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
Borrow J
(2020)
Cosmological baryon transfer in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Fattahi A
(2019)
The origin of galactic metal-rich stellar halo components with highly eccentric orbits
in Monthly Notices of the Royal Astronomical Society
Ganeshaiah Veena P
(2019)
The Cosmic Ballet II: spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
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
Gómez J
(2022)
Halo merger tree comparison: impact on galaxy formation models
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
Braspenning J
(2023)
Sensitivity of non-radiative cloud-wind interactions to the hydrodynamic solver
in Monthly Notices of the Royal Astronomical Society
Prole L
(2022)
Primordial magnetic fields in Population III star formation: a magnetized resolution study
in Monthly Notices of the Royal Astronomical Society
Zheng Y
(2022)
Rapidly quenched galaxies in the Simba cosmological simulation and observations
in Monthly Notices of the Royal Astronomical Society
Bennett J
(2024)
The growth of the gargantuan black holes powering high-redshift quasars and their impact on the formation of early galaxies and protoclusters
in Monthly Notices of the Royal Astronomical Society
Haworth T
(2021)
Warm millimetre dust in protoplanetary discs near massive stars
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2018)
Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Lara-López M
(2019)
Oxygen yields as a constraint on feedback processes in galaxies
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
Katz H
(2023)
The challenges of identifying Population III stars in the early Universe
in Monthly Notices of the Royal Astronomical Society
Gunawardhana M
(2018)
Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small-scale galaxy clustering
in Monthly Notices of the Royal Astronomical Society
Correa C
(2019)
The origin of the red-sequence galaxy population in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Trujillo-Gomez S
(2021)
The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Whitworth D
(2023)
Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Arnold C
(2022)
forge : the f ( R )-gravity cosmic emulator project - I. Introduction and matter power spectrum emulator
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
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
Elvis M
(2020)
Q wind code release: a non-hydrodynamical approach to modelling line-driven winds in active galactic nuclei
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
Trotta D
(2023)
Three-dimensional modelling of the shock-turbulence interaction
in Monthly Notices of the Royal Astronomical Society
Stafford S
(2021)
Testing extensions to ?CDM on small scales with forthcoming cosmic shear surveys
in Monthly Notices of the Royal Astronomical Society
Sorini D
(2022)
How baryons affect haloes and large-scale structure: a unified picture from the Simba simulation
in Monthly Notices of the Royal Astronomical Society
Smith A
(2021)
Reducing the variance of redshift space distortion measurements from mock galaxy catalogues with different lines of sight
in Monthly Notices of the Royal Astronomical Society
Pakmor R
(2023)
The MillenniumTNG Project: the hydrodynamical full physics simulation and a first look at its galaxy clusters
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
Mitchell M
(2019)
A general framework to test gravity using galaxy clusters II: A universal model for the halo concentration in f(R) 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
Goater A
(2024)
EDGE: The direct link between mass growth history and the extended stellar haloes of the faintest dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Simpson C
(2020)
The milky way total mass profile as inferred from Gaia DR2
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
Weinberger L
(2018)
Lyman-a emitters gone missing: the different evolution of the bright and faint populations
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
Ahad S
(2024)
An environment-dependent halo mass function as a driver for the early quenching of z = 1.5 cluster galaxies
in Monthly Notices of the Royal Astronomical Society
Bolton J
(2022)
Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman a forest
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
Sawala T
(2021)
Setting the stage: structures from Gaussian random fields
in Monthly Notices of the Royal Astronomical Society
Smith R
(2023)
On the distribution of the cold neutral medium in galaxy discs
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
Yankelevich V
(2023)
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
in Monthly Notices of the Royal Astronomical Society
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
Altamura E
(2023)
EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
in Monthly Notices of the Royal Astronomical Society
Hadzhiyska B
(2023)
The MillenniumTNG Project: an improved two-halo model for the galaxy-halo connection of red and blue galaxies
in Monthly Notices of the Royal Astronomical Society
Costa T
(2018)
Quenching star formation with quasar outflows launched by trapped IR radiation
in Monthly Notices of the Royal Astronomical Society
Li Y
(2022)
Non-linear reconstruction of features in the primordial power spectrum from large-scale structure
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
| 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 |