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
(2019)
Magnetogenesis at Cosmic Dawn: tracing the origins of cosmic magnetic fields
in Monthly Notices of the Royal Astronomical Society
Thomas N
(2019)
Black hole - Galaxy correlations in simba
in Monthly Notices of the Royal Astronomical Society
Teodoro L
(2019)
Planetary giant impacts: convergence of high-resolution simulations using efficient spherical initial conditions and swift
in Monthly Notices of the Royal Astronomical Society
Bourne M
(2019)
AGN jet feedback on a moving mesh: lobe energetics and X-ray properties in a realistic cluster environment
in Monthly Notices of the Royal Astronomical Society
Lander S
(2019)
Magnetic-field evolution in a plastically failing neutron-star crust
in Monthly Notices of the Royal Astronomical Society
Arnold C
(2019)
Simulating galaxy formation in f(R) modified gravity: matter, halo, and galaxy statistics
in Monthly Notices of the Royal Astronomical Society
Clough K
(2019)
Growth of massive scalar hair around a Schwarzschild black hole
in Physical Review D
Davé R
(2019)
simba: Cosmological simulations with black hole growth and feedback
in Monthly Notices of the Royal Astronomical Society
Henden N
(2019)
The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the fable simulations
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2019)
A general framework to test gravity using galaxy clusters II: A universal model for the halo concentration in f(R) gravity
in Monthly Notices of the Royal Astronomical Society
Smith M
(2019)
Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
in Monthly Notices of the Royal Astronomical Society
Wijers N
(2019)
The abundance and physical properties of O vii and O viii X-ray absorption systems in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Davies C
(2019)
The self-similarity of weak lensing peaks
in Monthly Notices of the Royal Astronomical Society
Sormani M
(2019)
The geometry of the gas surrounding the Central Molecular Zone: on the origin of localized molecular clouds with extreme velocity dispersions
in Monthly Notices of the Royal Astronomical Society
Li Q
(2019)
The dust-to-gas and dust-to-metal ratio in galaxies from z = 0 to 6
in Monthly Notices of the Royal Astronomical Society
Cristini A
(2019)
Dependence of convective boundary mixing on boundary properties and turbulence strength
in Monthly Notices of the Royal Astronomical Society
Fattahi A
(2019)
The origin of galactic metal-rich stellar halo components with highly eccentric orbits
in Monthly Notices of the Royal Astronomical Society
Ali A
(2019)
Massive star feedback in clusters: variation of the FUV interstellar radiation field in time and space
in Monthly Notices of the Royal Astronomical Society
Smith A
(2019)
Correcting for fibre assignment incompleteness in the DESI Bright Galaxy Survey
in Monthly Notices of the Royal Astronomical Society
Tröster T
(2019)
Painting with baryons: augmenting N-body simulations with gas using deep generative models
in Monthly Notices of the Royal Astronomical Society: Letters
Hernández-Aguayo C
(2019)
Large-scale redshift space distortions in modified gravity theories
in Monthly Notices of the Royal Astronomical Society
Puchwein E
(2019)
Consistent modelling of the meta-galactic UV background and the thermal/ionization history of the intergalactic medium
in Monthly Notices of the Royal Astronomical Society
Davies C
(2019)
Cosmological test of gravity using weak lensing voids
in Monthly Notices of the Royal Astronomical Society
Van Son L
(2019)
Galaxies with monstrous black holes in galaxy cluster environments
in Monthly Notices of the Royal Astronomical Society
Davis T
(2019)
Evolution of the cold gas properties of simulated post-starburst galaxies
in Monthly Notices of the Royal Astronomical Society
Correa C
(2019)
The origin of the red-sequence galaxy population in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Wang E
(2019)
The impact of black hole seeding in cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Baugh C
(2019)
Linear bias forecasts for emission line cosmological surveys
in Monthly Notices of the Royal Astronomical Society
Paillas E
(2019)
The Santiago-Harvard-Edinburgh-Durham void comparison II: unveiling the Vainshtein screening using weak lensing
in Monthly Notices of the Royal Astronomical Society
Müller B
(2019)
Three-dimensional simulations of neutrino-driven core-collapse supernovae from low-mass single and binary star progenitors
in Monthly Notices of the Royal Astronomical Society
Rodríguez Montero F
(2019)
Mergers, starbursts, and quenching in the simba simulation
in Monthly Notices of the Royal Astronomical Society
Lara-López M
(2019)
Oxygen yields as a constraint on feedback processes in galaxies
in Monthly Notices of the Royal Astronomical Society
Koudmani S
(2019)
Fast and energetic AGN-driven outflows in simulated dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Ganeshaiah Veena P
(2019)
The Cosmic Ballet II: spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Baes M
(2019)
The cosmic spectral energy distribution in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Shao S
(2019)
Evolution of galactic planes of satellites in the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Rose T
(2019)
Deep and narrow CO absorption revealing molecular clouds in the Hydra-A brightest cluster galaxy
in Monthly Notices of the Royal Astronomical Society
Kruijssen J
(2019)
The formation and assembly history of the Milky Way revealed by its globular cluster population
in Monthly Notices of the Royal Astronomical Society
Ludlow A
(2019)
Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
in Monthly Notices of the Royal Astronomical Society: Letters
Meru F
(2019)
Is the ring inside or outside the planet?: the effect of planet migration on dust rings
in Monthly Notices of the Royal Astronomical Society
Cowley W
(2019)
The evolution of the UV-to-mm extragalactic background light: evidence for a top-heavy initial mass function?
in Monthly Notices of the Royal Astronomical Society
Armitage T
(2019)
An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations
in Monthly Notices of the Royal Astronomical Society
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
Teyssier R
(2020)
The loss of the intracluster medium in globular clusters
in Monthly Notices of the Royal Astronomical Society
Li B
(2020)
Measuring the baryon acoustic oscillation peak position with different galaxy selections
in Monthly Notices of the Royal Astronomical Society
Simpson C
(2020)
The milky way total mass profile as inferred from Gaia DR2
in Monthly Notices of the Royal Astronomical Society
Wu X
(2020)
Photometric properties of reionization-epoch galaxies in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Cuesta-Lazaro C
(2020)
Towards a non-Gaussian model of redshift space distortions
in Monthly Notices of the Royal Astronomical Society
Benitez-Llambay A
(2020)
The detailed structure and the onset of galaxy formation in low-mass gaseous dark matter haloes
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 |