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J. Chem. Phys., Vol. 121, No. 15, 15 October 2004
Rakitzis et al.
to be 86Ϯ27% ͑2͒. The theoretical electron polarization for
the H atoms corresponding to Br(2P1/2) atoms is 100%.
Therefore, the overall H-atom electron polarization is about
88%. The degree of this polarization may be confirmed both
directly35 and theoretically,36 and the polarization may in-
crease at different photodissociation wavelengths.21 This
work shows that HBr photodissociation can be used as an
intense source of spin-polarized hydrogen.
3Ϫ2p͒
͑
͑1͒
a0 Ќ͒ϭϩ
,
͑14͒
͑
ͱ15
͑1͒
1
ʈ
Re a
,Ќ͒ ϭcA,a0 cos ⌬A,a0ϩca1,a0 cos ⌬
,
͓
͑
͔
a1,a0
͑15͒
͑2͒
a0 Ќ͒ϭϩ 4/5͒ 1Ϫ2p͒,
͑16͒
͑
͑
͑
͑2͒
Ќ͒ϭϪ 4ͱ2/5͒ͱp 1Ϫp͒cos ⌬
͑
a2
,
͑17͒
͑18͒
͑
͑
A,a1
2 1Ϫ4p͒
͑
ACKNOWLEDGMENTS
͑3͒
a0 Ќ͒ϭ
,
͑
5ͱ15
This work is conducted at the Ultraviolet Laser Facility
operating at FORTH-IESL ͑Improving Human Potential-
Transnational Access to major Research Infrastructures,
Grant No. HPRI-CT-1999-00074͒ and is also supported by
Grant Nos. HPRN-CT-2002-00183 ͑PICNIC͒ and HPRN-
CT-2000-0006 ͑REACTIVES͒.
where p is equal to p1 /(1Ϫp2); p1 and p2 is the probability
of nonadiabatic transfer from the A 1⌸ to the a 3⌸ state and
1 3⌺1 state, respectively. Notice that Eq. ͑18͒ differs from
Eq. ͑21͒ in Ref. ͑6͒, due to a different convention.
Using either Eq. ͑14͒ or Eq. ͑16͒, we can solve for p, and
obtain 0.93Ϯ0.13. The probability p2 was measured to be
about 2͑0.14͒/3;33,34 hence we determine p1 to be 0.80Ϯ0.10.
Therefore, after excitation to the primary absorber, the A 1⌸
state, only 6% dissociates adiabatically ͓Eq. ͑11͔͒, whereas
80% transfers nonadiabatically to the a 3⌸ state ͓Eq. ͑12͔͒
and 14% to the 1 3⌺1 state, both of which involve an H spin
flip. Using pϭ0.93 and Eq. ͑17͒, we see that ⌬A,a1ϭ0. The
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(1)
1
ʈ
Re a ( ,Ќ) parameter is small, and therefore we cannot
͓
͔
separate the possibility that both the contributions from
⌬ and ⌬ are small ͓Eq. ͑15͔͒, or that they are
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A,a0
A,a0
canceling each other.
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direction are given in terms of the a(qk)(p) by
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830 ͑1996͒.
1
9
p Jϭ3/2,m ϭϮ3/2͒ϭ 1Ϯ
a1 Ќ͒
͑
͑
Z
ͫ
0
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123001 ͑2001͒.
4
ͱ
15
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Phys. 110, 6749 ͑1999͒.
ͱ15
2
5
4
ϩ
a2 Ќ͒Ϯ
a3 Ќ͒ , ͑19͒
͑
͑
ͬ
0
0
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1
3
p Jϭ3/2,m ϭϮ1/2͒ϭ 1Ϯ
a1 Ќ͒
͑
͑
Z
ͫ
0
15 T. P. Rakitzis, P. C. Samartzis, R. L. Toomes, T. N. Kitsopoulos, A. Brown,
G. G. Balint-Kurti, O. S. Vasyutinskii, and J. A. Beswick, Science 2003,
300 ͑1936͒.
4
ͱ
15
3ͱ15
2
5
4
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17 C. R. Gebhardt, T. P. Rakitzis, P. C. Samartzis, V. Ladopoulos, and T. N.
Kitsopoulos, Rev. Sci. Instrum. 72, 3848 ͑2001͒.
Ϫ
a2 Ќ͒ϯ
a3 Ќ͒ .
͑
͑
ͬ
0
0
18 R. L. Toomes, P. C. Samartzis, T. P. Rakitzis, and T. N. Kitsopoulos,
Chem. Phys. 301, 209 ͑2004͒.
͑20͒
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21 R. N. Zare, Mol. Photochem. 4, 1 ͑1972͒.
The electron polarization Pe of the nascent H atoms, also
recoiling parallel to the photodissociation polarization direc-
tion, is given by the difference in population between the
mϭ1/2 and mϭ3/2 states of the halogen (2P3/2) state:
22 A. J. Alexander, Z. H. Kim, S. A. Kandel, R. N. Zare, T. P. Rakitzis, Y.
Asano, and S. Yabushita, J. Chem. Phys. 113, 9022 ͑2000͒.
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press͒.
1
4
6
5
2
2
0
3
0
a1 Ќ͒ϩ
͑21͒
a Ќ͒ϩ2ͱ15a Ќ͒ .
͑
PeϭϪ
͑
͑
ͫ
ͬ
0
25 P. C. Samartzis, I. Sakellariou, T. Gougousi, and T. N. Kitsopoulos, J.
Chem. Phys. 107, 43 ͑1997͒.
ͱ15
26 S. Arepalli, N. Presser, D. Robie, and R. J. Gordon, Chem. Phys. Lett. 118,
88 ͑1985͒.
Using Eqs. ͑8͒ and ͑21͒, and the measured values of
a(01)(Ќ) and a(02)(Ќ), the nascent electron polarization for
the H atoms ͑parallel to the photodissociation propagation
direction͒ from the photodissociation of HBr is determined
27 C. E. Moore, Atomic Energy Levels as Derived From the Analyses of
Optical Spectra ͑U.S. Dept. of Commerce, National Bureau of Standards,
Washington, 1949͒.
130.88.90.140 On: Mon, 22 Dec 2014 18:21:49