Low energy orbital magnetic dipole excitations of heavy nonspherical nuclei

1991 ◽  
Vol 339 (1) ◽  
pp. 97-109 ◽  
Author(s):  
D. Zawischa ◽  
J. Speth
Keyword(s):  
2013 ◽  
Vol 111 (23) ◽  
Author(s):  
R. Schwengner ◽  
S. Frauendorf ◽  
A. C. Larsen

Author(s):  
D. Bohle ◽  
Th. Guhr ◽  
U. Hartmann ◽  
K.-D. Hummel ◽  
G. Kilgus ◽  
...  

2018 ◽  
Vol 98 (6) ◽  
Author(s):  
J. E. Midtbø ◽  
A. C. Larsen ◽  
T. Renstrøm ◽  
F. L. Bello Garrote ◽  
E. Lima
Keyword(s):  

1999 ◽  
Vol 650 (3) ◽  
pp. 267-280 ◽  
Author(s):  
P. von Neumann-Cosel ◽  
A. Richter ◽  
C. Schlegel ◽  
R. Schulz

2020 ◽  
Vol 2 (1) ◽  
pp. 015006 ◽  
Author(s):  
J Horn-Stanja ◽  
E V Stenson ◽  
M R Stoneking ◽  
M Singer ◽  
U Hergenhahn ◽  
...  

2010 ◽  
Vol 168-169 ◽  
pp. 113-116 ◽  
Author(s):  
Mikhail V. Eremin ◽  
Joachim Deisenhofer ◽  
M.A. Fayzullin ◽  
C. Kant ◽  
Alois Loidl

We propose a new mechanism of exciton-magnon absorption in the 1D Heisenberg antiferromagnet KCuF3. It yields the correct description of the relative intensity of the spectral lines in both polarizations E c and E‖c. The magnon density of states has been calculated. The origin of the fine sideband structure in KCuF3 can be explained. The sharp magnon lines, observed in Ref. [1], correspond to the low energy singularities in the magnon density of states.


2003 ◽  
Vol 727 (1-2) ◽  
pp. 41-55 ◽  
Author(s):  
R.W. Fearick ◽  
G. Hartung ◽  
K. Langanke ◽  
G. Martínez-Pinedo ◽  
P. von Neumann-Cosel ◽  
...  

1999 ◽  
Vol 14 (23) ◽  
pp. 1599-1608 ◽  
Author(s):  
OLEG V. KECHKIN

We construct new class of solutions which describes a rotating electric–magnetic dipole in the low energy heterotic string theory. Our method is based on the use of symmetries which preserve asymptotic flatness property; the generation of the solution is performed in the variables which linearize the action of these symmetries. The constructed solution possesses nontrivial values of mass, dilaton and axion charges; the maximal value of angular momentum is defined by some combination of the electric and magnetic dipole moments which is invariant under the action of the electric–magnetic duality.


Author(s):  
Andrew J Coates

Titan is the only Moon in the Solar System with a significant permanent atmosphere. Within this nitrogen–methane atmosphere, an ionosphere forms. Titan has no significant magnetic dipole moment, and is usually located inside Saturn's magnetosphere. Atmospheric particles are ionized both by sunlight and by particles from Saturn's magnetosphere, mainly electrons, which reach the top of the atmosphere. So far, the Cassini spacecraft has made over 45 close flybys of Titan, allowing measurements in the ionosphere and the surrounding magnetosphere under different conditions. Here we review how Titan's ionosphere and Saturn's magnetosphere interact, using measurements from Cassini low-energy particle detectors. In particular, we discuss ionization processes and ionospheric photoelectrons, including their effect on ion escape from the ionosphere. We also discuss one of the unexpected discoveries in Titan's ionosphere, the existence of extremely heavy negative ions up to 10 000 amu at 950 km altitude.


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