HIGH-TEMPERATURE PLASMA CREATED BY EXTERNAL INTENSIVE X-RAY RADIATION

To use the hollow ion spectra for diagnosing of the plasma affected by strong X-ray radiation have been proposed recently in the papers by Vinko et al. (Reference Vinko, Ciricosta, Cho, Engelhorn, Chung, Brown, Burian, Chalupský, Falcone, Graves, Hájková, Higginbotham, Juha, Krzywinski, Lee, Messerschmidt, Murphy, Ping, Scherz, Schlotter, Toleikis, Turner, Vysin, Wang, Wu, Zastrau, Zhu, Lee, Heimann, Nagler and Wark2012) and Colgan et al. (Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013). It should be noted that the properties of such high energy density plasma are under increasing scrutiny in recent years due to their importance to our understanding of stellar interiors, the cores of giant planets (Chabrier, Reference Chabrier2009; Kalman, Reference Kalman2010), and the properties of hot plasma in inertial confinement fusion devices (Atzeni & Meyer-Ter-Vehn, Reference Atzeni and Meyer-Ter-Vehn2004). These high-energy density systems are relevant to study photoionized plasmas found in active galactic nuclei and X-ray binaries (Behar et al., Reference Behar, Sako and Kahn2001). With irradiation by X-rays, electrons in the inner-shells are ionized first, which creates atoms or ions with empty internal electron shells, i.e., hollow atoms or ions. Note that the powerful new X-ray sources, namely, free electron lasers, are now available and could provide laser intensities larger than 10¹⁷ W/cm² for creation in laboratory conditions of novel states of matter that also must show clear signatures of hollow ions formation.

Recently, it was shown that strong X-ray radiation can also be formed with long wavelength laser fields, if the laser intensity is sufficiently large and approaches the radiation dominant regime (Zhidkov et al., Reference Zhidkov, Koga, Sasaki and Uesaka2002). In this case, a high-intensity laser rapidly ionizes valence electrons from a thin target through field ionization (Zhidkov & Sasaki, Reference Zhidkov and Sasaki2000). Such electrons are accelerated in the strong electric field of the laser and can quickly reach very high energies (> 10 MeV) if the laser is sufficiently intense. During the interaction of an intense laser pulse with a thin foil some of these hot electrons oscillate through the foil (Nakamura et al., Reference Nakamura, Koga, Esirkepov, Kando, Korn and Bulanov2012; Antici et al., Reference Antici, Fuchs, D'humières, Lefebvre, Borghesi, Brambrink, Cecchetti, Gaillard, Romagnani, Sentoku, Toncian, Willi, Audebert and Pépin2007), due to reflection by the fields on each surface, known as refluxing. These electrons radiate X-rays via Thomson scattering of the incident and scattered laser light and via Bremsstrahlung through the strong plasma field at the foil surfaces. It was estimated by Colgan et al., (Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013) that both of such processes can produce X-rays in the few KeV range and at intensities of around 10¹⁹ W/cm², when conventional optical laser intensity exceed 10²⁰ W/cm². The proposed concept (see Fig. 2) was tested at the Vulcan Petawatt Laser Facility at Rutherford Appleton Laboratory. Details of the experiments are described by Colgan et al. (Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013). Note here that when in such experiments the maximum laser intensity of 3 × 10²⁰ W/cm² was achieved, laser pulse duration was 0.7 ps, and the laser contrast was about 10⁹.

Fig. 2. A schematic diagram of hollow atoms formation by the ultra intense optical laser pulse (Colgan et al., Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013). Laser field of >10²⁰ W/cm² in central area of the focal spot accelerates MeV and multi-MeV electrons from a target and produces bright X-ray radiation range via Thomson scattering and Bremsstrahlung processes. In turn, X-ray photons of keV energies create hollow atoms in outer area of a target.

The spectra were measured in this paper using a focusing spectrometer with spatial resolution (FSSR) equipped with spherically bent mica crystals (Faenov et al., Reference Faenov, Pikuz, Erko, Bryunetkin, Dyakin, Ivanenkov, Mingaleev, Pikuz, Romanova and Shelkovenko1994; Skobelev et al., Reference Skobelev, Faenov, Bryunetkin, Dyakin, Pikuz, Pikuz, Shelkovenko, Romanova and Mingaleev1995; Blasco et al., Reference Blasco, Stenz, Salin, Faenov, Magunov, Pikuz and Skobelev2001). FSSR was tuned to observe radiation in the wavelength range from 7.0 to 8.4 Å containing the K-shell spectra from multi-charged and neutral Al ions. The spectra were acquired from the front, laser irradiated surface, at 45° to the target normal. X-ray spectra from pure aluminum foils of 1.5 and 20 mkm thicknesses were investigated at different laser pulse energies.

As shown in Figure 3, the reduction of the laser pulse energy from 160 J to 64 J leads to remarkable changes in the spectra. For the lower laser energy case, little emission was observed, with prominent peaks just below 7.8 and 7.2 Å corresponding to He_α and Ly_α transitions. In the full laser energy case, the spectra are dramatically different. The “usual” He_α and Ly_α lines are dominated by significant emission between 7.3 and 7.7 Å (which was identified as arising from KK hollow atoms) and between 7.9 and 8.3 Å (which was associated with emission from KL hollow atoms). These spectra differ notably from observations previously made with high contrast optical lasers (See for example, Andiel et al., Reference Andiel, Eidmann, Hakel, Mancini, Junkel-Vives, Abdallah and Witte2002a; Reference Andiel, Eidmann, Witte, Uschmann and Förster2002b) and rather high laser intensities about 10¹⁷ W/cm². The new emission at wavelengths lower than the He_α line is due to the radiative decay from the L-shell to the K-shell within ions that have a double K-shell vacancy, as well as several L-shell vacancies, quite distinct from earlier studies of hollow atoms (McPherson et al., Reference McPherson, Thompson, Borisov, Boyer and Rhodes1994), which involved LM transitions. Possible hollow atom configurations are shown schematically in Figure 1 and the inset of Figure 2. The substantial decrease in the yield of hollow ion spectral lines occurs, consistent with the strong dependence of the X-ray yield on laser intensity (Zhidkov & Sasaki, Reference Zhidkov and Sasaki2000; Zhidkov et al., Reference Zhidkov, Koga, Sasaki and Uesaka2002).

Fig. 3. Upper panel: Experimental spectra measured at Vulcan PW laser with Al foil targets of 1.5 µm thickness and laser energies of 160 or 64 J (Colgan et al., Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013; Hansen et al., Reference Hansen, Colgan, Faenov, Abdallah, Pikuz, Skobelev, Wagenaars, Booth, Culfa, Dance, Tallents, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Schulze, Uschmann, Zhidkov and Woolsey2014). Comparison of SCRAM modeled results, which fits to experimental spectra at two different laser intensities. Lower panel: ATOMIC comparison to the experimental spectra for the 160 J laser interaction with Al foil target of 1.5 µm thickness

Emission arises from many ion stages of Al, from Al III through Al X. For emission to be observed from such ion stages at these high field intensities, implies that the electron density remains high (greater than 10²³ cm⁻³), so that three-body recombination drives the ions back toward the neutral stage. The emission in the longer wavelength range (7.9 to 8.3 Å) results from a similar radiative decay process, except that in this case, the initial state has only one K-shell vacancy. This emission occurs at slightly later times, when the electron density is smaller and the radiation field has significantly decreased. Such transitions are less energetic and so occur at longer wavelengths. Refluxing of fast electrons, which are responsible for X-ray radiation, between the target's front and rear occurs only in thin foils and vanishes in thick ones. This is the primary reason for the difference of spectra observed by Colgan et al. (Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013) for the 1. 5 and 20 mkm foils.

It is clear that the large energy deposited in the present experiment leads to a quite different physical picture than that used for lower energy laser experiments. The intense Vulcan laser rapidly ionizes valence electrons from the Al target through field ionization (Zhidkov & Sasaki, Reference Zhidkov and Sasaki2000). These electrons are accelerated in the strong electric and magnetic fields of the laser, and the ponderomotive electron energy (Gavrila, Reference Gavrila1992) in a laser field at an intensity of >10²⁰ W/cm², approaches to 10 MeV. The thin Al target is essentially transparent to these highly-relativistic electrons (Zhidkov & Sasaki, Reference Zhidkov and Sasaki2000), but the electrons quickly lose energy through plasma bremsstrahlung (Nozaw et al., Reference Nozaw, Itoh and Kohyama1998) and (non-linear) Thomson scattering (Sarachik & Schappert, Reference Sarachik and Schappert1970; Landau & Lifshitz, Reference Landau and Lifshitz1961). The scaling for the radiation power P, with the laser amplitude a ₀ = eE _L /mcω (E _L is the electric field strength, ω is the field frequency, m is the electron mass, and c is the speed of light) can be estimated with the use of radiation friction force (Zhidkov et al., Reference Zhidkov, Koga, Sasaki and Uesaka2002).

These X-rays interact with the Al ions and atoms in the target by interacting with electrons in the inner atomic shells and ejecting multiple K and L-shell electrons. Inner-shell electrons are preferentially ionized by high-energy photons so that the excess recoil momentum can be absorbed by the nucleus. High-energy photons are much more efficient at removing K-shell electrons than electrons of similar energies (Skobelev et al., Reference Skobelev, Faenov, Pikuz and Fortov2012). A previous measurement (Evans et al., Reference Evans, Clark, Eagleton, Dunne, Edwards, Garbett, Goldsack, James, Smith, Thomas, Clarke, Neely and Rose2005), which used similar laser intensities to the present measurement but a much thicker target, found that electron pumping of hollow ions was the main ionizing mechanism. In this case, it was found that the generation of hollow ions was not efficient.

To produce a sufficient number of the KK hollow ions, the photoionization must be the main channel of the auto-ionization state decay. That means the condition (I_X-ray/ħω)σ^ph > Γ must be satisfied (here I _X-ray is the X-ray flux, ħω is the energy of X-ray photons, σ^ph is the photoionization cross-section, and Γ is the probability of autoionization). For Al XII ion, the K-shell photoionization cross-section at ħω ~ 2 keV is about 5.5 × 10⁻²⁰ cm², probabilities of autoionization decay are about 10¹⁵ s⁻¹. Therefore the X-ray flux greater than 10¹⁹ W/cm² must be realized to provide such intense hollow ions spectra. We believe that radiation dominant regime is the most suitable mechanism for production so bright X-ray source.

X-ray spectra of hollow atom radiation were analyzed by performing atomic kinetics calculations using the ATOMIC code ((Mazevet & Abdallah, Reference Mazevet and Abdallah2006; Colgan et al., Reference Colgan, Abdallah, Fontes, Kilcrease, Dunn, Purvis and Lee2010; Reference Colgan, Abdallah, Faenov, Pikuz, Skobelev, Fukuda, Hayashi, Pirozhkov, Kawase, Shimomura, Kiriyama, Kato, Bulanov and Kando2011; Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013) and the hybrid structure Spectroscopic Collisional-Radiative Atomic Mode (SCRAM) (Hansen et al., Reference Hansen, Bauche, Bauche-Arnoult and Gu2007; Reference Hansen, Colgan, Faenov, Abdallah, Pikuz, Skobelev, Wagenaars, Booth, Culfa, Dance, Tallents, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Schulze, Uschmann, Zhidkov and Woolsey2014). These codes include all relevant atomic processes, that is, photoionization, collisional ionization, autoionization, collisional and radiative excitation and de-excitation, and all recombination processes. Preliminary time-dependent calculations using a simplified atomic model were performed to determine the bulk plasma conditions. They show that, at the high electron densities under consideration here, the system reaches steady-state very quickly. As it was shown by Hansen et al. (Reference Hansen, Colgan, Faenov, Abdallah, Pikuz, Skobelev, Wagenaars, Booth, Culfa, Dance, Tallents, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Schulze, Uschmann, Zhidkov and Woolsey2014) for correctly modeling of the exotic plasma created experimentally, it is necessary to include over 21000 atomic configurations, representing Al ions in which up to five electrons have been removed from the K- and L-shells and placed in excited states. Multiply excited states were found to be important in accurately reproducing the observed emission spectra. In particular, it was demonstrated that the radiative decay from the L- to K-shell in any one specific configuration results in a relatively weak line, but that the very large number of configurations with different combinations of spectator electrons in excited states, in which this radiative transition occurs, allows the observed transition to become prominent.

Performed detailed steady-state calculations at various plasma conditions allowed to compute (Colgan et al., Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013; Pikuz et al., Reference Pikuz, Faenov, Colgan, Dance, Abdallah, Wagenaars, Booth, Culfa, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013; Hansen et al., Reference Hansen, Colgan, Faenov, Abdallah, Pikuz, Skobelev, Wagenaars, Booth, Culfa, Dance, Tallents, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Schulze, Uschmann, Zhidkov and Woolsey2014) the emission spectrum as a function of electron temperature (including non-Maxwellian effects such as hot electron tails) and density. Additionally, opacity effects are included via escape factors. Influence of radiation temperature was included assuming that the radiation field seen by the plasma was a Planckian distribution in the keV range. Typical dependencies of spectra radiation form such parameters are presented in Figures 4–7. As it is seen from Figure 4 no emission lines due to KK hollow ions are observed, particularly in the region between 7.2 and 7.7 Å, in the case of absence external radiation field. Figure 4 obviously demonstrated that the incorporation in modeling radiation field leads to dramatic effect. The blue line shows the effect of radiation on the calculation while omitting the hot-electron tail. Modeling shows that the hot electrons do excite hollow ions, but provide only a small part of the measured intensity of the hollow ion spectral lines. It was also found (see Fig. 7) that at a radiation temperature of 1 keV only a few spectral features exist in the region 7.2–7.6 A. However, for T _r = 2 keV, we see a dramatic change; a series of intense lines are now prominent. As we move to T _r = 3 keV the intensity of these features is modified somewhat (and is in better agreement with the observed spectrum).

Fig. 4. Aluminum K-shell spectra calculated (Colgan et al., Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013) by the ATOMIC code. Calculations are made at plasma conditions: bulk T _e = 55 eV, Ne = 3 µ × 10²³ cm⁻³, 5% of 5 keV hot electrons, T _rad = 3 keV. The inset shows the ion charge distribution for the combined calculation (pink line in both panels) that includes the radiation field and hot electrons. Experimental spectra were measured for Al foil targets of 1.5 µm thickness and with laser energies of 160 J.

Fig. 5. Aluminum K-shell spectra calculated by the ATOMIC code (Pikuz et al., Reference Pikuz, Faenov, Colgan, Dance, Abdallah, Wagenaars, Booth, Culfa, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013). ATOMIC calculations are made for four different electron temperatures and the following other plasma conditions:Ne-3 × 10²³ cm⁻³, 5% of 5 keV hot electrons, T _rad = 3 keV. Spectra measured in Colgan et al. (Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013) is shown as the grey line.

Fig. 6. Aluminum K-shell spectra calculated by the ATOMIC code (Pikuz et al., Reference Pikuz, Faenov, Colgan, Dance, Abdallah, Wagenaars, Booth, Culfa, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013). ATOMIC calculations are made for four different electron densities and the following other plasma conditions: T _e = 55 eV, 5% of 5 keV hot electrons, T _rad = 3 keV. The inset shows the ion charge distribution for the combined calculation (pink line in both panels) that includes the radiation field and hot electrons. Spectra measured in Colgan et al. (Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013) is shown as the grey line.

Fig. 7. Calculated (Hansen et al., Reference Hansen, Colgan, Faenov, Abdallah, Pikuz, Skobelev, Wagenaars, Booth, Culfa, Dance, Tallents, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Schulze, Uschmann, Zhidkov and Woolsey2014) optically thin emission from the SCRAM model showing dependence of emission on Te, Tr, and hot electron fraction, assuming a 5 keV Maxwellian hot electron distribution.

Figures 4–7 demonstrate strong dependence of emitted spectra intensities from all plasma parameters. It is necessary to stress that intensity of KK and KL hollow ions spectra are the most pronounced for bulk electron temperatures around 10–100 eV and electron densities about 10²³ cm⁻³ or higher. At the same time, for observation of intensive, KK hollow ions spectra high radiation temperature are crucial parameters. Presented results of theoretical modeling allow concluding that if X-ray spectra with high (λ/Δλ more than 2000) spectral resolution are observed, it is allowed to determine parameters of warm, dense plasma with rather high accuracy.

Comparisons of modeled by SCRAM and by ATOMIC codes spectra with experimental one obtained at laser energy 160 J are presented in Figure 3. It is clearly seen that both codes model experimental spectra rather well. At the same time it was shown that it is impossible to model all lines intensities using only one set of plasma parameters. From Figure 3 (upper panel) we could conclude that the emission comes from three almost equally weighted regions, all assumed to be at solid density. The first region includes the entire depth of the 1.5 mkm target at a relatively cold thermal temperature (7 eV), with 5% hot electrons and a 2.5 keV radiation field. This region contributes the cold K_α and the KL and KK emission from near-Ne-like ions. The second region has a higher thermal temperature of 50 eV and a lower radiation temperature of 1.7 keV, and is responsible for the KL and KK emission from mid-L-shell ions. Finally, there is a hotter region with Te = 400 eV and 5% hot electrons with no radiation field that includes only about a tenth of the original target thickness, but with a larger weighting factor that could be attributable to a larger area or longer duration. The spectrum measured from the 64 J laser pulse incident on a 1.5 mkm target is also shown in Figure 3 (upper panel) and it is quite different compared with the spectra emitted by plasma irradiated by laser with energy 160 J. This spectrum does not have significant hollow-ion emission and is reasonably well fit by the high-temperature region with no radiation field. Such strong change in spectra intensity and processes responsible for it production is consistent with the mechanism for radiation production due to radiation dominant regime, which were discussed above and was proposed in Colgan et al. (Reference Colgan, Abdallah, Faenov, Pikuz, Wagenaars, Booth, Culfa, Dance, Evans, Gray, Kaempfer, Lancaster, Mckenna, Rossall, Skobelev, Schulze, Uschmann, Zhidkov and Woolsey2013).

So, we see that hollow-ion emission from radiation-dominated hot, dense plasmas provides a new opportunity for diagnosing high-intensity X-ray radiation fields interaction with warm dense matter. However, constructing adequate non-LTE atomic models remains a challenge, since there remains uncertainty in the ionization potential depression at these conditions, configuration interaction plays a significant role in the structure of the emission, and multiply excited states with many holes in both valence and inner shells can lead to enormous structural and computational complexity. Developing atomic kinetics model that systematically and self-consistently accounts for all these effects is state-of-the-art for atomic and plasma physics today.

HIGH-TEMPERATURE PLASMA WITH ENHANCED ROLE OF THE CHARGE-EXCHANGE PROCESSES

When a gas is utilized as a laser target, there are favorable conditions for the penetration of multi-charged ions, which are generated in the focal region, into peripheral regions containing primarily low-charged ions, and even neutral atoms of the gas. This has the consequence that the charge exchange processes may give rise to an efficient population of the states of hollow ions.

This effect was first discovered and explained by Rosmej et al. (Reference Rosmej, Faenov, Pikuz, Magunov, Skobelev, Auguste, D'oliveira, Hulin, Monot, Andreev, Chegotov and Veisman1999), which was dedicated to the experimental and theoretical investigation of intense femtosecond laser pulses with high-pressure nitrogen. The experiments of Rosmej et al. (Reference Rosmej, Faenov, Pikuz, Magunov, Skobelev, Auguste, D'oliveira, Hulin, Monot, Andreev, Chegotov and Veisman1999) were performed on the titanium-sapphire laser of the Saclay Research Center (France). Laser pulses with a linear p-polarization were focused onto a pulsed nitrogen gas target. The atomic number density was amounted to 1.5 × 10¹⁹ cm⁻³ for the highest pressure in the valve equal to 20 bar. The pulse energy was 750 mJ, the laser contrast ratio was 10⁵, and intensity was equal to 10¹⁹ W/cm². Under this intensity, the optical field ionization could take place up to the instant of formation of bare nitrogen nuclei (Ammosov et al., Reference Ammosov, Delone and Krainov1986). The space-resolved X-ray spectra of nitrogen ions were recorded using a spectrograph with a spherically mica crystal (Skobelev et al., Reference Skobelev, Faenov, Bryunetkin, Dyakin, Pikuz, Pikuz, Shelkovenko, Romanova and Mingaleev1995; Faenov et al., Reference Faenov, Pikuz, Erko, Bryunetkin, Dyakin, Ivanenkov, Mingaleev, Pikuz, Romanova and Shelkovenko1994) bent to a radius of 150 mm. The observed spectra contained very broad structures about the resonance lines of the H-like ion (see Fig. 8).

Fig. 8. Comparison of the experimental spectrum of the nitrogen target with the spectrum calculated using the Maria code (Rosmej et al., Reference Rosmej, Faenov, Pikuz, Magunov, Skobelev, Auguste, D'oliveira, Hulin, Monot, Andreev, Chegotov and Veisman1999).

Rosmej et al. (Reference Rosmej, Faenov, Pikuz, Magunov, Skobelev, Auguste, D'oliveira, Hulin, Monot, Andreev, Chegotov and Veisman1999) hypothesized that these structures arise from radiative transitions from the highly excited nln₀l₀ states of hollow He-like nitrogen ions. Atomic calculations performed using the multi-configuration Hartree-Fock method with the inclusion of relativistic corrections for hollow configurations (3l5l₀, 4l5l₀, 5l5l₀, 3l6l₀, 4l6l₀, 5l6l₀, 6l6l₀, 3l7l₀, 4l7l₀, 5l7l₀, 6l7l₀, 7l7l₀, 3l8l₀, 4l8l₀, 5l8l₀, 6l8l₀, 7l8l₀, and 8l8l₀) confirmed this assumption, at least for the wavelengths of the observed spectral peaks. It turned out that the spectra of the structures listed above are really quite broad because of the mutual overlap of a huge number of closely spaced transitions and lie in the spectral region of interest. Furthermore, the total emission spectrum of these hollow ion states provides a qualitatively and even quantitatively good description of the experimental spectrum (a comparison is given in Fig. 8) with the exception of the H-like ion resonance lines themselves. This signifies that, in this case, the hollow ion states for some reasons are anomalously densely populated in comparison with the singly excited states of hydrogen-like ions. To explain this anomalous behavior of level populations, Rosmej et al. (Reference Rosmej, Faenov, Pikuz, Magunov, Skobelev, Auguste, D'oliveira, Hulin, Monot, Andreev, Chegotov and Veisman1999) proposed a physical mechanism involving charge exchange in collisions of multi-charged and low-charged nitrogen ions. The scenario of this mechanism is as follows.

After the optical field ionization of N₂ molecules to the state of bare nuclei, they penetrate the surrounding gas that contains neutral atoms or singly and doubly ionized ions. The reason is that the laser intensity decreases rapidly with distance from the central spot, and at distances of about 30 mkm from the focused point, the laser field cannot ionize even N₂ molecules. We note, however, that N₂ molecules, even though far away from the central spot, may be destroyed by sufficiently high-energy particles (photons and electrons) generated in the central region. That is why, in accordance with Rosmej et al. (Reference Rosmej, Faenov, Pikuz, Magunov, Skobelev, Auguste, D'oliveira, Hulin, Monot, Andreev, Chegotov and Veisman1999), it will be assumed that the nuclei collide with N⁺⁰, N⁺¹‡ and N⁺²‡ ions, resulting in the following single- or double-electron charge-exchange reactions N⁶⁺ + N⁰ → N⁵⁺(nl) + N¹⁺, N⁶⁺ + N¹⁺ → N⁵⁺(nl) + N²⁺, N⁶⁺ + N²⁺ → N⁵⁺(nl) + N³⁺, N⁶⁺ + N⁰→ N⁴⁺(nln‘l’) + N²⁺, N⁶⁺ + N¹⁺ → N⁴⁺(nln‘l’) + N³⁺, N⁶⁺ + N²⁺ → N⁴⁺(nln‘l’) + N³⁺. It means that the charge exchange mechanisms do turn out to be most significant in the population of hollow ion states.

One can see from the Figure 8 that comparison of the calculated hollow ion spectra with observed ones allow to measure plasma parameters. For example, in the experiment of Rosmej et al. (Reference Rosmej, Faenov, Pikuz, Magunov, Skobelev, Auguste, D'oliveira, Hulin, Monot, Andreev, Chegotov and Veisman1999) plasma density was known, and value of T _e = 30 eV was measured by this method.

EMISSION OF HOLLOW IONS SPECTRA IN HIGH-TEMPERATURE PLASMA WITH FAST CHARGED PARTICLES

It is well-known that in the laser-produced plasma and particular in plasma produced by relativistic laser intensities, a large amount of fast electrons and ions are generated. However, as it was mentioned above, the creation of the hollow ions by charged particle impact ionization is less effective than by X-ray photons. Moreover, the extra high plasma density is needed for the good excitation of the hollow ion states. At the same time in the laser-produced plasma, the electron plasma density usually is limited by critical value, depending on laser wavelength. This limitation is not important only for super short laser pulses (femtosecond or sub-picosecond) and for short wavelength lasers (vacuum-ultraviolet- or X-ray). Therefore, until now, hollow ion spectra were observed practically only in the femtosecond laser-produced plasma in the cases when laser did not produce preplasma due to the rather low laser intensity (Gauthier et al., Reference Gauthier, Geindre, Audebert, Rousse, Dos Santos, Grillon, Antonetti and Mancini1995) or due to very high (above 10⁹) laser contrast (see, for example, Faenov et al., Reference Faenov, Abdallah, Clark, Cohen, Johnson, Kyrala, Magunov, Pikuz, Skobelev and Wilke1997; Reference Faenov, Magunov, Pikuz, Skobelev, Pikuz, Urnov, Abdallah, Clark, Cohen, Johnson, Kyrala, Wilke, Maksimchuk, Umstadter, Nantel, Doron, Behar, Mandelbaum, Schwob, Dubau, Rosmej and Osterheld1999; Reference Faenov, Pikuz, Skobelev, Fukuda, Colgan and Abdallah2009; Reference Faenov, Skobelev, Pikuz, Fortov, Boldarev, Gasilov, Chen, Zhang, Yan, Yaun, Mao and Wang2011; Reference Faenov, Skobelev, Pikuz, Pikuz, Fortov, Fukuda, Hayashi, Pirozhkov, Kotaki, Shimomura, Kiriyama, Kanazawa, Kato, Colgan, Abdallah and Kando2012; Urnov et al., Reference Urnov, Dyubo, Faenov, Pikuz, Skobelev, Abdallah, Clark, Cohen, Johnson, Kyrala, Wilke and Osterheld1998; Rosmej et al., Reference Rosmej, Funk, Geissel, Hofmann, Tausehwitz, Faenov, Pikuz, Skobelev, Flora, Bollanti, Di Lazzaro, Letardi, Grilli, Palladino, Reale, Scafati, Reale, Auguste, D'oliveira, Hulin, Monot, Maksimchuk, Pikuz, Umstadter, Nanatel, Bock, Dornik, Stetter, Stoewe, Yakushev, Kulish and Shilkin2000; Colgan et al., Reference Colgan, Abdallah, Faenov, Pikuz, Skobelev, Fortov, Fukuda, Akahane, Aoyama, Inoue and Yamakawa2008; Reference Colgan, Abdallah, Faenov, Pikuz, Skobelev, Fukuda, Hayashi, Pirozhkov, Kawase, Shimomura, Kiriyama, Kato, Bulanov and Kando2011; Skobelev et al., Reference Skobelev, Faenov, Pikuz and Fortov2012). For longer laser pulse, hollow ion spectra have been observed where short wavelength eximer XeCl-laser or 2w of Nd laser were used (Abdallah et al., Reference Abdallah, Skobelev, Faenov, Magunov, Pikuz, Flora, Bollanti, Di Lazzaro, Letardi, Burattini, Grilli, Reale, Palladino, Tomassetti, Scafati and Reale2000; Colgan et al., Reference Colgan, Abdallah, Faenov, Pikuz and Skobelev2008a; Colgan Reference Colgan, Abdallah, Fontes, Kilcrease, Dunn, Purvis and Lee2010).

For the plasma created by fast heavy ion beam situation must be better, because in this case the beam energy will be inputted directly in the solid state target and plasma density will be higher (the critical density does not exist in this case). It means that such plasma hollow ions will be created independently on the ion pulse duration (see for example, Moribayashi et al., Reference Moribayashi, Suto, Zhidkov, Sasaki and Kagawa2001a). The ion energy for effective ionization of inner atom electrons must be higher than the energy of fast electrons, of course, but the experiments, carried out at the different accelerators, showed that energy of nowadays used heavy projectile ions are enough for ionization of the K-electrons in the different atoms (see, for example, MacFarlane et al., Reference Macfarlane, Wang, Bailey, Mehlhorn, Dukart and Mancini1993; Rosmej et al., Reference Rosmej, More, Rosmej, Wieser, Borisenko, Shevelko, Geißel, Blazevic, Jacoby, Dewald, Roth, Brambrink, Weyrich, Hoffmann, Golubev, Turtikov, Fertman, Sharkov, Faenov, Pikuz, Magunov and Skobelev2002; Rosmej, O. et al., Reference Rosmej, Pikuz, Wieser, Blazevic, Brambrink, Roth, Efremov, Faenov, Pikuz, Skobelev and Hoffmann2003; Reference Rosmej, Blazevic, Korostiy, Bock, Hoffmann, Pikuz, Efremov, Fortov, Fertman, Mutin, Pikuz and Faenov2005b; Reference Rosmej, Pikuz, Korostiy, Blazevic, Brambrink, Fertman, Mutin, Efremov, Pikuz, Faenov, Loboda, Golubev and Hoffmann2005a; Pikuz et al., Reference Pikuz, Efremov, Rosmej, Blazevic, Korostiy, Fertman, Shutov, Norman and Hoffmann2006; Rzadkiewicz et al., Reference Rzadkiewicz, Gojska, Rosmej, Polasik and Słabkowska2010; Kawamura et al., Reference Kawamura, Horioka and Koike2011; McMahon et al., Reference Mcmahon, Kavanagh, Watanabe, Sun, Tona, Nakamura, Ohtani and Currell2011; Nakano et al., Reference Nakano, Suda, Hatakeyama, Nakai, Komaki, Takada, Murakami and Azuma2012).

To the present time KK hollow ion spectra were used for diagnostics of high-temperature plasma with fast charged particles only in the case of the laser-produced plasma. The observations of the KK-hollow ion spectra (spectra of the ions with two holes in the K-shell) in the plasma heated by heavy ion beam are absent yet. We would like to note that there are no objective reasons for this and consider that such observations in future will allow obtaining important information on heavy ion beam plasma. It should be noted that KL-hollow ions (ions with one hole in the K-shell and one hole in the L-shell) have been observed in aluminum plasma heated by intensive proton beam (Bailey et al., Reference Bailey, Carlson, Chandler, Derzon, Dukart, Hammel, Lockner, Maenchen, Mcguire, Mehlhorn, Nelson, Ruggles, Stygar and Wenger1990). In the papers by Wang et al. (Reference Wang, MacFarlane and Moses1993) and MacFarlane et al. (Reference Macfarlane, Wang, Bailey, Mehlhorn, Dukart and Mancini1993) it was shown that K_α satellite lines of aluminum ions observed by Bailey et al. (Reference Bailey, Carlson, Chandler, Derzon, Dukart, Hammel, Lockner, Maenchen, Mcguire, Mehlhorn, Nelson, Ruggles, Stygar and Wenger1990) can be classified into two distinct groups: one involving transitions of type 1s2s^r2p^q - 1s²2s^r2p^q-1, the other 1s2s^r2p^q-13l - 1s²2s^r2p^q-23l. The second group is just KL-hollow ion configurations.

In the case of the laser-produced plasma, the hollow ion spectra will be prominent in the densest regions, while emission spectra of the hot low dense plasma are being caused by usual spectral transitions. Just for diagnostics of these regions, the hollow ion spectra are the most suitable. For example, Colgan et al. (Reference Colgan, Abdallah, Faenov, Pikuz, Skobelev, Fukuda, Hayashi, Pirozhkov, Kawase, Shimomura, Kiriyama, Kato, Bulanov and Kando2011) and Faenov et al. (Reference Faenov, Skobelev, Pikuz, Fortov, Boldarev, Gasilov, Chen, Zhang, Yan, Yaun, Mao and Wang2011; Reference Faenov, Skobelev, Pikuz, Pikuz, Fortov, Fukuda, Hayashi, Pirozhkov, Kotaki, Shimomura, Kiriyama, Kanazawa, Kato, Colgan, Abdallah and Kando2012) have suggested the use of such spectra to diagnose the early stage of the heating of argon clusters by a femtosecond laser pulse. Experiments were carried out at the Xtreme Light III (XL-III) laser facility at the Institute of Physics, Chinese Academy of Sciences. The laser pulse has energy up to 1 J, duration is about 100 fs, and contrast is about 10¹⁰. A laser beam was focused onto a pulsed gas-cluster argon target. The laser energy flux density reached q _las = 2.6 × 10¹⁹ W/cm². The pressure of the gas supplied to the nozzle was optimized to increase the yield of clusters with a radius of R _cl ~ 0.15 µm. According to the calculations of Boldarev et al. (Reference Boldarev, Gasilov and Faenov2004; Reference Boldarev, Gasilov, Faenov, Fukuda and Yamakawa2006), a cluster diameter of 0.3 µm and a maximum atomic density of N _Ar ~ 1.5 × 10²⁰ cm⁻³ at a distance of 1 mm from the nozzle edge are achieved at a gas pressure of 70 bar. The experiments indicated that the maximum X-ray emission was observed at this gas pressure.

In our previous experiments, the spectra of the argon plasma were studied in the laser-droplet interaction (the size of cluster was about 1 µm) regime (see Fig. 9). Dependences of intensities of argon spectra from contrast and pulse duration are presented in Figure 9 and demonstrated that in the case of high laser contrast and very short laser pulse duration the strong KL hollow ions spectra are radiated. It was found that various stages of the evolution of the produced plasma contribute to the observed time-integrated X-ray emission spectrum. The long-wavelength part of the spectrum shown in Figure 9 is formed at the initial heating stage by the densest regions heated not too strong, whereas the short-wavelength part is formed by the less dense, hotter plasma at the much later stage. Since the size of clusters in these experiments was about 1 µm, i.e., was much larger than the thickness of the skin layer, the heating of the cluster was non-uniform. When its surface layer had been already heated to a high temperature and began to expand, the inner part still remained cold and immobile.

Fig. 9. Typical traces of the spectra in the wavelength range 3.9–4.3 Å emitted by large size Ar clusters, irradiated by ultra-intense laser radiation (Colgan et al., Reference Colgan, Abdallah, Faenov, Pikuz, Skobelev, Fukuda, Hayashi, Pirozhkov, Kawase, Shimomura, Kiriyama, Kato, Bulanov and Kando2011; Faenov et al., Reference Faenov, Skobelev, Pikuz, Pikuz, Fortov, Fukuda, Hayashi, Pirozhkov, Kotaki, Shimomura, Kiriyama, Kanazawa, Kato, Colgan, Abdallah and Kando2012): Upper panel: dependence from different laser contrast. Bottom panel: dependence from different pulse durations.

In the case under consideration, all parts of the cluster will be heated simultaneously and the plasma created at the heating stage will be much more uniform. Using developed stationary kinetic model and the atomic constants calculated for argon ions (Colgan et al., Reference Colgan, Abdallah, Faenov, Pikuz, Skobelev, Fukuda, Hayashi, Pirozhkov, Kawase, Shimomura, Kiriyama, Kato, Bulanov and Kando2011) the emission spectrum corresponding to this stage of the plasma evolution were calculated. It was shown that until the cluster does not noticeably expand (i.e., until time T _exp ~ R _cl/v _ion ~ 150 fs at a typical value of v _ion ~ 10⁸ cm/s), its atomic density can be treated as constant N _Ar = 2.1 × 10²² cm⁻². In this case, the spectrum will depend on only one parameter, i.e., the electron temperature T _e of the plasma, because its electron density (and the ionization degree) will be determined by the balance equations. In Figure 10, spectra calculated for various T _e and N _e according to this model, which include into the kinetic equations also the influence of the 1% fraction of hot electrons with a mean energy of 7 keV, are presented.

Fig. 10. Emission spectra of Ar plasma calculated (Faenov et al., Reference Faenov, Skobelev, Pikuz, Fortov, Boldarev, Gasilov, Chen, Zhang, Yan, Yaun, Mao and Wang2011) in the stationary kinetic model: for various electron temperatures (upper panel); with and without contribution of hollow ions (middle panel); spectra at a fixed temperature but for different electron densities (bottom panel).

The spectral range shown in Figure 10 includes three broad spectral structures with the average wavelengths of 4.11–4.13, 4.14–4.15, and 4.18–4.20 Å. Each of these structures can generally consist of a number of various spectral transitions both well-known transitions (K_α lines and dielectronic satellites) and transitions in hollow ions or hypersatellites.

It can be seen from Figure 10 that an increase in the temperature of the plasma is accompanied by a noticeable change in the emission spectrum. To demonstrate the contribution to the emission spectrum from radiative transitions of various types, calculations disregarding transitions in hollow ions were performed by Faenov et al. (Reference Faenov, Skobelev, Pikuz, Fortov, Boldarev, Gasilov, Chen, Zhang, Yan, Yaun, Mao and Wang2011) and results are presented in Figure 10 (middle panel). These calculations showed that, for low temperatures below 50 eV, the emission spectrum almost completely consists of lines of hollow ions. At a temperature of 100 eV, hollow ions completely determine the right spectral structure, making an approximately 50% contribution to the intensity of the central structure, and could be recognized in the left structure (see Fig. 10). It means that the emission of clusters at low temperatures is almost completely determined by transitions in hollow ions. It should be stressed that their contribution in the longest-wavelength part of the spectrum under consideration is noticeable even for the high-temperature plasma. It can be seen also from Figure 10 (bottom panel) that an increase in the electron density leads to a decrease in the plasma ionization degree. This is obvious because an increase in the density is accompanied by a fast increase in the collisional recombination rate and by a transition from the coronal ionization equilibrium to the Saha equilibrium. Note that the effect of an increase in N _e on the emission spectrum is similar to that of a decrease in T _e because, in both cases, the plasma ionization degree decreases. Thus, we could conclude that the spectra of hollow ions can be used for the diagnostics of the heating of clusters at the stage of the action of the main laser pulse.

If a high intensive femtosecond pulse interacts with clusters and laser contrast is not large enough, the laser prepulse may destroy cluster and the main pulse will interacts with plasma not with dense cluster core. Therefore, development of the diagnostic methods allowing to directly obtain information about the cluster destruction by laser prepulses is very important. In paper by Faenov et al. (Reference Faenov, Skobelev, Pikuz, Pikuz, Fortov, Fukuda, Hayashi, Pirozhkov, Kotaki, Shimomura, Kiriyama, Kanazawa, Kato, Colgan, Abdallah and Kando2012), it was shown that the key information regarding the existence (or non-existence) of the dense cluster core at the moment of the main laser pulse arrival can be obtained by means of the observation of the hollow ion spectra. Really, for observation of such radiation, the existence of two conditions is necessary (1) presence of cold matter and (2) presence of the electrons with energy sufficient for K-shell excitation, i.e., at least several keV. As high energy electrons can be generated only after irradiation of the cluster by the main laser pulse, K_α lines will be observed only in the case when the cold dense cluster core remains after irradiation by the laser prepulses.

As it is seen from Figure 9 (upper panel) at very high laser contrast >10⁸ observable spectra contain intense Kα line which is not observed at contrast 2 × 10⁵. It means that in the latter case the laser prepulse was strong enough to ionize all cluster atoms before the arrival of the main pulse. At higher laser contrasts the cold dense part of cluster survived after the laser prepulse. In such case, the Hollow ions and neutral K_α spectral structures with wavelengths of about 4.18 Å are clearly seen. Since generation of these states require hot electrons, generated by the main laser pulse, and cold dense plasma therefore an observation of such structure near 4.18 Å will also suggest the existence of a dense core at the moment of arrival of the main pulse. Moreover, a comparison of the experimental and the calculated spectra of hollow ions can be used for estimation of the parameters of the most dense plasma regions generated by the laser prepulse. Such type of calculations were done by atomic and kinetic models (Colgan et al., Reference Colgan, Abdallah, Faenov, Pikuz, Skobelev, Fukuda, Hayashi, Pirozhkov, Kawase, Shimomura, Kiriyama, Kato, Bulanov and Kando2011; Faenov et al., Reference Faenov, Skobelev, Pikuz, Fortov, Boldarev, Gasilov, Chen, Zhang, Yan, Yaun, Mao and Wang2011) and their results show that the spectrum of the hollow ions obtained for laser contrast 10¹⁰, is described adequately by the modeling for the plasma with T _e = 50 eV and N _e = 5 × 10²² cm⁻³ in which there is 1% fraction of hot electrons.