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
Upadhyay A
(2021)
Star formation histories of Coma cluster galaxies matched to simulated orbits hint at quenching around first pericenter
in Astronomy & Astrophysics
Pagano P
(2018)
Contribution of phase-mixing of Alfvén waves to coronal heating in multi-harmonic loop oscillations
in Astronomy & Astrophysics
Reid J
(2018)
Coronal energy release by MHD avalanches: continuous driving
in Astronomy & Astrophysics
Bemporad A
(2018)
Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test
in Astronomy & Astrophysics
Vandenbroucke B
(2020)
CMACIONIZE 2.0: a novel task-based approach to Monte Carlo radiation transfer
in Astronomy & Astrophysics
Fyfe L
(2021)
Forward modelling of heating within a coronal arcade
in Astronomy & Astrophysics
Chubb K
(2021)
The ExoMolOP database: Cross sections and k -tables for molecules of interest in high-temperature exoplanet atmospheres
in Astronomy & Astrophysics
Johnston C
(2021)
A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method
in Astronomy & Astrophysics
Goldstraw E
(2018)
Comparison of methods for modelling coronal magnetic fields
in Astronomy & Astrophysics
Witstok J
(2021)
Prospects for observing the low-density cosmic web in Lyman- a emission
in Astronomy & Astrophysics
Howson T
(2021)
Magnetic reconnection and the Kelvin-Helmholtz instability in the solar corona
in Astronomy & Astrophysics
Pagano P
(2017)
Contribution of mode-coupling and phase-mixing of Alfvén waves to coronal heating
in Astronomy & Astrophysics
Vandenbroucke B
(2021)
Polarised emission from aligned dust grains in nearby galaxies: Predictions from the Auriga simulations
in Astronomy & Astrophysics
Clough K
(2021)
Continuity equations for general matter: applications in numerical relativity
in Classical and Quantum Gravity
Helfer T
(2022)
Malaise and remedy of binary boson-star initial data
in Classical and Quantum Gravity
Di Carlo M
(2022)
Electromagnetic finite-size effects beyond the point-like approximation
in EPJ Web of Conferences
Oman K
(2017)
The "Building Blocks" of Stellar Halos
in Galaxies
Dietrich W
(2018)
Anelastic spherical dynamos with radially variable electrical conductivity
in Icarus
Pedersen C
(2021)
An emulator for the Lyman-a forest in beyond-?CDM cosmologies
in Journal of Cosmology and Astroparticle Physics
Leo M
(2018)
Nonlinear growth of structure in cosmologies with damped matter fluctuations
in Journal of Cosmology and Astroparticle Physics
Leo M
(2018)
A new smooth- k space filter approach to calculate halo abundances
in Journal of Cosmology and Astroparticle Physics
Leo M
(2018)
N-body simulations of structure formation in thermal inflation cosmologies
in Journal of Cosmology and Astroparticle Physics
Nazari Z
(2021)
Oscillon collapse to black holes
in Journal of Cosmology and Astroparticle Physics
Fa W
(2018)
Unravelling the Mystery of Lunar Anomalous Craters Using Radar and Infrared Observations
in Journal of Geophysical Research: Planets
Allanson O
(2021)
Electron Diffusion and Advection During Nonlinear Interactions With Whistler-Mode Waves
in Journal of Geophysical Research: Space Physics
Drach V
(2021)
Scattering of Goldstone bosons and resonance production in a composite Higgs model on the lattice
in Journal of High Energy Physics
Nightingale J
(2021)
PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
in Journal of Open Source Software
Andrade T
(2021)
GRChombo: An adaptable numerical relativity code for fundamental physics
in Journal of Open Source Software
Nightingale J
(2021)
PyAutoLens: Open-Source Strong Gravitational Lensing
in Journal of Open Source Software
Agudelo Rueda J
(2021)
Three-dimensional magnetic reconnection in particle-in-cell simulations of anisotropic plasma turbulence
in Journal of Plasma Physics
Pagano P
(2018)
A new technique for observationally derived boundary conditions for space weather
in Journal of Space Weather and Space Climate
Downing E
(2023)
The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions
in Monthly Notices of the Royal Astronomical Society
Cataneo M
(2022)
The matter density PDF for modified gravity and dark energy with Large Deviations Theory
in Monthly Notices of the Royal Astronomical Society
Barrera M
(2023)
The MillenniumTNG Project: semi-analytic galaxy formation models on the past lightcone
in Monthly Notices of the Royal Astronomical Society
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
(2019)
Magnetogenesis at Cosmic Dawn: tracing the origins of cosmic magnetic fields
in Monthly Notices of the Royal Astronomical Society
Thomas N
(2019)
Black hole - Galaxy correlations in simba
in Monthly Notices of the Royal Astronomical Society
Wareing C
(2018)
A new mechanical stellar wind feedback model for the Rosette Nebula
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2022)
How gas flows shape the stellar-halo mass relation in the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Dillamore A
(2022)
Merger-induced galaxy transformations in the artemis simulations
in Monthly Notices of the Royal Astronomical Society
Brown S
(2022)
Towards a universal model for the density profiles of dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Yankelevich V
(2023)
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
in Monthly Notices of the Royal Astronomical Society
Vijayan A
(2022)
First Light And Reionisation Epoch Simulations (FLARES) - III. The properties of massive dusty galaxies at cosmic dawn
in Monthly Notices of the Royal Astronomical Society
Li N
(2021)
The impact of line-of-sight structures on measuring H 0 with strong lensing time delays
in Monthly Notices of the Royal Astronomical Society
Mateu C
(2017)
Predictions for the detection of tidal streams with Gaia using great-circle methods
in Monthly Notices of the Royal Astronomical Society
Barnes D
(2017)
The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
in Monthly Notices of the Royal Astronomical Society
Bose S
(2023)
The progenitor galaxies of stellar haloes as 'failed' Milky Ways
in Monthly Notices of the Royal Astronomical Society
Mastromarino C
(2023)
Properties and observables of massive galaxies in self-interacting dark matter cosmologies
in Monthly Notices of the Royal Astronomical Society
Teyssier R
(2020)
The loss of the intracluster medium in globular clusters
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
| 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 |