ASTROPHYSICAL PROBLEMS OF CONDENSED MATTER IN HUGE MAGNETIC FIELDS

A large occurrence of weak magnetic fields in hot stars would also have a direct impact on stellar evolution models by providing the first direct constraints on the value of

Reste dès lors à envisager la conséquence de cette opposition, pour tâcher de comprendre en quoi l’affordance de liste engage une action particulière de son lecteur lorsque

(2005) determined the field strengths and the inclinations of magnetic dipoles by comparing the observed spectra visually with model spectra calculated using a simplified

As a result, the star reaches an equilibrium rotation law close to uniform (see models in the above ref.), with always a strong thermal instability amplifying meridional circulation

The theory predicts that both the density of electron states p(EF) and the electron mean lifetime =(EF) at the Fermi energy EF will oscillate while changing magnetic

L’archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des

as the neutrons enter the magnetic field at the sample position they are subject to a force produced by the magnetic field gradient of the sample magnet and

An axial map of the shield for the initial field of 150 microgauss is shown in figure 5. The field perpendicular to the axis was also less than 2 micro-