Article
Plasma Investigations
2001. V. 39. № 1. P. 22–30
Vostrikov A.A., Dubov D.Yu., Agarkov A.A.
Inelastic interaction of an electron with a C60 cluster
Annotation
The method of intersecting beams of C60 fullerene clusters and of electrons is used to investigate the production of C+60 and C−60 ions and the radiation in the wavelength range from 300 to 800 nm for the electron energy Ee ranging from zero to 100 eV. The absolute values of the ionization and electron-attachment cross sections [σ+(Ee) and σ−(Ee), respectively] are determined. A maximum of σ+(Ee) of 0.53 nm2 is observed at Ee=52 eV. For a C60 cluster excited by electron impact, "delayed" (∼150μs) ionization initiated by collision with the surface and ionization due to thermionic emission (its characteristic time at Ee=60 eV is 6μs) is observed. It is found that, for Ee<0.4 eV, the formation of C−60 is defined by the polarization capture of an s-electron (σ−∼E−1e), and a formula is suggested for determining σ−(Ee). In the region of Ee from 1 to 6 eV, the cross section σ−(Ee) shows only slight variations about σ−(Ee)=0.36±0.03 nm2. For Ee>7.5 eV, C−60 ions proved to be unstable to electron autodetachment. In the region of intersection of C60 and electron beams, radiation of a quasicontinuous spectrum described by a modified Planck formula for the thermal emission of spherical particles of diameter d≪λ is recorded. For Ee>47 eV, the brightness temperature proved to be 3150±50 K. It is found that this radiation is emitted predominantly by hot C+∗60 ions produced as a result of thermionic emission from C∗60. The rate of radiation loss of energy by a C+∗60 ion and the cross section for the formation of radiating C+∗60 ions are found to be, respectively, 5.5×105 eV/s at T=3150 K and 2×10−2 nm2 at Ee=60 eV.
Article reference:
Vostrikov A.A., Dubov D.Yu., Agarkov A.A. Inelastic interaction of an electron with a C60 cluster, High Temp., 2001. V. 39. № 1. P. 22
Vostrikov A.A., Dubov D.Yu., Agarkov A.A. Inelastic interaction of an electron with a C60 cluster, High Temp., 2001. V. 39. № 1. P. 22