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
Gray A
(2021)
Uncertainty Propagation in SINBAD Fusion Benchmarks with Total Monte Carlo and Imprecise Probabilities
in Fusion Science and Technology
Granelli A
(2023)
ULYSSES, Universal LeptogeneSiS Equation Solver: version 2
Granelli A
(2023)
ULYSSES, universal LeptogeneSiS equation solver: Version 2
in Computer Physics Communications
Ratnasingam R
(2020)
Two-dimensional simulations of internal gravity waves in the radiation zones of intermediate-mass stars
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
Katz H
(2023)
Two modes of LyC escape from bursty star formation: implications for [C ii ] deficits and the sources of reionization
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
Vidal J
(2020)
Turbulent Viscosity Acting on the Equilibrium Tidal Flow in Convective Stars
in The Astrophysical Journal Letters
Guervilly C
(2019)
Turbulent convective length scale in planetary cores.
in Nature
Vizgan D
(2022)
Tracing Molecular Gas Mass in z ? 6 Galaxies with [C ii]
in The Astrophysical Journal
Ruan C
(2022)
Towards an accurate model of small-scale redshift-space distortions in modified gravity
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
Cuesta-Lazaro C
(2020)
Towards a non-Gaussian model of redshift space distortions
in Monthly Notices of the Royal Astronomical Society
Cuesta-Lazaro C
(2020)
Towards a non-Gaussian model of redshift space distortions
Parrott W
(2021)
Toward accurate form factors for B -to-light meson decay from lattice QCD
in Physical Review D
Pallero D
(2022)
Too dense to go through: the role of low-mass clusters in the pre-processing of satellite galaxies
in Monthly Notices of the Royal Astronomical Society
Yip K
(2024)
To Sample or Not to Sample: Retrieving Exoplanetary Spectra with Variational Inference and Normalizing Flows
in The Astrophysical Journal
Astoul A
(2023)
Tidally Excited Inertial Waves in Stars and Planets: Exploring the Frequency-dependent and Averaged Dissipation with Nonlinear Simulations
in The Astrophysical Journal Letters
Wang M
(2017)
Tidal features of classical Milky Way satellites in a ? cold dark matter universe
in Monthly Notices of the Royal Astronomical Society
Ploeckinger S
(2018)
Tidal dwarf galaxies in cosmological simulations
in Monthly Notices of the Royal Astronomical Society
De Vries N
(2023)
Tidal dissipation due to the elliptical instability and turbulent viscosity in convection zones in rotating giant planets and stars
in Monthly Notices of the Royal Astronomical Society
Cufari M
(2023)
Tidal capture of stars by supermassive black holes: implications for periodic nuclear transients and quasi-periodic eruptions
in Monthly Notices of the Royal Astronomical Society: Letters
Müller B
(2019)
Three-dimensional simulations of neutrino-driven core-collapse supernovae from low-mass single and binary star progenitors
in Monthly Notices of the Royal Astronomical Society
Vanon R
(2023)
Three-dimensional Simulations of Massive Stars. II. Age Dependence
in The Astrophysical Journal
Trotta D
(2023)
Three-dimensional modelling of the shock-turbulence interaction
in Monthly Notices of the Royal Astronomical Society
Igoshev A
(2023)
Three-dimensional magnetothermal evolution of off-centred dipole magnetic field configurations in neutron stars
in Monthly Notices of the Royal Astronomical Society
Agudelo Rueda J
(2021)
Three-dimensional magnetic reconnection in particle-in-cell simulations of anisotropic plasma turbulence
in Journal of Plasma Physics
Owens A
(2021)
Theoretical rovibronic spectroscopy of the calcium monohydroxide radical (CaOH).
in The Journal of chemical physics
Ashworth G
(2018)
Theoretical predictions for IMF diagnostics in UV spectroscopy of star clusters
in Monthly Notices of the Royal Astronomical Society
Wijers N
(2022)
The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray-line emission
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
Montargès M
(2023)
The VLT/SPHERE view of the ATOMIUM cool evolved star sample I. Overview: Sample characterization through polarization analysis
in Astronomy & Astrophysics
Read P
(2020)
The turbulent dynamics of Jupiter's and Saturn's weather layers: order out of chaos?
in Geoscience Letters
Santos-Santos I
(2022)
The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
Santos-Santos I
(2023)
The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
in Monthly Notices of the Royal Astronomical Society
Newton O
(2018)
The total satellite population of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2023)
The timeless timing argument and the total mass of the Local Group
in Monthly Notices of the Royal Astronomical Society: Letters
Sawala T
(2023)
The Timeless Timing Argument and the Mass of the Local Group
| 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 |