DiRAC: Memory Intensive 2.5y

Lead Research Organisation: Durham University
Department Name: Physics

Abstract

Physicists across the astronomy, nuclear and particle physics communities are focussed on understanding how the Universe works at a very fundamental level. The distance scales with which they work vary by 50 orders of magnitude from the smallest distances probed by experiments at the Large Hadron Collider, deep within the atomic nucleus, to the largest scale galaxy clusters discovered out in space. The Science challenges, however, are linked through questions such as: How did the Universe begin and how is it evolving? and What are the fundamental constituents and fabric of the Universe and how do they interact?

Progress requires new astronomical observations and experimental data but also new theoretical insights. Theoretical understanding comes increasingly from large-scale computations that allow us to confront the consequences of our theories very accurately with the data or allow us to interrogate the data in detail to extract information that has impact on our theories. These computations test the fastest computers that we have and push the boundaries of technology in this sector. They also provide an excellent environment for training students in state-of-the-art techniques for code optimisation and data mining and visualisation.

The DiRAC2 HPC facility has been operating since 2012, providing computing resources for theoretical research in all areas of particle physics, astronomy, cosmology and nuclear physics supported by STFC. It is a highly productive facility, generating 200-250 papers annually in international, peer-reviewed journals. However, the DiRAC facility risks becoming uncompetitive as it has remained static in terms of overall capability since 2012. The DiRAC-2.5x investment in 2017/18 mitigated the risk of hardware failures, by replacing our oldest hardware components. However, as the factor 5 oversubscription of the most recent RAC call demonstrated, the science programme in 2019/20 and beyond requires a significant uplift in DiRAC's compute capability. The main purpose of the requested funding for the DiRAC2.5y project is to provide a factor 2 increase in computing across all DiRAC services to enable the facility to remain competitive during 2019/20 in anticipation of future funding for DiRAC-3.

DiRAC2.5y builds on the success of the DiRAC HPC facility and will provide the resources needed to support cutting-edge research during 2019 in all areas of science supported by STFC. While the funding is required to remain competitive, the science programme will continue to be world-leading. Examples of the projects which will benefit from this investment include:

(i) lattice quantum chromodynamics (QCD) calculations of the properties of fundamental particles from first principles;

(ii) improving the potential of experiments at CERN's Large Hadron Collider for discovery of new physics by increasing the accuracy of theoretical predictions for rare processes involving the fundamental constituents of matter known as quarks;

(iii) simulations of the merger of pairs of black holes and which generate gravitational waves such as those recently discovered by the LIGO consortium;

(iv) the most realistic simulations to date of the formation and evolution of galaxies in the Universe;

(v) the accretion of gas onto supermassive black holes, the most efficient means of extracting energy from matter and the engine which drives galaxy evolution; (vi) new models of our own Milky Way galaxy calibrated using new data from the European Space Agency's GAIA satellite; (vii) detailed simulations of the interior of the sun and of planetary interiors; (viii) the formation of stars in clusters - for the first time it will be possible to follow the formation of massive stars.

Planned Impact

The anticipated impact of the DiRAC2.5y HPC facility aligns closely with the recently published UK Industrial Strategy. As such, many of our key impacts will be driven by our engagements with industry. Each service provider for DiRAC2.5y has a local industrial strategy to deliver increased levels of industrial returns over the next three years. The "Pathways to impact" document which is attached to the lead (Leicester) proposal describes the overall industrial strategy for the DiRAC facility, including our strategic goals and key performance indicators.

Publications

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Glowacki M (2021) The redshift evolution of the baryonic Tully-Fisher relation in SIMBA in Monthly Notices of the Royal Astronomical Society

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Barrera M (2023) The MillenniumTNG Project: semi-analytic galaxy formation models on the past lightcone in Monthly Notices of the Royal Astronomical Society

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Richings A (2022) The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry in Monthly Notices of the Royal Astronomical Society

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Rodríguez Montero F (2019) Mergers, starbursts, and quenching in the simba simulation in Monthly Notices of the Royal Astronomical Society

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Robson D (2023) Redshift evolution of galaxy group X-ray properties in the Simba simulations in Monthly Notices of the Royal Astronomical Society

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

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Van Loon M (2021) Explaining the scatter in the galaxy mass-metallicity relation with gas flows in Monthly Notices of the Royal Astronomical Society

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Thomas N (2019) Black hole - Galaxy correlations in simba in Monthly Notices of the Royal Astronomical Society

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Evans T (2022) Observing EAGLE galaxies with JWST : predictions for Milky Way progenitors and their building blocks in Monthly Notices of the Royal Astronomical Society

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Borrow J (2020) Cosmological baryon transfer in the simba simulations in Monthly Notices of the Royal Astronomical Society

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Smith A (2022) Solving small-scale clustering problems in approximate light-cone mocks in Monthly Notices of the Royal Astronomical Society

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Monaco P (2020) The accuracy of weak lensing simulations in Monthly Notices of the Royal Astronomical Society

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Bahé Y (2022) The importance of black hole repositioning for galaxy formation simulations in Monthly Notices of the Royal Astronomical Society

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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

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Vidal J (2020) Efficiency of tidal dissipation in slowly rotating fully convective stars or planets in Monthly Notices of the Royal Astronomical Society

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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

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Glowacki M (2020) The baryonic Tully-Fisher relation in the simba simulation in Monthly Notices of the Royal Astronomical Society

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Hutt M (2022) The effect of local Universe constraints on halo abundance and clustering in Monthly Notices of the Royal Astronomical Society