2023)
qwind 3: UV line-driven accretion disc wind models for AGN feedback
in Monthly Notices of the Royal Astronomical Society
Costa T
(2018)
Quenching star formation with quasar outflows launched by trapped IR radiation
in Monthly Notices of the Royal Astronomical Society
Font A
(2022)
Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations
in Monthly Notices of the Royal Astronomical Society
Bamber J
(2021)
Quasinormal modes of growing dirty black holes
in Physical Review D
Arthuis P
(2023)
Quantum Monte Carlo calculations in configuration space with three-nucleon forces
in Physical Review C
Buividovich P.
(2023)
Quantum chaos in supersymmetric Yang-Mills-like model: equation of state, entanglement, and spectral form-factors
in Proceedings of Science
Buividovich P
(2022)
Quantum chaos in supersymmetric quantum mechanics: an exact diagonalization study
Elvis M
(2020)
Q wind code release: a non-hydrodynamical approach to modelling line-driven winds in active galactic nuclei
in Monthly Notices of the Royal Astronomical Society
Nightingale J
(2021)
PyAutoLens: Open-Source Strong Gravitational Lensing
Nightingale J
(2021)
PyAutoLens: Open-Source Strong Gravitational Lensing
in Journal of Open Source Software
Nightingale J
(2023)
PyAutoGalaxy: Open-Source Multiwavelength Galaxy Structure & Morphology
in Journal of Open Source Software
Nightingale J
(2023)
PyAutoGalaxy: Open-Source Multiwavelength Galaxy Structure & Morphology
Nightingale J
(2021)
PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
in Journal of Open Source Software
Aresté Saló L
(2023)
Puncture gauge formulation for Einstein-Gauss-Bonnet gravity and four-derivative scalar-tensor theories in d + 1 spacetime dimensions
in Physical Review D
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
Witstok J
(2021)
Prospects for observing the low-density cosmic web in Lyman- a emission
in Astronomy & Astrophysics
Štofanová L
(2024)
Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
in Monthly Notices of the Royal Astronomical Society
Koponen J
(2022)
Properties of low-lying charmonia and bottomonia from lattice QCD + QED
in Suplemento de la Revista Mexicana de Física
Mastromarino C
(2023)
Properties and observables of massive galaxies in self-interacting dark matter cosmologies
in Monthly Notices of the Royal Astronomical Society
Becker C
(2020)
Proca-stinated cosmology. Part I. A N -body code for the vector Galileon
in Journal of Cosmology and Astroparticle Physics
Gaikwad P
(2020)
Probing the thermal state of the intergalactic medium at z > 5 with the transmission spikes in high-resolution Ly a forest spectra
in Monthly Notices of the Royal Astronomical Society
De Pontieu B
(2022)
Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal Heating
in The Astrophysical Journal
Šoltinský T
(2023)
Probing quasar lifetimes with proximate 21-centimetre absorption in the diffuse intergalactic medium at redshifts z = 6
in Monthly Notices of the Royal Astronomical Society
Prole L
(2022)
Primordial magnetic fields in Population III star formation: a magnetized resolution study
in Monthly Notices of the Royal Astronomical Society
Brough S
(2024)
Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions
in Monthly Notices of the Royal Astronomical Society
Zarrouk P
(2022)
Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
in Monthly Notices of the Royal Astronomical Society
Mateu C
(2017)
Predictions for the detection of tidal streams with Gaia using great-circle methods
in Monthly Notices of the Royal Astronomical Society
| Description | See Dirac annual report https://dirac.ac.uk |
| Exploitation Route | See Dirac annual report https://dirac.ac.uk |
| Sectors | Digital/Communication/Information Technologies (including Software),Education |
| URL | https://dirac.ac.uk |