1997
DOI: 10.1063/1.473097
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Impact induced vibrational excitation in surface scattering of hyperthermal neutral C60 molecule

Abstract: Articles you may be interested inAn advanced molecule-surface scattering instrument for study of vibrational energy transfer in gas-solid collisions Rev. Sci. Instrum. 78, 104104 (2007); 10.1063/1.2796149Theoretical investigation of the stability of highly charged C 60 molecules produced with intense near-infrared laser pulses Negative ion formation in near grazing surface scattering of hyperthermal neutral C 60 : Image charge effects

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Cited by 38 publications
(14 citation statements)
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“…More energy is imparted to the film as the projectile velocity increases, making the collision less elastic. This description of reflection is consistent with C 60 -graphite simulations involving the Brenner [20] and Takai-Lee-Halicioglu-Tiller potentials [9] as well as with experiment [15,17]. There are also similarities to the qualitative reflection mechanism in surface impact studies of C 60 and a diamond surface [21].…”
Section: Resultssupporting
confidence: 80%
“…More energy is imparted to the film as the projectile velocity increases, making the collision less elastic. This description of reflection is consistent with C 60 -graphite simulations involving the Brenner [20] and Takai-Lee-Halicioglu-Tiller potentials [9] as well as with experiment [15,17]. There are also similarities to the qualitative reflection mechanism in surface impact studies of C 60 and a diamond surface [21].…”
Section: Resultssupporting
confidence: 80%
“…Finally, with the help of Eq. (13) and using the canonical expression from Tsipinyuk et al [29], an explicit approximate relation between the internal energy and the microcanonical temperature is obtained:…”
Section: ͑23͒mentioning
confidence: 99%
“…1, this expression leads to Ē v − ZPE ϵ E v eff Ϸ 79, 103, and 134 eV for E 0 = 300, 600, and 900 eV correspondingly ͑here ZEP is the C 60 zero point energy and equals 9.7 eV͒. 20 These values of E v eff exceed ͑or are nearly the same as͒ the normal components of the kinetic energy loss of the precursor species calculated as ⌬E Ќ ͑E 0 ͒ = ͓E 0 cos 2 i − n͑E 0 ͒cos 2 r ͔: 52, 103, and 152 eV correspondingly ͑ i = 63°, r = 72°͒. Taking into account also an appreciable part ␤ of ⌬E Ќ which is lost to surface excitation, one gets E v eff ӷ ͑1−␤͒⌬E Ќ ͑E 0 ͒, thus leading to the conclusion that a substantial part of E v eff is contributed by the parallel component of the kinetic energy loss ⌬E ʈ .…”
Section: Maxwellianmentioning
confidence: 98%