TY - JOUR
T1 - Efficiency-optimized relativistic plasma harmonics for extreme fields
AU - Timmis, Robin J.L.
AU - Fitzpatrick, Colm R.J.
AU - Kennedy, Jonathan P.
AU - Huddleston, Holly M.
AU - Denis, Elliott
AU - James, Abigail
AU - Baird, Chris
AU - Symes, Dan
AU - McGonegle, David
AU - Atonga, Eduard
AU - Martin, Heath
AU - Rebenstock, Jeremy
AU - Neely, John
AU - Lee, Jordan
AU - Redfern, Joshua
AU - Bourgeois, Nicolas
AU - Finlay, Oliver
AU - Ruskov, Rusko
AU - Astbury, Sam
AU - Hawkes, Steve
AU - Zhang, Zixin
AU - Zepf, Matt
AU - Krushelnick, Karl
AU - Gumbrell, Edward
AU - Rajeev, Paramel Pattathil
AU - Yeung, Mark
AU - Dromey, Brendan
AU - Norreys, Peter
PY - 2026/4/22
Y1 - 2026/4/22
N2 - Bright harmonic radiation from relativistically oscillating laser plasmas offers a direct route for generating extreme electromagnetic fields. Theory predicts that under optimized conditions, the plasma medium can support strong spatiotemporal compression of laser energy in a coherent harmonic focus (CHF), delivering intensity boosts many orders of magnitude greater than the incident driving laser pulse1, 2, 3–4. Although diffraction-limited performance5 (spatial compression) and attosecond phase locking6, 7–8 (temporal compression) have been demonstrated experimentally, efficient coupling of relativistically intense laser pulse energy into the emitted harmonic cone has not been realized so far. Here we demonstrate that this highly nonlinear interaction can be tailored to deliver the maximum conversion efficiencies predicted from simulations. By fine-tuning the temporal profile of the driving laser on sub-picosecond (<10−12 s) timescales, energies >9 mJ between the 12th and 47th harmonics are observed. These results are in agreement with the theoretically expected efficiency dependence on harmonic order, verifying that optimal conditions have been achieved in the generation process. This is the important final element required to achieve the expected intensity boosts from a CHF in experiments. Although obtaining spatiotemporal compression and optimal efficiency simultaneously remains challenging, the path to realizing extreme optical field strengths approaching the critical field of quantum electrodynamics (the Schwinger limit at >1016 V cm−1 or >1029 W cm−2) is now open, permitting all-optical studies of the quantum vacuum and new frontiers for intense attosecond science.
AB - Bright harmonic radiation from relativistically oscillating laser plasmas offers a direct route for generating extreme electromagnetic fields. Theory predicts that under optimized conditions, the plasma medium can support strong spatiotemporal compression of laser energy in a coherent harmonic focus (CHF), delivering intensity boosts many orders of magnitude greater than the incident driving laser pulse1, 2, 3–4. Although diffraction-limited performance5 (spatial compression) and attosecond phase locking6, 7–8 (temporal compression) have been demonstrated experimentally, efficient coupling of relativistically intense laser pulse energy into the emitted harmonic cone has not been realized so far. Here we demonstrate that this highly nonlinear interaction can be tailored to deliver the maximum conversion efficiencies predicted from simulations. By fine-tuning the temporal profile of the driving laser on sub-picosecond (<10−12 s) timescales, energies >9 mJ between the 12th and 47th harmonics are observed. These results are in agreement with the theoretically expected efficiency dependence on harmonic order, verifying that optimal conditions have been achieved in the generation process. This is the important final element required to achieve the expected intensity boosts from a CHF in experiments. Although obtaining spatiotemporal compression and optimal efficiency simultaneously remains challenging, the path to realizing extreme optical field strengths approaching the critical field of quantum electrodynamics (the Schwinger limit at >1016 V cm−1 or >1029 W cm−2) is now open, permitting all-optical studies of the quantum vacuum and new frontiers for intense attosecond science.
U2 - 10.1038/s41586-026-10400-2
DO - 10.1038/s41586-026-10400-2
M3 - Article
C2 - 42020740
AN - SCOPUS:105037062366
SN - 0028-0836
VL - 652
SP - 1153
EP - 1158
JO - Nature
JF - Nature
ER -