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
Wang M
(2017)
Tidal features of classical Milky Way satellites in a ? cold dark matter universe
in Monthly Notices of the Royal Astronomical Society
Astoul A
(2023)
Tidally Excited Inertial Waves in Stars and Planets: Exploring the Frequency-dependent and Averaged Dissipation with Nonlinear Simulations
in The Astrophysical Journal Letters
Yip K
(2024)
To Sample or Not to Sample: Retrieving Exoplanetary Spectra with Variational Inference and Normalizing Flows
in The Astrophysical Journal
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
Parrott W
(2021)
Toward accurate form factors for B -to-light meson decay from lattice QCD
in Physical Review D
Cuesta-Lazaro C
(2020)
Towards a non-Gaussian model of redshift space distortions
in Monthly Notices of the Royal Astronomical Society
Cuesta-Lazaro C
(2020)
Towards a non-Gaussian model of redshift space distortions
Brown S
(2022)
Towards a universal model for the density profiles of dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2022)
Towards an accurate model of small-scale redshift-space distortions in modified gravity
in Monthly Notices of the Royal Astronomical Society
Vizgan D
(2022)
Tracing Molecular Gas Mass in z ? 6 Galaxies with [C ii]
in The Astrophysical Journal
Guervilly C
(2019)
Turbulent convective length scale in planetary cores.
in Nature
Vidal J
(2020)
Turbulent Viscosity Acting on the Equilibrium Tidal Flow in Convective Stars
in The Astrophysical Journal Letters
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
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
Le Saux A
(2023)
Two-dimensional simulations of internal gravity waves in a 5 M? zero-age-main-sequence model
in Monthly Notices of the Royal Astronomical Society
Ratnasingam R
(2020)
Two-dimensional simulations of internal gravity waves in the radiation zones of intermediate-mass stars
in Monthly Notices of the Royal Astronomical Society
Granelli A
(2023)
ULYSSES, Universal LeptogeneSiS Equation Solver: version 2
Granelli A
(2023)
ULYSSES, universal LeptogeneSiS equation solver: Version 2
in Computer Physics Communications
Gray A
(2021)
Uncertainty Propagation in SINBAD Fusion Benchmarks with Total Monte Carlo and Imprecise Probabilities
in Fusion Science and Technology
Schwinn J
(2018)
Uncovering substructure with wavelets:proof of concept using Abell 2744
in Monthly Notices of the Royal Astronomical Society
Yang T
(2022)
Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the simba and TNG simulations
in Monthly Notices of the Royal Astronomical Society
Evstafyeva T
(2023)
Unequal-mass boson-star binaries: initial data and merger dynamics
in Classical and Quantum Gravity
Hellwing W
(2018)
Uneven flows: On cosmic bulk flows, local observers, and gravity
in Physical Review D
Deason A
(2023)
Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function
in Monthly Notices of the Royal Astronomical Society
Fa W
(2018)
Unravelling the Mystery of Lunar Anomalous Craters Using Radar and Infrared Observations
in Journal of Geophysical Research: Planets
Richings A
(2021)
Unravelling the physics of multiphase AGN winds through emission line tracers
in Monthly Notices of the Royal Astronomical Society
Iršic V
(2024)
Unveiling dark matter free streaming at the smallest scales with the high redshift Lyman-alpha forest
in Physical Review D
D'Silva J
(2023)
Unveiling the main sequence of galaxies at z = 5 with the JWST : predictions from simulations
in Monthly Notices of the Royal Astronomical Society
Blum T
(2023)
Update of Euclidean windows of the hadronic vacuum polarization
in Physical Review D
Irodotou D
(2021)
Using angular momentum maps to detect kinematically distinct galactic components
in Monthly Notices of the Royal Astronomical Society
Sullivan D
(2018)
Using artificial neural networks to constrain the halo baryon fraction during reionization
in Monthly Notices of the Royal Astronomical Society
Bilimogga P
(2022)
Using eagle simulations to study the effect of observational constraints on the determination of H i asymmetries in galaxies
in Monthly Notices of the Royal Astronomical Society
Wu Y
(2023)
Using planet migration and dust drift to weigh protoplanetary discs
in Monthly Notices of the Royal Astronomical Society
Barrera-Hinojosa C
(2021)
Vector modes in ?CDM: the gravitomagnetic potential in dark matter haloes from relativistic N -body simulations
in Monthly Notices of the Royal Astronomical Society
Piccirillo E
(2022)
Velocity-dependent annihilation radiation from dark matter subhalos in cosmological simulations
in Journal of Cosmology and Astroparticle Physics
| 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 |