2d Geometry of Quadrapole Magnetic field Lines from Neutron Star and Associated Radiation Pressure

dc.contributor.advisorWetro, Legesse (PhD)
dc.contributor.authorGirma, Melkameshet
dc.date.accessioned2018-06-29T06:20:52Z
dc.date.accessioned2023-11-09T11:24:01Z
dc.date.available2018-06-29T06:20:52Z
dc.date.available2023-11-09T11:24:01Z
dc.date.issued2011-06
dc.description.abstractIn this thesis we have derived the vector potential to determine the analytic expressions for the magnetic eld of dipole and quadrupole components of neutron star, we develop the eld line equations and the magnetic eld line geometry of both dipole and quadrupole terms. The magnetic eld varies with time and as well as the induced electric eld. As a result the neutron star can generate electromagnetic radiation. This electromagnetic radiation has pressure. We have derived the radiation pressure at any distance r out side of the surface of the neutron staren_US
dc.identifier.urihttp://10.90.10.223:4000/handle/123456789/4803
dc.language.isoenen_US
dc.publisherAddis Ababa Universityen_US
dc.subject2d Geometry of Quadrapoleen_US
dc.title2d Geometry of Quadrapole Magnetic field Lines from Neutron Star and Associated Radiation Pressureen_US
dc.typeThesisen_US

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