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
Aumer M
(2017)
Migration and kinematics in growing disc galaxies with thin and thick discs
in Monthly Notices of the Royal Astronomical Society
Aurrekoetxea J
(2023)
Oscillon formation during inflationary preheating with general relativity
in Physical Review D
Baes M
(2019)
The cosmic spectral energy distribution in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Bahé Y
(2022)
The importance of black hole repositioning for galaxy formation simulations
in Monthly Notices of the Royal Astronomical Society
Bahé Y
(2021)
Strongly lensed cluster substructures are not in tension with ?CDM
in Monthly Notices of the Royal Astronomical Society
Bahé Y
(2019)
Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
in Monthly Notices of the Royal Astronomical Society
Bamber J
(2023)
Black hole merger simulations in wave dark matter environments
in Physical Review D
Bamber J
(2021)
Quasinormal modes of growing dirty black holes
in Physical Review D
Bamber J
(2021)
Growth of accretion driven scalar hair around Kerr black holes
in Physical Review D
Barber C
(2018)
Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
in Monthly Notices of the Royal Astronomical Society
Barmentloo S
(2023)
Determining satellite infall times using machine learning
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
Barnes D
(2021)
Characterizing hydrostatic mass bias with mock-X
in Monthly Notices of the Royal Astronomical Society
Barnes L
(2018)
Galaxy formation efficiency and the multiverse explanation of the cosmological constant with EAGLE simulations
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
Barrera-Hinojosa C
(2021)
Vector modes in ?CDM: the gravitomagnetic potential in dark matter haloes from relativistic N -body simulations
in Monthly Notices of the Royal Astronomical Society
Barrera-Hinojosa C
(2022)
Looking for a twist: probing the cosmological gravitomagnetic effect via weak lensing-kSZ cross-correlations
in Monthly Notices of the Royal Astronomical Society
Baugh C
(2022)
Modelling emission lines in star-forming galaxies
in Monthly Notices of the Royal Astronomical Society
Baugh C
(2019)
Linear bias forecasts for emission line cosmological surveys
in Monthly Notices of the Royal Astronomical Society
Baxter E
(2021)
The correlation of high-redshift galaxies with the thermal Sunyaev-Zel'dovich effect traces reionization
in Monthly Notices of the Royal Astronomical Society
Beane S
(2021)
Charged multihadron systems in lattice QCD + QED
in Physical Review D
Becker G
(2021)
The mean free path of ionizing photons at 5 < z < 6: evidence for rapid evolution near reionization
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
Belokurov V
(2023)
Energy wrinkles and phase-space folds of the last major merger
in Monthly Notices of the Royal Astronomical Society
Bemporad A
(2018)
Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test
in Astronomy & Astrophysics
| 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 |