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
Tsang Y
(2024)
Scaling of the geomagnetic secular variation timescale
in Geophysical Journal International
Aurrekoetxea JC
(2024)
Effect of Wave Dark Matter on Equal Mass Black Hole Mergers.
in Physical review letters
Bennett J
(2024)
The growth of the gargantuan black holes powering high-redshift quasars and their impact on the formation of early galaxies and protoclusters
in Monthly Notices of the Royal Astronomical Society
Feron J
(2024)
The Lyman-limit photon mean free path at the end of late reionization in the Sherwood-Relics simulations
in Monthly Notices of the Royal Astronomical Society
Coleman G
(2024)
Constraining the formation history of the TOI-1338/BEBOP-1 circumbinary planetary system
in Monthly Notices of the Royal Astronomical Society
Talbot R
(2024)
Simulations of spin-driven AGN jets in gas-rich galaxy mergers
in Monthly Notices of the Royal Astronomical Society
Yurchenko S
(2024)
ExoMol line lists - LIV. Empirical line lists for AlH and AlD and experimental emission spectroscopy of AlD in A1? ( v = 0, 1, 2)
in Monthly Notices of the Royal Astronomical Society
Manzoni G
(2024)
The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation
in Monthly Notices of the Royal Astronomical Society
Keating L
(2024)
The origin of the characteristic shape and scatter of intergalactic damping wings during reionization
in Monthly Notices of the Royal Astronomical Society: Letters
Ibrahim D
(2024)
The impact of supernova feedback on the mass-metallicity relations
in Monthly Notices of the Royal Astronomical Society
Hamilton E
(2024)
Catalog of precessing black-hole-binary numerical-relativity simulations
in Physical Review D
Ibrahim D
(2024)
The impact of supernova feedback on the mass-metallicity relations
in Monthly Notices of the Royal Astronomical Society
Fenton A
(2024)
The 3D structure of disc-instability protoplanets
in Astronomy & Astrophysics
Hafen Z
(2024)
The Halo21 absorption modelling challenge: lessons from 'observing' synthetic circumgalactic absorption spectra
in Monthly Notices of the Royal Astronomical Society
Prole L
(2024)
Heavy black hole seed formation in high- z atomic cooling halos
in Astronomy & Astrophysics
Armijo J
(2024)
A new test of gravity - I. Introduction to the method
in Monthly Notices of the Royal Astronomical Society
Householder A
(2024)
Investigating the Atmospheric Mass Loss of the Kepler-105 Planets Straddling the Radius Gap
in The Astronomical Journal
Schoettler C
(2024)
The effect of dynamical interactions in stellar birth environments on the orbits of young close-in planetary systems
in Monthly Notices of the Royal Astronomical Society
Changeat Q
(2024)
Is the Atmosphere of the Ultra-hot Jupiter WASP-121 b Variable?
in The Astrophysical Journal Supplement Series
CamposĀ Estrada B
(2024)
On the likely magnesium-iron silicate dusty tails of catastrophically evaporating rocky planets
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2024)
Anisotropies in the spatial distribution and kinematics of dwarf galaxies in the Local Group and beyond
in Monthly Notices of the Royal Astronomical Society
Georgy C
(2024)
3D simulations of a neon burning convective shell in a massive star
in Monthly Notices of the Royal Astronomical Society
Keating L
(2024)
JWST observations of galaxy-damping wings during reionization interpreted with cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Sirks E
(2024)
Hydrodynamical simulations of merging galaxy clusters: giant dark matter particle colliders, powered by gravity
in Monthly Notices of the Royal Astronomical Society
Gayer L
(2025)
Highly excited B, Bs and Bc meson spectroscopy from lattice QCD
in Journal of High Energy Physics
Fragkoudi F
(2025)
Bar formation and evolution in the cosmological context: inputs from the Auriga simulations
in Monthly Notices of the Royal Astronomical Society
Zhang M
(2025)
The Three Hundred project: The relationship between the shock and splashback radii of simulated galaxy clusters
in Publications of the Astronomical Society of Australia
Elley M
(2025)
Robustness of inflation to kinetic inhomogeneities
in Journal of Cosmology and Astroparticle Physics
| 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 |