Kinetic theory in k=0 Friedmann-Robertson-Walker cosmology

dc.contributor	Graduate Program in Physics.
dc.contributor.advisor	Akant, Levent.
dc.contributor.author	Tülümen, Nimet.
dc.date.accessioned	2023-03-16T10:37:14Z
dc.date.available	2023-03-16T10:37:14Z
dc.date.issued	2016.
dc.identifier.other	PHYS 2016 T86
dc.identifier.uri	http://digitalarchive.boun.edu.tr/handle/123456789/13606
dc.description.abstract	In the thesis we calculated Boltzmann Equation in RW metric. After that in the at space-like slices we showed that for RW metric it is not possible to nd any equilibrium solutions. However we looked for the equilibrium solutions in the two limits when mass goes to zero and when mass goes to in nity. Then we applied these result to the Bose-Einstein and to the Fermi-Dirac statistics for nding the equilibrium solution in the limits. Finally in the Bose-Einstein Condensation we calculated critical temperature.
dc.format.extent	30 cm.
dc.publisher	Thesis (M.S.) - Bogazici University. Institute for Graduate Studies in Science and Engineering, 2016.
dc.subject.lcsh	Kinetic theory of matter.
dc.subject.lcsh	Cosmology.
dc.title	Kinetic theory in k=0 Friedmann-Robertson-Walker cosmology
dc.format.pages	viii, 44 leaves ;