Research summary

Sir Harry Kroto's main research areas and research highlights.

Flash photolysis diagram
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Main research areas

  • Spectroscopy of unstable species and reaction intermediates (Infrared, Photoelectron, Microwave and Mass Spectrometry)
  • Astrophysics (Interstellar Molecules and Circumstellar Dust)
  • Cluster science (Carbon and Metal Clusters, Microparticles, Nanofibres)
  • Fullerene chemistry, nanoscience and nanotechnology

Research highlights

  • first detection of 1Δ state of a polyatomic free radical (NCN by flash photolysis)
  • theoretical studies of ground and electronically excited sates of small molecules
  • detection of liquid phase intermolecular interactions using Raman Spectroscopy
  • breakthrough in the detection of new unstable species (thioaldehydes, thiocarbonyls thioborines) using combination of microwave and photoelectron spectroscopy techniques
  • synthesis in 1976 of the first phoaphaalkenes (compounds containing the free carbon phosphorus double bond) in particular CH2=PH (with N P C Simmons and J F Nixon, Sussex)
  • monograph “Molecular Rotation Spectra
  • synthesis in 1976 of the first analogues of HCP, the phosphaalkynes which contain the carbon phoshorus triple bond – in particular CH3CP (with N P C Simmons and J F Nixon, Sussex)
  • the discovery in 1976-8 of the cyanopolyynes, HCnN (n=5,7,9), in interstellar space (with D R M Walton, A J Alexander and C Kirby (Sussex) and T Oka, L W Avery, N W Broten and J M MacLeod (NRC Ottawa)), Ref 4-6, based on microwave measurements made at Sussex.
  • the discovery of C60: Buckminsterfullerene in 1985 (with J R Heath, S C O’Brien, R F Curl and R E Smalley)
  • the detection of endohedral metallofullerene complexes (with J R Heath, S C O’Brien, Q Zhang, Y Liu, R F Curl, F K Tittel and R E Smalley)
  • the prediction that C60 should be produced in combustion processes and might indicate how soot is formed (with Q L Zhang, S C O’Brien, J R Heath, Y Liu, R F Curl and R E Smalley)
  • the explanation of why C70 is the second stable fullerene (after C60) and the discovery of the Pentagon Isolation Rule as a criterion for fullerene stability in general
  • the prediction of the tetrahedral structure of C28 and the possible stability of “tetravalent” derivatives such as C28H4
  • in 1987 the first prediction that C60 and its analogues such as C60+, endohedral species M@C60, and complexes M.C60, will survive in space and are the best candidates for carriers of the diffuse interstellar bands
  • the prediction that giant fullerenes have quasi-icosahedral shapes and the detailed structure of concentric shell graphite microparticles (with K G McKay)
  • the mass spectrometric identification and solvent extraction (with J P Hare and A Abdul-Sada) of C60 from arc processed carbon in 1990 – independently from and simultaneously with the Heidelberg/Tucson group
  • the chromatographic separation/purification of C60 and C70 and 13C NMR measurements which provided unequivocal proof that these species had fullerene cage structures (with J P Hare and R Taylor, Sussex)
  • crystal structure of C60

Main Fullerene chemistry breakthroughs

  • C60(ferrocene)2
  • characterisation of C60Hal6
  • C60(P4)2

Nanoscience and Nanotechnology advances

  • condensed phase nanotubes
  • nanoscale BN structures
  • partly aligned-nanotube bundles
  • nanotube formation mechanisms
  • silicon oxide nanostructures
  • Si surface-deposited fullererene studies
  • insulated carbon nanotube conductors

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