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
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
Tillman M
(2023)
Efficient Long-range Active Galactic Nuclei (AGNs) Feedback Affects the Low-redshift Lya Forest
in The Astrophysical Journal Letters
Chen C
(2023)
Can a binary star host three giant circumbinary planets?
in Monthly Notices of the Royal Astronomical Society
Rosca-Mead R
(2023)
Stochastic gravitational wave background from supernovae in massive scalar-tensor gravity
in Physical Review D
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
Shingles L
(2023)
Self-consistent 3D Radiative Transfer for Kilonovae: Directional Spectra from Merger Simulations
in The Astrophysical Journal Letters
Belokurov V
(2023)
Energy wrinkles and phase-space folds of the last major merger
in Monthly Notices of the Royal Astronomical Society
Ferlito F
(2023)
The MillenniumTNG Project: the impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
in Monthly Notices of the Royal Astronomical Society
Baraffe I
(2023)
A study of convective core overshooting as a function of stellar mass based on two-dimensional hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Ali A
(2023)
Star cluster formation and feedback in different environments of a Milky Way-like galaxy
in Monthly Notices of the Royal Astronomical Society
Ananyev V
(2023)
Collider constraints on electroweakinos in the presence of a light gravitino
in The European Physical Journal C
Betts J
(2023)
Machine learning and structure formation in modified gravity
in Monthly Notices of the Royal Astronomical Society
Beraldo E Silva L
(2023)
Orbital Support and Evolution of Flat Profiles of Bars (Shoulders)
in The Astrophysical Journal
Bose S
(2023)
The MillenniumTNG Project: the large-scale clustering of galaxies
in Monthly Notices of the Royal Astronomical Society
Changeat Q
(2023)
ESA-Ariel Data Challenge NeurIPS 2022: introduction to exo-atmospheric studies and presentation of the Atmospheric Big Challenge (ABC) Database
in RAS Techniques and Instruments
Bartlett D
(2023)
Marginalised Normal Regression: Unbiased curve fitting in the presence of x-errors
in The Open Journal of Astrophysics
Schaller M
(2023)
On the anisotropic distribution of clusters in the local Universe
Kirchschlager F
(2023)
Dust survival rates in clumps passing through the Cas A reverse shock - II. The impact of magnetic fields
in Monthly Notices of the Royal Astronomical Society
Doneva D
(2023)
Testing the limits of scalar-Gauss-Bonnet gravity through nonlinear evolutions of spin-induced scalarization
in Physical Review D
Czakon M
(2023)
NNLO B-fragmentation fits and their application to $$ t\overline{t} $$ production and decay at the LHC
in Journal of High Energy Physics
Barmentloo S
(2023)
Determining satellite infall times using machine learning
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2023)
Distinct distributions of elliptical and disk galaxies across the Local Supercluster as a ?CDM prediction
in Nature Astronomy
Theuns T
(2023)
A halo model for cosmological Lyman-limit systems
Forzano N
(2023)
Lattice studies of Sp(2N) gauge theories using GRID
Seeyave L
(2023)
First light and reionization epoch simulations (FLARES) X iii : the lyman-continuum emission of high-redshift galaxies
in Monthly Notices of the Royal Astronomical Society
Roper W
(2023)
First light and reionization epoch simulations (FLARES) IX: the physical mechanisms driving compact galaxy formation and evolution
in Monthly Notices of the Royal Astronomical Society
Daly RT
(2023)
Successful kinetic impact into an asteroid for planetary defence.
in Nature
| 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 |