Stability of C59 Knockout Fragments from Femtoseconds to Infinity

• Published in: The Astrophysical journal 2024-05, Vol.966 (2), p.146
• Main Authors: Gatchell, Michael, Florin, Naemi, Indrajith, Suvasthika, Navarro Navarrete, José Eduardo, Martini, Paul, Ji, MingChao, Reinhed, Peter, Rosén, Stefan, Simonsson, Ansgar, Cederquist, Henrik, Schmidt, Henning T., Zettergren, Henning
• Format: Article
• Language: English
• Subjects: Anions; Astrochemistry; Buckminsterfullerene; Chemical reactions; Collision physics; Collisions; Fragments; Fullerenes; Helium; Interstellar chemistry; Interstellar molecules; Ion beams; Ion-storage rings; Ions; Molecular dynamics; Shock waves; Stability; Stellar winds; Winds
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/ad3930

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 C59− 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 C59− 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.