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
Hamilton E
(2023)
Ringdown frequencies in black holes formed from precessing black-hole binaries
in Physical Review D
Regan J
(2018)
Rise of the first supermassive stars
in Monthly Notices of the Royal Astronomical Society
Semenov M
(2021)
Rovibronic spectroscopy of PN from first principles.
in Physical chemistry chemical physics : PCCP
Olsen K
(2021)
sígame v3: Gas Fragmentation in Postprocessing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
in The Astrophysical Journal
Santos-Santos I
(2022)
Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
in Monthly Notices of the Royal Astronomical Society
Karunakaran A
(2021)
Satellites around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations versus Simulations
in The Astrophysical Journal Letters
Drach V
(2021)
Scattering of Goldstone bosons and resonance production in a composite Higgs model on the lattice
in Journal of High Energy Physics
Mukherjee S
(2018)
SEAGLE - I. A pipeline for simulating and modelling strong lenses from cosmological hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Mukherjee S
(2021)
SEAGLE - II. Constraints on feedback models in galaxy formation from massive early-type strong-lens galaxies
in Monthly Notices of the Royal Astronomical Society
Braspenning J
(2023)
Sensitivity of non-radiative cloud-wind interactions to the hydrodynamic solver
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2021)
Setting the stage: structures from Gaussian random fields
in Monthly Notices of the Royal Astronomical Society
Decataldo D
(2020)
Shaping the structure of a GMC with radiation and winds
in Monthly Notices of the Royal Astronomical Society
Davé R
(2019)
simba: Cosmological simulations with black hole growth and feedback
in Monthly Notices of the Royal Astronomical Society
Sorini D
(2020)
simba: the average properties of the circumgalactic medium of 2 = z = 3 quasars are determined primarily by stellar feedback
in Monthly Notices of the Royal Astronomical Society
Arnold C
(2019)
Simulating galaxy formation in f(R) modified gravity: matter, halo, and galaxy statistics
in Monthly Notices of the Royal Astronomical Society
Yardley S
(2021)
Simulating the Coronal Evolution of Bipolar Active Regions to Investigate the Formation of Flux Ropes
in Solar Physics
Chaikin E
(2022)
Simulations of 60Fe entrained in ejecta from a near-Earth supernova: effects of observer motion
in Monthly Notices of the Royal Astronomical Society
Tress R
(2020)
Simulations of the Milky Way's central molecular zone - I. Gas dynamics
in Monthly Notices of the Royal Astronomical Society
Sormani M
(2020)
Simulations of the Milky Way's Central Molecular Zone - II. Star formation
in Monthly Notices of the Royal Astronomical Society
Tress R
(2020)
Simulations of the star-forming molecular gas in an interacting M51-like galaxy
in Monthly Notices of the Royal Astronomical Society
Chan T
(2021)
Smoothed particle radiation hydrodynamics: two-moment method with local Eddington tensor closure
in Monthly Notices of the Royal Astronomical Society
Smith A
(2022)
Solving small-scale clustering problems in approximate light-cone mocks
in Monthly Notices of the Royal Astronomical Society
Brady S
(2023)
Solving the initial conditions problem for modified gravity theories
in Physical Review D
Salcido J
(2023)
SP(k) - a hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
in Monthly Notices of the Royal Astronomical Society
Huško F
(2022)
Spin-driven jet feedback in idealized simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Wang D
(2023)
Star formation concentration as a tracer of environmental quenching in action: a study of the eagle and c-eagle simulations
in Monthly Notices of the Royal Astronomical Society
Upadhyay A
(2021)
Star formation histories of Coma cluster galaxies matched to simulated orbits hint at quenching around first pericenter
in Astronomy & Astrophysics
Norman S
(2021)
Stars Crushed by Black Holes. I. On the Energy Distribution of Stellar Debris in Tidal Disruption Events
in The Astrophysical Journal
Kordov Z
(2021)
State mixing and masses of the p 0 , ? and ? ' mesons from n f = 1 + 1 + 1 lattice QCD + QED
in Physical Review D
Buividovich P
(2021)
Static magnetic susceptibility in finite-density $$SU\left( 2\right) $$ lattice gauge theory
in The European Physical Journal A
Huško F
(2022)
Statistics of galaxy mergers: bridging the gap between theory and observation
in Monthly Notices of the Royal Astronomical Society
Gunawardhana M
(2020)
Stellar populations and physical properties of starbursts in the antennae galaxy from self-consistent modelling of MUSE spectra
in Monthly Notices of the Royal Astronomical Society
Deason A
(2021)
Stellar splashback: the edge of the intracluster light
in Monthly Notices of the Royal Astronomical Society
Bahé Y
(2021)
Strongly lensed cluster substructures are not in tension with ?CDM
in Monthly Notices of the Royal Astronomical Society
Errani R
(2022)
Structure and kinematics of tidally limited satellite galaxies in LCDM
in Monthly Notices of the Royal Astronomical Society
Cao K
(2021)
Studying galaxy cluster morphological metrics with mock-X
in Monthly Notices of the Royal Astronomical Society
Peters A
(2018)
Supercluster simulations: impact of baryons on the matter power spectrum and weak lensing forecasts for Super-CLASS
in Monthly Notices of the Royal Astronomical Society
Habouzit M
(2021)
Supermassive black holes in cosmological simulations I: M BH - M ? relation and black hole mass function
in Monthly Notices of the Royal Astronomical Society
Smith M
(2018)
Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
in Monthly Notices of the Royal Astronomical Society
Müller B
(2017)
Supernova simulations from a 3D progenitor model - Impact of perturbations and evolution of explosion properties
in Monthly Notices of the Royal Astronomical Society
Wang Z
(2022)
Superradiance in massive vector fields with spatially varying mass
in Physical Review D
Stafford S
(2021)
Testing extensions to ?CDM on small scales with forthcoming cosmic shear surveys
in Monthly Notices of the Royal Astronomical Society
Hassan S
(2020)
Testing galaxy formation simulations with damped Lyman-a abundance and metallicity evolution
in Monthly Notices of the Royal Astronomical Society
Armijo J
(2018)
Testing modified gravity using a marked correlation function
in Monthly Notices of the Royal Astronomical Society
Tramonte D
(2017)
Testing the conditional mass function of dark matter haloes against numerical N-body simulations
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
Oman K
(2017)
The "Building Blocks" of Stellar Halos
in Galaxies
Wijers N
(2019)
The abundance and physical properties of O vii and O viii X-ray absorption systems in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Monaco P
(2020)
The accuracy of weak lensing simulations
in Monthly Notices of the Royal Astronomical Society
Font A
(2020)
The artemis simulations: stellar haloes of Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
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| Exploitation Route | See Dirac annual report https://dirac.ac.uk |
| Sectors | Digital/Communication/Information Technologies (including Software),Education |
| URL | https://dirac.ac.uk |