CF3Br agust,www,....cf3br/PPT ak.ppt agust,heima,....Sept10/XLS ak.xls

Slides:



Advertisements
Similar presentations
I 2 fs REMPI 1) Energetics / excitation calculations....slide 2 2) Absorption spectrum slides 3-6 3)REMPI spectrum slide.
Advertisements

CH3Br, Energy for CH3Br ->->-> CH3 + Br
Molecular Bonds Molecular Spectra Molecules and Solids CHAPTER 10 Molecules and Solids Johannes Diderik van der Waals (1837 – 1923) “You little molecule!”
CH3Br, Relative ion signals (I(M + )/I(CH 3 + )) vs Rydberg states agust,www,....Nov09/PPT ak.ppt agust,heima,...CH3Br-Overall +mass km ak.pxp.
CH2Br2: 1) Absorption 2) REMPI scans: overview (slides 12-15) 3) C+ REMPI vs absorption spectrum agust,www,....ch2br2/PPT ak.ppt agust,heima,...CH2Br2/PXP ak.pxp.
CF3Br Literature survey on energetics: agust,www,....cf3br/PPT ak.ppt Updated: ; 13:35 o´clock.
CH2Br2 agust,www,....ch2br2/PPT ak.ppt agust,heima,....CH2Br2/Long, Sept-11/Merged CH2Br2 spectra jlak.pxp agust,heima,....CH2Br2/Long, Sept-11/Merged.
HBr, F1D2, v´=1
Spectroscopy Molecules move Movement can be monitored with electromagnetic radiation, e.g. light.
HBr, F 1  2, v´=1
Physics for Scientists and Engineers, 6e Chapter 43 - Molecules and Solids.
CH3Br, HBr detection agust, www,...Sept09/PPT ak.ppt.
CF3Br Data handeling agust,heima,....CF3Br/Sept-10/PXP ak.pxp : agust,heima,....CF3Br/Sept-10/XLS ak.xls agust, www,......cf3br/PPT ak.ppt.
CH 3 Br: & Literature survey on Direct ion-pair state excitation vs Ion pair fomation via initial Rydberg state excitation (Rydberg doorway.
1 CH 3 Br Br atomic lines. summary : agust. heima.....Sept09/Br Atomic lines vhw.ppt agust. heima.....Sept09/Br Atomic lines summary vhwak.xls.
CH3Br, )PD summary status 2)Thresholds for direct excitations 3)CH3+ formation energetics / thresholds (direct and indirect)/ PD agust, heima,.....Dec09/CH3Br-Overall.
CH 2 Br 2 agust,www,...rempi/ch2br2/PPT ak.ppt agust,heima,....CH2Br2/Long, Sept-11/Merged CH2Br2 spectra jl ak.pxp.
CF3Br agust,heima,....CF3Br/Sept10/PXP ks/Br 1D-REMPImW ks ak.pxp agust,heima,....CF3Br/Sept10/PXP ks/Br 1D-REMPImW ks ak.pxp.
CF3Br agust,heima,....Mars11/XLS ak.xls agust,www,......April11/PPT ak.xls agust,heima,....Mars11/PXP ak.pxp agust,heima,....Mars11/CF3HBr.
CH3Br, HBr spectra Agust, heima,... Jan10/CH3Br18750_19250-Hbr-sim km ak.pxp Agust, www,...Jan10/PPT ak.ppt.
CH3Br, Relative ion intensities and trend summary & “impurity threshold” agust,heima,...Nov09/CH3Br-Overall +mass km ak.pxp agust,heima,...Nov09/CH3Br-Overall.
1 CH3Br, C, C* and C** dissociation formation channels vs C+ spectra Explanation for enhanced C+ Rydberg state spectra in the cm-1.
Agust,heima,...january09/PPT ak.ppt cm cm-1 F, v´= cm-1 Agust,heima,..january09/PXP ak.pxp.
1 CH3Br, agust, heima,....Sept09/XLS ak.xls agust, www,....Sept09/PPT ak.ppt agust,heima,....Sept09/C ion lines vhw.pxp.
CH3Br agust,www,...Sept09/PPt ak.ppt agust,heima,....Sept09/CH3BR avhwak.pxp agust,heima,....Sept09/CH3BR bvhwak.pxp.
CF3Br, Impurity background correction: agust,www,...cf3br/PPT ak.ppt PC,LHj,...CF3Br/PXP ak.pxp agust,heima,...
Time out—states and transitions Spectroscopy—transitions between energy states of a molecule excited by absorption or emission of a photon h =  E = E.
TOPIC D: SPECTROMETRY AND SPECTROSCOPY. Mass spectrometry is used to detect isotopes. mass spectrometer uses an ionizing beam of electrons to analyze.
HCl, negative ion detections 1hv ion-pair spectra (slides 3-4) Loock´s prediction about H+ + Cl- formation channels(slides 5-6) Energetics vs Dye for V(v´= )
HI Relevant to the HI- Perturb.II paper:pages: H(2) ion intensities (system (b))………………………2-9
Electronic spectroscopy of CHBr and CDBr Chong Tao, Calvin Mukarakate, Mihaela Deselnicu and Scott A. Reid Department of Chemistry, Marquette University.
1.1Excited electronic states Each electron has unique set of quantum numbers (Pauli Exclusion Principle) n principle (1s, 2s, 3s,…) langular momentum (l.
Liquid Oxygen is Blue, Why? The electronic properties of oxygen (i.e. the distribution of electrons) give rise to some interesting optical properties -
Eirík´s project(?) CH3I: agust,www,...rempi/ch3i/PPT ak.ppt ( )
Of all the transitions that are allowed, how do I figure out intensities?
PHOTOFRAGMENTATIONS, STATE INTERACTIONS AND ENERGETICS OF HALOGEN CONTAINING MOLECULES: TWO-DIMENSIONAL (2+n) REMPI ÁGÚST KVARAN, et al. Science Institute,
HCl, E(v´=2) agust,www,…..hcl/June11/PPT ak.ppt agust,heima,…HCl/June11/HCl E2 spectra jl.pxp agust,heima,…HCl/June11/HCl E2 spectra jlaka.pxp.
LITERATURE SEARCH ASSIGNMENT A) Properties of diatomic molecules A diatomic molecule is a molecule composed of two atoms. For homonuclear diatomics the.
HBr; Updated: Imaging experiments in Crete Labtop..C:……/Crete/HBr/PPT aka.pptx &
MD (here)MD*EXP (kcal/mole)  (D) D (cm/s) 298K ENHANCED H ION TRANSPORT AND HYDRONIUM ION FORMATION T. S. Mahadevan.
HBr Energetics agust,www,....hbr/PPT ak.ppt agust, heima,...HBr/XLS ak.xls.
2.4 CLASSIFICATION OF UV ABSORPTION BANDS
CH3Br, one-color exp.: CHn+, iBr+ and CiBr+ ions vs CH3Br(Ry) states: Content: pages:
CH3Br, (2+n)REMPI spectra assignments for region – cm-1
Molecular Spectroscopy
CH3Br, one-color exp.: CHn+, iBr+ and CiBr+ ions vs CH3Br(Ry) states: Content: pages:
CH3I VMI-REMPI data and analysis:
Eirík´s project(?) CH3I: agust,www,...rempi/ch3i/PPT ak.ppt
Introduction and Principle of IR Spectrophotometry
Updated (p:15-16, refs. & p:50-51)
First principles calculation on field emission of boron/nitrogen doped carbon nanotube I’m going to talk about the first principles calculation on field.
DCl (HCl) Heavy Rydberg states work Exploring V state spectra
Resolution of Transient States of Nitrile Anions via Photodissociation Action Spectroscopy; Our Progress to Date The 2 traces show resonant Cu atomic.
H(0), one-color, VMI and slicing images
Chapter 13, Unnumbered Figure 1, Page 535
2 color VMI exp. CH3(X;v1v2v3v4) detection; hi
VMI-fitting results for V(m+i), i=4-10
6pp 3S- vs l / J´ Updated: One color, H+ detection: pages
HBr Mass resolved REMPI and Imaging REMPI.
HBr, dep. Calc. E0,Vm+4,Vm+5
HBr 6pp.. vs. V(m+17) state interactions.
CH3I VMI-REMPI data and analysis:
1hv spectrum corrected/shifted
HI Absorption REMPI references (slide 9) Energetics (slides 10-)
CH3Br Negative particle detections; Electrons /PES:
HBr The cm-1 system (slides 2-16)
Bgr nLASER/ cm
HCl, Deperturbation E1, V14, V15 (slides 2-7 )
Br+ (n=?) agust,heima,...Sept10/Br ks ak.ppt
MODE SPECIFIC DYNAMICS IN THE PREDISSOCIATED, QUASILINEAR
Presentation transcript:

CF3Br agust,www,....cf3br/PPT-081210ak.ppt agust,heima,....Sept10/XLS-081210ak.xls agust, heima,...PXP-291110ks/Leiðrétt-291110ks-081210ak.pxp (CF3+) agust,heima,... PXP-291110ks/Br 1D-REMPImW-291110ks-081210ak.pxp (Br+)

Bond dissociation for CF3Br revisited: The value used in http://notendur.hi.is/agust/rannsoknir/rempi/cf3br/PPT-090910ak.ppt (25 986.80 cm-1)is based on a paper from 1966 (see slide 3 in http://notendur.hi.is/agust/rannsoknir/rempi/cf3br/PPT-090910ak.ppt) The value used by Suto and Lee (JCP, 79(3), 1127, (´83) (see: http://notendur.hi.is/agust/rannsoknir/papers/jcp79-1127-83.pdf page 1131), based on Thermochemical data (Okabe, “Photochemistry of small molecules”, (1978)) is 2.98 eV (*8065.54093 cm-1/eV) = 24035.31 cm-1 which is is significantly lower. CF3+ + Br- threshold revisited: This affects the estimate of the CF3+ + Br- threshold: E(CF3+ + Br-) = 24035.31 + 72912.48 - 27129.17 = 69818.62197 cm-1 agust,heima,....Sept10/XLS-081210ak.xls

CF3* + Br thresholds: Suto and Lee (JCP, 79(3), 1127, (´83) (see: http://notendur.hi.is/agust/rannsoknir/papers/jcp79-1127-83.pdf page 1132): UV spectrum: 6.38 + 2.98 eV =.... 75493.46 cm-1 Vis spectrum: 6.36 + 2.98 eV = ....75332.15 cm-1

UV spectrum: 75493.46 cm-1 Vis spectrum: 75332.15 cm-1 CF3* + Br thresholds agust, heima,...PXP-291110ks/Leiðrétt-291110ks-081210ak.pxp

CF3* + Br thresholds UV spectrum: 75493.46 cm-1 Vis spectrum: 75332.15 cm-1 agust,heima,... PXP-291110ks/Br 1D-REMPImW-291110ks-081210ak.pxp

Now let´s look at the energetics with respect to CF3+ formation via CF3* formation (see fig. Next slide)

(Semi) schematic energy figure: E/cm -1 CF3 + + Br 96947.79 cm-1 CF3Br+ + e- 91980 cm-1 80 000 cm-1 CF3 * + Br 75493.46/75332.15 cm-1 CF3 + + Br- 69818.62 cm-1 {CF3+Br-}? Ion-pair state? ca. 24035.31 cm-1 CF3 + Br CF3Br(?) R(CF3 –Br) Agust,heima,...CF3Br/Sept10/PXP-081210ak.pxp; Layout::0, Graph: 0, Table::0

Possible dissociation mechanism(1): Ry -> Ion-pair -> CF3+ + Br- formation E/cm -1 CF3 + + Br 96947.79 cm-1 CF3Br+ + e- 91980 cm-1 (1) 80 000 cm-1 CF3 * + Br CF3 + + Br- 75493.46/75332.15 cm-1 CF3 + + Br- 69818.62 cm-1 {CF3+Br-}? Ion-pair state? ca. 24035.31 cm-1 CF3 + Br CF3Br(?) R(CF3 –Br) Agust,heima,...CF3Br/Sept10/PXP-081210ak.pxp; Layout::0, Graph: 0, Table::0

Possible dissociation mechanism(2): Ry -> CF3* + Br dissociation E/cm -1 CF3 + + Br 96947.79 cm-1 CF3Br+ + e- 91980 cm-1 (2) 80 000 cm-1 CF3 * + Br 75493.46/75332.15 cm-1 CF3 + + Br- 69818.62 cm-1 {CF3+Br-}? Ion-pair state? ca. 24035.31 cm-1 CF3 + Br CF3Br(?) R(CF3 –Br) Agust,heima,...CF3Br/Sept10/PXP-081210ak.pxp; Layout::0, Graph: 0, Table::0

This brake in CF3+ intensity could be because UV spectrum: 75493.46 cm-1 Vis spectrum: 75332.15 cm-1 This brake in CF3+ intensity could be because -for 2hv < 75332 cm-1 only channels occurs (i.e. CF3Br** ->-> CF3+ + Br-) b) for hv > 75332 cm-1, competition Between (1)(direct CF3+ formation) and (2)(CF3* formation) However based on PD data the observed CF3+ signal all over most probably is mainly due to (1) (i.e. direct CF3+ formation) CF3* + Br thresholds agust, heima,...PXP-291110ks/Leiðrétt-291110ks-081210ak.pxp

Now let´s compare the “spin-orbit splitting” structure observed in the fluorescenec Spectrum for CF3Br and mentioned by Suto and Lee (JCP, 79(3), 1127, (´83) (see: http://notendur.hi.is/agust/rannsoknir/papers/jcp79-1127-83.pdf page 1132), i.e.

Fluorescence maxima (a) (b) (c) (d) agust, heima,...PXP-291110ks/Leiðrétt-291110ks-081210ak.pxp

The fluorescenec maxima do not match CF3+ signal maxima The fluorescenec maxima do not match CF3+ signal maxima. On the contrary It looks more as if the maxima are in between peaks or close to minima in CF3+ signals (peaks (a)- (c). This could further indicate that there is a competition between channels (1) and (2)! http://notendur.hi.is/agust/rannsoknir/papers/jcp101-2069-94.pdf : 2) 11.7 eV 1) 11.4 eV Try to search for systematic spacing between peaks close to 0.3 and 0.46 eV:

Now let´s look at quantum defects: 0.3 eV 0.46 eV 0.2 eV 0.264 eV 0.35 eV 1) En = 74546.9 cm-1 = 9.24 eV 2) En = 9.24+0.3 = 9.24 eV agust, heima,...PXP-291110ks/Leiðrétt-291110ks-081210ak.pxp

= n – sqrt(R/(EI-En)); n = 5, R = 13.61 eV 1) d = 2.5 2) d = 2.5 Which is what one might expect for d for R-Br, p orbitals (and better value than that given by Eden et al. (http://notendur.hi.is/agust/rannsoknir/papers/cp323-313-06.pdf ) of 2.71) : See: http://notendur.hi.is/agust/rannsoknir/papers/jpcA112-7170-08.pdf (CH3Br) and http://notendur.hi.is/agust/rannsoknir/papers/CP148-315-90.pdf (Br2) Ergo: I conclude that the peaks at 1) just below 76000 cm-1 and 2) ca 78000 cm-1 are due to transitions to the Rydberg states: 1) [CF3Br+ (X 2E3/2)]c 5p and 2) [CF3Br+ (X 2E1/2)]c 5p Possibly the peak near 80500 cm-1 is due to transition to [CF3Br+ (A 2E1/2)]c 5p

but what about the “peak” just below 77000 cm-1, i ...but what about the “peak” just below 77000 cm-1, i.e ca 1000 cm-1 above The peak for [CF3Br+ (X 2E3/2)]c 5p . Could that be a vibrational Band? NIST => ERGO: yes it could indeed be a vibrational band such as CF3 stretching(?)