TY - JOUR
T1 - Mechanism of the conversion of ethene to ethylidyne on rhodium (111): evidence for a vinylic intermediate
AU - Borg, H.J.
AU - van Hardeveld, R.M.
AU - Niemantsverdriet, J.W.
PY - 1995
Y1 - 1995
N2 - Temperature-programmed static secondary ion mass spectrometry (TPSSIMS) and temperature-programmed desorption (TPD) have been used to study the mechanism of ethene to ethylidyne conversion on Rh(111). Ethene is adsorbed molecularly on Rh(111) at 100 K. During temperature-programmed reaction of small coverages of ethene, hydrogen accumulates on the surface at 140 K, followed by the formation of ethylidyne at 190 K. Scission of a C—H bond being the first step in the decomposition of ethene points to a vinyl (either ¿1-CHCH2 or µ3-¿2-CHCH2) intermediate in the reaction to ethylidyne. The temperature at which the vinylic intermediate forms increases with increasing coverage until it coincides with the ethylidyne formation temperature, which remains at 190 K, irrespective of coverage. This behaviour is explained by an ensemble size requirement for C—H scission: the number of vacant ensembles decreases with increasing coverage, thus obstructing C—H cleavage, but increases again during the formation of ethylidyne. Similarities and differences in ethylidyne formation on Rh(111) and Pt(111) are discussed.
AB - Temperature-programmed static secondary ion mass spectrometry (TPSSIMS) and temperature-programmed desorption (TPD) have been used to study the mechanism of ethene to ethylidyne conversion on Rh(111). Ethene is adsorbed molecularly on Rh(111) at 100 K. During temperature-programmed reaction of small coverages of ethene, hydrogen accumulates on the surface at 140 K, followed by the formation of ethylidyne at 190 K. Scission of a C—H bond being the first step in the decomposition of ethene points to a vinyl (either ¿1-CHCH2 or µ3-¿2-CHCH2) intermediate in the reaction to ethylidyne. The temperature at which the vinylic intermediate forms increases with increasing coverage until it coincides with the ethylidyne formation temperature, which remains at 190 K, irrespective of coverage. This behaviour is explained by an ensemble size requirement for C—H scission: the number of vacant ensembles decreases with increasing coverage, thus obstructing C—H cleavage, but increases again during the formation of ethylidyne. Similarities and differences in ethylidyne formation on Rh(111) and Pt(111) are discussed.
U2 - 10.1039/ft9959103679
DO - 10.1039/ft9959103679
M3 - Article
SN - 0956-5000
VL - 91
SP - 3679
EP - 3684
JO - Journal of the Chemical Society, Faraday Transactions
JF - Journal of the Chemical Society, Faraday Transactions
IS - 20
ER -