Abstract

Damaged regions of cylindrical shapes called ion tracks, typically in nano-meters wide and tens micro-meters long, are formed along the ion trajectories in many insulators, when high energy ions in the electronic stopping regime are injected. In most cases, the ion tracks were assumed as consequences of dense electronic energy deposition from the high energy ions, except some cases where the synergy effect with the nuclear energy deposition plays an important role. In crystalline Si (c-Si), no tracks have been observed with any monomer ions up to GeV. Tracks are formed in c-Si under 40 MeV fullerene (C60) cluster ion irradiation, which provides much higher energy deposition than monomer ions. The track diameter decreases with decreasing the ion energy until they disappear at an extrapolated value of ~ 17 MeV. However, here we report the track formation of 10 nm in diameter under C60 ion irradiation of 6 MeV, i.e., much lower than the extrapolated threshold. The diameters of 10 nm were comparable to those under 40 MeV C60 irradiation. Furthermore, the tracks formed by 6 MeV C60 irradiation consisted of damaged crystalline, while those formed by 40 MeV C60 irradiation were amorphous. The track formation was observed down to 1 MeV and probably lower with decreasing the track diameters. The track lengths were much shorter than those expected from the drop of Se below the threshold. These track formations at such low energies cannot be explained by the conventional purely electronic energy deposition mechanism, indicating another origin, e.g., the synergy effect between the electronic and nuclear energy depositions, or dual transitions of transient melting and boiling.

Highlights

  • We report the ion track formation in crystalline Si (c-Si) induced by ­C60+ ion irradiation between 1 and 6 MeV, which are much lower than the above-mentioned threshold of 17 MeV

  • The energy dependencies of the electronic and nuclear stopping powers, Se and Sn, of C­ 60 ions in c-Si are plotted in Fig. 1b, which were approximated as the sum of sixty independent carbon monomer ions with the energy of (E/60) each, and expressed as, Si(E, C60) = 60Si(E/60, C1)

  • At E > 20 MeV, Se is more than 10 times greater than Sn, and the former increases with the energy while the latter decreases

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Summary

Methods

Institute (TARRI), of the National Institutes for Quantum and Radiological Science and Technology (QST), using a 3 MV tandem accelerator and a newly developed high-flux ­C60 negative ion source. The samples were mostly irradiated to a low fluence of 5 × 1010 ­C60/cm[2] to avoid overlaps between the tracks. For precise control of the low fluence, the ion flux was reduced to below 50 pA through an aperture of 3 mm in diameter, while using the high-flux ion source. Since cos (7°) = 0.993, beams deviating from the normal incidence did not significantly modify the shapes of the tracks. Some samples were irradiated with 200 MeV X­ e14+ ions from the tandem accelerator in the Japan Atomic energy Agency (JAEA), Tokai Research and Development Center

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