High-harmonic generation in lanthanide-containing plasmas
Source abstract
Abstract
High-order harmonic generation (HHG) in atoms and molecules allows the study of the static and dynamic properties of these systems. We present the results of HHG studies in the plasmas produced using femtosecond and picosecond laser pulses on the surfaces of lanthanides and their oxides (La, Yb, Pr6O11, and Tb4O7). The plasmas induced by femtosecond pulses have proven to be a more efficient medium for HHG than the plasmas produced by picosecond pulses in the case of two-color pump HHG. We analyze the advantages of laser ablation using femtosecond pulses for the extension of the cutoff energy of generated harmonic in lanthanide plasma. We have shown that Yb plasma is the efficient medium for the harmonic generation up to the 73rd order, which is one of the largest orders generated in laser-produced plasmas.
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Research context
OpenAlex topics: Laser-Matter Interactions and Applications · Laser-induced spectroscopy and plasma · Mass Spectrometry Techniques and Applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Physics, American University of Sharjah 1 , P.O. Box 26666, Sharjah, United Arab Emirates
Faculty of Physics, National University of Uzbekistan 2 , Tashkent 100174, Uzbekista
Faculty of Physics, Voronezh State University 3 , Voronezh 394006, Russia
References (38)
Show source-provided references
1. J. Opt. Soc. Am. B · 1987 · 4 · 59510.1364/josab.4.000595 ↗
2. J. Phys. B · 1988 · 21 · L3110.1088/0953-4075/21/3/001 ↗
3. Phys. Rev. Lett. · 1992 · 69 · 217610.1103/physrevlett.69.2176 ↗
4. Opt. Commun. · 1997 · 135 · 25110.1016/s0030-4018(96)00633-5 ↗
5. Phys. Rev. Lett. · 1992 · 68 · 353510.1103/physrevlett.68.3535 ↗
6. Phys. Rev. Lett. · 1993 · 71 · 199410.1103/physrevlett.71.1994 ↗
7. Phys. Rev. A · 1994 · 49 · 211710.1103/physreva.49.2117 ↗
8. Phys. Rev. A · 2007 · 76 · 02380510.1103/physreva.76.023805 ↗
9. Phys. Rev. A · 2009 · 79 · 02380710.1103/physreva.79.023807 ↗
10. Appl. Phys. Lett. · 2011 · 98 · 10110410.1063/1.3558999 ↗
11. Opt. Express · 2011 · 19 · 367710.1364/oe.19.003677 ↗
12. New J. Phys. · 2013 · 15 · 01305110.1088/1367-2630/15/1/013051 ↗
13. J. Appl. Phys. · 2014 · 115 · 03310410.1063/1.4862302 ↗
14. Phys. Rev. Lett. · 2015 · 115 · 13390110.1103/physrevlett.115.133901 ↗
15. Appl. Phys. Lett. · 2016 · 108 · 12410410.1063/1.4944640 ↗
16. Nat. Commun. · 2017 · 8 · 1606110.1038/ncomms16061 ↗
17. Opt. Express · 2018 · 26 · 1452410.1364/oe.26.014524 ↗
18. Opt. Express · 2018 · 26 · 1574510.1364/oe.26.015745 ↗
19. Phys. Rev. Lett. · 2018 · 121 · 02320110.1103/physrevlett.121.023201 ↗
20. Phys. Rev. A · 2019 · 99 · 06342010.1103/physreva.99.063420 ↗
21. J. Appl. Phys. · 2019 · 125 · 15590210.1063/1.5093575 ↗
22. J. Phys. B: At., Mol. Opt. Phys. · 2012 · 45 · 07401710.1088/0953-4075/45/7/074017 ↗
23. OSA Continuum · 2019 · 2 · 238110.1364/osac.2.002381 ↗
24. Phys. Rev. A · 2012 · 85 · 02383210.1103/physreva.85.023832 ↗
25. Phys. Rev. A · 2011 · 83 · 01382010.1103/physreva.83.013820 ↗
26. Phys. Rev. A · 2014 · 89 · 03382110.1103/physreva.89.033821 ↗
27. 2012
28. Phys. Rev. Lett. · 2005 · 94 · 24390110.1103/physrevlett.94.243901 ↗
29. Phys. Rev. Lett. · 2006 · 97 · 01300110.1103/physrevlett.97.013001 ↗
30. Phys. Rev. A · 2009 · 80 · 03384510.1103/physreva.80.033845 ↗
31. Phys. Rev. A · 2010 · 82 · 05383110.1103/physreva.82.053831 ↗
32. Appl. Phys. Lett. · 2008 · 92 · 02112510.1063/1.2836252 ↗
33. Phys. Rev. A · 2005 · 71 · 06380810.1103/physreva.71.063808 ↗
34. Phys. Rev. A · 2006 · 74 · 06382410.1103/physreva.74.063824 ↗
35. Phys. Rev. A · 2007 · 76 · 02383210.1103/physreva.76.023832 ↗
36. Appl. Surf. Sci. · 1998 · 127-129 · 19310.1016/s0169-4332(97)00631-4 ↗
37. Phys. Rev. A · 2007 · 75 · 03380410.1103/physreva.75.033804 ↗
38. J. Phys. B: At., Mol. Opt. Phys. · 2012 · 45 · 16540210.1088/0953-4075/45/16/165402 ↗