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 P
(2020)
Galactic inflow and wind recycling rates in the EAGLE simulations
Mitchell P
(2019)
Galactic outflow rates in the EAGLE simulations
Mitchell P
(2020)
Galactic inflow and wind recycling rates in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2020)
Galactic outflow rates in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Mocz P
(2023)
Cosmological structure formation and soliton phase transition in fuzzy dark matter with axion self-interactions
in Monthly Notices of the Royal Astronomical Society
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
Molaro M
(2022)
The effect of inhomogeneous reionization on the Lyman a forest power spectrum at redshift z > 4: implications for thermal parameter recovery
in Monthly Notices of the Royal Astronomical Society
Monaco P
(2020)
The accuracy of weak lensing simulations
in Monthly Notices of the Royal Astronomical Society
Montargès M
(2023)
The VLT/SPHERE view of the ATOMIUM cool evolved star sample I. Overview: Sample characterization through polarization analysis
in Astronomy & Astrophysics
Montero F
(2019)
Mergers, Starbursts, and Quenching in the Simba Simulation
Morello G
(2023)
Spitzer thermal phase curve of WASP-121 b
in Astronomy & Astrophysics
Moreno V
(2021)
Baryon-driven decontraction in Milky Way mass haloes
Moreno V
(2022)
Galactic satellite systems in CDM, WDM and SIDM
Mosbech M
(2023)
Gravitational-wave event rates as a new probe for dark matter microphysics
in Physical Review D
Mukherjee S
(2018)
SEAGLE - I. A pipeline for simulating and modelling strong lenses from cosmological hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Mukherjee S
(2021)
SEAGLE - II. Constraints on feedback models in galaxy formation from massive early-type strong-lens galaxies
in Monthly Notices of the Royal Astronomical Society
Müller B
(2017)
Supernova simulations from a 3D progenitor model - Impact of perturbations and evolution of explosion properties
in Monthly Notices of the Royal Astronomical Society
Müller B
(2018)
Multidimensional simulations of ultrastripped supernovae to shock breakout
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
Navarro J
(2018)
The innate origin of radial and vertical gradients in a simulated galaxy disc
in Monthly Notices of the Royal Astronomical Society
Nazari Z
(2021)
Oscillon collapse to black holes
in Journal of Cosmology and Astroparticle Physics
Negri A
(2022)
The luminosity of cluster galaxies in the Cluster-EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Newton O
(2018)
The total satellite population of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Newton O
(2021)
Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way
in Journal of Cosmology and Astroparticle Physics
Nightingale J
(2021)
PyAutoLens: Open-Source Strong Gravitational Lensing
Nightingale J
(2023)
PyAutoGalaxy: Open-Source Multiwavelength Galaxy Structure & Morphology
in Journal of Open Source Software
Nightingale J
(2021)
PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
in Journal of Open Source Software
Nightingale J
(2023)
PyAutoGalaxy: Open-Source Multiwavelength Galaxy Structure & Morphology
Nightingale J
(2021)
PyAutoLens: Open-Source Strong Gravitational Lensing
in Journal of Open Source Software
Nixon C
(2021)
Partial, Zombie, and Full Tidal Disruption of Stars by Supermassive Black Holes
in The Astrophysical Journal
Nixon C
(2021)
Accretion discs with non-zero central torque
in New Astronomy
Nobels F
(2022)
The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Norman S
(2021)
Stars Crushed by Black Holes. I. On the Energy Distribution of Stellar Debris in Tidal Disruption Events
in The Astrophysical Journal
Oleskiewicz P
(2019)
The connection between halo concentrations and assembly histories: a probe of gravity?
in Monthly Notices of the Royal Astronomical Society
Olsen K
(2021)
sígame v3: Gas Fragmentation in Postprocessing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
in The Astrophysical Journal
Oman K
(2017)
The "Building Blocks" of Stellar Halos
in Galaxies
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
Orkney M
(2023)
EDGE: the shape of dark matter haloes in the faintest galaxies
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2021)
EDGE: two routes to dark matter core formation in ultra-faint dwarfs
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 |