Formation of methane and cyclohexane through the hydrogenation of toluene
A. T. Hopkinson, F. G. Doktor, J. Pitfield, M. Moll, J. D. Thrower, L. Hornekær
TL;DR
This study investigates how a single methyl group in toluene affects hydrogen atom reactivity relevant to interstellar chemistry by exposing a toluene monolayer on graphite to H atoms and monitoring hydrogenation products with temperature-programmed desorption and mass spectrometry. The experiments reveal progressive hydrogenation to methyl-cyclohexane, followed by demethylation to cyclohexane and methane, with the initial H-addition cross-section significantly smaller than that of larger PAHs, consistent with a smaller molecular footprint. Complementary DFT calculations show substantial energy release during hydrogenation and identify feasible scission pathways that can liberate CH4 and generate radical species, potentially enabling further chemistry on grain surfaces. Collectively, the results illuminate how methylated PAHs may evolve in the ISM, contribute to small hydrocarbon formation, and influence PAH growth via hydrogenation and demethylation processes under varying radiation environments.
Abstract
Methylated polycyclic aromatic hydrocarbons (PAHs) have been hypothesised to be present in the interstellar medium (ISM) through their 3.4 and 6.9 $μ$m absorption bands. To investigate the hydrogenation of these methylated PAHs, the simplest, toluene ($\mathrm{CH_3C_6H_5}$), was exposed to H-atoms. This demonstrated how the presence of a methyl group changes the reactivity towards atomic hydrogen as compared to benzene and other PAHs and how this may alter its chemistry in the ISM. Toluene was deposited onto a graphite surface in an ultrahigh vacuum (UHV) chamber and then exposed to a H-atom beam. Temperature programmed desorption (TPD) measurements were used to investigate the reaction between H-atoms and toluene and the masses of hydrogenation products were measured with a quadrupole mass spectrometer (QMS). H-atom exposure of toluene leads to superhydrogenation of toluene and the formation of methyl-cyclohexane ($\mathrm{CH_3C_6H_{11}}$) at long exposure times. The initial cross-section of H-addition is lower than that of other PAHs. Methyl-cyclohexane can be further hydrogenated, leading to the detachment of the methyl group and production of cyclohexane ($\mathrm{C_6H_{12}}$) and methane ($\mathrm{CH_4}$). Toluene may be fully hydrogenated through its interaction with H-atoms, although it has a smaller initial cross-section for H-atom addition compared to other PAHs. This likely reflects it having a smaller geometric cross-section and the low flexibility of the benzene ring when undergoing sp$^3$ hybridization. The removal of the methyl group at high H-atom fluences provides a top down formation route to smaller molecules with the possibility of the formation of a radical cyclohexane combining with other species in an interstellar environment to form prebiotic molecules.
