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HI Absorption REMPI references (slide 9) Energetics (slides 10-) Files: www= open; heima: closed agust,www,...hi/PPT ak.ppt ( agust,heima,...HI/PXP ak.pxp (abs. spectrum) ( ) agust,heima,...HI/PXP ak.pxp (energetics) ( ) agust,heima,....HI/XLS ak.xls ( ) o.fl.
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Slide 4 Slide 5 Slides 6 and 7 & IGOR
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https://notendur.hi.is/agust/rannsoknir/papers/jesrp144-127-05.pdf :
nm agust,heima,...HI/PXP ak.pxp =
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https://notendur.hi.is/agust/rannsoknir/papers/jesrp144-127-05.pdf :
nm agust,heima,...HI/PXP ak.pxp =
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https://notendur.hi.is/agust/rannsoknir/papers/jesrp144-127-05.pdf :
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2) REMPI references: i.e: And our paper from 1998: Abs. Ref.:
i.e: And our paper from 1998: Abs. Ref.: :HI DI See more in slide 23
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3) Energetics: : H & H (book): D00= 3.054(1) eV
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NIST:
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HI D: 295 kJ mol-1 cm-1 3.054 eV H&H book Factors: f1: 8.36E+01 cm-1 / (kJ mol-1) f2: 3.50E+02 cm-1 / (kcal mol-1) f3: cm-1/eV E(6s) = E(6s)+D= IE(HI)= 10.386 IE(I)= E(S/O;I)= E(H+I*(1/2))= E(H+I+ + e)= IE(H) = E(H+ + e + I) EA(I) = E(H+ + I-)= E(I+)-E(I*)= agust,heima,....HI/XLS ak.xls; =
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cm-1 H+ + e + I; H+ + I H + I+ + e; HI+ + e; H + I**(min) H + I* H + I cm-1 HI agust,heima,...HI/PXP ak.pxp (energetics)=
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Abs. spectrum HI+ + e; 83768.7081 74000 cm-1 64500 cm-1 HI
H+ + e + I; H+ + I H + I+ + e; Abs. spectrum HI+ + e; H + I**(min) 74000 cm-1 64500 cm-1 H + I* H + I cm-1 HI
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74000 cm-1 72618.17 Threshold for H + I+ +e 64500 cm-1 73092.05
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HI+ + e; 83768.7081 74000 cm-1 Abs. spectrum 64500 cm-1 The A-band
64500 cm-1 The A-band x100
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Experiments:
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THE first HI-REMPI data!:
Dye: C540A
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Is this I atomic line? Dye: C540A 70814.3 cm-1 Large I(I+)/I(HI+)
Is this I atomic line? cm-1 Dye: C540A Large I(I+)/I(HI+) ratio! ..and seems to increase with J´(?) 70854 cm-1
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NIST (http://www.nist.gov/pml/data/asd.cfm ):
I atomic line: 1.5 0.5 exp. Peak NIST ( ): i.e. 5s25p4(1D2)6p, 2[1]°, (J=3/2) <-<- 5s25p5 2P° (J=1/2) and (5s25p4(3P0)7s, 2[0] , (J=1/2) <-<- 5s25p5 2P° (J=1/2)) The latter of which should not be allowed (s <-<- p)
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ERGO: one would indeed expect the I(I+)/I(HI+)
Judging from E(v´=0) is very close to V(v´=m+6), which is slightly higher in energy: ERGO: one would indeed expect the I(I+)/I(HI+) ratio to increase with J´ (see slide 19)
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The first data are promishing, indeed!
Abs. Spectra and assignments: :
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