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
Lovell C
(2022)
A machine learning approach to mapping baryons on to dark matter haloes using the eagle and C-EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
McAlpine S
(2020)
Galaxy mergers in eagle do not induce a significant amount of black hole growth yet do increase the rate of luminous AGN
in Monthly Notices of the Royal Astronomical Society
Yankelevich V
(2023)
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
in Monthly Notices of the Royal Astronomical Society
Gómez J
(2022)
Halo merger tree comparison: impact on galaxy formation models
in Monthly Notices of the Royal Astronomical Society
Bennett J
(2022)
A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
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
Garzilli A
(2021)
How to constrain warm dark matter with the Lyman-a forest
in Monthly Notices of the Royal Astronomical Society
D'Silva J
(2023)
Unveiling the main sequence of galaxies at z = 5 with the JWST : predictions from simulations
in Monthly Notices of the Royal Astronomical Society
Molaro M
(2022)
The effect of inhomogeneous reionization on the Lyman a forest power spectrum at redshift z > 4: implications for thermal parameter recovery
in Monthly Notices of the Royal Astronomical Society
Barrera M
(2023)
The MillenniumTNG Project: semi-analytic galaxy formation models on the past lightcone
in Monthly Notices of the Royal Astronomical Society
Herzog G
(2023)
The present-day gas content of simulated field dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Li N
(2021)
The impact of line-of-sight structures on measuring H 0 with strong lensing time delays
in Monthly Notices of the Royal Astronomical Society
Thomas P
(2023)
First light and reionization epoch simulations ( Flares ) X: environmental galaxy bias and survey variance at high redshift
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
Kugel R
(2023)
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning.
in Monthly notices of the Royal Astronomical Society
Santos-Santos I
(2021)
Magellanic satellites in ?CDM cosmological hydrodynamical simulations of the Local Group
in Monthly Notices of the Royal Astronomical Society
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
Glowacki M
(2021)
The redshift evolution of the baryonic Tully-Fisher relation in SIMBA
in Monthly Notices of the Royal Astronomical Society
Peñarrubia J
(2017)
What galaxy masses perturb the local cosmic expansion?
in Monthly Notices of the Royal Astronomical Society
Davé R
(2019)
simba: Cosmological simulations with black hole growth and feedback
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
Sorini D
(2020)
simba: the average properties of the circumgalactic medium of 2 = z = 3 quasars are determined primarily by stellar feedback
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
| 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 |