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
Goater A
(2024)
EDGE: The direct link between mass growth history and the extended stellar haloes of the faintest dwarf galaxies
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
Yip K
(2024)
To Sample or Not to Sample: Retrieving Exoplanetary Spectra with Variational Inference and Normalizing Flows
in The Astrophysical Journal
Changeat Q
(2024)
Is the Atmosphere of the Ultra-hot Jupiter WASP-121 b Variable?
in The Astrophysical Journal Supplement Series
Rey M
(2024)
Boosting galactic outflows with enhanced resolution
in Monthly Notices of the Royal Astronomical Society
Rowan C
(2024)
Black hole binaries in AGN accretion discs - II. Gas effects on black hole satellite scatterings
in Monthly Notices of the Royal Astronomical Society
Witten C
(2024)
Deciphering Lyman-a emission deep into the epoch of reionization
in Nature Astronomy
Pizzati E
(2024)
Revisiting the extreme clustering of z ˜ 4 quasars with large volume cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Feng J
(2024)
On the evolution of the observed mass-to-length relationship for star-forming filaments
in Monthly Notices of the Royal Astronomical Society
Chan T
(2024)
The impact and response of mini-haloes and the interhalo medium on cosmic reionization
in Monthly Notices of the Royal Astronomical Society
Wilkins S
(2024)
First Light and Reionization Epoch Simulations ( flares ) - XIV. The Balmer/4000 Å breaks of distant galaxies
in Monthly Notices of the Royal Astronomical Society
Bennett E
(2024)
Singlets in gauge theories with fundamental matter
in Physical Review D
Ploeckinger S
(2024)
Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multiphase interstellar medium
in Monthly Notices of the Royal Astronomical Society
Bartlett D
(2024)
Exhaustive Symbolic Regression
in IEEE Transactions on Evolutionary Computation
Hamilton E
(2024)
Catalog of precessing black-hole-binary numerical-relativity simulations
in Physical Review D
Ghosh S
(2024)
First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence
in Physical Review D
Dai Z
(2024)
Physics-informed neural networks in the recreation of hydrodynamic simulations from dark matter
in Monthly Notices of the Royal Astronomical Society
Yurchenko S
(2024)
ExoMol line lists - LIV. Empirical line lists for AlH and AlD and experimental emission spectroscopy of AlD in A1? ( v = 0, 1, 2)
in Monthly Notices of the Royal Astronomical Society
Gonzalo T
(2024)
PEANUTS: a software for the automatic computation of solar neutrino flux and its propagation within Earth
in The European Physical Journal C
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
Pakmor R
(2024)
Magnetic field amplification in cosmological zoom simulations from dwarf galaxies to galaxy groups
in Monthly Notices of the Royal Astronomical Society
Owens A
(2024)
ExoMol line lists - LI. Molecular line lists for lithium hydroxide (LiOH)
in Monthly Notices of the Royal Astronomical Society
Carrillo A
(2024)
Can we really pick and choose? Benchmarking various selections of Gaia Enceladus/Sausage stars in observations with simulations
in Monthly Notices of the Royal Astronomical Society
Edwards B
(2024)
Measuring Tracers of Planet Formation in the Atmosphere of WASP-77A b: Substellar O/H and C/H Ratios, with a Stellar C/O Ratio and a Potentially Superstellar Ti/H Ratio
in The Astrophysical Journal Letters
Fenton A
(2024)
The 3D structure of disc-instability protoplanets
in Astronomy & Astrophysics
Ibrahim D
(2024)
The impact of supernova feedback on the mass-metallicity relations
in Monthly Notices of the Royal Astronomical Society
Mayes R
(2024)
The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
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 |