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
Koudmani S
(2021)
A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Xia Q
(2021)
Intergalactic filaments spin
in Monthly Notices of the Royal Astronomical Society
Coulton W
(2020)
Weak lensing minima and peaks: Cosmological constraints and the impact of baryons
in Monthly Notices of the Royal Astronomical Society
Wilkins S
(2023)
First Light And Reionization Epoch Simulations (FLARES) VII: The star formation and metal enrichment histories of galaxies in the early Universe
in Monthly Notices of the Royal Astronomical Society
Bennett J
(2020)
Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
in Monthly Notices of the Royal Astronomical Society
Kelly A
(2021)
The origin of X-ray coronae around simulated disc galaxies
in Monthly Notices of the Royal Astronomical Society
Pichon C
(2020)
And yet it flips: connecting galactic spin and the cosmic web
in Monthly Notices of the Royal Astronomical Society
Cowley W
(2017)
Blending bias impacts the host halo masses derived from a cross-correlation analysis of bright submillimetre galaxies
in Monthly Notices of the Royal Astronomical Society
Huško F
(2022)
Spin-driven jet feedback in idealized simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Hutt M
(2022)
The effect of local Universe constraints on halo abundance and clustering
in Monthly Notices of the Royal Astronomical Society
Deason A
(2021)
The mass of the Milky Way out to 100 kpc using halo stars
in Monthly Notices of the Royal Astronomical Society
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
Mitchell P
(2020)
Galactic inflow and wind recycling rates in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Dai Z
(2024)
Physics-informed neural networks in the recreation of hydrodynamic simulations from dark matter
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
Mitchell M
(2022)
A general framework to test gravity using galaxy clusters - VI. Realistic galaxy formation simulations to study clusters in modified gravity
in Monthly Notices of the Royal Astronomical Society
Smith A
(2022)
A light-cone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
in Monthly Notices of the Royal Astronomical Society
Sana T
(2023)
Plasma sheath around sunlit moon: monotonic and non-monotonic structures
in Monthly Notices of the Royal Astronomical Society
Huscher E
(2021)
The changing circumgalactic medium over the last 10 Gyr - I. Physical and dynamical properties
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
Mukherjee S
(2021)
SEAGLE - II. Constraints on feedback models in galaxy formation from massive early-type strong-lens galaxies
in Monthly Notices of the Royal Astronomical Society
Yurchenko S
(2024)
ExoMol line lists - LIV. Empirical line lists for AlH and AlD and experimental emission spectroscopy of AlD in A1? ( v = 0, 1, 2)
in Monthly Notices of the Royal Astronomical Society
Christiansen J
(2020)
Jet feedback and the photon underproduction crisis in simba
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
Veresvarska M
(2023)
Outer disc edge: properties of low-frequency aperiodic variability in ultracompact interacting binaries
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
Teyssier R
(2020)
The loss of the intracluster medium in globular clusters
in Monthly Notices of the Royal Astronomical Society
Tagore A
(2018)
Reducing biases on H0 measurements using strong lensing and galaxy dynamics: results from the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
A general framework to test gravity using galaxy clusters IV: cluster and halo properties in DGP gravity
in Monthly Notices of the Royal Astronomical Society
Wu Y
(2023)
Using planet migration and dust drift to weigh protoplanetary discs
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2023)
Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
in Monthly Notices of the Royal Astronomical Society
Oppenheimer B
(2020)
Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
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
Keating L
(2020)
Constraining the second half of reionization with the Ly ß forest
in Monthly Notices of the Royal Astronomical Society
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
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
Salcido J
(2023)
SP(k) - a hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
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
Wang E
(2019)
The impact of black hole seeding in cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Talbot R
(2022)
Blandford-Znajek jets in galaxy formation simulations: exploring the diversity of outflows produced by spin-driven AGN jets in Seyfert galaxies
in Monthly Notices of the Royal Astronomical Society
Evans T
(2022)
Observing EAGLE galaxies with JWST : predictions for Milky Way progenitors and their building blocks
in Monthly Notices of the Royal Astronomical Society
McCarthy I
(2018)
The BAHAMAS project: the CMB-large-scale structure tension and the roles of massive neutrinos and galaxy formation
in Monthly Notices of the Royal Astronomical Society
Appleby S
(2021)
The low-redshift circumgalactic medium in simba
in Monthly Notices of the Royal Astronomical Society
Farahi A
(2018)
Localized massive halo properties in bahamas and MACSIS simulations: scalings, lognormality, and covariance
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2024)
An emulator-based halo model in modified gravity - I. The halo concentration-mass relation and density profile
in Monthly Notices of the Royal Astronomical Society
Prole L
(2022)
Fragmentation-induced starvation in Population III star formation: a resolution study
in Monthly Notices of the Royal Astronomical Society
Cataneo M
(2022)
The matter density PDF for modified gravity and dark energy with Large Deviations Theory
in Monthly Notices of the Royal Astronomical Society
Zamyatina M
(2023)
Observability of signatures of transport-induced chemistry in clear atmospheres of hot gas giant exoplanets
in Monthly Notices of the Royal Astronomical Society
Davé R
(2020)
Galaxy cold gas contents in modern cosmological hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Manera M
(2021)
Obtaining nonlinear galaxy bias constraints from galaxy-lensing phase differences
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 |