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
Moews B
(2021)
Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Mocz P
(2023)
Cosmological structure formation and soliton phase transition in fuzzy dark matter with axion self-interactions
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2020)
Galactic inflow and wind recycling rates in the EAGLE simulations
Mitchell P
(2020)
Galactic outflow rates in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2020)
Galactic inflow and wind recycling rates in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2018)
Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2019)
Galactic outflow rates in the EAGLE simulations
Mitchell P
(2022)
How gas flows shape the stellar-halo mass relation in the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2022)
Baryonic mass budgets for haloes in the eagle simulation, including ejected and prevented gas
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
A general framework to test gravity using galaxy clusters IV: cluster and halo properties in DGP gravity
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
A general framework to test gravity using galaxy clusters - V. A self-consistent pipeline for unbiased constraints of f ( R ) gravity
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2022)
A general framework to test gravity using galaxy clusters - VI. Realistic galaxy formation simulations to study clusters in modified gravity
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
The impact of modified gravity on the Sunyaev-Zeldovich effect
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2019)
A general framework to test gravity using galaxy clusters II: A universal model for the halo concentration in f(R) gravity
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2020)
The impact of modified gravity on the Sunyaev-Zel'dovich effect
Mitchell M
(2021)
The impact of modified gravity on the Sunyaev-Zeldovich effect
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
A general framework to test gravity using galaxy clusters III: observable-mass scaling relations in f ( R ) gravity
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
A general framework for unbiased tests of gravity using galaxy clusters
Mills B
(2024)
Spectral Calculations of 3D Radiation Magnetohydrodynamic Simulations of Super-Eddington Accretion onto a Stellar-mass Black Hole
in The Astrophysical Journal
Meru F
(2019)
Is the ring inside or outside the planet?: the effect of planet migration on dust rings
in Monthly Notices of the Royal Astronomical Society
Merson A
(2019)
Linear bias forecasts for emission line cosmological surveys
Mercier W
(2024)
The COSMOS-Web ring: In-depth characterization of an Einstein ring lensing system at z ~ 2
in Astronomy & Astrophysics
Mellor T
(2021)
Artificial Symmetries for Calculating Vibrational Energies of Linear Molecules
in Symmetry
Mellor T
(2023)
MARVEL analysis of high-resolution spectra of thioformaldehyde (H 2 CS)
in Journal of Molecular Spectroscopy
McNally C
(2018)
Low-mass planet migration in magnetically torqued dead zones - II. Flow-locked and runaway migration, and a torque prescription
in Monthly Notices of the Royal Astronomical Society
McCarthy I
(2020)
The imprint of dark subhaloes on the circumgalactic medium
McCarthy I
(2023)
The FLAMINGO project: revisiting the S 8 tension and the role of baryonic physics
in Monthly Notices of the Royal Astronomical Society
McCarthy I
(2020)
The imprint of dark subhaloes on the circumgalactic medium
in Monthly Notices of the Royal Astronomical Society
McCarthy I
(2018)
The BAHAMAS project: the CMB-large-scale structure tension and the roles of massive neutrinos and galaxy formation
in Monthly Notices of the Royal Astronomical Society
McAlpine S
(2020)
Galaxy mergers in eagle do not induce a significant amount of black hole growth yet do increase the rate of luminous AGN
in Monthly Notices of the Royal Astronomical Society
McAlpine S
(2018)
The rapid growth phase of supermassive black holes
in Monthly Notices of the Royal Astronomical Society
Mayes R
(2021)
Testing the tidal stripping scenario of ultracompact dwarf galaxy formation by using internal properties
in Monthly Notices of the Royal Astronomical Society
Mayes R
(2021)
Contribution of stripped nuclei to the ultracompact dwarf galaxy population in the Virgo cluster
in Monthly Notices of the Royal Astronomical Society
Mayes R
(2024)
The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Mayes R
(2024)
The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Maunder T
(2024)
Synthetic light curves and spectra from a self-consistent 2D simulation of an ultra-strippped supernova
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 |