AClassical Description >E = T + V Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  CSolve the Hamiltonian > Energy Levels E (n) = -R/n i 2 Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  CSolve the Hamiltonian > Energy Levels E (n) = -R/n i 2 DSelection Rules > Allowed Transitions  n = n 2 – n 1,  J = ±1 Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  CSolve the Hamiltonian > Energy Levels E (n) = -R/n i 2 DSelection Rules > Allowed Transitions  n = n 2 – n 1,  J = ±1 ETransition Frequencies >  F = - R[ 1/n 2 2 – 1/n 1 2 ] Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  CSolve the Hamiltonian > Energy Levels E (n) = -R/n i 2 DSelection Rules > Allowed Transitions  n = n 2 – n 1,  J = ±1 ETransition Frequencies >  F = - R[ 1/n 2 2 – 1/n 1 2 ] FIntensities > THE SPECTRUM Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  CSolve the Hamiltonian > Energy Levels E (n) = -R/n i 2 DSelection Rules > Allowed Transitions  n = n 2 – n 1,  J = ±1 ETransition Frequencies >  F = - R[ 1/n 2 2 – 1/n 1 2 ] FIntensities > THE SPECTRUM G Analysis > Pattern recognition; assign Q numbers Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  CSolve the Hamiltonian > Energy Levels E (n) = -R/n i 2 DSelection Rules > Allowed Transitions  n = n 2 – n 1,  J = ±1 ETransition Frequencies >  F = - R[ 1/n 2 2 – 1/n 1 2 ] FIntensities > THE SPECTRUM GAnalysis > Pattern recognition; assign Q numbers HExperimental Details > spectrometers, laser fluorescence Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  CSolve the Hamiltonian > Energy Levels E (n) = -R/n i 2 DSelection Rules > Allowed Transitions  n = n 2 – n 1,  J = ±1 ETransition Frequencies >  F = - R[ 1/n 2 2 – 1/n 1 2 ] FIntensities > THE SPECTRUM J Analysis > Pattern recognition; assign Q numbers HExperimental Details > spectrometers, laser fluorescence IMore Advanced Details > Relativistic Effects; Fermi contact term Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  CSolve the Hamiltonian > Energy Levels E (n) = -R/n i 2 DSelection Rules > Allowed Transitions  n = n 2 – n 1,  J = ±1 ETransition Frequencies >  F = - R[ 1/n 2 2 – 1/n 1 2 ] FIntensities > THE SPECTRUM J Analysis > Pattern recognition; assign Q numbers HExperimental Details > spectrometers, laser fluorescence IMore Advanced Details > Relativistic Effects; Fermi contact term JInformation obtainable from the spectrum > B values structures Harry Kroto 2004

AClassical Description >E = T + V B QM description > the Hamiltonian H  = E  CSolve the Hamiltonian > Energy Levels E (n) = -R/n i 2 DSelection Rules > Allowed Transitions  n = n 2 – n 1,  J = ±1 ETransition Frequencies >  F = - R[ 1/n 2 2 – 1/n 1 2 ] FIntensities > THE SPECTRUM J Analysis > Pattern recognition; assign Q numbers HExperimental Details > spectrometers, laser fluorescence IMore Advanced Details > Relativistic Effects; Fermi contact term JInformation obtainable from the spectrum > B values structures Harry Kroto 2004