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
Kannan R
(2023)
The MillenniumTNG project: the galaxy population at z = 8
in Monthly Notices of the Royal Astronomical Society
Karunakaran A
(2021)
Satellites around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations versus Simulations
in The Astrophysical Journal Letters
Katsianis A
(2021)
The specific star formation rate function at different mass scales and quenching: a comparison between cosmological models and SDSS
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
Katz H
(2017)
Interpreting ALMA observations of the ISM during the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
Katz H
(2023)
Two modes of LyC escape from bursty star formation: implications for [C ii ] deficits and the sources of reionization
in Monthly Notices of the Royal Astronomical Society
Katz H
(2023)
The SPHINX Public Data Release: Forward Modelling High-Redshift JWST Observations with Cosmological Radiation Hydrodynamics Simulations
in The Open Journal of Astrophysics
Katz H
(2019)
Magnetogenesis at Cosmic Dawn: tracing the origins of cosmic magnetic fields
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
Keating L
(2020)
Constraining the second half of reionization with the Ly ß forest
in Monthly Notices of the Royal Astronomical Society
Keating L
(2024)
The origin of the characteristic shape and scatter of intergalactic damping wings during reionization
in Monthly Notices of the Royal Astronomical Society: Letters
Keating L
(2024)
JWST observations of galaxy-damping wings during reionization interpreted with cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Kegerreis J
(2022)
Immediate Origin of the Moon as a Post-impact Satellite
in The Astrophysical Journal Letters
Kegerreis J
(2022)
Immediate origin of the Moon as a post-impact satellite
Kegerreis J
(2018)
Consequences of Giant Impacts on Early Uranus for Rotation, Internal Structure, Debris, and Atmospheric Erosion
in The Astrophysical Journal
Kelly A
(2021)
The origin of X-ray coronae around simulated disc galaxies
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
Kelly A
(2022)
Apostle-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Kelly A
(2020)
The origin of X-ray coronae around simulated disc galaxies
Kesri K
(2024)
Dependence of Spicule Properties on the Magnetic Field-Results from Magnetohydrodynamics Simulations
in The Astrophysical Journal
Khrykin I
(2024)
The cosmic baryon partition between the IGM and CGM in the SIMBA simulations
in Monthly Notices of the Royal Astronomical Society
Kirchschlager F
(2023)
Dust survival rates in clumps passing through the Cas A reverse shock - II. The impact of magnetic fields
in Monthly Notices of the Royal Astronomical Society
Kirchschlager F
(2024)
From total destruction to complete survival: dust processing at different evolutionary stages in the supernova remnant Cassiopeia A
in Monthly Notices of the Royal Astronomical Society
Knebe A
(2018)
Cosmic CARNage I: on the calibration of galaxy formation models
in Monthly Notices of the Royal Astronomical Society
Kobayashi C
(2020)
New Type Ia Supernova Yields and the Manganese and Nickel Problems in the Milky Way and Dwarf Spheroidal Galaxies
in The Astrophysical Journal
Kobayashi C
(2020)
The Origin of Elements from Carbon to Uranium
in The Astrophysical Journal
Komissarov S
(2019)
Magnetic inhibition of centrifugal instability
in Monthly Notices of the Royal Astronomical Society
Komissarov S
(2019)
Magnetic Inhibition of Centrifugal Instability in Astrophysical Jets
Kong S
(2022)
Filament formation via collision-induced magnetic reconnection - formation of a star cluster
in Monthly Notices of the Royal Astronomical Society
Koponen J
(2022)
Properties of low-lying charmonia and bottomonia from lattice QCD + QED
in Suplemento de la Revista Mexicana de FÃsica
Kordov Z
(2021)
State mixing and masses of the p 0 , ? and ? ' mesons from n f = 1 + 1 + 1 lattice QCD + QED
in Physical Review D
Koskela T
(2023)
Principles for Automated and Reproducible Benchmarking
Koudmani S
(2019)
Fast and energetic AGN-driven outflows in simulated dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Koudmani S
(2021)
A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Koudmani S
(2024)
A unified accretion disc model for supermassive black holes in galaxy formation simulations: method and implementation
in Monthly Notices of the Royal Astronomical Society
Koudmani S
(2018)
Fast and energetic AGN-driven outflows in simulated dwarf galaxies
Koudmani S
(2021)
A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
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
Kraljic K
(2019)
And yet it flips: connecting galactic spin and the cosmic web
Kraljic K
(2020)
And yet it flips: connecting galactic spin and the cosmic web
in Monthly Notices of the Royal Astronomical Society
Kraljic K
(2020)
The impact of the connectivity of the cosmic web on the physical properties of galaxies at its nodes
in Monthly Notices of the Royal Astronomical Society
Kruijssen J
(2019)
The formation and assembly history of the Milky Way revealed by its globular cluster population
in Monthly Notices of the Royal Astronomical Society
Kugel R
(2023)
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning.
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 |