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
Ray G
(2022)
Determination of hybrid charmonium meson masses
Hatton D
(2021)
Determination of m ¯ b / m ¯ c and m ¯ b from n f = 4 lattice QCD + QED
in Physical Review D
Barmentloo S
(2023)
Determining satellite infall times using machine learning
in Monthly Notices of the Royal Astronomical Society
Barmentloo S
(2022)
Determining Satellite Infall Times Using Machine Learning
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
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
Yardley S
(2021)
Determining the source and eruption dynamics of a stealth CME using NLFFF modelling and MHD simulations
in Astronomy & Astrophysics
Gurung-López S
(2021)
Determining the systemic redshift of Lyman a emitters with neural networks and improving the measured large-scale clustering
in Monthly Notices of the Royal Astronomical Society
Gurung-López S
(2021)
Determining the systemic redshift of Lyman a emitters with neural networks and improving the measured large-scale clustering
in Monthly Notices of the Royal Astronomical Society
MacTaggart D
(2021)
Direct evidence that twisted flux tube emergence creates solar active regions.
in Nature communications
Zhang Z
(2024)
Disentangling the anisotropic radio sky: Fisher forecasts for 21 cm arrays
in Monthly Notices of the Royal Astronomical Society
Zhang Z
(2024)
Disentangling the anisotropic radio sky: Fisher forecasts for 21 cm arrays
in Monthly Notices of the Royal Astronomical Society
Raj A
(2021)
Disk Tearing: Implications for Black Hole Accretion and AGN Variability
in The Astrophysical Journal
Raj A
(2021)
Disk Tearing: Numerical Investigation of Warped Disk Instability
in The Astrophysical Journal
Bahé Y
(2019)
Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2023)
Distinct distributions of elliptical and disk galaxies across the Local Supercluster as a ?CDM prediction
in Nature Astronomy
Yeo J
(2024)
DK/Dp scattering and an exotic virtual bound state at the SU(3) flavour symmetric point from lattice QCD
in Journal of High Energy Physics
Gonzalez-Perez V
(2020)
Do model emission line galaxies live in filaments at z ~ 1?
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2020)
Do model emission line galaxies live in filaments at z~1?
Costa T
(2018)
Driving gas shells with radiation pressure on dust in radiation-hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Kirchschlager F
(2023)
Dust survival rates in clumps passing through the Cas A reverse shock - II. The impact of magnetic fields
in Monthly Notices of the Royal Astronomical Society
Sanati M
(2024)
Dwarf galaxies as a probe of a primordially magnetized Universe
in Astronomy & Astrophysics
Deason A
(2022)
Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
in Monthly Notices of the Royal Astronomical Society
Strigari L
(2018)
Dynamical Constraints on the Dark Matter Distribution of the Sculptor Dwarf Spheroidal from Stellar Proper Motions
in The Astrophysical Journal
Silva HO
(2021)
Dynamical Descalarization in Binary Black Hole Mergers.
in Physical review letters
Traykova D
(2021)
Dynamical friction from scalar dark matter in the relativistic regime
Traykova D
(2021)
Dynamical friction from scalar dark matter in the relativistic regime
in Physical Review D
Traykova D
(2021)
Dynamical friction from scalar dark matter in the relativistic regime
in Physical Review D
Bourne M
(2024)
Dynamics and spin alignment in massive, gravito-turbulent circumbinary discs around supermassive black hole binaries
in Monthly Notices of the Royal Astronomical Society
Andrassy R
(2022)
Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes
in Astronomy & Astrophysics
Altamura E
(2023)
EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
in Monthly Notices of the Royal Astronomical Society
Pontzen A
(2021)
EDGE: a new approach to suppressing numerical diffusion in adaptive mesh simulations of galaxy formation
in Monthly Notices of the Royal Astronomical Society
Goater A
(2024)
EDGE: The direct link between mass growth history and the extended stellar haloes of the faintest dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2023)
EDGE: the shape of dark matter haloes in the faintest galaxies
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2021)
EDGE: two routes to dark matter core formation in ultra-faint dwarfs
in Monthly Notices of the Royal Astronomical Society
Pagano P
(2020)
Effect of Coronal Loop Structure on Wave Heating by Phase Mixing
Pagano P
(2020)
Effect of coronal loop structure on wave heating through phase mixing
in Astronomy & Astrophysics
Aurrekoetxea JC
(2024)
Effect of Wave Dark Matter on Equal Mass Black Hole Mergers.
in Physical review letters
Zerbo M
(2024)
Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Camps P
(2021)
Effects of Spatial Discretization in Lya Line Radiation Transfer Simulations
in The Astrophysical Journal
Vidal J
(2020)
Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
in Monthly Notices of the Royal Astronomical Society
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
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
| 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 |