The data-driven future of high energy density physics

Nature Springer Nature 593 (2021) 351-361

Authors:

Peter Hatfield, Jim Gaffney, Gemma Anderson, Suzanne Ali, Luca Antonelli, Suzan Başeğmez du Pree, Jonathan Citrin, Marta Fajardo, Patrick Knapp, Brendan Kettle, Bogdan Kustowski, Michael MacDonald, Derek Mariscal, Madison Martin, Taisuke Nagayama, Charlotte Palmer, Jl Peterson, Steven Rose, Jj Ruby, Carl Shneider, Matt Streeter, Will Trickey, Ben Williams

Abstract:

High-energy-density physics is the field of physics concerned with studying matter at extremely high temperatures and densities. Such conditions produce highly nonlinear plasmas, in which several phenomena that can normally be treated independently of one another become strongly coupled. The study of these plasmas is important for our understanding of astrophysics, nuclear fusion and fundamental physics—however, the nonlinearities and strong couplings present in these extreme physical systems makes them very difficult to understand theoretically or to optimize experimentally. Here we argue that machine learning models and data-driven methods are in the process of reshaping our exploration of these extreme systems that have hitherto proved far too nonlinear for human researchers. From a fundamental perspective, our understanding can be improved by the way in which machine learning models can rapidly discover complex interactions in large datasets. From a practical point of view, the newest generation of extreme physics facilities can perform experiments multiple times a second (as opposed to approximately daily), thus moving away from human-based control towards automatic control based on real-time interpretation of diagnostic data and updates of the physics model. To make the most of these emerging opportunities, we suggest proposals for the community in terms of research design, training, best practice and support for synthetic diagnostics and data analysis.

The SAMI Galaxy Survey: stellar population and structural trends across the Fundamental Plane

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 504:4 (2021) 5098-5130

Authors:

Francesco D’Eugenio, Matthew Colless, Nicholas Scott, Arjen van der Wel, Roger L Davies, Jesse van de Sande, Sarah M Sweet, Sree Oh, Brent Groves, Rob Sharp, Matt S Owers, Joss Bland-Hawthorn, Scott M Croom, Sarah Brough, Julia J Bryant, Michael Goodwin, Jon S Lawrence, Nuria PF Lorente, Samuel N Richards

The double-peaked Type Ic supernova 2019cad: another SN 2005bf-like object

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 504:4 (2021) 4907-4922

Authors:

CP Gutiérrez, MC Bersten, M Orellana, A Pastorello, K Ertini, G Folatelli, G Pignata, JP Anderson, S Smartt, M Sullivan, M Pursiainen, C Inserra, N Elias-Rosa, M Fraser, E Kankare, S Moran, A Reguitti, TM Reynolds, M Stritzinger, J Burke, C Frohmaier, L Galbany, D Hiramatsu, DA Howell, H Kuncarayakti, S Mattila, T Müller-Bravo, C Pellegrino, M Smith

Probabilistic Reconstruction of Type Ia Supernova SN 2002bo

(2021)

Authors:

John T O'Brien, Wolfgang E Kerzendorf, Andrew Fullard, Marc Williamson, Ruediger Pakmor, Johannes Buchner, Stephan Hachinger, Christian Vogl, James H Gillanders, Andreas Floers, Patrick van der Smagt

The hybrid radio/X-ray correlation of the black hole transient MAXI J1348-630

(2021)

Authors:

F Carotenuto, S Corbel, E Tremou, TD Russell, A Tzioumis, RP Fender, PA Woudt, SE Motta, JCA Miller-Jones, AJ Tetarenko, GR Sivakoff