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
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
Porth L
(2020)
Fast estimation of aperture mass statistics - I. Aperture mass variance and an application to the CFHTLenS data
in Monthly Notices of the Royal Astronomical Society
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
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
Šoltinskí T
(2021)
The detectability of strong 21 centimetre forest absorbers from the diffuse intergalactic medium in late reionisation models
in Monthly Notices of the Royal Astronomical Society
Vidal J
(2020)
Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
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
Cautun M
(2018)
The Santiago-Harvard-Edinburgh-Durham void comparison - I. SHEDding light on chameleon gravity tests
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
Acuto A
(2021)
The BAHAMAS project: evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
in Monthly Notices of the Royal Astronomical Society
Schaye J
(2023)
The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
in Monthly Notices of the Royal Astronomical Society
Rodríguez Montero F
(2019)
Mergers, starbursts, and quenching in the simba simulation
in Monthly Notices of the Royal Astronomical Society
Wilkins S
(2023)
First light and reionization epoch simulations (FLARES) V: the redshift frontier
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
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
Katz H
(2018)
A Census of the LyC photons that form the UV background during reionization
in Monthly Notices of the Royal Astronomical Society
Martin-Alvarez S
(2023)
The Pandora project - I. The impact of radiation, magnetic fields, and cosmic rays on the baryonic and dark matter properties of dwarf galaxies
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
Bahé Y
(2021)
Strongly lensed cluster substructures are not in tension with ?CDM
in Monthly Notices of the Royal Astronomical Society
Huško F
(2022)
Statistics of galaxy mergers: bridging the gap between theory and observation
in Monthly Notices of the Royal Astronomical Society
Theuns T
(2021)
Connecting cosmological accretion to strong Ly a absorbers
in Monthly Notices of the Royal Astronomical Society
Pearce F
(2021)
Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
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
Borrow J
(2023)
The impact of stochastic modelling on the predictive power of galaxy formation simulations
in Monthly Notices of the Royal Astronomical Society
He J
(2020)
Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
in Monthly Notices of the Royal Astronomical Society
Zenocratti L
(2022)
The origin of correlations between mass, metallicity, and morphology in galaxies from the eagle simulation
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
Hillier A
(2023)
The role of cooling induced by mixing in the mass and energy cycles of the solar atmosphere
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
Richings A
(2021)
Unravelling the physics of multiphase AGN winds through emission line tracers
in Monthly Notices of the Royal Astronomical Society
Owens A
(2021)
ExoMol line lists - XLI. High-temperature molecular line lists for the alkali metal hydroxides KOH and NaOH
in Monthly Notices of the Royal Astronomical Society
Šoltinský T
(2023)
Probing quasar lifetimes with proximate 21-centimetre absorption in the diffuse intergalactic medium at redshifts z = 6
in Monthly Notices of the Royal Astronomical Society
Bourne M
(2017)
AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
in Monthly Notices of the Royal Astronomical Society
Han J
(2018)
hbt+: an improved code for finding subhaloes and building merger trees in cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Huško F
(2023)
The buildup of galaxies and their spheroids: The contributions of mergers, disc instabilities, and star formation
in Monthly Notices of the Royal Astronomical Society
Koudmani S
(2019)
Fast and energetic AGN-driven outflows in simulated dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Gunawardhana M
(2020)
Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra
in Monthly Notices of the Royal Astronomical Society
Costa T
(2018)
Driving gas shells with radiation pressure on dust in radiation-hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Mayes R
(2021)
Contribution of stripped nuclei to the ultracompact dwarf galaxy population in the Virgo cluster
in Monthly Notices of the Royal Astronomical Society
Schirra A
(2021)
Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Hernández-Aguayo C
(2023)
The MillenniumTNG Project: high-precision predictions for matter clustering and halo statistics
in Monthly Notices of the Royal Astronomical Society
Henden N
(2020)
The baryon content of groups and clusters of galaxies in the FABLE simulations
in Monthly Notices of the Royal Astronomical Society
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
Wang W
(2017)
What to expect from dynamical modelling of galactic haloes
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
Dutta R
(2021)
Metal-enriched halo gas across galaxy overdensities over the last 10 billion years
in Monthly Notices of the Royal Astronomical Society
Ragusa E
(2021)
Circumbinary and circumstellar discs around the eccentric binary IRAS 04158+2805 - a testbed for binary-disc interaction
in Monthly Notices of the Royal Astronomical Society
Sullivan D
(2018)
Using artificial neural networks to constrain the halo baryon fraction during reionization
in Monthly Notices of the Royal Astronomical Society
Borrow J
(2021)
Inconsistencies arising from the coupling of galaxy formation sub-grid models to pressure-smoothed particle hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Reid J
(2021)
Linking computational models to follow the evolution of heated coronal plasma
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 |