scholarly journals Consolidating the concept of low-energy magnetic dipole decay radiation

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

scholarly journals Low-Energy Enhancement of Magnetic Dipole Radiation

2013 ◽  
Vol 111 (23) ◽  
Author(s):  
R. Schwengner ◽  
S. Frauendorf ◽  
A. C. Larsen
Keyword(s):  
Magnetic Dipole ◽  
Low Energy ◽  
Dipole Radiation

Properties of a New Magnetic Dipole Mode Discovered in Low Energy Electron Scattering

1986 ◽  
pp. 311-320 ◽  
Author(s):  
D. Bohle ◽  
Th. Guhr ◽  
U. Hartmann ◽  
K.-D. Hummel ◽  
G. Kilgus ◽  
...  
Keyword(s):  
Magnetic Dipole ◽  
Electron Scattering ◽  
Low Energy ◽  
Energy Electron ◽  
Dipole Mode ◽  
Low Energy Electron

Low-energy magnetic dipole response in the 57Fe(γ,γ′) reaction

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

scholarly journals Injection of intense low-energy reactor-based positron beams into a supported magnetic dipole trap

2020 ◽  
Vol 2 (1) ◽  
pp. 015006 ◽  
Author(s):  
J Horn-Stanja ◽  
E V Stenson ◽  
M R Stoneking ◽  
M Singer ◽  
U Hergenhahn ◽  
...  
Keyword(s):  
Magnetic Dipole ◽  
Low Energy ◽  
Dipole Trap ◽  
Positron Beams

Exchange-Induced Magnetic Dipole Mechanism of Magnon Sideband

2010 ◽  
Vol 168-169 ◽  
pp. 113-116 ◽  
Author(s):  
Mikhail V. Eremin ◽  
Joachim Deisenhofer ◽  
M.A. Fayzullin ◽  
C. Kant ◽  
Alois Loidl
Keyword(s):  
Magnetic Dipole ◽  
Density Of States ◽  
Relative Intensity ◽  
Low Energy ◽  
Spectral Lines ◽  
Heisenberg Antiferromagnet ◽  
Correct Description

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.

Low-energy magnetic dipole response in 56Fe from high-resolution electron scattering

2003 ◽  
Vol 727 (1-2) ◽  
pp. 41-55 ◽  
Author(s):  
R.W. Fearick ◽  
G. Hartung ◽  
K. Langanke ◽  
G. Martínez-Pinedo ◽  
P. von Neumann-Cosel ◽  
...  
Keyword(s):  
High Resolution ◽  
Magnetic Dipole ◽  
Electron Scattering ◽  
Low Energy ◽  
Resolution Electron ◽  
Dipole Response

ROTATING BONNOR SOLUTION IN DILATON–AXION GRAVITY

1999 ◽  
Vol 14 (23) ◽  
pp. 1599-1608 ◽  
Author(s):  
OLEG V. KECHKIN
Keyword(s):  
Angular Momentum ◽  
String Theory ◽  
Magnetic Dipole ◽  
Dipole Moments ◽  
Low Energy ◽  
Heterotic String ◽  
Heterotic String Theory ◽  
New Class ◽  
Asymptotic Flatness ◽  
Flatness Property

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.

Interaction of Titan's ionosphere with Saturn's magnetosphere

2008 ◽  
Vol 367 (1889) ◽  
pp. 773-788 ◽  
Author(s):  
Andrew J Coates
Keyword(s):  
Dipole Moment ◽  
Solar System ◽  
Magnetic Dipole ◽  
Magnetic Dipole Moment ◽  
Negative Ions ◽  
Low Energy ◽  
Energy Particle ◽  
Particle Detectors ◽  
Ion Escape ◽  
Ionization Processes

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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