Show simple item record

dc.contributor.authorVenter, Christo
dc.date.accessioned2009-01-30T06:41:23Z
dc.date.available2009-01-30T06:41:23Z
dc.date.issued2004
dc.identifier.urihttp://hdl.handle.net/10394/215
dc.descriptionThesis (M.Sc. (Physics))--North-West University, Potchefstroom Campus, 2004.
dc.description.abstractIt has been noted by several authors that General Relativistic frame dragging in rotating neutron stars is a first order effect which has to be included in a self-consistent model of pulsar magnetospheric structure and associated radiation and transport processes. To this end, I undertook the present study with the aim of investigating the effect of General Relativity (GR) on millisecond pulsar (MSP) visibility. I developed a numerical code for simulating a pulsar magnetosphere, incorporating the GR-corrected expressions for the electric potential and field. I included curvature radiation (CR) due to primary electrons accelerated above the stellar surface, as well as inverse Compton scattering (ICS) of thermal X-ray photons by these electrons. I then applied the model to PSR J0437-4715, a prime candidate for testing the GR-Electrodynamic theory, and examined its visibility for the H.E.S.S. telescope. I also considered the question of whether magnetic photon absorption would take place for this particular pulsar. In addition, I developed a classical model for comparison with the GR results. I found that the typical electron energies and associated CR photon energies are functions of position above the polar cap (PC). These energies are also quite smaller in the GR case than in the classical case due to the different functional forms of the GR and classical electric fields. I found the CR energy cut-off to be ~ 4 GeV compared to the well-known classical value of ~ 100 GeV. Since the H.E.S.S. energy threshold is ~ 100 GeV, it seems as though the CR component will not be visible, contrary to wide-held opinion. However, the ICS component seems to be well in excess of the H.E.S.S. energy threshold and is expected to be visible. I also found that no pair production will take place for PSR J0437-4715. Hopefully, forthcoming H.E.S.S. observations will provide validation of these results. KEY WORDS: General relativistic frame dragging, GR electrodynamics, millisecond pulsar visibility, non-thermal radiation processes, pair production, H.E.S.S., individual pulsars: PSR J0437-4715.
dc.publisherNorth-West University
dc.subjectGeneral relativistic frame draggingen
dc.subjectGR electrodynamics, millisecond pulsar visibilityen
dc.subjectNon-thermal radiation processesen
dc.subjectPair productionen
dc.subjectH.E.S.S.en
dc.subjectIndividual pulsars: PSR J0437-4715en
dc.titleThe effect of general relativistic frame dragging on millisecond pulsar visibility for the H.E.S.S. telescope / C. Venteren
dc.typeThesisen
dc.description.thesistypeMasters


Files in this item

Thumbnail

This item appears in the following Collection(s)

  • ETD@PUK [6299]
    This collection contains the original digitized versions of research conducted at the North-West University (Potchefstroom Campus)

Show simple item record