Download presentation
Presentation is loading. Please wait.
1
How do nuclei rotate? 2. High Spin
2
Coincidence measurements
select rotational bands.
4
Stability against fission
Homogenously charged droplet
5
fission instable fission barrier 8MeV
6
Rotational bands in 5/17
7
Semiclassics High angular momentum
can be treated as a classical quantity For uniform rotation the rotational frequency (angular velocity) is given by the classical relation
8
Experimental rotational frequency
9
M1 radiation intensity also well described by classical radiation theory E2 radiation
10
M1 radiation - high spin limit
K J
11
Angular momentum, moment of inertia and routhians as functions of the frequency
Long bands permit us to derive the classical functions
12
Includes a quantal correction
Zero point fluctuation I I+1/2 10/17
14
Rotational bands in the non-adiabatic regime
How are the spectral lines arranged into bands?
15
Rotational bands in
16
band EAB band E bandcrossing
17
Summary Nuclei can be studied at high spin where intrinsic and rotational motion are on the same time scale. The levels still organize into rotational bands, the states of which are connected by fast electromagnetic transitions. Bands cross each other. High spin allows us to use classical concepts for the rotational degree of freedom. The angular velocity becomes a well defined concept. It is very useful to study physical quantities as functions of the angular frequency.
Similar presentations
© 2024 SlidePlayer.com Inc.
All rights reserved.