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
Shao S
(2021)
The survival of globular clusters in a cuspy Fornax
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
Hafen Z
(2024)
The Halo21 absorption modelling challenge: lessons from 'observing' synthetic circumgalactic absorption spectra
in Monthly Notices of the Royal Astronomical Society
Hill A
(2021)
The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Hernández-Aguayo C
(2021)
Galaxy formation in the brane world I: overview and first results
in Monthly Notices of the Royal Astronomical Society
Wilkins S
(2023)
First light and reionization epoch simulations (FLARES) V: the redshift frontier
in Monthly Notices of the Royal Astronomical Society
Katz H
(2018)
A Census of the LyC photons that form the UV background during reionization
in Monthly Notices of the Royal Astronomical Society
Barnes D
(2017)
The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
in Monthly Notices of the Royal Astronomical Society
Armijo J
(2024)
A new test of gravity - I. Introduction to the method
in Monthly Notices of the Royal Astronomical Society
Beckett A
(2021)
The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet
in Monthly Notices of the Royal Astronomical Society
Elbers W
(2021)
An optimal non-linear method for simulating relic neutrinos
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
Wilkins S
(2022)
First Light and Reionisation Epoch Simulations (FLARES) - VI. The colour evolution of galaxies z = 5-15
in Monthly Notices of the Royal Astronomical Society
Tress R
(2020)
Simulations of the star-forming molecular gas in an interacting M51-like galaxy
in Monthly Notices of the Royal Astronomical Society
Yang T
(2022)
Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the simba and TNG simulations
in Monthly Notices of the Royal Astronomical Society
Hou J
(2021)
How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
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
Theuns T
(2021)
Connecting cosmological accretion to strong Ly a absorbers
in Monthly Notices of the Royal Astronomical Society
Downing E
(2023)
The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions
in Monthly Notices of the Royal Astronomical Society
Wijers N
(2020)
The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray and UV line absorption
in Monthly Notices of the Royal Astronomical Society
Gu Q
(2022)
The spatial distribution of satellites in galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Genina A
(2018)
The core-cusp problem: a matter of perspective
in Monthly Notices of the Royal Astronomical Society
Oppenheimer B
(2020)
Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
in Monthly Notices of the Royal Astronomical Society
Towler I
(2023)
Gas clumping and its effect on hydrostatic bias in the MACSIS simulations
in Monthly Notices of the Royal Astronomical Society
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
Kafle P
(2018)
Galaxy tagging: photometric redshift refinement and group richness enhancement
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
Bennett J
(2020)
Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
in Monthly Notices of the Royal Astronomical Society
Wareing C
(2018)
A new mechanical stellar wind feedback model for the Rosette Nebula
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
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
Campos Estrada B
(2024)
On the likely magnesium-iron silicate dusty tails of catastrophically evaporating rocky planets
in Monthly Notices of the Royal Astronomical Society
Sana T
(2023)
Plasma sheath around sunlit moon: monotonic and non-monotonic structures
in Monthly Notices of the Royal Astronomical Society
Müller B
(2017)
Supernova simulations from a 3D progenitor model - Impact of perturbations and evolution of explosion properties
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
Correa C
(2018)
The formation of hot gaseous haloes around galaxies
in Monthly Notices of the Royal Astronomical Society
Zarrouk P
(2021)
Baryon acoustic oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
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
Lovell C
(2021)
First Light And Reionization Epoch Simulations (FLARES) - I. Environmental dependence of high-redshift galaxy evolution
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2018)
The E-MOSAICS project: simulating the formation and co-evolution of galaxies and their star cluster populations
in Monthly Notices of the Royal Astronomical Society
Pereira-Wilson M
(2023)
The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Herrington N
(2023)
The role of previous generations of stars in triggering star formation and driving gas dynamics
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2022)
Baryonic mass budgets for haloes in the eagle simulation, including ejected and prevented gas
in Monthly Notices of the Royal Astronomical Society
Brown S
(2022)
Towards a universal model for the density profiles of dark matter haloes
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
Porth L
(2021)
Fast estimation of aperture-mass statistics - II. Detectability of higher order statistics in current and future surveys
in Monthly Notices of the Royal Astronomical Society
Le Saux A
(2023)
Two-dimensional simulations of internal gravity waves in a 5 M? zero-age-main-sequence model
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
Smith G
(2020)
The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451-03
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 |