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
Ruan C
(2022)
Fast full N-body simulations of generic modified gravity: conformal coupling models
in Journal of Cosmology and Astroparticle Physics
Ruan C
(2022)
Towards an accurate model of small-scale redshift-space distortions in modified gravity
in Monthly Notices of the Royal Astronomical Society
Rowan C
(2024)
Black hole binaries in AGN accretion discs - II. Gas effects on black hole satellite scatterings
in Monthly Notices of the Royal Astronomical Society
Roth A
(2024)
Hot Jupiter diversity and the onset of TiO/VO revealed by a large grid of non-grey global circulation models
in Monthly Notices of the Royal Astronomical Society
Rose T
(2019)
Deep and narrow CO absorption revealing molecular clouds in the Hydra-A brightest cluster galaxy
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
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
Roper W
(2022)
First Light And Reionisation Epoch Simulations ( flares ) - IV. The size evolution of galaxies at z = 5
in Monthly Notices of the Royal Astronomical Society
Roper W
(2020)
MEGA: Merger graphs of structure formation
in Monthly Notices of the Royal Astronomical Society
Roper W
(2020)
MEGA: Merger graphs of structure formation
Rogers J
(2023)
Exoplanet atmosphere evolution: emulation with neural networks
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
RodrĂguez Montero F
(2019)
Mergers, starbursts, and quenching in the simba simulation
in Monthly Notices of the Royal Astronomical Society
RodrĂguez Montero F
(2024)
The impact of cosmic rays on the interstellar medium and galactic outflows of Milky Way analogues
in Monthly Notices of the Royal Astronomical Society
Robson D
(2020)
X-ray emission from hot gas in galaxy groups and clusters in simba
in Monthly Notices of the Royal Astronomical Society
Robson D
(2021)
Redshift Evolution of Galaxy Group X-ray Properties in Simba
Robson D
(2023)
Redshift evolution of galaxy group X-ray properties in the Simba simulations
in Monthly Notices of the Royal Astronomical Society
Robson D
(2023)
Redshift evolution of galaxy group X-ray properties in the Simba simulations
in Monthly Notices of the Royal Astronomical Society
Robertson A
(2021)
The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
in Monthly Notices of the Royal Astronomical Society
Robertson A
(2023)
Why weak lensing cluster shapes are insensitive to self-interacting dark matter
in Monthly Notices of the Royal Astronomical Society
Robertson A
(2021)
The galaxy-galaxy strong lensing cross-sections of simulated ?CDM galaxy clusters
in Monthly Notices of the Royal Astronomical Society: Letters
Robertson A
(2021)
The galaxy-galaxy strong lensing cross-sections of simulated ?CDM galaxy clusters
in Monthly Notices of the Royal Astronomical Society: Letters
Rizzuti F
(2023)
3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star
in Monthly Notices of the Royal Astronomical Society
Rizzuti F
(2022)
Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
in Monthly Notices of the Royal Astronomical Society
Rizzuti F
(2024)
Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Rizzuti F
(2022)
3D hydrodynamics simulations of massive stars with the PROMPI code
in Journal of Physics: Conference Series
Richings J
(2021)
A high-resolution cosmological simulation of a strong gravitational lens
in Monthly Notices of the Royal Astronomical Society
Richings A
(2021)
Unravelling the physics of multiphase AGN winds through emission line tracers
in Monthly Notices of the Royal Astronomical Society
Richings A
(2021)
Unravelling the physics of multiphase AGN winds through emission line tracers
in Monthly Notices of the Royal Astronomical Society
Richings A
(2022)
The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
in Monthly Notices of the Royal Astronomical Society
Rey M
(2024)
Boosting galactic outflows with enhanced resolution
in Monthly Notices of the Royal Astronomical Society
Reina-Campos M
(2022)
Radial distributions of globular clusters trace their host dark matter halo: insights from the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Reid J
(2018)
Coronal energy release by MHD avalanches: continuous driving
in Astronomy & Astrophysics
Reid J
(2021)
Linking computational models to follow the evolution of heated coronal plasma
in Monthly Notices of the Royal Astronomical Society
Regan J
(2018)
Fragmentation inside atomic cooling haloes exposed to Lyman-Werner radiation
in Monthly Notices of the Royal Astronomical Society
Regan J
(2018)
Rise of the first supermassive stars
in Monthly Notices of the Royal Astronomical Society
Reeves A
(2023)
Constraining quenching time-scales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
in Monthly Notices of the Royal Astronomical Society
Read P
(2020)
Baroclinic and barotropic instabilities in planetary atmospheres: energetics, equilibration and adjustment
in Nonlinear Processes in Geophysics
Read P
(2020)
The turbulent dynamics of Jupiter's and Saturn's weather layers: order out of chaos?
in Geoscience Letters
Ray G
(2022)
Determination of hybrid charmonium meson masses
| 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 |