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
Gavardi A
(2023)
NNLO+PS W+W- production using jet veto resummation at NNLL'
in Journal of High Energy Physics
Genina A
(2018)
The core-cusp problem: a matter of perspective
in Monthly Notices of the Royal Astronomical Society
Ghosh S
(2024)
First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence
in Physical Review D
Givans J
(2022)
Non-linearities in the Lyman-a forest and in its cross-correlation with dark matter halos
in Journal of Cosmology and Astroparticle Physics
Glowacki M
(2020)
The baryonic Tully-Fisher relation in the simba simulation
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2021)
The redshift evolution of the baryonic Tully-Fisher relation in SIMBA
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2022)
ASymba: H i global profile asymmetries in the simba simulation
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2020)
The redshift evolution of the baryonic Tully-Fisher relation in Simba
Glowacki M
(2022)
ASymba: HI global profile asymmetries in the Simba simulation
Glowacki M
(2020)
The baryonic Tully-Fisher relation in the Simba simulation
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
Goldstraw E
(2018)
Comparison of methods for modelling coronal magnetic fields
in Astronomy & Astrophysics
Gonzalez-Perez V
(2020)
Do model emission line galaxies live in filaments at z~1?
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
(2017)
The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2020)
Multiwavelength consensus of large-scale linear bias
in Monthly Notices of the Royal Astronomical Society
Gonzalo T
(2024)
PEANUTS: a software for the automatic computation of solar neutrino flux and its propagation within Earth
in The European Physical Journal C
Gourgouliatos K
(2020)
Nonaxisymmetric Hall instability: A key to understanding magnetars
Grand R
(2018)
Aurigaia: mock Gaia DR2 stellar catalogues from the auriga cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Granelli A
(2023)
ULYSSES, Universal LeptogeneSiS Equation Solver: version 2
Granelli A
(2023)
ULYSSES, universal LeptogeneSiS equation solver: Version 2
in Computer Physics Communications
Gray A
(2021)
Uncertainty Propagation in SINBAD Fusion Benchmarks with Total Monte Carlo and Imprecise Probabilities
in Fusion Science and Technology
Gu Q
(2022)
The spatial distribution of satellites in galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Guervilly C
(2019)
Turbulent convective length scale in planetary cores.
in Nature
| 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 |