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First high-resolution IR spectra of buckyballs

Advanced cooling and optical techniques made it possible

by Sam Lemonick
January 9, 2019 | APPEARED IN VOLUME 97, ISSUE 2


Credit: Michael Ströck/Wikimedia Commons
State-of-the-art techniques allowed scientists to obtain the first high-resolution infrared spectra of the buckyball.

Buckyballs’ large size and intricate structure have long captured scientists’ interest, even if practical applications for the 60-carbon molecules remain elusive. Now, more than 30 years after their discovery, scientists using cutting-edge techniques have captured high-resolution infrared spectra of buckyballs for the first time (Science 2019, DOI: 10.1126/science.aav2616).

The size and structure that make buckyballs so fascinating also frustrate spectroscopists. One atom’s rotation or vibration propagates across the molecule, producing a spectrum that looks more like a low hill than a series of sharp peaks. To get clear spectra, Jun Ye of the University of Colorado and colleagues first had to cool buckyballs down to near 100 K. Ye likens it to a crowd holding hands and dancing. Each person’s movement will cause their neighbors and their neighbors’ neighbors to move a little in response. At lower temperatures he says it’s like most of the dancers are lying down, allowing a small number of dancers’ movements to stand out. At room temperature, a buckyball has thousands of rotational and vibrational modes. That number approaches one at 100 K.

The researchers injected gas-phase buckyballs into a chamber of cold argon atoms, which cooled the buckyballs down as they collided with them. Then they used comb spectroscopy to see the movements happening in buckyballs, in which an optical comb produces a wide spectrum of light divided into discrete lines at different frequencies, like the teeth of a comb. The researchers could see which frequencies correspond to buckyball motion by looking at which teeth were knocked out or absorbed after interacting with the molecule. Ye’s group used mirrors in their cold cell to bounce the light back and forth tens of thousands of times, increasing the sensitivity of their measurements.

“It is a spectroscopic tour-de-force,” says Daniel Neumark, a spectroscopist at the University of California, Berkeley. He says spectroscopists usually throw their hands up at molecules this large, but that state-of-the-art technology made this work possible.

Ye says their spectra largely confirm the past 20 years of theoretical work on C60 fullerene, but notes there is one discrepancy between simulated spectra and what the group observed. The researchers say simulated spectra fail to predict transitions that are likely due to centrifugal distortion caused by the buckyballs’ motions. They’re still trying to understand those higher-order effects to reach a more complete understanding of the buckyball.



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Dr.Paul C. Li (April 15, 2019 5:55 AM)
Dear Honorable Pioneering IR Spectroscopists: What a great achievement in the real world of spectroscopy. Thank you the outstanding publication got me re-educated called rotational vibrational modes in gas phase.
I personally, used an empirical equation initiated by Richar M. Badger to estimate the force constant k between two half shells in C60. A speherical breathing mode according to the radius of fulleren could be roughly matched where u, the reduced mass of two shells containing 30 carbons in each is assumed and delta X, the maximal extension of the ring size so as to get a good match
Any one can do this with ease.
Submitted to your attention by a life long chemist in humbleness.

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