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
Glowacki M
(2020)
The baryonic Tully-Fisher relation in the Simba simulation
Glasscock K
(2024)
Statistical estimation of full-sky radio maps from 21 cm array visibility data using Gaussian constrained realizations
in RAS Techniques and Instruments
Givans J
(2022)
Non-linearities in the Lyman-a forest and in its cross-correlation with dark matter halos
in Journal of Cosmology and Astroparticle Physics
Ghosh S
(2024)
First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence
in Physical Review D
Georgy C
(2024)
3D simulations of a neon burning convective shell in a massive star
in Monthly Notices of the Royal Astronomical Society
Genina A
(2018)
The core-cusp problem: a matter of perspective
in Monthly Notices of the Royal Astronomical Society
Gayer L
(2025)
Highly excited B, Bs and Bc meson spectroscopy from lattice QCD
in Journal of High Energy Physics
Gavardi A
(2023)
NNLO+PS W+W- production using jet veto resummation at NNLL'
in Journal of High Energy Physics
Garzilli A
(2021)
How to constrain warm dark matter with the Lyman-a forest
in Monthly Notices of the Royal Astronomical Society
Garver B
(2023)
Exploring the Evolution of Massive Clumps in Simulations That Reproduce the Observed Milky Way a-element Abundance Bimodality
in The Astrophysical Journal
Garron N
(2023)
Nonperturbative renormalization with interpolating momentum schemes
in Physical Review D
Garg P
(2022)
The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High Redshift
in The Astrophysical Journal
Garg P
(2024)
Theoretical Strong-line Metallicity Diagnostics for the JWST Era
in The Astrophysical Journal
Ganeshaiah Veena P
(2021)
Cosmic Ballet III: Halo spin evolution in the cosmic web
in Monthly Notices of the Royal Astronomical Society
Ganeshaiah Veena P
(2019)
The Cosmic Ballet II: spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Ganeshaiah Veena P
(2021)
Cosmic Ballet III: Halo spin evolution in the cosmic web
in Monthly Notices of the Royal Astronomical Society
Galbiati M
(2024)
MUSE Analysis of Gas around Galaxies (MAGG) VI. The cool and enriched gas environment of z ? 3 Ly a emitters
in Astronomy & Astrophysics
Gaire B
(2024)
Maintaining spherical polarization in solar wind plasma
in Nature Astronomy
Gaikwad P
(2020)
Probing the thermal state of the intergalactic medium at z > 5 with the transmission spikes in high-resolution Ly a forest spectra
in Monthly Notices of the Royal Astronomical Society
Gaikwad P
(2021)
A consistent and robust measurement of the thermal state of the IGM at 2 = z = 4 from a large sample of Ly a forest spectra: evidence for late and rapid He ii reionization
in Monthly Notices of the Royal Astronomical Society
Gaikwad P
(2023)
Measuring the photoionization rate, neutral fraction, and mean free path of H i ionizing photons at 4.9 = z = 6.0 from a large sample of XShooter and ESI spectra
in Monthly Notices of the Royal Astronomical Society
Gaikwad P
(2021)
A consistent and robust measurement of the thermal state of the IGM at 2 = z = 4 from a large sample of Ly a forest spectra: evidence for late and rapid He ii 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 |
