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

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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 ;


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