Effect of antiferromagnetic RKKY interaction and magnetic field in a two-impurity Kondo system

2010 ◽  
Vol 82 (15) ◽  
Author(s):  
Emi Minamitani ◽  
Wilson Agerico Diño ◽  
Hiroshi Nakanishi ◽  
Hideaki Kasai
Keyword(s):  
Magnetic Field ◽  
Rkky Interaction ◽  
Kondo System

scholarly journals Effect of magnetic field and chemical potential on the RKKY interaction in the α−T3 lattice

2021 ◽  
Vol 103 (7) ◽  
Author(s):  
Oleksiy Roslyak ◽  
Godfrey Gumbs ◽  
Antonios Balassis ◽  
Heba Elsayed
Keyword(s):  
Magnetic Field ◽  
Chemical Potential ◽  
Rkky Interaction

scholarly journals Temperature and magnetic field dependence of a Kondo system in the weak coupling regime

2013 ◽  
Vol 4 (1) ◽  
Author(s):  
Yong-hui Zhang ◽  
Steffen Kahle ◽  
Tobias Herden ◽  
Christophe Stroh ◽  
Marcel Mayor ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Field Dependence ◽  
Weak Coupling ◽  
Magnetic Field Dependence ◽  
Weak Coupling Regime ◽  
Kondo System

Magnetic Field Depreciation of a Kondo System

1972 ◽  
Vol 5 (9) ◽  
pp. 3788-3790 ◽  
Author(s):  
E. W. Fenton
Keyword(s):  
Magnetic Field ◽  
Kondo System

RKKY interaction in semiconductors: Effects of magnetic field and screening

2004 ◽  
Vol 70 (7) ◽  
Author(s):  
C. H. Ziener ◽  
S. Glutsch ◽  
F. Bechstedt
Keyword(s):  
Magnetic Field ◽  
Rkky Interaction

Magnetic-field strengths from optical polarization data

1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg
Keyword(s):  
Magnetic Field ◽  
Optical Polarization ◽  
Polarization Data ◽  
Term Model ◽  
Source Of Information ◽  
Field Strengths

Van de Hulst (Paper 64, Table 1) has marked optical polarization as a questionable or marginal source of information concerning magnetic field strengths. Rather than arguing about this–I should rate this method asq+-, or quarrelling about the term ‘model-sensitive results’, I wish to stress the historical point that as recently as two years ago there were still some who questioned that optical polarization was definitely due to magnetically-oriented interstellar particles.

Observing the galactic magnetic field

1967 ◽  
Vol 31 ◽  
pp. 375-380
Author(s):  
H. C. van de Hulst
Keyword(s):  
Magnetic Field ◽  
Fair Agreement ◽  
Solar Neighbourhood ◽  
Galactic Magnetic Field ◽  
The Magnetic Field

Various methods of observing the galactic magnetic field are reviewed, and their results summarized. There is fair agreement about the direction of the magnetic field in the solar neighbourhood:l= 50° to 80°; the strength of the field in the disk is of the order of 10-5gauss.

Sign in / Sign up

Export Citation Format

Share Document