ELECTRON SPECTROSCOPY AND ELECTRON SPECTROSCOPY AND MASS SPECTROMETRIC STUDY MASS SPECTROMETRIC STUDY OF PENNING IONIZATION OF OF PENNING IONIZATION OF MOLECULES MOLECULES F. Vecchiocattivi F. Vecchiocattivi Dipartimento d’Ingegneria Civile ed Ambientale Dipartimento d’Ingegneria Civile ed Ambientale Università degli Studi di Perugia Università degli Studi di Perugia Perugia - Italy Perugia - Italy
40
Embed
ELECTRON SPECTROSCOPY AND MASS SPECTROMETRIC STUDY OF PENNING IONIZATION OF MOLECULES
ELECTRON SPECTROSCOPY AND MASS SPECTROMETRIC STUDY OF PENNING IONIZATION OF MOLECULES. F. Vecchiocattivi Dipartimento d’Ingegneria Civile ed Ambientale Università degli Studi di Perugia Perugia - Italy. … it’s elementary, my dear Watson. The Penning ionization process …. (1894-1953). - PowerPoint PPT Presentation
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
ELECTRON SPECTROSCOPY ELECTRON SPECTROSCOPY AND MASS SPECTROMETRIC AND MASS SPECTROMETRIC
STUDY OF PENNING STUDY OF PENNING IONIZATION OF MOLECULESIONIZATION OF MOLECULES
F. VecchiocattiviF. Vecchiocattivi Dipartimento d’Ingegneria Civile ed Ambientale Dipartimento d’Ingegneria Civile ed Ambientale Università degli Studi di PerugiaUniversità degli Studi di PerugiaPerugia - ItalyPerugia - Italy
… … it’s elementary, my dear Watson.it’s elementary, my dear Watson.
The Penning ionization process …The Penning ionization process …
(1894-1953)
F. M. Penning,Naturwissenschaften 15, 818 (1927)
(1894-1953)
A* + M A* + M (A…M)* (A…M)* (A…M) (A…M)++ + e + e--
Perugia molecular beam Perugia molecular beam apparatus for Penning apparatus for Penning ionization studiesionization studies
He*(2He*(211S, 2S, 233S) + Ar S) + Ar He + ArHe + Ar++((22PP3/23/2, , 22PP1/21/2) + e) + e--
0.01 0.1 1
1
10
100
Collision energy (eV)
Ioni
zatio
n cr
oss
sect
ion
(Å2 ) Ar+
HeAr+
He*(2He*(233S) + Ar S) + Ar He + Ar He + Ar++((22PP1/21/2) + e) + e--
He*(2He*(211S) + Ar S) + Ar He + Ar He + Ar++((22PP3/23/2) + e) + e--
He*(2He*(211S) + Ar S) + Ar He + Ar He + Ar++((22PP1/21/2) + e) + e--
He*(2He*(233S) + Ar S) + Ar He + Ar He + Ar++((22PP3/23/2) + e) + e-- 3,3/23,3/2
3,1/23,1/2
1,3/21,3/2
1,1/21,1/2
3,3/2
3,1/2= 2.1±0.2
3.6 3.8 4.0 4.2 4.4 4.6 4.8
Ar+(2P1/2
)
Ar+(2P1/2
)
Ar+(2P3/2
)
Ar+(2P3/2
)
He*(21S)-Ar
He*(23S)-Ar
Electron energy (eV)
B. Brunetti, P. Candori, S. Falcinelli, B. Lescop, G. Liuti, F. Pirani, F. Vecchiocattivi (2005) to be published
He*(He*(33S) + Ar S) + Ar [He-Ar]* [He-Ar]* [He-M][He-M]++ + e + e--
He*(He*(33S)S) ArAr
HeHeArAr++
He + ArHe + Ar++((22PP1/21/2))
He + ArHe + Ar++((22PP3/23/2))
The relative population of the J=1/2 and J=3/2 states of the Ar+ product practically reflects the character of the final He-Ar+ state.
Ne*(Ne*(33PP2,02,0) + Ar ) + Ar [Ne-Ar]* [Ne-Ar]* [Ne-M][Ne-M]++ + e + e--
Ne*(Ne*(33PP2,02,0))
ArAr++
NeNe++ ArAr
NeNe ArAr++
e-
e-
symmetry symmetry
NeNe++ ArAr
NeNe ArAr++
e-
e-
symmetry symmetry
1.8 2.0 2.2 2.4 2.6 2.8 3.0
NeNe**((33PP00))
NeNe**((33PP22))
NeNe**((33PP00))
NeNe**((33PP22))
KrKr++((22PP3/23/2))KrKr
++((22PP1/21/2))
EEcollcoll=0.050 eV=0.050 eV
electron energy (eV)
B. Brunetti, P. Candori, S. Falcinelli, B. Lescop, G. Liuti, F. Pirani, F. Vecchiocattivi (2005) to be published
0.0 0.1 0.2 0.3 0.4 0.50
1
2
3
4
5
6
J=0 (present experiment)J=0 (present experiment) J=0 (Hotop and coworkers)J=0 (Hotop and coworkers)
J=2 (present experiment)J=2 (present experiment) J=2 (Hotop and coworkers)J=2 (Hotop and coworkers)
Qj,3
/2/Q
j,1/2
collision energy (eV)
NeNe**((33PP22))
NeNe**((33PP00))
Penning ionization occurs through the Penning ionization occurs through the transfer of an outer shell electron from the transfer of an outer shell electron from the target particle into the inner shell vacancy of target particle into the inner shell vacancy of the metastable atom. the metastable atom.
The process is therefore governed by the The process is therefore governed by the mutual orientation of atomic orbitals.mutual orientation of atomic orbitals.
In the case of atom-molecule systems, this In the case of atom-molecule systems, this also implies a strong effect of the also implies a strong effect of the orientation of the target molecule.orientation of the target molecule.
+ -hexapole filter
CH3Cl beam
rotatable plate
Ar* beam
high voltage
Ion detector
Ar* + CHAr* + CH33Cl Cl CH CH33ClCl++ + Ar + e + Ar + e--
H. Ohoyama, M.Yamato, S. Okada, T. Kasai, B. G. Brunetti, F. Vecchiocattivi, Phys.Chem.Chem.Phys. 3, 3598 (2001).
B. G. Brunetti, P. Candori, S. Falcinelli, T. Kasai, H. Ohoyama, F. Vecchiocattivi, Phys.Chem.Chem.Phys. 3, 807 (2001).
V. Aquilanti, F. Pirani, D. Cappelletti, F. Vecchiocattivi, T. Kasai, in: “Theory of chemical reaction dynamics”, Kluwer Academic, the Netherlands, p.243 (2004).
V.Aquilanti, M. Bartolomei, F. Pirani, D. Cappelletti, F. Vecchiocattivi, Y. Shimizu, T. Kasai. Phys.Chem.Chem.Phys. 7, 291 (2005)
ArAr**
0-1 +1
cos ()
CHCH33 end end
Cl endCl end
Ar* CHAr* CH33ClCl
cos(cos()=0)=0
cos(cos()=-1)=-1
cos(cos()=+1)=+1
stereo-opacitystereo-opacity
ArAr**
0.8
1.2
Rg* + NRg* + N22O O [Rg…N [Rg…N22OO++] + e] + e--
[Rg…N[Rg…N22OO++] ] N N22OO++
NONO++ + N + N
OO++ + N + N22
RgNRgN22OO++
Rg = He, NeRg = He, Ne
tot
Cro
ss
Se
ctio
n (
Cro
ss
Se
ctio
n (
ÅÅ22 ))
Collision Energy (eV)Collision Energy (eV)0.1 0.2
0.1
1
10 N2O+
NO+
O+
NeN2O+
Ne* + NNe* + N22OO
He*(23S, 21S)-N2O
0.06
0.08
0.10
0.12
Collision Energy (e
V)
LUMOLUMO HOMOHOMO
NitrogenNitrogen““lone pair”lone pair”
OxygenOxygen““lone pair”lone pair”
Molecular orbitals of NMolecular orbitals of N22OO
NN22OO++ ion ionin the ground in the ground 22 state state
N N O
He*
NN22OO++ ion ionin the excited in the excited 22 state state
N N OHe*
He*(2He*(211S) + NS) + N22OO
He*He*…… NNO NNO
NNO NNO …… He* He*
Ne*(Ne*(33P) + HP) + H22O O Ne + HNe + H22OO++ + e + e--
He*(He*(33S) + HS) + H22O O He + HHe + H22OO++ + e + e-- 77.9%77.9%
B. Brunetti, P. Candori, S. Falcinelli, B. Lescop, G. Liuti, D. Malfatti, F. Pirani, F. Vecchiocattivi (2005) to be published
1b1
(2p non bonding orbital)
3a1
(sp2 lone pair orbital)
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0
Electron Energy (eV)
~~X (X (22BB11))
~~A (A (22AA11))
Photoionization Photoionization electron spectrum, electron spectrum, energy scaledenergy scaled
Ne* + HNe* + H22OO
B. Brunetti, P. Candori, S. Falcinelli, B. Lescop, G. Liuti, D. Malfatti, F. Pirani, F. Vecchiocattivi (2005) to be published
Ne* + HNe* + H22OO
The Penning ionization of molecules The Penning ionization of molecules strongly depends on the orientation of the strongly depends on the orientation of the molecule with respect to the approach molecule with respect to the approach direction of the metastable atom. direction of the metastable atom.
The orientation not only affects the ionization The orientation not only affects the ionization probability, but also the specific reaction probability, but also the specific reaction following following the ionization event (dissociation, the ionization event (dissociation, rearrangement, etc.) rearrangement, etc.)
Optical Potential Model (H. Bethe, 1940):Optical Potential Model (H. Bethe, 1940):
and therefore the phase shift is also complexand therefore the phase shift is also complex
== + + ii
The Potential is assumed to be complexThe Potential is assumed to be complex
Total Ionization Cross Section:Total Ionization Cross Section:
B. Brunetti, F. Vecchiocattivi, B. Brunetti, F. Vecchiocattivi, Current Topic on Ion Chemistry and PhysicsCurrent Topic on Ion Chemistry and Physics , , edited by C.Y. Ng, T. Baer, I. Powis (John Wiley & Sons Ltd, New York, 1993), p. 359edited by C.Y. Ng, T. Baer, I. Powis (John Wiley & Sons Ltd, New York, 1993), p. 359