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
Banfi A
(2024)
A POWHEG generator for deep inelastic scattering
in Journal of High Energy Physics
Fu B
(2022)
A predictive and testable unified theory of fermion masses, mixing and leptogenesis
in Journal of High Energy Physics
Pagano P
(2019)
A Prospective New Diagnostic Technique for Distinguishing Eruptive and Noneruptive Active Regions
in The Astrophysical Journal
Hoy C
(2024)
A rapid multi-modal parameter estimation technique for LISA
in Classical and Quantum Gravity
Teodoro L
(2023)
A Recent Impact Origin of Saturn's Rings and Mid-sized Moons
in The Astrophysical Journal
Teodoro L
(2023)
A recent impact origin of Saturn's rings and mid-sized moons
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
Icaza-Lizaola M
(2022)
A sparse regression approach for populating dark matter halos and subhalos with galaxies
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
(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
Baraffe I
(2023)
A study of convective core overshooting as a function of stellar mass based on two-dimensional hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Welsh L
(2024)
A survey of extremely metal-poor gas at cosmic noon Evidence of elevated [O/Fe]
in Astronomy & Astrophysics
Chaikin E
(2023)
A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
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
Oman K
(2024)
A warm dark matter cosmogony may yield more low-mass galaxy detections in 21-cm surveys than a cold dark matter one
in Monthly Notices of the Royal Astronomical Society
Xiao M
(2024)
Accelerated formation of ultra-massive galaxies in the first billion years.
in Nature
Nixon C
(2021)
Accretion discs with non-zero central torque
in New Astronomy
Huško F
(2023)
Active galactic nuclei jets simulated with smoothed particle hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Bourne M
(2017)
AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
in Monthly Notices of the Royal Astronomical Society
Bourne M
(2021)
AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
in Monthly Notices of the Royal Astronomical Society
Bourne M
(2019)
AGN jet feedback on a moving mesh: lobe energetics and X-ray properties in a realistic cluster environment
in Monthly Notices of the Royal Astronomical Society
Matteini L
(2024)
Alfvénic fluctuations in the expanding solar wind: Formation and radial evolution of spherical polarization
in Physics of Plasmas
Williams C
(2021)
ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z ~ 1.5
in The Astrophysical Journal
Chadha-Day F
(2024)
ALP anarchy
in Journal of Cosmology and Astroparticle Physics
Somogyi W
(2024)
An ab initio spectroscopic model of the molecular oxygen atmospheric and infrared bands.
in Physical chemistry chemical physics : PCCP
Van der Werf P
(2020)
An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies
in Monthly Notices of the Royal Astronomical Society
Laitinen T
(2023)
An Analytical Model of Turbulence in Parker Spiral Geometry and Associated Magnetic Field Line Lengths
in The Astrophysical Journal
Armitage T
(2019)
An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations
in Monthly Notices of the Royal Astronomical Society
Pedersen C
(2021)
An emulator for the Lyman-a forest in beyond-?CDM cosmologies
in Journal of Cosmology and Astroparticle Physics
Ruan C
(2024)
An emulator-based halo model in modified gravity - I. The halo concentration-mass relation and density profile
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2024)
An emulator-based halo model in modified gravity - I. The halo concentration-mass relation and density profile
in Monthly Notices of the Royal Astronomical Society
Ahad S
(2024)
An environment-dependent halo mass function as a driver for the early quenching of z = 1.5 cluster galaxies
in Monthly Notices of the Royal Astronomical Society
Elbers W
(2021)
An optimal non-linear method for simulating relic neutrinos
in Monthly Notices of the Royal Astronomical Society
Elbers W
(2021)
An optimal non-linear method for simulating relic neutrinos
in Monthly Notices of the Royal Astronomical Society
Elbers W
(2020)
An optimal nonlinear method for simulating relic neutrinos
Lovell C
(2022)
An orientation bias in observations of submillimetre galaxies
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 |