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
Srisawat C
(2020)
MEGA: Merger graphs of structure formation
in Monthly Notices of the Royal Astronomical Society
Sormani M
(2020)
Simulations of the Milky Way's Central Molecular Zone - II. Star formation
in Monthly Notices of the Royal Astronomical Society
Sorini D
(2020)
simba: the average properties of the circumgalactic medium of 2 = z = 3 quasars are determined primarily by stellar feedback
in Monthly Notices of the Royal Astronomical Society
Somà V
(2021)
Moving away from singly-magic nuclei with Gorkov Green's function theory
in The European Physical Journal A
Smith R
(2023)
On the distribution of the cold neutral medium in galaxy discs
in Monthly Notices of the Royal Astronomical Society
Smith M
(2018)
Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
in Monthly Notices of the Royal Astronomical Society
Smith M
(2019)
Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
in Monthly Notices of the Royal Astronomical Society
Smith G
(2020)
The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451-03
in Monthly Notices of the Royal Astronomical Society
Smith A
(2020)
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N -body mock challenge for the quasar sample
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
Smith A
(2022)
Solving small-scale clustering problems in approximate light-cone mocks
in Monthly Notices of the Royal Astronomical Society
Smith A
(2019)
Correcting for fibre assignment incompleteness in the DESI Bright Galaxy Survey
in Monthly Notices of the Royal Astronomical Society
Smail R
(2023)
Constraining beyond the standard model nucleon isovector charges
in Physical Review D
Simpson C
(2020)
The milky way total mass profile as inferred from Gaia DR2
in Monthly Notices of the Royal Astronomical Society
Silva HO
(2021)
Dynamical Descalarization in Binary Black Hole Mergers.
in Physical review letters
Shingles L
(2023)
Self-consistent 3D Radiative Transfer for Kilonovae: Directional Spectra from Merger Simulations
in The Astrophysical Journal Letters
Shi D
(2017)
Environmental screening of dark matter haloes in f ( R ) gravity
in Monthly Notices of the Royal Astronomical Society
Sherletov A
(2023)
Lattice Studies of 3D Maximally Supersymmetric Yang-Mills
Sharma M
(2018)
CEMPlifying reionization
in Monthly Notices of the Royal Astronomical Society
Shao S
(2021)
The survival of globular clusters in a cuspy Fornax
in Monthly Notices of the Royal Astronomical Society
Sergeev D
(2023)
Simulations of idealised 3D atmospheric flows on terrestrial planets using LFRic-Atmosphere
in Geoscientific Model Development
Semenov M
(2021)
Rovibronic spectroscopy of PN from first principles.
in Physical chemistry chemical physics : PCCP
Seeyave L
(2023)
First light and reionization epoch simulations (FLARES) X iii : the lyman-continuum emission of high-redshift galaxies
in Monthly Notices of the Royal Astronomical Society
Scott L
(2021)
Convective core entrainment in 1D main-sequence stellar models
in Monthly Notices of the Royal Astronomical Society
Schönrich R
(2017)
Assessing distances and consistency of kinematics in Gaia/TGAS
in Monthly Notices of the Royal Astronomical Society
Schönrich R
(2018)
Warp, waves, and wrinkles in the Milky Way
in Monthly Notices of the Royal Astronomical Society
Schwinn J
(2018)
Uncovering substructure with wavelets:proof of concept using Abell 2744
in Monthly Notices of the Royal Astronomical Society
Scholtz J
(2018)
Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Scholtz J
(2023)
GN-z11: The environment of an AGN at $z=$10.603
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
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
Schaller M
(2024)
On the anisotropic distribution of clusters in the local Universe
in Monthly Notices of the Royal Astronomical Society: Letters
Sawala T
(2021)
The SIBELIUS Project: E Pluribus Unum
Sawala T
(2023)
Distinct distributions of elliptical and disk galaxies across the Local Supercluster as a ?CDM prediction
in Nature Astronomy
Sawala T
(2023)
The timeless timing argument and the total mass of the Local Group
in Monthly Notices of the Royal Astronomical Society: Letters
Sawala T
(2023)
The Timeless Timing Argument and the Mass of the Local Group
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| Sectors | Digital/Communication/Information Technologies (including Software) Education |
| URL | https://dirac.ac.uk |