Home > Publications database > Decreasing ultrafast X-ray pulse durations with saturable absorption and resonant transitions > print |
001 | 490197 | ||
005 | 20250715173520.0 | ||
024 | 7 | _ | |a 10.1103/PhysRevE.107.015205 |2 doi |
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100 | 1 | _ | |a Cardoch, Sebastian |0 P:(DE-H253)PIP1096981 |b 0 |e Corresponding author |
245 | _ | _ | |a Decreasing ultrafast X-ray pulse durations with saturable absorption and resonant transitions |
260 | _ | _ | |a Woodbury, NY |c 2023 |b Inst. |
336 | 7 | _ | |a article |2 DRIVER |
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520 | _ | _ | |a Saturable absorption is a nonlinear effect where a material’s ability to absorb light is frustrated due to a high influx of photons and the creation of electron vacancies. Experimentally induced saturable absorption in copper revealed a reduction in the temporal duration of transmitted X-ray laser pulses, but a detailed account of changes in opacity and emergence of resonances is still missing. In this computational work, we employ non-local thermodynamic equilibrium plasma simulations to study the interaction of femtosecond X-rays and copper. Following the onset of frustrated absorption, we find that a K–M resonant transition occurring at highly charged states turns copper opaque again. The changes in absorption generate a transient transparent window responsible for the shortened transmission signal. We also propose using fluorescence induced by the incident beam as an alternative source to achieve shorter X-ray pulses. Intense femtosecond X-rays are valuable to probe the structure and dynamics of biological samples or to reach extreme states of matter. Shortened pulses could be relevant for emerging imaging techniques. |
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700 | 1 | _ | |a Trost, Fabian |0 P:(DE-H253)PIP1082226 |b 1 |
700 | 1 | _ | |a Scott, Howard |0 P:(DE-H253)PIP1085046 |b 2 |
700 | 1 | _ | |a Chapman, Henry N. |0 P:(DE-H253)PIP1006324 |b 3 |
700 | 1 | _ | |a Caleman, Carl |0 P:(DE-H253)PIP1011740 |b 4 |
700 | 1 | _ | |a Timneanu, Nicusor |0 P:(DE-H253)PIP1008264 |b 5 |e Corresponding author |
773 | _ | _ | |a 10.1103/PhysRevE.107.015205 |g Vol. 107, no. 1, p. 015205 |0 PERI:(DE-600)2844562-4 |n 1 |p 015205 |t Physical review / E |v 107 |y 2023 |x 2470-0045 |
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