CH 2 Br 2 agust,www,...rempi/ch2br2/PPT ak.ppt agust,heima,....CH2Br2/Long, Sept-11/Merged CH2Br2 spectra jl ak.pxp

agust,heima,....CH2Br2/Long, Sept-11/Merged CH2Br2 spectra jl ak.pxp; Gr4, Lay0 Br(1/2) ( 3 P 2 )5p( 3 P 1 )5p( 3 P 0 )5p( 3 P 2 )6p Br(3/2) ( 3 P 2 )5p( 3 P 1 )5p( 3 P 0 )5p

Br(1/2) Br(3/2) agust,heima,....CH2Br2/Long, Sept-11/Merged CH2Br2 spectra jl ak.pxp; Gr4, Lay0

Comments: It is interesting to see that the Br(3/2) atomic lines, generally, are much stronger than the Br(1/2) lines. Similar effect was seen for CF 3 Br except for atomic lines close to cm -1 (article). Similar effect was also seen for CH 3 Br, but not as dramatic differencearticle This suggests that formation of Br(3/2) is favored over Br(1/2). Lets compare this with photodissociation studied via excitations to repulsive states. The Br atomic peaks at and cm-1 (Br(3/2) ->->( 3 P 0 )5p)are enhanced (compared to both CF 3 Br and CH 3 Br) and happen to coinside with the Rydberg state peak(s) near cm -1 which has been assigned to a 6d Rydberg state (?) ( This strongly suggests that indeed the corresponding Br(3/2) atoms are formed via excitation to thehttp://notendur.hi.is/agust/rannsoknir/rempi/ch2br2/PPT ak.ppt Rydberg state (6d). Lets compare the Br atomic line spectra from the three compounds (CH 3 Br, CF 3 Br and CH 2 Br 2 by putting them all into one PXP file /figure.