Solution of the dirac equation in curved Space time in the presence of a strong Back ground magnetic field

dc.contributor.advisorWotro, Legesse (PhD)
dc.contributor.authorMekonnen, Eshetu
dc.date.accessioned2018-06-22T08:37:33Z
dc.date.accessioned2023-11-09T11:23:30Z
dc.date.available2018-06-22T08:37:33Z
dc.date.available2023-11-09T11:23:30Z
dc.date.issued2013-06
dc.description.abstractIn this thesis we propose a curved spacetime version of the Dirac equation. The equation has been developed mainly to try and account in a natural way for the solution of the Dirac equation in curved spacetime in an open cosmological universe with a partially horn topology in the presence of a time dependent magnetic eld. Since the exact solution cannot be obtained explicitly for arbitrary time dependence of the eld, we discuss the asymptotic behavior of the solutions with the help of the relativistic Hamilton-Jacobi equationen_US
dc.identifier.urihttp://10.90.10.223:4000/handle/123456789/2949
dc.language.isoenen_US
dc.publisherAddis Ababa Universityen_US
dc.subjectSolution of the Dirac Equationen_US
dc.titleSolution of the dirac equation in curved Space time in the presence of a strong Back ground magnetic fielden_US
dc.typeThesisen_US

Files

Original bundle
Now showing 1 - 1 of 1
No Thumbnail Available
Name:
Eshetu Mekonnen Abebe.pdf
Size:
380.31 KB
Format:
Adobe Portable Document Format
License bundle
Now showing 1 - 1 of 1
No Thumbnail Available
Name:
license.txt
Size:
1.71 KB
Format:
Plain Text
Description:

Collections