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
Hausammann L
(2022)
Continuous Simulation Data Stream: A dynamical timescale-dependent output scheme for simulations
in Astronomy and Computing
Trotta D
(2022)
Single-spacecraft techniques for shock parameters estimation: A systematic approach
in Frontiers in Astronomy and Space Sciences
Huško F
(2022)
Spin-driven jet feedback in idealized simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Hutt M
(2022)
The effect of local Universe constraints on halo abundance and clustering
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2022)
A general framework to test gravity using galaxy clusters - VI. Realistic galaxy formation simulations to study clusters in modified gravity
in Monthly Notices of the Royal Astronomical Society
Smith A
(2022)
A light-cone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
in Monthly Notices of the Royal Astronomical Society
Koudmani S
(2022)
Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
in Monthly Notices of the Royal Astronomical Society
Kannan R
(2022)
The MillenniumTNG Project: The galaxy population at $z\geq 8$
Fu B
(2022)
A predictive and testable unified theory of fermion masses, mixing and leptogenesis
in Journal of High Energy Physics
Clough K
(2022)
Ghost Instabilities in Self-Interacting Vector Fields: The Problem with Proca Fields.
in Physical review letters
Talbot R
(2022)
Blandford-Znajek jets in galaxy formation simulations: exploring the diversity of outflows produced by spin-driven AGN jets in Seyfert galaxies
in Monthly Notices of the Royal Astronomical Society
Evans T
(2022)
Observing EAGLE galaxies with JWST : predictions for Milky Way progenitors and their building blocks
in Monthly Notices of the Royal Astronomical Society
Prole L
(2022)
Fragmentation-induced starvation in Population III star formation: a resolution study
in Monthly Notices of the Royal Astronomical Society
Cataneo M
(2022)
The matter density PDF for modified gravity and dark energy with Large Deviations Theory
in Monthly Notices of the Royal Astronomical Society
Bernal N
(2022)
Rescuing high-scale leptogenesis using primordial black holes
in Physical Review D
Ramírez-Galeano L
(2022)
Why most molecular clouds are gravitationally dominated
Pryer D
(2022)
The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
in Journal of Cosmology and Astroparticle Physics
Vizgan D
(2022)
Tracing Molecular Gas Mass in z ? 6 Galaxies with [C ii]
in The Astrophysical Journal
Kelly A
(2022)
Apostle-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Belokurov V
(2022)
Energy wrinkles and phase-space folds of the last major merger
Harrison J
(2022)
B s ? D s * form factors for the full q 2 range from lattice QCD
in Physical Review D
Hernández-Aguayo C
(2022)
The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
Barmentloo S
(2022)
Determining Satellite Infall Times Using Machine Learning
Poci A
(2022)
Comparing lensing and stellar orbital models of a nearby massive strong-lens galaxy
in Monthly Notices of the Royal Astronomical Society
Chaikin E
(2022)
The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
in Monthly Notices of the Royal Astronomical Society
Yankelevich V
(2022)
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
Vernon I
(2022)
Bayesian Emulation and History Matching of JUNE
Bolton JS
(2022)
Comparison of Low-Redshift Lyman-a Forest Observations to Hydrodynamical Simulations with Dark Photon Dark Matter.
in Physical review letters
Kegerreis J
(2022)
Immediate origin of the Moon as a post-impact satellite
| 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 |