In the solid crusts of neutron stars, the advection of the magnetic field by the current-carrying electrons, an effect known as Hall drift, should play a very important role as the ions remain essentially fixed (as long as the solid does not break). Although Hall drift preserves the magnetic field e...

Full description

Autores:
Tipo de recurso:
Fecha de publicación:
2014
Institución:
Universidad de Medellín
Repositorio:
Repositorio UDEM
Idioma:
eng
OAI Identifier:
oai:repository.udem.edu.co:11407/1374
Acceso en línea:
http://hdl.handle.net/11407/1374
Palabra clave:
instabilities
magnetic fields
stars: magnetars
stars: magnetic field
stars: neutron
Rights
restrictedAccess
License
http://purl.org/coar/access_right/c_16ec