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.

Publications

10 25 50

publication icon
Ali A (2021) The growth of H ii regions around massive stars: the role of metallicity and dust in Monthly Notices of the Royal Astronomical Society

publication icon
Allanson O (2021) Electron Diffusion and Advection During Nonlinear Interactions With Whistler-Mode Waves in Journal of Geophysical Research: Space Physics

publication icon
Andrade T (2021) GRChombo: An adaptable numerical relativity code for fundamental physics in Journal of Open Source Software

publication icon
Appleby S (2020) The impact of quenching on galaxy profiles in the simba simulation in Monthly Notices of the Royal Astronomical Society

publication icon
Appleby S (2021) The low-redshift circumgalactic medium in simba in Monthly Notices of the Royal Astronomical Society

publication icon
Armijo J (2018) Testing modified gravity using a marked correlation function in Monthly Notices of the Royal Astronomical Society

publication icon
Armijo J (2022) Making use of sub-resolution haloes in N -body simulations in Monthly Notices of the Royal Astronomical Society: Letters

publication icon
Armitage T (2019) An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations in Monthly Notices of the Royal Astronomical Society

publication icon
Armitage T (2018) The Cluster-EAGLE project: velocity bias and the velocity dispersion-mass relation of cluster galaxies in Monthly Notices of the Royal Astronomical Society

publication icon
Ashworth G (2018) Theoretical predictions for IMF diagnostics in UV spectroscopy of star clusters in Monthly Notices of the Royal Astronomical Society

publication icon
Ashworth G (2017) Exploring the IMF of star clusters: a joint SLUG and LEGUS effort in Monthly Notices of the Royal Astronomical Society

publication icon
Aumer M (2017) Migration and kinematics in growing disc galaxies with thin and thick discs in Monthly Notices of the Royal Astronomical Society

publication icon
Aumer M (2017) The structural evolution of galaxies with both thin and thick discs in Monthly Notices of the Royal Astronomical Society

publication icon
Baes M (2019) The cosmic spectral energy distribution in the EAGLE simulation in Monthly Notices of the Royal Astronomical Society

publication icon
Bahé Y (2021) Strongly lensed cluster substructures are not in tension with ?CDM in Monthly Notices of the Royal Astronomical Society

publication icon
Bamber J (2021) Quasinormal modes of growing dirty black holes in Physical Review D

publication icon
Barnes D (2021) Characterizing hydrostatic mass bias with mock-X in Monthly Notices of the Royal Astronomical Society

publication icon
Barnes D (2017) The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies in Monthly Notices of the Royal Astronomical Society

publication icon
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

publication icon
Barrera-Hinojosa C (2022) Looking for a twist: probing the cosmological gravitomagnetic effect via weak lensing-kSZ cross-correlations in Monthly Notices of the Royal Astronomical Society

publication icon
Baugh C (2022) Modelling emission lines in star-forming galaxies in Monthly Notices of the Royal Astronomical Society

publication icon
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

publication icon
Beane S (2021) Charged multihadron systems in lattice QCD + QED in Physical Review D

publication icon
Becker G (2021) The mean free path of ionizing photons at 5 < z < 6: evidence for rapid evolution near reionization in Monthly Notices of the Royal Astronomical Society

publication icon
Beckett A (2021) The relationship between gas and galaxies at z  < 1 using the Q0107 quasar triplet in Monthly Notices of the Royal Astronomical Society

publication icon
Benitez-Llambay A (2021) The Tail of Late-forming Dwarf Galaxies in ?CDM in The Astrophysical Journal Letters

publication icon
Benitez-Llambay A (2020) The detailed structure and the onset of galaxy formation in low-mass gaseous dark matter haloes in Monthly Notices of the Royal Astronomical Society

publication icon
Bennett E (2021) Glueballs and strings in S p ( 2 N ) Yang-Mills theories in Physical Review D

publication icon
Bose B (2020) On the road to per cent accuracy IV: ReACT - computing the non-linear power spectrum beyond ?CDM in Monthly Notices of the Royal Astronomical Society

publication icon
Bourne M (2017) AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence in Monthly Notices of the Royal Astronomical Society

publication icon
Brown S (2020) Connecting the structure of dark matter haloes to the primordial power spectrum in Monthly Notices of the Royal Astronomical Society

publication icon
Brown S (2022) Towards a universal model for the density profiles of dark matter haloes in Monthly Notices of the Royal Astronomical Society

publication icon
Cai Y (2017) Gravitational redshift and asymmetric redshift-space distortions for stacked 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