• Matter and Radiation at Extremes
  • Vol. 10, Issue 2, 027201 (2025)
X. Li1,* and F. B. Rosmej2,3
Author Affiliations
  • 1Key Laboratory of Ultra-Intense Laser Science and Technology, Shanghai Institute of Optics and Fine Mechanics (SIOM), Chinese Academy of Sciences (CAS), Shanghai 201800, China
  • 2Sorbonne University, Faculty of Science and Engineering, UMR 7605, case128, 4 Place Jussieu, F-75252 Paris Cedex 05, France
  • 3LULI, Ecole Polytechnique, Laboratoire pour l’Utilisation des Lasers Intenses, Physique Atomique dans les Plasmas Denses, F-91128 Palaiseau, France
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    DOI: 10.1063/5.0235418 Cite this Article
    X. Li, F. B. Rosmej. X-ray transition and K-edge energies in dense finite-temperature plasmas: Challenges of a generalized approach with spectroscopic precision[J]. Matter and Radiation at Extremes, 2025, 10(2): 027201 Copy Citation Text show less
    Schematic illustration of valence-band-like features with bound and free states in the framework of an ion-sphere model (R is the radius of the ion sphere) coupled to atomic wave equations: (a) Case of Al I with 13 bound electrons; (b) case of Al II with 12 bound electrons and one free electron.
    Fig. 1. Schematic illustration of valence-band-like features with bound and free states in the framework of an ion-sphere model (R is the radius of the ion sphere) coupled to atomic wave equations: (a) Case of Al I with 13 bound electrons; (b) case of Al II with 12 bound electrons and one free electron.
    Schematic illustration of core-hole vacancies production in the framework of the VB-BFC valence band model. Case (a) depicts Al I with 13 bound electrons corresponding to the excitation of a K-electron, while case (b) shows Al II with 12 bound electrons and one free electron corresponding to the ionization of a K-electron.
    Fig. 2. Schematic illustration of core-hole vacancies production in the framework of the VB-BFC valence band model. Case (a) depicts Al I with 13 bound electrons corresponding to the excitation of a K-electron, while case (b) shows Al II with 12 bound electrons and one free electron corresponding to the ionization of a K-electron.
    Heβ line-shift measurements of Cl15+ ions in dense laser-produced plasmas (open and solid circles) and comparison with the present generalized model (red crosses) for Te = 600 eV. Very good agreement between theory and experiment is observed, demonstrating the spectroscopic precision of the present generalized model, even in dense plasmas.
    Fig. 3. Heβ line-shift measurements of Cl15+ ions in dense laser-produced plasmas (open and solid circles) and comparison with the present generalized model (red crosses) for Te = 600 eV. Very good agreement between theory and experiment is observed, demonstrating the spectroscopic precision of the present generalized model, even in dense plasmas.
    Averaged radius of the 2p and 3p orbitals for different aluminum ionic states in solid-density Al plasma. The black dashed line is the average atomic size (or the radius of the ion sphere) calculated from the crystal constant of Al (0.404 nm, corresponding to 7.64a0).
    Fig. 4. Averaged radius of the 2p and 3p orbitals for different aluminum ionic states in solid-density Al plasma. The black dashed line is the average atomic size (or the radius of the ion sphere) calculated from the crystal constant of Al (0.404 nm, corresponding to 7.64a0).
    Distribution of photon absorption oscillator strengths with respect to excitation energy. The excitation energy is the XFEL photon energy to induce a 1s − 3p transition in channels 1–4 for aluminum with a Ne-like ion core. The labels 1–4 correspond to the production of nonresonance Kα radiation via the lowest-energy channels 1–4 listed in the text at the start of Sec. II D. The gray areas indicate the experimental uncertainty in measuring the XFEL photon energy corresponding to the appearance of the Kα lines. The label 5 corresponds to channel 5 of 1s ionization. The black and red vertical dashed lines show the 1s ionization energy of Ne-like Al in vacuum and in solid-density plasma, respectively. The plasma conditions used in the calculations with the present generalized model are Te = 100 eV, ni = 5.97 × 1022 cm−3, and ne = Nfni.
    Fig. 5. Distribution of photon absorption oscillator strengths with respect to excitation energy. The excitation energy is the XFEL photon energy to induce a 1s − 3p transition in channels 1–4 for aluminum with a Ne-like ion core. The labels 1–4 correspond to the production of nonresonance Kα radiation via the lowest-energy channels 1–4 listed in the text at the start of Sec. II D. The gray areas indicate the experimental uncertainty in measuring the XFEL photon energy corresponding to the appearance of the Kα lines. The label 5 corresponds to channel 5 of 1s ionization. The black and red vertical dashed lines show the 1s ionization energy of Ne-like Al in vacuum and in solid-density plasma, respectively. The plasma conditions used in the calculations with the present generalized model are Te = 100 eV, ni = 5.97 × 1022 cm−3, and ne = Nfni.
    Spontaneous transition probabilities of Kα transitions with respect to transition energies, where the labels 1–5 are the same as in Fig. 4. The gray areas indicate the experimentally recorded transition intervals where the Kα radiation intensity increases from zero to a nearly constant value.
    Fig. 6. Spontaneous transition probabilities of Kα transitions with respect to transition energies, where the labels 1–5 are the same as in Fig. 4. The gray areas indicate the experimentally recorded transition intervals where the Kα radiation intensity increases from zero to a nearly constant value.
    Comparison of 1s − 3p excitation energies and corresponding photon absorption oscillator strengths in the framework of the free-atom model (hollow circles) and the present model (solid circles). Simulations are performed for the Ne-like core in pure aluminum plasma at Te = 100 eV and ni = 5.97 × 1022 cm−3 (corresponding to a mass density of ρ = 2.7 g/cm3).
    Fig. 7. Comparison of 1s − 3p excitation energies and corresponding photon absorption oscillator strengths in the framework of the free-atom model (hollow circles) and the present model (solid circles). Simulations are performed for the Ne-like core in pure aluminum plasma at Te = 100 eV and ni = 5.97 × 1022 cm−3 (corresponding to a mass density of ρ = 2.7 g/cm3).
    Theoretical 1s − 3p excitation energies for the B-like core of aluminum using Maxwell–Boltzmann and Fermi–Dirac statistics for the free electrons. The plasma density is ni = 5.97 × 1022 cm−3, which corresponds to solid-density aluminum. The plasma temperatures are 10 and 100 eV. The excitation channel considered is (1s)2(2s)2(2p)13s23p3F3−(1s)1(2s)2(2p)13s23p4F3. The gray area is the experimental uncertainty interval. The red circles are the calculations in vacuum, the green circles show the calculations in the framework of the uniform electron gas model (UEGM), while the light blue circles/pink crosses and dark blue circles/red crosses are calculations from the present generalized model (GM) for 100 and 10 eV, respectively. The circles and crosses are calculated assuming Maxwell–Boltzmann (MB) and Fermi–Dirac (FD) statistics, respectively, for the free electrons.
    Fig. 8. Theoretical 1s − 3p excitation energies for the B-like core of aluminum using Maxwell–Boltzmann and Fermi–Dirac statistics for the free electrons. The plasma density is ni = 5.97 × 1022 cm−3, which corresponds to solid-density aluminum. The plasma temperatures are 10 and 100 eV. The excitation channel considered is (1s)2(2s)2(2p)13s23p3F3(1s)1(2s)2(2p)13s23p4F3. The gray area is the experimental uncertainty interval. The red circles are the calculations in vacuum, the green circles show the calculations in the framework of the uniform electron gas model (UEGM), while the light blue circles/pink crosses and dark blue circles/red crosses are calculations from the present generalized model (GM) for 100 and 10 eV, respectively. The circles and crosses are calculated assuming Maxwell–Boltzmann (MB) and Fermi–Dirac (FD) statistics, respectively, for the free electrons.
    Comparison of experimental data (solid orange squares) with calculations (solid black circles) on IPD with the results of the present VB-BFC model for solid-density pure aluminum at ni = 5.97 × 1022 cm−3. The solid black circles are calculated for the real experimental temperatures Te related to different aluminum ions:41 8 eV for Al3+, 30 eV for Al4+, 42.5 eV for Al5+, 58 eV for Al6+, 72 eV for Al7+, 104 eV for Al8+, and 132 eV for Al9+. The long-dashed red line “EK-fit C = 1” is a fit to the data from Ref. 34, while the short-dashed red line is the result from the original Ecker–Kröll model18,19 for the respective plasma parameters. The short-dashed blue curve is the result from the Stewart–Pyatt model17 as given in Ref. 34.
    Fig. 9. Comparison of experimental data (solid orange squares) with calculations (solid black circles) on IPD with the results of the present VB-BFC model for solid-density pure aluminum at ni = 5.97 × 1022 cm−3. The solid black circles are calculated for the real experimental temperatures Te related to different aluminum ions:41 8 eV for Al3+, 30 eV for Al4+, 42.5 eV for Al5+, 58 eV for Al6+, 72 eV for Al7+, 104 eV for Al8+, and 132 eV for Al9+. The long-dashed red line “EK-fit C = 1” is a fit to the data from Ref. 34, while the short-dashed red line is the result from the original Ecker–Kröll model18,19 for the respective plasma parameters. The short-dashed blue curve is the result from the Stewart–Pyatt model17 as given in Ref. 34.
    The same as in Fig. 5, but for the 1s − 3p excitation energy of Ne-like Al in Al2O3 plasma and for the excitation channels 1–4 (open circles). The plasma conditions for Al2O3 are set as ni = 1.2 × 1023 cm−3 and Te = 100 eV. The 1s − 3p excitation energies in a pure solid-density Al plasma (ni = 5.97 × 1022 cm−3 and Te = 100 eV) are also included for comparison (solid circles). All the theoretical results are calculated with the present VB-BFC model.
    Fig. 10. The same as in Fig. 5, but for the 1s − 3p excitation energy of Ne-like Al in Al2O3 plasma and for the excitation channels 1–4 (open circles). The plasma conditions for Al2O3 are set as ni = 1.2 × 1023 cm−3 and Te = 100 eV. The 1s − 3p excitation energies in a pure solid-density Al plasma (ni = 5.97 × 1022 cm−3 and Te = 100 eV) are also included for comparison (solid circles). All the theoretical results are calculated with the present VB-BFC model.
    Comparison of IPD for different charge states (core states) of aluminum between experiment and the present theory for the solid-density compound Al2O3 (ni = 1.2 × 1023 cm−3). The plasma temperature used in the calculations is Te = 100 eV (solid green circles). The red-bar vertical line for the F-like core shows the theoretical range of IPD between (ni = 1.2 × 1023 cm−3, Te = 30 eV) and (ni = 1.2 × 1022 cm−3, Te = 100 eV). Also indicated in the figure are the results from the Ecker–Kröll model, where the lattice function Cne,Te,Z has been replaced by a simple fitting constant34 (curves designated with “EK-fit C = 1”).
    Fig. 11. Comparison of IPD for different charge states (core states) of aluminum between experiment and the present theory for the solid-density compound Al2O3 (ni = 1.2 × 1023 cm−3). The plasma temperature used in the calculations is Te = 100 eV (solid green circles). The red-bar vertical line for the F-like core shows the theoretical range of IPD between (ni = 1.2 × 1023 cm−3, Te = 30 eV) and (ni = 1.2 × 1022 cm−3, Te = 100 eV). Also indicated in the figure are the results from the Ecker–Kröll model, where the lattice function Cne,Te,Z has been replaced by a simple fitting constant34 (curves designated with “EK-fit C = 1”).
    The same as in Fig. 5, except that the 1s − 3p excitation channels with F-like core are considered in an Al2O3 plasma. Compound Al2O3: Te = 100 eV, ni = 1.2 × 1023 cm−3.
    Fig. 12. The same as in Fig. 5, except that the 1s − 3p excitation channels with F-like core are considered in an Al2O3 plasma. Compound Al2O3: Te = 100 eV, ni = 1.2 × 1023 cm−3.
    The same as in Fig. 5, except that the 1s − 3p excitation channels with F-like core are considered in an Al2O3 plasma. Compound Al2O3: Te = 30 eV, ni = 1.2 × 1023 cm−3.
    Fig. 13. The same as in Fig. 5, except that the 1s − 3p excitation channels with F-like core are considered in an Al2O3 plasma. Compound Al2O3: Te = 30 eV, ni = 1.2 × 1023 cm−3.
    The same as in Fig. 5 except that the 1s − 3p excitation channels with F-like core are considered in an Al2O3 plasma. Compound Al2O3: Te = 100 eV, ni = 1.2 × 1022 cm−3.
    Fig. 14. The same as in Fig. 5 except that the 1s − 3p excitation channels with F-like core are considered in an Al2O3 plasma. Compound Al2O3: Te = 100 eV, ni = 1.2 × 1022 cm−3.
    The same as in Fig. 5, except that the 1s − 3p excitation channels with F-like core are considered in an Al2O3 plasma. Compound Al2O3: Te = 30 eV, ni = 1.2 × 1022 cm−3.
    Fig. 15. The same as in Fig. 5, except that the 1s − 3p excitation channels with F-like core are considered in an Al2O3 plasma. Compound Al2O3: Te = 30 eV, ni = 1.2 × 1022 cm−3.
    TransitionReference 52Present GM
    Kedge (for Al I)1559.891559.4
    Kα (for Al II)1487.531488.0
    Kβ (for Al II)1557.571558.7
    Table 1. Comparison of energies (in units of eV) of Kedge, Kα, and Kβ transitions from reference data52 and the present generalized model (GM).
    TransitionNISTPresent GM
    W27.75737.7624
    Y27.80707.8125
    W36.63486.6395
    Y36.64476.6503
    Table 2. Comparison of wavelengths (in units of Å) of the He-like resonance and intercombination lines of aluminum obtained from the present generalized model (GM) with reference data from NIST.53
    X. Li, F. B. Rosmej. X-ray transition and K-edge energies in dense finite-temperature plasmas: Challenges of a generalized approach with spectroscopic precision[J]. Matter and Radiation at Extremes, 2025, 10(2): 027201
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