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
Katz H
(2023)
The challenges of identifying Population III stars in the early Universe
in Monthly Notices of the Royal Astronomical Society
Whitworth D
(2023)
Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Thomas P
(2023)
First light and reionization epoch simulations ( Flares ) X: environmental galaxy bias and survey variance at high redshift
in Monthly Notices of the Royal Astronomical Society
Ibrahim D
(2023)
The impact of supernova feedback on the mass-metallicity relations
Trotta D
(2023)
Three-dimensional modelling of the shock-turbulence interaction
in Monthly Notices of the Royal Astronomical Society
Pakmor R
(2023)
The MillenniumTNG Project: the hydrodynamical full physics simulation and a first look at its galaxy clusters
in Monthly Notices of the Royal Astronomical Society
De Jong E
(2023)
Spinning primordial black holes formed during a matter-dominated era
in Journal of Cosmology and Astroparticle Physics
Smith R
(2023)
On the distribution of the cold neutral medium in galaxy discs
in Monthly Notices of the Royal Astronomical Society
Teodoro L
(2023)
A recent impact origin of Saturn's rings and mid-sized moons
Yankelevich V
(2023)
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
in Monthly Notices of the Royal Astronomical Society
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
Hadzhiyska B
(2023)
The MillenniumTNG Project: an improved two-halo model for the galaxy-halo connection of red and blue galaxies
in Monthly Notices of the Royal Astronomical Society
De Jong E
(2023)
Spinning primordial black holes formed during a matter-dominated era
Huško F
(2023)
The buildup of galaxies and their spheroids: The contributions of mergers, disc instabilities, and star formation
in Monthly Notices of the Royal Astronomical Society
Heyl J
(2023)
Data quality and autism: Issues and potential impacts
in International Journal of Medical Informatics
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
Huško F
(2023)
The complex interplay of AGN jet-inflated bubbles and the intracluster medium
in Monthly Notices of the Royal Astronomical Society
Trotta D
(2023)
Irregular Proton Injection to High Energies at Interplanetary Shocks
in The Astrophysical Journal Letters
Chung-Jukko L
(2023)
Electromagnetic instability of compact axion stars
in Physical Review D
Debattista V
(2023)
The Imprint of Clump Formation at High Redshift. II. The Chemistry of the Bulge
in The Astrophysical Journal
Katz H
(2023)
The SPHINX Public Data Release: Forward Modelling High-Redshift JWST Observations with Cosmological Radiation Hydrodynamics Simulations
in The Open Journal of Astrophysics
Beraldo E Silva L
(2023)
Orbital Support and Evolution of Flat Profiles of Bars (Shoulders)
in The Astrophysical Journal
Vanon R
(2023)
Three-dimensional Simulations of Massive Stars. II. Age Dependence
in The Astrophysical Journal
Chan T
(2023)
Simulations of the reionization of the clumpy intergalactic medium with a novel particle-based two-moment radiative transfer scheme
in Proceedings of the International Astronomical Union
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 |