Creation and characterization of warm dense matter isochorically heated by an intense laser-driven proton beam to temperatures exceeding 100 eV

The warm dense matter (WDM) is an exotic state of matter encountered in inertial confinement implosions for fusion energy, as well as the interiors of giant planets like Jupiter, brown dwarfs, the atmospheres of white dwarfs, neutron star crusts, and newly discovered exo-planets. One efficient way to create WDM is to use protons accelerated by a high-intensity short-pulse laser to isochorically heat dense samples to WDM states. Despite its importance, direct temperature measurements within WDM targets are scarce. This study utilizes an intense proton beam generated by the kilojoule EP laser further focused and guided by a curved foil and cone structure to efficiently heat a thin copper sample. A high-resolution streaked spectrometer tuned to copper K_α fluorescence lines provided bulk temperature measurements every ~2 ps, revealing temperatures exceeding 100 eV in under 50 ps. Particle-in-cell simulations of proton transport and energy deposition closely matched the observed heating dynamics, including transverse temperature gradients revealed by the broadening of K_α lines.. Authors: Bailly-Grandvaux, M. [University of California, San Diego, CA (United States)] (ORCID:0000000175294013); Bolaños, S. [University of California, San Diego, CA (United States)]; Kim, J. [University of California, San Diego, CA (United States)] (ORCID:0000000161963044); Saret, J. [University of California, San Diego, CA (United States)]; McGuffey, C. [General Atomics, San Diego, CA (United States)] (ORCID:000000028162192X). DOE Contract: 89233124CNA000365; NA0003842; NA0004144. Subjects: 70 PLASMA PHYSICS AND FUSION TECHNOLOGY; Astrophysical plasmas; Characterization and analytical techniques; Laser-produced plasmas