Dirac states of an electron in a circular intense magnetic field

21 Mar 2017 Voisin Guillaume LUTH Bonazzola Silvano LUTH Mottez Fabrice CNRS, LUTH

Neutron-star magnetospheres are structured by very intense magnetic fields extending from 100 to 10 5 km traveled by very energetic electrons and positrons with Lorentz factors up to $\sim$ 10 7. In this context, particles are forced to travel almost along the magnetic field with very small gyro-motion, potentially reaching the quantified regime... (read more)

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Categories


  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • HIGH ENERGY PHYSICS - THEORY
  • QUANTUM PHYSICS