scholarly journals The Pulsar Magnetosphere – A Stationary Self-Consistent Solution

1996 ◽  
Vol 160 ◽  
pp. 429-430
Author(s):  
Bernhard Hofmann ◽  
Heinz Herold ◽  
Hanns Ruder

AbstractUsing fundamental equations of physics we determine with a simple model a globally self-consistent state of a pulsar magnetosphere.

1988 ◽  
Vol 03 (03) ◽  
pp. 295-301 ◽  
Author(s):  
A.P. CONTOGOURIS ◽  
N. MEBARKI ◽  
D. ATWOOD ◽  
H. TANAKA

Possible strong interaction effects arising when the Higgs mass MH is sufficiently large are investigated in the system of interacting Higgs, using dispersion relations (N/D method). A simple model indicates that for MH≳1 TeV several such effects are present: an 1=0 bound state, large s-wave phase shifts and a resonance-like state. In the range 1.5≲MH≲3.5 TeV the above bound state amounts to an approximate bootstrap (self-consistent) solution for the Higgs with respect to both its mass and coupling. Other aspects of the H-H strong interaction system are also investigated.


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