A review focused on plasma induced on solid target by GW-level pulsed laser source is presented. A description of the Tor Vergata laser-plasma source (TVLPS), at the Tor Vergata University in Rome, is given. Such a facility uses a 1? GW, tabletop, multistage Nd:YAG/Glass laser system, delivering infrared (IR) pulses with nanosecond width and 1064?nm wavelength (TEM00 mode). Its applications are discussed providing: wide analysis of IR → soft X-ray conversion efficiency (1.3–1.55?keV); measures and modeling of line emission in soft X-ray spectra, such as those from zinc plasma near Ne-like Zn XXI and from barium plasma near Ni-like Ba XXIX. Particular attention is devoted to high-n dielectronic Rydberg satellites for finding a useful diagnostic tool for plasma conditions. Dependence of plasma spectra on laser parameters is shown. Finally, microradiography applications are presented for thin biological samples. Images permit to visualize specific structures and detect bioaccumulation sites due to contamination from pollutants. 1. Introduction Plasma [1] is a particular state of the matter beside ordinary solid, liquid, and gaseous ones usually called fourth state. It is constituted by neutral atoms, negative (electrons) and positive (ions) charged particles subjected to the action of long-range electromagnetic fields, governing the motion, and able to produce electric and magnetic forces. The charge separation can be properly generated by heating the matter to high temperatures (around 104°C at least), giving a validation of the plasma definition in terms of high-temperature ionized gas. It represents an interesting, original, very intricate matter state whose study has required the development of specific scientific disciplines and advanced research fields. The survey of the matter in the plasma state is important, because it constitutes the 99% of the universe matter. Specifically, the stars (e.g., the sun) are the more common and prevailing examples of natural plasmas. Here, temperatures can achieve the hundreds of millions of degrees, and the produced high energies cannot be explained in terms of chemical reactions but only by nuclear fusion processes induced by high temperatures. It is also possible to generate plasma in artificial way for scientific and industrial purposes. This usually occurs in research laboratories and industries, especially for surveys in the fields of the radiation-matter interaction, mechanical processing (welding, cutting, drilling, etc.), and material treatment, such as the plasma-enhanced chemical vapour deposition (PECVD).
References
[1]
R. Goldston and P. H. Rutherford, Introduction to Plasma Physics, Institute of Physics Publishing, Philadelphia, Pa, USA, 1995.
[2]
M. D. Perry and G. Mourou, “Terawatt to petawatt subpicosecond lasers,” Science, vol. 264, no. 5161, pp. 917–924, 1994.
[3]
G. A. Mourou, C. P. J. Barty, and M. D. Perry, “Ultrahigh-intensity lasers: Physics of the extreme on a tabletop,” Physics Today, vol. 51, no. 1, pp. 22–28, 1998.
[4]
S. Martellucci, M. Francucci, and P. Ciuffa, “Ultraintense tabletop laser system and plasma applications,” in Progress in Ultrafast Intense Laser Science (PUILS), vol. I of Springer Series in Chemical Physics, Springer, Berlin, Germany, 2006.
[5]
S. Martellucci, C. Bellecci, M. Francucci et al., “Soft x-ray generation by a tabletop Nd:YAG/glass laser system,” Journal of Physics Condensed Matter, vol. 18, no. 33, pp. S2039–S2044, 2006.
[6]
W. L. Kruer, Physics of Laser Plasma Interaction, Addison Wesley, Redwood City, Calif, USA, 1988.
[7]
I. C. E. Turcu and J. B. Dance, X rays from laser plasma: Generation and Applications, Wiley & Sons, London, UK, 1998.
[8]
E. P. Liang, S. C. Wilks, and M. Tabak, “Pair production by ultraintense lasers,” Physical Review Letters, vol. 81, no. 22, pp. 4887–4890, 1998.
[9]
J. Lindl, “Development of the indirect-drive approach to inertial confinement fusion and the target physics basis for ignition and gain,” Physics of Plasmas, vol. 2, no. 11, pp. 3933–4024, 1995.
[10]
W. J. Hogan, R. Bangerter, and G. L. Kulcinski, “Energy from inertial fusion,” Physics Today, vol. 45, no. 9, pp. 42–50, 1992.
[11]
B. A. Remington, D. Arnett, R. P. Drake, and H. Takabe, “Modelling astrophysical phenomena in the laboratory with intense lasers,” Science, vol. 284, no. 5419, pp. 1488–1493, 1999.
[12]
B. A. Remington, R. P. Drake, H. Takabe, and D. Arnett, “A review of astrophysics experiments on intense lasers,” Physics of Plasmas, vol. 7, no. 5, pp. 1641–1652, 2000.
[13]
K. B. Fournier, A. Y. Faenov, T. A. Pikuz et al., “Observations of high-n transitions in the spectra of near-neon-like copper ions from laser-produced plasmas,” Journal of Physics B, vol. 35, no. 15, pp. 3347–3364, 2002.
[14]
I. Y. Skobelev, A. Y. Faenov, T. A. Pikuz et al., “Spectral transitions from the rydberg autoionization states of a Li-like Mg X ion,” Journal of Experimental and Theoretical Physics, vol. 95, no. 3, pp. 421–428, 2002.
[15]
K. B. Fournier, A. Y. Faenov, T. A. Pikuz et al., “Rydberg transitions in the spectra of near-neon-like Cu and Zn ions in different laser-produced plasmas: Observations and modeling,” Journal of Quantitative Spectroscopy & Radiative Transfer, vol. 81, no. 1-4, pp. 167–182, 2003.
[16]
K. B. Fournier, A. Y. Faenov, T. A. Pikuz et al., “Identification and precise measurements of the wavelengths of high-n transitions in N-, O-, and F-like Zn ions,” Journal of Physics B, vol. 36, no. 18, pp. 3787–3796, 2003.
[17]
A. Y. Faenov, T. A. Pikuz, and I. Y. Skobelev, “X-ray spectroscopic observations of a superdense plasma in nanoparticles irradiated by superintense femtosecond laser radiation,” Journal of Experimental and Theoretical Physics Letters, vol. 80, pp. 730–733, 2004.
[18]
K. B. Fournier, A. Y. Faenov, T. A. Pikuz et al., “Analysis of high-n dielectronic Rydberg satellites in the spectra of Na-like Zn XX and Mg-like Zn XIX,” Physical Review E, vol. 70, no. 1, Article ID 016406, 2004.
[19]
M. J. May, P. Beiersdorfer, J. Dunn et al., “Accurate wavelength measurements and modeling of Fe XV to Fe XIX spectra recorded in high-density plasmas between 13.5 and 17 ?,” Astrophysical Journal, vol. 158, no. 2, pp. 230–241, 2005.
[20]
J. Colgan, J. Abdallah, A. Y. Faenov et al., “Model calculations and measurements of the emission of a barium plasma in the spectral range of high-n rydberg levels in a near Ni-like state,” Journal of Physics B, vol. 43, no. 17, Article ID 175701, 2010.
[21]
L. Reale, A. Lai, A. Tucci et al., “Differences in X-ray absorption due to cadmium treatment in Saponaria Officinalis leaves,” Microscopy Research and Technique, vol. 64, no. 1, pp. 21–29, 2004.
[22]
T. Pikuz, A. Faenov, I. Skobelev et al., “Easy spectrally tunable highly efficient X-ray backlighting schemes based on spherically bent crystals,” Laser and Particle Beams, vol. 22, no. 3, pp. 289–300, 2004.
[23]
C. Bellecci, L. Coniglio, M. Francucci et al., “Laser-plasma soft-X-rays analysis by means of a CCD camera: A first application to digital micro-radiography,” Nuovo Cimento della Societa Italiana di Fisica B, vol. 121, no. 8, pp. 811–822, 2007.
[24]
K. W. D. Ledingham and P. A. Norreys, “Nuclear physics merely using a light source,” Contemporary Physics, vol. 40, no. 6, pp. 367–383, 1999.
[25]
T. Tajima and J. M. Dawson, “Laser electron accelerator,” Physical Review Letters, vol. 43, no. 4, pp. 267–270, 1979.
[26]
A. Pukhov, Z. M. Sheng, and J. Meyer-ter-Vehn, “Particle acceleration in relativistic laser channels,” Physics of Plasmas, vol. 6, no. 7, pp. 2847–2854, 1999.
[27]
M. Gavrila, Advances in Atomic, Molecular and Optical Physics: Atoms in Intense Laser Fields, Academic Press, New York, NY, USA, 1992.
[28]
P. M. Celliers, G. W. Collins, L. B. Da Silva et al., “Shock-induced transformation of liquid deuterium into a metallic fluid,” Physical Review Letters, vol. 84, no. 24, pp. 5564–5567, 2000.
[29]
K. B. Fournier, A. Y. Faenov, T. A. Pikuz et al., “Influence of optical thickness and hot electrons on Rydberg spectra of Ne-like and F-like copper ions,” Physical Review E, vol. 67, no. 1, Article ID 016402, 2003.
[30]
R. W. Falcone and M. M. Murnane, “Proposal for a femtosecond X-ray light source,” AIP Conference Proceedings, vol. 147, pp. 81–85, 1986.
[31]
M. M. Murnane, H. C. Kapteyn, M. D. Rosen, and R. W. Falcone, “Ultrafast X-ray pulses from laser-produced plasmas,” Science, vol. 251, no. 4993, pp. 531–536, 1991.
[32]
C. Bellecci, I. Bellucci, P. Gaudio, S. Martellucci, G. Petrocelli, and M. Richetta, “Beam characterization of a high power Nd:YAG-GLASS laser,” in Proceedings of the 6th International Workshop on Laser Beam and Optics Characterization (LBOC '6), Munich, Germany, June 2001.
[33]
M. Francucci, “Sistemi per la generazione di raggi X da plasma indotto da laser e possibili applicazioni,” , Ph.D. thesis, University of Rome “Tor Vergata”, 2005.
[34]
A. Y. Faenov, S. A. Pikuz, A. I. Erko, et al., “High-performance X-ray spectroscopic devices for plasma microsources investigations,” Physica Scripta, vol. 50, pp. 333–338, 1994.
[35]
I. Y. Skobelev, A. Y. Faenov, and B. A. Bryunetkin, “Investigating the emission properties of plasma structures with x-ray imaging spectroscopy,” Journal of Experimental and Theoretical Physics, vol. 81, no. 4, pp. 692–718, 1995.
[36]
B. K. F. Young, A. L. Osterheld, D. F. Price et al., “High-resolution x-ray spectrometer based on spherically bent crystals for investigations of femtosecond laser plasmas,” Review of Scientific Instruments, vol. 69, no. 12, pp. 4049–4053, 1998.
[37]
J. R. Janesick and S. T. Elliot, “Astronomical CCD imaging and reduction,” in Astronomical Society of the Pacific Conference Series, S. B. Howell and D. H. McNamara, Eds., vol. 23 of Managing Editors of Conference Series, Bookcrafters, 1992.
[38]
D. Nanni, R. Viotti, M. Badiali, A. M. Di Lellis, and M. Ferrari, “A new 30?cm three-reflection telescope for wide-field Astronomy on the Antarctic Plateau,” in Proceedings of the Future research Direction and Visions for Astronomy, vol. 4835 of Proceedings of SPIE, pp. 192–202, Waikoloa, Hawaii, USA, August 2002.
[39]
G. Agnelli, D. Nanni, S. Cola, A. Vignato, A. Di Lellis, and C. D. La Padula, “A thermo electric cooled 2k × 2k CCD imaging camera for wide-field telescopes,” in Proceedings of the Optical Astronomical Instrumentation, vol. 3355 of Proceedings of SPIE, pp. 703–712, Kona, Hawaii, USA, March 1998.
[40]
A. Zigler, P. G. Burkhalter, D. J. Nagel et al., “Measurement of energy penetration depth of subpicosecond laser energy into solid density matter,” Applied Physics Letters, vol. 59, no. 5, pp. 534–536, 1991.
[41]
Z. Jiang, J. C. Kieffer, J. P. Matte et al., “X-ray spectroscopy of hot solid density plasmas produced by subpicosecond high contrast laser pulses at 1018–1019?W/cm2,” Physics of Plasmas, vol. 2, no. 5, pp. 1702–1711, 1995.
[42]
B. K. F. Young, B. G. Wilson, D. F. Price, and R. E. Stewart, “Measurement of x-ray emission and thermal transport in near-solid-density plasmas heated by 130 fs laser pulses,” Physical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics, vol. 58, no. 4, pp. 4929–4936, 1998.
[43]
K. B. Fournier, B. K. F. Young, S. J. Moon et al., “Characterization of time resolved, buried layer plasmas produced by ultrashort laser pulses,” Journal of Quantitative Spectroscopy & Radiative Transfer, vol. 71, no. 2–6, pp. 339–354, 2001.
[44]
H. R. Griem, Spectral Line Broadening by Plasmas, Academic Press, New York, NY, USA, 1974.
[45]
R. C. Mancini, A. S. Shlyaptseva, P. Audebert et al., “Stark broadening of satellite lines in silicon plasmas driven by femtosecond laser pulses,” Physical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics, vol. 54, no. 4, pp. 4147–4154, 1996.
[46]
U. Andiel, K. Eidmann, P. Hakel et al., “Demonstration of aluminum K-shell line shifts in isochorically heated targets driven by ultrashort laser pulses,” Europhysics Letters, vol. 60, no. 6, pp. 861–867, 2002.
[47]
K. Eidmann, U. Andiel, F. Pisani et al., “K-shell spectra from hot dense aluminum layers buried in carbon and heated by ultrashot laser pulses,” Journal of Quantitative Spectroscopy & Radiative Transfer, vol. 81, no. 1–4, pp. 133–146, 2003.
[48]
P. Audebert, R. Shepherd, K. B. Fournier et al., “Time-resolved plasma spectroscopy of thin foils heated by a relativistic-intensity short-pulse laser,” Physical Review E, vol. 66, no. 6, Article ID 066412, 2002.
[49]
R. Shepherd, P. Audebert, H. K. Chen et al., “Satellite and opacity effects on resonance line shapes produced from short-pulse laser heated foils,” Journal of Quantitative Spectroscopy & Radiative Transfer, vol. 81, no. 1–4, pp. 431–440, 2003.
[50]
Y. Ralchenko, et al., 16th APS Topical Conference on Atomic Processes in Plasmas, AIP Conference Proceedings, Melville, NY, USA, 2009.
[51]
S. H. Glenzer, K. B. Fournier, B. G. Wilson, R. W. Lee, and L. J. Suter, “Ionization balance in inertial confinement fusion hohlraum plasmas,” Journal of Quantitative Spectroscopy & Radiative Transfer, vol. 71, no. 2-6, pp. 355–363, 2001.
[52]
B. Lipschultz, D. G. Whyte, J. Irby, B. Labombard, and G. M. Wright, “Hydrogenic retention with high-Z plasma facing surfaces in Alcator C-Mod,” Nuclear Fusion, vol. 49, no. 4, Article ID 045009, 2009.
[53]
J. Abdallah, R. E. H. Clark, and R. D. Cowan, “Los Alamos Manual,” No. LA 11436-M-I, Los Alamos National Laboratory, 1988.
[54]
R. E. H. Clark, J. Abdallah Jr., and J. B. Mann, “Integral and differential cross sections for electron impact ionization,” Astrophysical Journal, vol. 381, no. 2, pp. 597–600, 1991.
[55]
J. Abdallah Jr., H. L. Zhang, C. J. Fontes, D. P. Kilcrease, and B. J. Archer, “Model comparisons for high-Z non-LTE steady-state calculations,” Journal of Quantitative Spectroscopy & Radiative Transfer, vol. 71, no. 2–6, pp. 107–116, 2001.
[56]
N. H. Magee, J. Abdallah Jr., J. Colgan, et al., “Los Alamos opacities: Transition from LEDCOP to ATOMIC,” in 14th Topical Conference on Atomic Processes in Plasma, J. S. Cohen, S. Mazevet, and D. P. Kilcrease, Eds., AIP Conference Proceedings, pp. 168–179, New York, NY, USA, 2004.
[57]
S. Mazevet and J. Abdallah, “Mixed UTA and detailed line treatment for mid-Z opacity and spectral calculations,” Journal of Physics B, vol. 39, no. 16, article no. 022, pp. 3419–3429, 2006.
[58]
B. L. Henke, F. G. Fujiwara, M. A. Tester, C. H. Dittmore, and M. A. Palmer, “Low-energy X-ray response of photographic films. II. Experimental characterization,” Journal of the Optical Society of America B, vol. 1, no. 6, pp. 828–849, 1984.
[59]
T. Holstein, “Imprisonment of resonance radiation in gases,” Physical Review, vol. 72, no. 12, pp. 1212–1233, 1947.
[60]
T. Holstein, “Imprisonment of resonance radiation in gases. II,” Physical Review, vol. 83, no. 6, pp. 1159–1168, 1951.
[61]
J. P. Apruzese, “An analytic Voigt profile escape probability approximation,” Journal of Quantitative Spectroscopy & Radiative Transfer, vol. 34, no. 5, pp. 447–452, 1985.
[62]
R. Doron, E. Behar, M. Fraenkel et al., “High-resolution x-ray spectrum of a laser-produced barium plasma in the 9.10-9.36-? wavelength range,” Physical Review A - Atomic, Molecular, and Optical Physics, vol. 58, no. 3, pp. 1859–1866, 1998.
[63]
R. Doron, M. Fraenkel, P. Mandelbaum, A. Zigler, and J. L. Schwob, “X-ray spectrum emitted by laser-produced barium plasma in the 8 to 13.5 ? wavelength range,” Physica Scripta, vol. 58, no. 1, pp. 19–24, 1998.
[64]
V. S. Belyaev, V. I. Vinogradov, A. S. Kurilov et al., “On the role of prepulses during solid target heating by picosecond laser pulses,” Journal of Experimental and Theoretical Physics, vol. 96, no. 5, pp. 897–903, 2003.
[65]
T. Auguste, P. D'Oliveira, S. Hulin, et al., “The role of the prepulse in cluster heating by a high-power femtosecond laser pulse,” Journal of Experimental and Theoretical Physics Letters, vol. 72, pp. 38–41, 2000.
[66]
A. S. Shlyaptseva, S. B. Hansen, V. L. Kantsyrev et al., “Advanced spectroscopic analysis of 0.8-1.0-MA Mo x pinches and the influence of plasma electron beams on L-shell spectra of Mo ions,” Physical Review E, vol. 67, no. 2, Article ID 026409, 2003.
[67]
A. Bar-Shalom, M. Klapisch, and J. Oreg, “Hullac, an integrated computer package for atomic processes in plasmas,” Journal of Quantitative Spectroscopy & Radiative Transfer, vol. 71, no. 2–6, pp. 169–188, 2001.
[68]
D. Mihalas, Stellar Atmosheres, Freeman, San Francisco, Calif, USA, 1978.
[69]
F. B. Rosmej, D. H. H. Hoffmann, M. Gei?el et al., “Advanced x-ray diagnostics based on an observation of high-energy Rydberg transitions from autoionizing levels in dense laser-produced plasmas,” Physical Review A. Atomic, Molecular, and Optical Physics, vol. 63, no. 6, Article ID 063409, 2001.
[70]
G. V. Brown, P. Beiersdorfer, D. A. Liedahl, K. Widmann, and S. M. Kahn, “Laboratory measurements and modeling of the Fe XVII X-ray spectrum,” Astrophysical Journal, vol. 502, no. 2, pp. 1015–1026, 1998.
[71]
G. V. Brown, P. Beiersdorfer, D. A. Liedahl, K. Widmann, S. M. Kahn, and E. J. Clothiaux, “Laboratory measurements and identification of the Fe XVIII-XXIV L-shell X-ray line emission,” Astrophysical Journal, vol. 140, no. 2, pp. 589–607, 2002.
[72]
L. Reale, A. Lai, I. Bellucci et al., “Microradiography as a tool to detect heavy metal uptake in plants for phytoremediation applications,” Microscopy Research and Technique, vol. 69, no. 8, pp. 666–674, 2006.