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
Arnold C
(2019)
Simulating galaxy formation in f(R) modified gravity: matter, halo, and galaxy statistics
in Monthly Notices of the Royal Astronomical Society
Arthuis P
(2023)
Quantum Monte Carlo calculations in configuration space with three-nucleon forces
in Physical Review C
Ashworth G
(2017)
Exploring the IMF of star clusters: a joint SLUG and LEGUS effort
in Monthly Notices of the Royal Astronomical Society
Ashworth G
(2018)
Theoretical predictions for IMF diagnostics in UV spectroscopy of star clusters
in Monthly Notices of the Royal Astronomical Society
Asquith R
(2018)
Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
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
Aumer M
(2017)
Migration and kinematics in growing disc galaxies with thin and thick discs
in Monthly Notices of the Royal Astronomical Society
Aumer M
(2017)
The structural evolution of galaxies with both thin and thick discs
in Monthly Notices of the Royal Astronomical Society
Aurrekoetxea J
(2023)
Oscillon formation during inflationary preheating with general relativity
in Physical Review D
Aurrekoetxea J
(2023)
Oscillon formation during inflationary preheating with general relativity
Aurrekoetxea J
(2023)
GRDzhadzha: A code for evolving relativistic matter on analytic metric backgrounds
Aylett-Bullock J
(2021)
Operational response simulation tool for epidemics within refugee and IDP settlements: A scenario-based case study of the Cox's Bazar settlement.
in PLoS computational biology
Aylett-Bullock J
(2021)
June: open-source individual-based epidemiology simulation.
in Royal Society open science
Badger S
(2023)
Isolated photon production in association with a jet pair through next-to-next-to-leading order in QCD
in Journal of High Energy Physics
Bahé Y
(2021)
Strongly lensed cluster substructures are not in tension with ?CDM
in Monthly Notices of the Royal Astronomical Society
Ballard D
(2024)
Gravitational imaging through a triple source plane lens: revisiting the ?CDM-defying dark subhalo in SDSSJ0946+1006
in Monthly Notices of the Royal Astronomical Society
Bamber J
(2021)
Growth of accretion driven scalar hair around Kerr black holes
in Physical Review D
Bamber J
(2021)
Quasinormal modes of growing dirty black holes
in Physical Review D
Bamber J
(2022)
Black hole merger simulations in wave dark matter environments
Bantilan H
(2021)
Cauchy evolution of asymptotically global AdS spacetimes with no symmetries
in Physical Review D
Bantilan H
(2020)
Real-Time Dynamics of Plasma Balls from Holography.
in Physical review letters
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
Barber C
(2018)
Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
in Monthly Notices of the Royal Astronomical Society
Barmentloo S
(2022)
Determining Satellite Infall Times Using Machine Learning
Barmentloo S
(2023)
Determining satellite infall times using machine learning
in Monthly Notices of the Royal Astronomical Society
Barnes D
(2020)
Characterizing hydrostatic mass bias with Mock-X
Barnes D
(2017)
The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
in Monthly Notices of the Royal Astronomical Society
Barnes D
(2021)
Characterizing hydrostatic mass bias with mock-X
in Monthly Notices of the Royal Astronomical Society
Barnes L
(2018)
Galaxy formation efficiency and the multiverse explanation of the cosmological constant with EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Barone A
(2023)
Approaches to inclusive semileptonic B(s)-meson decays from Lattice QCD
in Journal of High Energy Physics
Barrera M
(2023)
The MillenniumTNG Project: semi-analytic galaxy formation models on the past lightcone
in Monthly Notices of the Royal Astronomical Society
Barrera-Hinojosa C
(2020)
GRAMSES: a new route to general relativistic N -body simulations in cosmology. Part II. Initial conditions
in Journal of Cosmology and Astroparticle Physics
Barrera-Hinojosa C
(2020)
GRAMSES: a new route to general relativistic N -body simulations in cosmology. Part I. Methodology and code description
in Journal of Cosmology and Astroparticle Physics
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
Bartlett D
(2023)
Marginalised Normal Regression: Unbiased curve fitting in the presence of x-errors
in The Open Journal of Astrophysics
Bartlett D
(2024)
Exhaustive Symbolic Regression
in IEEE Transactions on Evolutionary Computation
Bate M
(2023)
The statistical properties of stars at redshift, z = 5, compared with the present epoch
in Monthly Notices of the Royal Astronomical Society
Batelaan M
(2023)
Moments and power corrections of longitudinal and transverse proton structure functions from lattice QCD
in Physical Review D
Batelaan M
(2023)
Feynman-Hellmann approach to transition matrix elements and quasidegenerate energy states
in Physical Review D
Baugh C
(2021)
Modelling emission lines in star forming galaxies
Baugh C
(2019)
Linear bias forecasts for emission line cosmological surveys
in Monthly Notices of the Royal Astronomical Society
Baxter E
(2021)
The correlation of high-redshift galaxies with the thermal Sunyaev-Zel'dovich effect traces reionization
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 |