Stability of C59 Knockout Fragments from Femtoseconds to Infinity

Author:

Gatchell MichaelORCID,Florin NaemiORCID,Indrajith SuvasthikaORCID,Navarro Navarrete José EduardoORCID,Martini PaulORCID,Ji MingChaoORCID,Reinhed Peter,Rosén StefanORCID,Simonsson AnsgarORCID,Cederquist HenrikORCID,Schmidt Henning T.ORCID,Zettergren HenningORCID

Abstract

Abstract We have studied the stability of C59 anions as a function of time, from their formation on femtosecond timescales to their stabilization on second timescales and beyond, using a combination of theory and experiments. The C 59 fragments were produced in collisions between C60 fullerene anions and neutral helium gas at a velocity of 90 km s−1 (corresponding to a collision energy of 166 eV in the center-of-mass frame). The fragments were then stored in a cryogenic ion beam storage ring at the DESIREE facility, where they were followed for up to 1 minute. Classical molecular dynamics simulations were used to determine the reaction cross section and the excitation energy distributions of the products formed in these collisions. We find that about 15% of the C 59 ions initially stored in the ring are intact after about 100 ms and that this population then remains intact indefinitely. This means that C60 fullerenes exposed to energetic atoms and ions, such as stellar winds and shock waves, will produce stable, highly reactive products, like C59, that are fed into interstellar chemical reaction networks.

Funder

Vetenskapsrådet

Knut och Alice Wallenbergs Stiftelse

Publisher

American Astronomical Society

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