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
Leo M
(2018)
Nonlinear growth of structure in cosmologies with damped matter fluctuations
in Journal of Cosmology and Astroparticle Physics
Buividovich P
(2021)
Numerical study of the chiral separation effect in two-color QCD at finite density
in Physical Review D
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
Manera M
(2021)
Obtaining nonlinear galaxy bias constraints from galaxy-lensing phase differences
in Monthly Notices of the Royal Astronomical Society
Vincenzo F
(2018)
On the [a/Fe]-[Fe/H] relations in early-type galaxies
in Monthly Notices of the Royal Astronomical Society: Letters
Smith R
(2023)
On the distribution of the cold neutral medium in galaxy discs
in Monthly Notices of the Royal Astronomical Society
Drewes N
(2021)
On the Dynamics of Low-viscosity Warped Disks around Black Holes
in The Astrophysical Journal
Desmond H
(2017)
On the galaxy-halo connection in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society: Letters
Bose B
(2020)
On the road to per cent accuracy IV: ReACT - computing the non-linear power spectrum beyond ?CDM
in Monthly Notices of the Royal Astronomical Society
Cooke R
(2018)
One Percent Determination of the Primordial Deuterium Abundance
in The Astrophysical Journal
Davies C
(2021)
Optimal void finders in weak lensing maps
in Monthly Notices of the Royal Astronomical Society
Nazari Z
(2021)
Oscillon collapse to black holes
in Journal of Cosmology and Astroparticle Physics
Aurrekoetxea J
(2023)
Oscillon formation during inflationary preheating with general relativity
in Physical Review D
Veresvarska M
(2023)
Outer disc edge: properties of low-frequency aperiodic variability in ultracompact interacting binaries
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
Tröster T
(2019)
Painting with baryons: augmenting N-body simulations with gas using deep generative models
in Monthly Notices of the Royal Astronomical Society: Letters
Nixon C
(2021)
Partial, Zombie, and Full Tidal Disruption of Stars by Supermassive Black Holes
in The Astrophysical Journal
Elbers W
(2023)
Persistent topology of the reionization bubble network - II. Evolution and classification
in Monthly Notices of the Royal Astronomical Society
Wu X
(2020)
Photometric properties of reionization-epoch galaxies in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Teodoro L
(2019)
Planetary giant impacts: convergence of high-resolution simulations using efficient spherical initial conditions and swift
in Monthly Notices of the Royal Astronomical Society
Vandenbroucke B
(2021)
Polarised emission from aligned dust grains in nearby galaxies: Predictions from the Auriga simulations
in Astronomy & Astrophysics
Molaro M
(2023)
Possible evidence for a large-scale enhancement in the Lyman-a forest power spectrum at redshift z = 4
in Monthly Notices of the Royal Astronomical Society
Cowell J
(2023)
Potential signature of a quadrupolar hubble expansion in Pantheon+supernovae
in Monthly Notices of the Royal Astronomical Society
Mateu C
(2017)
Predictions for the detection of tidal streams with Gaia using great-circle methods
in Monthly Notices of the Royal Astronomical Society
Zarrouk P
(2022)
Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
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
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
Gaikwad P
(2020)
Probing the thermal state of the intergalactic medium at z > 5 with the transmission spikes in high-resolution Ly a forest spectra
in Monthly Notices of the Royal Astronomical Society
Mastromarino C
(2023)
Properties and observables of massive galaxies in self-interacting dark matter cosmologies
in Monthly Notices of the Royal Astronomical Society
Witstok J
(2021)
Prospects for observing the low-density cosmic web in Lyman- a emission
in Astronomy & Astrophysics
Nightingale J
(2021)
PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
in Journal of Open Source Software
Nightingale J
(2021)
PyAutoLens: Open-Source Strong Gravitational Lensing
in Journal of Open Source Software
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
Bamber J
(2021)
Quasinormal modes of growing dirty black holes
in Physical Review D
Font A
(2022)
Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations
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
Quera-Bofarull A
(2023)
qwind 3: UV line-driven accretion disc wind models for AGN feedback
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
Rizzuti F
(2022)
Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
in Monthly Notices of the Royal Astronomical Society
Syntelis P
(2017)
Recurrent CME-like Eruptions in Emerging Flux Regions. I. On the Mechanism of Eruptions
in The Astrophysical Journal
Cheek A
(2022)
Redshift effects in particle production from Kerr primordial black holes
in Physical Review D
Robson D
(2023)
Redshift evolution of galaxy group X-ray properties in the Simba simulations
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
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
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
Lovell C
(2021)
Reproducing submillimetre galaxy number counts with cosmological hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Bernal N
(2022)
Rescuing high-scale leptogenesis using primordial black holes
in Physical Review D
Mao T
(2018)
Resolution of the apparent discrepancy between the number of massive subhaloes in Abell 2744 and ?CDM
in Monthly Notices of the Royal Astronomical Society: Letters
De Beer S
(2023)
Resolving the physics of quasar Ly a nebulae (RePhyNe): I. Constraining quasar host halo masses through circumgalactic medium kinematics
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 |