(c) 2000-2003 by Akira Miyoshi. All rights reserved.
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Reaction Dynamics 2002 - section-1
1. Introduction
1.1 Statistical Theory for Canonical Ensemble - Review
Canonical Ensemble
- Under free and random energy exchange among molecules in the system
(normal gas-state)
- The total energy of the system is defined by temperature,
.
<Boltzmann Statistics>
Probability of finding a molecule in the state
(of energy
and multiplicity
)

ex.) |
Distribution of the ground triplet states of atomic
oxygen;
( 0,
= 5),
( = 158.5
,
= 3), and
( = 226.5
,
= 1); at 298 K (1 = 1.4388 K) |
|
 |
 |
 |
<Partition Function>
Probability of finding molecule A in the system
(e.g., A = HCN and not HNC, 1/2 H2 +
1/2 N2 + C, nor etc.) = Sum of the probability
of finding for all states of A
[partition function] (1.1.1)
ex.) |
Distribution of the triplet ground states
( =
+ +
) and the excited
( ) state
[ = 15867.7
,
= 5] of atomic oxygen at 298 K: |
|
 |
 |
ex.) |
Vibrational partition function of a harmonic oscillator
( ): |
|
(1.1.2) |
<Chemical Equilibrium>
Ratio of the distributions of molecule B to A:
(When the same zero energy point was used to calculate both
and
)
or
(1.1.3)
(When
and
are calculated from an each
ground sate)
<Transition-State Theory>
Rate coefficient (A
[TS*]
B)
(1.1.4)
- Probability of passing through the states in the transition
state obey Boltzmann distribution
1.2 Statistical Theory for Microcanonical Ensemble
- Isolated molecules (molecules after photolysis, molecules just after
reaction, or etc.j
- The system is defined by energy
.
- The prior distribution
<Multiplicity>
- Degeneracy of multiple solutions to a (time-independent) Schrodinger
equation with the same eigenvalue (energy).
- Ratio of the probabilities of finding a system in the state A
(multiplicity
) to that in the
state B (multiplicity
; at the
same energy as A) =
:
ex.) |
Atomic orbitals of H: =
( : principal q.n.),
=
( : azimuthal q.n.) |
K-shell ( = 1):
1s ( = 0,
= 1) only
= = 1 |
L-shell ( = 2):
2s ( = 0,
= 1),
2p ( = 1,
= 3)
=
= 4 |
M-shell ( = 3):
3s ( = 0,
= 1),
3p ( = 1,
= 3),
3d ( = 2,
= 5)
= = 9 |
ex.) |
Electronic states of H-atom: |
total multiplicity |
ground state: |
( ) [ =
= 2
1 = 2] |
(K-shell) 2 |
excited states: |
( ) [ =
2 3 = 6] |
(L-shell) 8 |
( )
[ = 2 1 = 2] |
ex.) |
Bending vibration ( ) of
CO2 ... 2-D harmonic oscillator |
,
;
( : vibrational q.n.) |
<Density of states>
- = Number of states per unit energy [states /
]
- Probability ratio between molecule A (density of states =
) and B
(
) =
:
ex.) |
Photodecomposition of HCl at 248 nm (40320
): |
HCl +
(40320 ) |
H +
Cl( ) +
(4240
) | (a) |
| H +
Cl( ) +
(3359
) | (b) |
Statistical branching ratio,
:
 |
= [Cl( )]
(4240
) : [Cl( )]
(3359
) |
=
 |
Problem-1
Calculate the statistical branching ratio between H +
I( ) [channel-a] and H +
I( ) [channel-b] upon the
photolysis of HI at 266 nm.
Use the bond dissociation energy of HI [
H + I( ) ] = 298
and excitation energy of
I( ) form
I( ) (ground state) =
0.943 eV.
|