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
Henden N
(2018)
The FABLE simulations: a feedback model for galaxies, groups, and clusters
in Monthly Notices of the Royal Astronomical Society
Henden N
(2019)
The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the fable simulations
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
Hernández-Aguayo C
(2021)
Galaxy formation in the brane world I: overview and first results
in Monthly Notices of the Royal Astronomical Society
Hernández-Aguayo C
(2018)
Marked clustering statistics in f(R) gravity cosmologies
in Monthly Notices of the Royal Astronomical Society
Hernández-Aguayo C
(2021)
Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
in Monthly Notices of the Royal Astronomical Society
Hernández-Aguayo C
(2019)
Large-scale redshift space distortions in modified gravity theories
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
Herzog G
(2023)
The present-day gas content of simulated field dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Hill A
(2021)
The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
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
Ho S
(2021)
How Identifying Circumgalactic Gas by Line-of-sight Velocity instead of the Location in 3D Space Affects O vi Measurements
in The Astrophysical Journal
Hou J
(2021)
How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
in Monthly Notices of the Royal Astronomical Society
Hou J
(2018)
A new gas cooling model for semi-analytic galaxy formation models
in Monthly Notices of the Royal Astronomical Society
Howson T
(2021)
Magnetic reconnection and the Kelvin-Helmholtz instability in the solar corona
in Astronomy & Astrophysics
Hughes M
(2021)
What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
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
Hutt M
(2022)
The effect of local Universe constraints on halo abundance and clustering
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
Huško F
(2023)
The complex interplay of AGN jet-inflated bubbles and the intracluster medium
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
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
Huško F
(2023)
Active galactic nuclei jets simulated with smoothed particle hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Icaza-Lizaola M
(2021)
A sparse regression approach to modelling the relation between galaxy stellar masses and their host haloes
in Monthly Notices of the Royal Astronomical Society
Icaza-Lizaola M
(2023)
A sparse regression approach for populating dark matter haloes and subhaloes with galaxies
in Monthly Notices of the Royal Astronomical Society
Irodotou D
(2021)
Using angular momentum maps to detect kinematically distinct galactic components
in Monthly Notices of the Royal Astronomical Society
Johnston C
(2021)
A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method
in Astronomy & Astrophysics
Kafle P
(2018)
Galaxy tagging: photometric redshift refinement and group richness enhancement
in Monthly Notices of the Royal Astronomical Society
Kalaghatgi C
(2021)
Investigating the effect of in-plane spin directions for precessing binary black hole systems
in Physical Review D
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
(2019)
Magnetogenesis at Cosmic Dawn: tracing the origins of cosmic magnetic fields
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
(2017)
Interpreting ALMA observations of the ISM during the epoch of reionization
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
(2018)
A Census of the LyC photons that form the UV background during reionization
in Monthly Notices of the Royal Astronomical Society
Kay S
(2020)
The intracluster light as a tracer of the total matter density distribution: a view from 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
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
(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
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
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
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
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
(2019)
Fast and energetic AGN-driven outflows in simulated dwarf galaxies
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
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| Exploitation Route | See Dirac annual report https://dirac.ac.uk |
| Sectors | Digital/Communication/Information Technologies (including Software),Education |
| URL | https://dirac.ac.uk |