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
Mayes R
(2024)
The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Witten C
(2024)
Deciphering Lyman-a emission deep into the epoch of reionization
in Nature Astronomy
Ereza J
(2024)
The Uchuu - glam BOSS and eBOSS LRG lightcones: exploring clustering and covariance errors
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2024)
An emulator-based halo model in modified gravity - I. The halo concentration-mass relation and density profile
in Monthly Notices of the Royal Astronomical Society
Dai Z
(2024)
Physics-informed neural networks in the recreation of hydrodynamic simulations from dark matter
in Monthly Notices of the Royal Astronomical Society
Bennett E
(2024)
Singlets in gauge theories with fundamental matter
in Physical Review D
Ploeckinger S
(2024)
Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multiphase interstellar medium
in Monthly Notices of the Royal Astronomical Society
Ferlito F
(2024)
Ray-tracing versus Born approximation in full-sky weak lensing simulations of the MillenniumTNG project
in Monthly Notices of the Royal Astronomical Society
Pakmor R
(2024)
Magnetic field amplification in cosmological zoom simulations from dwarf galaxies to galaxy groups
in Monthly Notices of the Royal Astronomical Society
Rowan C
(2024)
Black hole binaries in AGN accretion discs - II. Gas effects on black hole satellite scatterings
in Monthly Notices of the Royal Astronomical Society
Maunder T
(2024)
Synthetic light curves and spectra from a self-consistent 2D simulation of an ultra-strippped supernova
in Monthly Notices of the Royal Astronomical Society
Pizzati E
(2024)
Revisiting the extreme clustering of z ˜ 4 quasars with large volume cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Zhu Y
(2024)
Damping wing-like features in the stacked Ly a forest: Potential neutral hydrogen islands at z < 6
in Monthly Notices of the Royal Astronomical Society: Letters
Dong-Páez C
(2024)
The Uchuu-SDSS galaxy light-cones: a clustering, redshift space distortion and baryonic acoustic oscillation study
in Monthly Notices of the Royal Astronomical Society
Vijayan A
(2024)
First Light And Reionisation Epoch Simulations (FLARES) - XII: The consequences of star-dust geometry on galaxies in the EoR
in Monthly Notices of the Royal Astronomical Society
Brough S
(2024)
Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions
in Monthly Notices of the Royal Astronomical Society
Halim S
(2024)
Assessing the survival of carbonaceous chondrites impacting the lunar surface as a potential resource
in Planetary and Space Science
Koudmani S
(2024)
A unified accretion disc model for supermassive black holes in galaxy formation simulations: method and implementation
in Monthly Notices of the Royal Astronomical Society
Durán-Camacho E
(2024)
Self-consistent modelling of the Milky Way structure using live potentials
Somogyi W
(2024)
An ab initio spectroscopic model of the molecular oxygen atmospheric and infrared bands.
in Physical chemistry chemical physics : PCCP
Štofanová L
(2024)
Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
in Monthly Notices of the Royal Astronomical Society
Yang T
(2024)
Feedback-driven anisotropy in the circumgalactic medium for quenching galaxies in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Dhandha J
(2024)
Decaying turbulence in molecular clouds: how does it affect filament networks and star formation?
in Monthly Notices of the Royal Astronomical Society
Glasscock K
(2024)
Statistical estimation of full-sky radio maps from 21 cm array visibility data using Gaussian constrained realizations
in RAS Techniques and Instruments
Mayes R
(2024)
The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Broxterman J
(2024)
The FLAMINGO project: baryonic impact on weak gravitational lensing convergence peak counts
in Monthly Notices of the Royal Astronomical Society
Theuns T
(2024)
A halo model for cosmological Lyman-limit systems
in Monthly Notices of the Royal Astronomical Society
Wilkins S
(2024)
First Light and Reionization Epoch Simulations ( flares ) - XIV. The Balmer/4000 Å breaks of distant galaxies
in Monthly Notices of the Royal Astronomical Society
Rogers J
(2024)
Under the light of a new star: evolution of planetary atmospheres through protoplanetary disc dispersal and boil-off
in Monthly Notices of the Royal Astronomical Society
Turpin G
(2024)
Orbital evolution of close binary systems: comparing viscous and wind-driven circumbinary disc models
in Monthly Notices of the Royal Astronomical Society
Xiao M
(2024)
Accelerated formation of ultra-massive galaxies in the first billion years.
in Nature
Thompson O
(2024)
Predictions for CO emission and the CO-to-H2 conversion factor in galaxy simulations with non-equilibrium chemistry
in Monthly Notices of the Royal Astronomical Society
Iršic V
(2024)
Unveiling dark matter free streaming at the smallest scales with the high redshift Lyman-alpha forest
in Physical Review D
Matteini L
(2024)
Alfvénic fluctuations in the expanding solar wind: Formation and radial evolution of spherical polarization
in Physics of Plasmas
Nobels F
(2024)
Tests of subgrid models for star formation using simulations of isolated disc galaxies
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
Mills B
(2024)
Spectral Calculations of 3D Radiation Magnetohydrodynamic Simulations of Super-Eddington Accretion onto a Stellar-mass Black Hole
in The Astrophysical Journal
Prole L
(2024)
Heavy black hole seed formation in high- z atomic cooling halos
in Astronomy & Astrophysics
Braspenning J
(2024)
The FLAMINGO project: galaxy clusters in comparison to X-ray observations
in Monthly Notices of the Royal Astronomical Society
Dethero M
(2024)
The shape of convection in 2D and 3D global simulations of stellar interiors
in Astronomy & Astrophysics
Bartlett D
(2024)
Exhaustive Symbolic Regression
in IEEE Transactions on Evolutionary Computation
Banfi A
(2024)
A POWHEG generator for deep inelastic scattering
in Journal of High Energy Physics
Owens A
(2024)
ExoMol line lists - LI. Molecular line lists for lithium hydroxide (LiOH)
in Monthly Notices of the Royal Astronomical Society
Contreras S
(2024)
Validating the clustering predictions of empirical models with the FLAMINGO simulations
in Astronomy & Astrophysics
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
Zhang Z
(2024)
Disentangling the anisotropic radio sky: Fisher forecasts for 21 cm arrays
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
Dutta R
(2024)
Metal line emission around z < 1 galaxies
in Astronomy & Astrophysics
Jiang A
(2024)
Minkowski functionals of large-scale structure as a probe of modified gravity
in Physical Review D
Choustikov N
(2024)
The great escape: understanding the connection between Ly a emission and LyC escape in simulated JWST analogues
in Monthly Notices of the Royal Astronomical Society
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| Exploitation Route | See Dirac annual report https://dirac.ac.uk |
| Sectors | Digital/Communication/Information Technologies (including Software) Education |
| URL | https://dirac.ac.uk |