Roadmap for warm dense matter physics
Jan Vorberger, Frank Graziani, David Riley, Andrew D. Baczewski, Isabelle Baraffe, Mandy Bethkenhagen, Simon Blouin, Maximilian P. Böhme, Michael Bonitz, Michael Bussmann, Alexis Casner, Witold Cayzac, Peter Celliers, Gilles Chabrier, Nicolas Chamel, Dave Chapman, Mohan Chen, Jean Clérouin, Gilbert Collins, Federica Coppari, Tilo Döppner, Tobias Dornheim, Luke B. Fletcher, Dirk O. Gericke, Siegfried Glenzer, Alexander F. Goncharov, Gianluca Gregori, Sebastien Hamel, Stephanie B. Hansen, Nicholas J. Hartley, Suxing Hu, Omar A. Hurricane, Valentin V. Karasiev, Joshua J. Kas, Brendan Kettle, Thomas Kluge, Marcus D. Knudson, Alina Kononov, Zuzana Konôpkov á, Dominik Kraus, Andrea Kritcher, Sophia Malko, Gérard Massacrier, Burkhard Militzer, Zhandos A. Moldabekov, Michael S. Murillo, Bob Nagler, Nadine Nettelmann, Paul Neumayer, Benjamin K. Ofori-Okai, Ivan I. Oleynik, Martin Preising, Aurora Pribram-Jones, Tlekkabul Ramazanov, Alessandra Ravasio, Ronald Redmer, Baerbel Rethfeld, Alex P. L. Robinson, Gerd Röpke, François Soubiran, Charles E. Starrett, Gerd Steinle-Neumann, Phillip A. Sterne, Shigenori Tanaka, Aidan P. Thompson, Samuel B. Trickey, Tommaso Vinci, Sam M. Vinko, Lei Wang, Alexander J. White, Thomas G. White, Ulf Zastrau, Eva Zurek, Panagiotis Tolias
TL;DR
This Roadmap surveys warm dense matter (WDM) across theory, computation, and experiment, highlighting how strongly coupled, partially degenerate electrons coexisting with ions demand multi-scale, multi-physics modeling. It organizes advances into 26 sections that cover ab initio methods (PIMC, DFT/TD-DFT, Green's functions, and many-body response), experimental generation/diagnostics (DACs, laser heating, shocks, and beams), system-specific physics (hydrogen, H–He mixtures, ices, rocks, dwarfs/NS crusts), applied contexts (ICF, novel materials), and enabling tools (ML, databases, open-source software, and future facilities). A central theme is the synergy between exact or near-exact quantum methods (PIMC, GF, TD-DFT) and efficient, scalable models (AA/CM, OF-DFT, MLIPs) to predict EOS, transport, and opacities, validated by XRTS and other diagnostics. The roadmap emphasizes data-driven infrastructure, uncertainty quantification, and the development of finite-$T$ XC functionals/kernels to improve predictive capability, with a forward-looking view toward next-generation facilities and quantum-enabled computing. The work aims to deliver integrated, multi-scale predictions that inform planetary interiors, ICF, and material synthesis under extreme conditions, ultimately accelerating discovery and practical applications in WDM science.
Abstract
This roadmap presents the state-of-the-art, current challenges and near future developments anticipated in the thriving field of warm dense matter physics. Originating from strongly coupled plasma physics, high pressure physics and high energy density science, the warm dense matter physics community has recently taken a giant leap forward. This is due to spectacular developments in laser technology, diagnostic capabilities, and computer simulation techniques. Only in the last decade has it become possible to perform accurate enough simulations \& experiments to truly verify theoretical results as well as to reliably design experiments based on predictions. Consequently, this roadmap discusses recent developments and contemporary challenges that are faced by theoretical methods, and experimental techniques needed to create and diagnose warm dense matter. A large part of this roadmap is dedicated to specific warm dense matter systems and applications in astrophysics, inertial confinement fusion and novel material synthesis.
