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
Pallero D
(2022)
Too dense to go through: the role of low-mass clusters in the pre-processing of satellite galaxies
in Monthly Notices of the Royal Astronomical Society
Hellinger P
(2022)
Ion-scale transition of plasma turbulence: Pressure-strain effect
Wijers N
(2022)
The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray-line emission
in Monthly Notices of the Royal Astronomical Society
Lamberts A
(2022)
Constraining blazar heating with the 2 ? z ? 3 Lyman-a forest
in Monthly Notices of the Royal Astronomical Society
Moreno V
(2022)
Galactic satellite systems in CDM, WDM and SIDM
Andrassy R
(2022)
Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes
in Astronomy & Astrophysics
Saló LA
(2022)
Well-Posedness of the Four-Derivative Scalar-Tensor Theory of Gravity in Singularity Avoiding Coordinates.
in Physical review letters
Di Carlo M
(2022)
Electromagnetic finite-size effects beyond the point-like approximation
in EPJ Web of Conferences
Radia M
(2022)
Lessons for adaptive mesh refinement in numerical relativity
Font A
(2022)
Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations
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
Davies C
(2021)
Cosmological forecasts with the clustering of weak lensing peaks
Buividovich P
(2021)
Numerical study of the chiral separation effect in two-color QCD at finite density
in Physical Review D
Horst L
(2021)
Multidimensional low-Mach number time-implicit hydrodynamic simulations of convective helium shell burning in a massive star
in Astronomy & Astrophysics
Ganeshaiah Veena P
(2021)
Cosmic Ballet III: Halo spin evolution in the cosmic web
in Monthly Notices of the Royal Astronomical Society
Armijo J
(2021)
Making use of sub-resolution halos in N-body simulations
Chan T
(2021)
Smoothed particle radiation hydrodynamics: two-moment method with local Eddington tensor closure
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
Santos-Santos I
(2021)
Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
Borrow J
(2021)
Inconsistencies arising from the coupling of galaxy formation sub-grid models to pressure-smoothed particle hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Thomas N
(2021)
The radio galaxy population in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Davies C
(2021)
Optimal void finders in weak lensing maps
in Monthly Notices of the Royal Astronomical Society
Lovell M
(2021)
The spatial distribution of Milky Way satellites, gaps in streams, and the nature of dark matter
in Monthly Notices of the Royal Astronomical Society
Williams C
(2021)
ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z ~ 1.5
in The Astrophysical Journal
Gaikwad P
(2021)
A consistent and robust measurement of the thermal state of the IGM at 2 = z = 4 from a large sample of Ly a forest spectra: evidence for late and rapid He ii reionization
in Monthly Notices of the Royal Astronomical Society
Falck B
(2021)
Indra: a public computationally accessible suite of cosmological N -body simulations
in Monthly Notices of the Royal Astronomical Society
Porth L
(2021)
The Information Content of Projected Galaxy Fields
Nightingale J
(2021)
PyAutoLens: Open-Source Strong Gravitational Lensing
Gray A
(2021)
Uncertainty Propagation in SINBAD Fusion Benchmarks with Total Monte Carlo and Imprecise Probabilities
in Fusion Science and Technology
Yardley S
(2021)
Simulating the Coronal Evolution of Bipolar Active Regions to Investigate the Formation of Flux Ropes
in Solar Physics
Robertson A
(2021)
The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
in Monthly Notices of the Royal Astronomical Society
Foster C
(2021)
The MAGPI survey: Science goals, design, observing strategy, early results and theoretical framework
in Publications of the Astronomical Society of Australia
Elliott E
(2021)
Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
in Monthly Notices of the Royal Astronomical Society
Chubb K
(2021)
The ExoMolOP database: Cross sections and k -tables for molecules of interest in high-temperature exoplanet atmospheres
in Astronomy & Astrophysics
Olsen K
(2021)
sígame v3: Gas Fragmentation in Postprocessing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
in The Astrophysical Journal
Cui W
(2021)
The origin of galaxy colour bimodality in the scatter of the stellar-to-halo mass relation
in Nature Astronomy
Robertson A
(2021)
The galaxy-galaxy strong lensing cross-sections of simulated ?CDM galaxy clusters
in Monthly Notices of the Royal Astronomical Society: Letters
Macpherson H
(2021)
Erratum: Luminosity distance and anisotropic sky-sampling at low redshifts: A numerical relativity study [Phys. Rev. D 104 , 023525 (2021)]
in Physical Review D
Silva HO
(2021)
Dynamical Descalarization in Binary Black Hole Mergers.
in Physical review letters
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
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 |