Role of N-States in Molecular Photodissociation

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The role of (
n
/
)
* states in molecular
photodissociation processes
 
Mike Ashfold
University of Bristol
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2
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5
Leiden Observatory Workshop:  Photodissociation in Astrochemistry
  Plan for lecture
Short introduction to (
n
/
)
* states
O–H/S–H bond fission in H
2
O, H
2
S, alcohols/thiols, 
etc
N–H 
bond fission in ammonia, amines
C–H bond fission in methane, ethyne and HCN
Larger molecules?
(
n
/
)
* state mediated ring opening?
Conclusions and future prospects
Excited state photochemistry: (
n
/
π
)
* excited states
  
HF
  Archetypal 
*
 
n
/
 excitation.
  Repulsive excited state
       potential.
  Direct bond fission
       
 H + F atoms
H
2
O 
(
singlet state potentials shown only)
 
 
OH not spherically symmetric, presents 
p
 and 
p
 orbitals.
   1
 and 
1
 
potentials cross at linear geometry.
  1
A
 components avoid each other when bent 
 conical intersection (CI)
at 
HOH = 180
 and extended 
R
O–H
.
  Change in 
HOH with O–H bond extension 
 OH product rotation?
 
conical
intersection
How to test such predictions?
In case of H
2
O:
simple triatomic, light atoms, high I.P.
Experiment:
        photofragment translational spectroscopy (PTS) / imaging.
Theory:  
 
       
ab initio 
full-dimensional PESs, propagate  wavepackets.
What are key wavelengths to study?  
Experimentalists prefer  
> 200 nm or 
 = 121.6 nm, but almost any wavelength is
possible if the problem merits it.
Absorption cross-sections 
(
; 
T
) generally not available 
 an
issue for light molecules with structured Rydberg regions.
 
Tagging (366nm)
Molecular Beam
 
Photolysis
 
 
“High n” tagging
(366nm)
 
 
Lyman-
(121.6nm)
H Rydberg atom PTS {Karl Welge (Bielefeld)}
 
Hydrogen Atom
 
Rydberg State
(H*)
 
n=2
 
n=1
 
Cation
 
H*
H
2
O
 + h
 (
=121.6 nm) 
 H + OH(X/A, 
v
, 
N
)
Y
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a
n
 
e
t
 
a
l
.
,
 
P
N
A
S
 
2
0
0
8
 
1
0
5
 
1
9
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4
8
 
 
(
M
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.
,
 
J
C
P
 
1
9
9
4
 
1
0
0
 
7
3
6
0
)
 Product recoil anisotropy, e
lectronic branching in products, immune
to effects of OH predissociation, confirm massive OH product rotation.
(see also Dr 
Kaijun Yuan presentation, Wed 4 pm).
Hydrides (and halides)
Similar ideas go a long way to explaining/predicting photoinduced
excited state bond fission in 
all
 gas phase hydride molecules:
H
2
O 

 CH
3
OH, C
6
H
5
OH, … H
2
S, CH
3
SH, C
6
H
5
SH, ……
 
NH
3
 

 
CH
3
NH
2
, cyclic amines (pyrroline, morpholine, 
etc
),
heterocycles (azoles, indoles, adenine, 
etc
), C
6
H
5
NH
2
, …..
 
HCN, HCCH, 
etc
 
alkylated analogues (
e.g.
 ethers, thioethers, secondary amines, 
etc
)
(
P
C
C
P
 
2
0
1
0
 
1
2
 
1
2
1
8
)
 
families of halides
(
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.
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.
 
h
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,
 
.
.
)
(
P
C
C
P
 
 
2
0
1
1
 
1
3
 
8
0
7
5
;
 
J
C
P
 
2
0
1
3
 
1
3
8
 
1
6
4
3
1
8
)
H
2
S
W
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a
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,
 
M
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l
 
P
h
y
s
 
1
9
9
6
 
8
8
 
8
4
1
Similarities (but also differences) with H
2
O.
I.P.(H
2
S) < I.P.(H
2
O), 
D
0
(H–SH) < 
D
0
(H–OH) 
 observe
given photodissociation behaviour at longer 
 in H
2
S.
Near UV photolysis
*
 3p
x
(HOMO) continuum
spanning 190-250 nm.
H + SH(X) products formed
predominantly in 
v
 = 0, low 
N
states
Anisotropic recoil
Similar behaviour to that
shown by H
2
O in wavelength
range 150 < 
 < 190 nm.
 = 243.3 nm
H
2
S 
+ h
 (
=121.6 nm) 
 H + ?
C
o
o
k
 
e
t
 
a
l
.
,
 
J
 
C
h
e
m
 
P
h
y
s
 
2
0
0
1
 
1
1
4
 
1
6
7
2
Excite just below 1
st
 I.P. –
high density of states.
Populate (or couple to)
second 
n
* state.
Dissociate to H + SH(A) with:
      
v
 
 5 (and low 
N
), and
      
v
 = 0 with high 
N
.
No H + SH(X) products.
Dissociating molecules fail to
sample relevant CI in 
R
H–SH
at linear geometries.
3-body fragmentation
 H + H + S.
H
2
 + S yields?  
(
Mingli Niu
presentation, Thurs 11 am)
VUV photolysis of alkyl alcohols and thiols?
 
 
*
 
Y
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a
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t
 
a
l
,
 
C
h
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.
 
J
.
 
C
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m
.
 
P
h
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s
.
 
2
0
0
8
 
2
1
 
3
0
1
HRA-PTS studies of MeOH, EtOH photolysis at 
 = 
157.6 nm.*
Fast H atoms from H–OMe, H–OEt bond fission on 
n
* PES;
slower H atoms attributed to primary C–H bond fission and to
secondary decay of vibrationally ‘hot’ OMe and OEt products.
MeSH studied at 
 = 
193.3 nm (and longer wavelengths)
(Butler, Wittig, ourselves, Yang, Parker, ….).
H–SMe and HS–Me bond fissions studied in some detail.
121.6 nm photolysis 
of such larger polyatomic systems rarely
studied in a quantitative manner.  In many cases, photoexcitation
would project molecule above first I.P., myriad fragmentation
pathways (in principle), not that appealing to photodissociation
dynamicists.
NH
3
 
+ h
 
 H + ?
M
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.
,
 
J
 
C
h
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m
 
P
h
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s
 
1
9
9
6
 
1
0
4
 
6
4
6
0
3s
n 
excitation gives structured
A – X absorption band centred at
 ~200 nm, dominated by
progression in excited state
umbrella-bend vibration.
Conical intersection between
ground and first excited PESs in
R
H2N–H 
dissociation coordinate,
at planar geometries.
Upon dissociation, parent out-of-
plane vibrational motion maps
into 
a
-axis rotation of NH
2
fragments.
NH
3
 
+ h
 (
 = 216 nm) 
 H + NH
2
(X)
M
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.
,
 
J
 
C
h
e
m
 
P
h
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s
 
1
9
9
6
 
1
0
4
 
6
4
6
0
Excess energy channelled into
product translation and rotation
Broadly similar behaviour seen
at all wavelengths 
 
 193 nm.
NH
2
(A) products also identified
once above relevant energy
threshold.
Similar studies of NH
2
D, NHD
2
and ND
3
 photolysis at these
near UV wavelengths.
No similar quantitative study at 
= 121.6 nm (above I.P.)
MeNH
2
:
 Me–NH
2
 and MeNH–H bond fission following near UV
excitation, but nothing quantitative at shorter wavelengths.
HCN + 
h
 (
 = 121.6 nm) 
 ?
C
o
o
k
 
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t
 
a
l
.
,
 
J
 
C
h
e
m
 
P
h
y
s
 
 
2
0
0
0
 
1
1
3
 
9
9
4
H + CN(A) products dominate,
     bimodal rotational state population
     distribution.
No H + CN(X) products identified.
Fully consistent with dissociation via 

* PES.  Predict same for
HC
2n
CN, given same X
2
 vs A
2
 ordering in C
2n
CN radicals.
(
HCN = 180
 )
C
2
H
2
 + 
h
 
 ?
M
o
r
d
a
u
n
t
 
 
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t
 
a
l
.
,
 
J
 
C
h
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P
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s
 
 
1
9
9
8
 
1
0
8
 
5
1
9
;
 
 
 
 
 
 
 
 
L
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f
f
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.
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J
 
C
h
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m
 
P
h
y
s
 
 
1
9
9
8
 
1
0
9
 
5
2
3
1
~210 nm:
Excite (bent) valence states,
‘Slow’  dissociation (ISC) via
triplet states 
 H +
 C
2
H(X)
products.
Beautifully quantum state
resolved problem.
121.6 nm:
Region of high state density,
Efficient coupling to 

* PES
Dissociate to H + C
2
H(A) products,
with obvious activity in C=C stretch
mode.
CH
4
 + 
h
 (
 = 121.6 nm) 
 ?
A long standing challenge.
CH
4
 only absorbs at 
 137 nm.
H + CH
3
 identified as major
primary products when exciting
at 121.6 nm as long ago as
1993.
Also see slow H atoms from
three-body dissociation.
Mechanism?
H
 
a
t
o
m
s
 
s
h
o
w
 
s
p
e
e
d
 
d
e
p
e
n
d
e
n
t
r
e
c
o
i
l
 
a
n
i
s
o
t
r
o
p
y
.
(
W
a
n
g
 
e
t
 
a
l
.
,
 
J
.
 
C
h
e
m
.
 
P
h
y
s
.
 
2
0
0
0
 
1
1
3
 
4
1
4
6
)
.
M
o
r
d
a
u
n
t
 
e
t
 
a
l
.
 
1
9
9
3
 
9
8
 
2
0
5
4
CH
4
 + 
h
 (
 = 121.6 nm) 
 ?
Recent clarifications.
E
x
p
e
r
i
m
e
n
t
s
 
a
t
 
~
1
3
0
 
n
m
(
Z
h
a
n
g
 
e
t
 
a
l
.
,
 
J
.
 
P
h
y
s
.
 
C
h
e
m
.
L
e
t
t
s
.
 
2
0
1
0
 
1
 
4
7
5
.
Structure in TKER spectrum
confirms H + CH
3
 products;
latter carry high 
N
 (and 
v
)
excitation.
T
h
e
o
r
y
 
(
v
a
n
 
H
a
r
r
e
v
e
l
t
,
 
J
.
 
C
h
e
m
.
 
P
h
y
s
.
 
2
0
0
6
 
1
2
5
 
1
2
4
3
0
2
)
Identifies conical intersections between S
1 
and S
0
 PESs at planar
geometries that offer potential routes to the observed fragmentation
products.
Summary
Focus of talk – photodissociation dynamics of hydride molecules,
using H (Rydberg) tagging methods.
Ion imaging methods applicable to many other small fragments.
In almost all cases, level of study (and understanding) much better
for near UV wavelengths than at 
 = 121.6 nm.
(
n
/
)
* PESs enable 
excited state 
photofragmentation.
Radiationless transfer to S
0
 PES, and unimolecular decay of
vibrationally ‘hot’ S
0
 molecules becomes ever more important for
larger polyatomic molecules.
Outstanding issues – for experiment and theory:
     identification of 
all
 products
  
product branching ratios
     
(
T
) dependence of 
total
 (and 
partial
 for forming possible products)
 
Acknowledgements
Bielefeld:  
Karl Welge, Ludger Schnieder, Eckart Wrede (Bielefeld)
Bristol:
   PhD students:  
Greg Morley, David Mordaunt, Steve Wilson, Claire Reed,
Phil Cook, Brid Cronin, Mike Nix, Adam Devine, Graeme King, Tom Oliver,
Tolga Karsili, Barbara Marchetti, Rebecca Ingle.
   PDRAs:   
Ian Lambert, Steve Langford, Emma Feltham.
   Academic colleagues:  
Richard Dixon, Colin Western, A
ndrew Orr-Ewing.
 
 
 
 
 
 
 
 
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The influence of N-states in molecular photodissociation processes, this study delves into topics like bond fission in various molecules, excited state photochemistry, singlet state potentials of H2O, and testing predictions through experiments and theory.

  • Molecular Photodissociation
  • Excited States
  • H2O
  • Photochemistry
  • Experimental Study

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  1. The role of (n/)* states in molecular photodissociation processes Mike Ashfold University of Bristol http://www.bristoldynamics.com Leiden Observatory Workshop: Photodissociation in Astrochemistry 3-5 February 2015 Kasteel Oud Poelgeest, Leiden

  2. Plan for lecture Short introduction to (n/ ) * states O H/S H bond fission in H2O, H2S, alcohols/thiols, etc N H bond fission in ammonia, amines C H bond fission in methane, ethyne and HCN Larger molecules? (n/ ) * state mediated ring opening? Conclusions and future prospects

  3. Excited state photochemistry: (n/)* excited states HF Archetypal * n/ excitation. Repulsive excited state potential. Direct bond fission H + F atoms

  4. H2O (singlet state potentials shown only) conical intersection OH not spherically symmetric, presents p and p orbitals. 1 and 1 potentials cross at linear geometry. 1A components avoid each other when bent conical intersection (CI) at HOH = 180 and extended RO H. Change in HOH with O H bond extension OH product rotation?

  5. How to test such predictions? In case of H2O: simple triatomic, light atoms, high I.P. Experiment: photofragment translational spectroscopy (PTS) / imaging. Theory: ab initio full-dimensional PESs, propagate wavepackets. What are key wavelengths to study? Experimentalists prefer > 200 nm or = 121.6 nm, but almost any wavelength is possible if the problem merits it. Absorption cross-sections ( ; T) generally not available an issue for light molecules with structured Rydberg regions.

  6. H Rydberg atom PTS {Karl Welge (Bielefeld)} Cation Detector Rydberg State (H*) Tagging (366nm) n=2 Photolysis Lyman- (121.6nm) H* n=1 Hydrogen Atom Molecular Beam High n tagging (366nm) Lyman- (121.6nm)

  7. H2O + h (=121.6 nm) H + OH(X/A, v, N) Product recoil anisotropy, electronic branching in products, immune to effects of OH predissociation, confirm massive OH product rotation. (see also Dr Kaijun Yuan presentation, Wed 4 pm). Yuan et al., PNAS 2008 105 19148 (Mordaunt et al., JCP 1994 100 7360)

  8. Hydrides (and halides) Similar ideas go a long way to explaining/predicting photoinduced excited state bond fission in all gas phase hydride molecules: H2O CH3OH, C6H5OH, H2S, CH3SH, C6H5SH, NH3 CH3NH2, cyclic amines (pyrroline, morpholine, etc), heterocycles (azoles, indoles, adenine, etc), C6H5NH2, .. HCN, HCCH, etc alkylated analogues (e.g. ethers, thioethers, secondary amines, etc) (PCCP 201012 1218) families of halides (e.g. hydrogenhalides alkyl halides,aryl halides,halophenols, ..) (PCCP 2011 13 8075; JCP 2013 138 164318)

  9. H2S Similarities (but also differences) with H2O. I.P.(H2S) < I.P.(H2O), D0(H SH) < D0(H OH) observe given photodissociation behaviour at longer in H2S. Near UV photolysis * 3px(HOMO) continuum spanning 190-250 nm. H + SH(X) products formed predominantly in v = 0, low N states Anisotropic recoil Similar behaviour to that shown by H2O in wavelength range 150 < < 190 nm. = 243.3 nm Wilson et al., Mol Phys 1996 88 841

  10. H2S + h (=121.6 nm) H + ? Excite just below 1st I.P. high density of states. Populate (or couple to) second n * state. Dissociate to H + SH(A) with: v 5 (and low N), and v = 0 with high N. No H + SH(X) products. Dissociating molecules fail to sample relevant CI in RH SH at linear geometries. 3-body fragmentation H + H + S. H2 + S yields? (Mingli Niu presentation, Thurs 11 am) Cook et al., J Chem Phys 2001 114 1672

  11. VUV photolysis of alkyl alcohols and thiols? HRA-PTS studies of MeOH, EtOH photolysis at = 157.6 nm.* Fast H atoms from H OMe, H OEt bond fission on n * PES; slower H atoms attributed to primary C H bond fission and to secondary decay of vibrationally hot OMe and OEt products. MeSH studied at = 193.3 nm (and longer wavelengths) (Butler, Wittig, ourselves, Yang, Parker, .). H SMe and HS Me bond fissions studied in some detail. 121.6 nm photolysis of such larger polyatomic systems rarely studied in a quantitative manner. In many cases, photoexcitation would project molecule above first I.P., myriad fragmentation pathways (in principle), not that appealing to photodissociation dynamicists. * Yuan et al, Chin. J. Chem. Phys. 2008 21 301

  12. NH3 + h H + ? 3s n excitation gives structured A X absorption band centred at ~200 nm, dominated by progression in excited state umbrella-bend vibration. Conical intersection between ground and first excited PESs in RH2N H dissociation coordinate, at planar geometries. Upon dissociation, parent out-of- plane vibrational motion maps into a-axis rotation of NH2 fragments. Mordaunt et al., J Chem Phys 1996 104 6460

  13. NH3 + h ( = 216 nm) H + NH2(X) Excess energy channelled into product translation and rotation Broadly similar behaviour seen at all wavelengths 193 nm. NH2(A) products also identified once above relevant energy threshold. Similar studies of NH2D, NHD2 and ND3 photolysis at these near UV wavelengths. No similar quantitative study at = 121.6 nm (above I.P.) MeNH2: Me NH2 and MeNH H bond fission following near UV excitation, but nothing quantitative at shorter wavelengths. Mordaunt et al., J Chem Phys 1996 104 6460

  14. HCN + h ( = 121.6 nm) ? H + CN(A) products dominate, bimodal rotational state population distribution. No H + CN(X) products identified. Fully consistent with dissociation via * PES. Predict same for HC2nCN, given same X2 vs A2 ordering in C2nCN radicals. ( HCN = 180 ) Cook et al., J Chem Phys 2000 113 994

  15. C2H2 + h ? ~210 nm: Excite (bent) valence states, Slow dissociation (ISC) via triplet states H + C2H(X) products. Beautifully quantum state resolved problem. 121.6 nm: Region of high state density, Efficient coupling to * PES Dissociate to H + C2H(A) products, with obvious activity in C=C stretch mode. Mordaunt et al., J Chem Phys 1998 108 519; Loeffler et al., J Chem Phys 1998 109 5231

  16. CH4 + h ( = 121.6 nm) ? A long standing challenge. CH4 only absorbs at 137 nm. H + CH3 identified as major primary products when exciting at 121.6 nm as long ago as 1993. Also see slow H atoms from three-body dissociation. Mechanism? H atoms show speed dependent recoil anisotropy. (Wang et al., J. Chem. Phys. 2000 113 4146). Mordaunt et al. 1993 98 2054

  17. CH4 + h ( = 121.6 nm) ? Recent clarifications. Experiments at ~130 nm (Zhang et al., J. Phys. Chem. Letts. 2010 1 475. Structure in TKER spectrum confirms H + CH3 products; latter carry high N (and v) excitation. Theory (van Harrevelt, J. Chem. Phys. 2006 125 124302) Identifies conical intersections between S1 and S0 PESs at planar geometries that offer potential routes to the observed fragmentation products.

  18. Summary Focus of talk photodissociation dynamics of hydride molecules, using H (Rydberg) tagging methods. Ion imaging methods applicable to many other small fragments. In almost all cases, level of study (and understanding) much better for near UV wavelengths than at = 121.6 nm. (n/ ) * PESs enable excited state photofragmentation. Radiationless transfer to S0 PES, and unimolecular decay of vibrationally hot S0 molecules becomes ever more important for larger polyatomic molecules. Outstanding issues for experiment and theory: identification of all products product branching ratios (T) dependence of total (and partial for forming possible products)

  19. Acknowledgements Bielefeld: Karl Welge, Ludger Schnieder, Eckart Wrede (Bielefeld) Bristol: PhD students: Greg Morley, David Mordaunt, Steve Wilson, Claire Reed, Phil Cook, Brid Cronin, Mike Nix, Adam Devine, Graeme King, Tom Oliver, Tolga Karsili, Barbara Marchetti, Rebecca Ingle. PDRAs: Ian Lambert, Steve Langford, Emma Feltham. Academic colleagues: Richard Dixon, Colin Western, Andrew Orr-Ewing.

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