Environmental Engineering Reference
In-Depth Information
neutron energy, is determined by again making use of Bragg-reflection
in a single-crystal analyser, so that only neutrons with energies in a
small interval dE around ( hk ) 2 / 2 M strike the counter. The number of
neutrons in this range, corresponding to a state vector
| k s n > for the
scattered neutrons, is
δN = V (2 π ) 3 ( k ) 2 dk d Ω= V (2 π ) 3 ( Mk /h 2 ) dEd .
The number of neutrons arriving at the counter per unit time and per
incident neutron is proportional to the scattering area =
| 1
| j ( ks n )
×
W ( ks n , k s n ) δN ,ortothe differential scattering cross-section
M
2 πh 2
2
d 2 σ
dEd =
k
k
2 δ ( + E i
| s n ; f>
P i |
< s n ; i
|H int (
κ
)
|
E f ) ,
if
(4 . 1 . 4 a )
where
)=
H int e −i κ · r n d r n .
H int (
κ
(4 . 1 . 4 b )
This result of time-dependent perturbation theory, in the first Born ap-
proximation, is accurate because of the very weak interaction between
the neutrons and the constituents of the sample.
In order to proceed further, it is necessary to specify the interaction
Hamiltonian
H int . The magnetic moment of the neutron is
m
M µ B =
eh
2 Mc ,
µ n =
g n µ N s n
;
g n =3 . 827
;
µ N
=
1
with s n =
2 . In this chapter, in the interest of conformity with the rest
of the literature, we do not reverse the signs of the electronic angular-
momentum vectors, which are therefore antiparallel to the corresponding
magnetic moments, as is also the case for the neutron.
This magnetic dipole moment at r n gives rise to a vector potential,
at the position r e ,
µ n × r /r 3 ,
A n ( r e , r n )= A n ( r = r e r n )=
with r =
. The magnetic-interaction Hamiltonian for a neutron at r n
with a single electron of charge
| r |
e , with coordinate r e ,momentum p ,
and spin s is
p + e
c ( A n + A e ) 2
p + e
c A e 2 +2 µ B s · B n
1
2 m
1
2 m
H int ( r e , r n )=
=2 µ B 1
∇× A n ) ,
h A n · p + s ·
(
(4 . 1 . 5)
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