dc.date.accessioned |
2024-01-09T10:11:38Z |
|
dc.date.available |
2024-01-09T10:11:38Z |
|
dc.date.issued |
2024-01-09 |
|
dc.identifier.uri |
http://repository.cuilahore.edu.pk/xmlui/handle/123456789/3889 |
|
dc.description.abstract |
In thisthesis,weassumeFRWuniverseincontextof¯ve-dimensional
Einstein Chern-Simonstheoryofgravity.TheBarrowholographicdark
energy densitywithHubblehorizonasboundaryoftheuniverseistaken
intoaccounttostudycosmicevolutionoftheuniverse.Wediscusssome
cosmological parameterssuchascoincidenceparameter,densityparame-
ter, EoSparameteranddecelerationparameter.Moreover,wealsodiscuss
the thermalstabilityincontextofunderlyingscenario.Weplotcoinci-
dence parameterwhichexhibitaDEdominatedphaseoftheuniverse.We
consider Barrowholographicdarkenergymodelwithbothinteractingand
non-interactingscenarioofdarkcomponentstoevaluatetheseparameters
and thermalstability.Itismentionedherethatweobtainsomeconsistent
results representingacceleratedexpansionoftheuniverse. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Comsats CUI Lahore |
en_US |
dc.relation.ispartofseries |
FA21-RMT-043;8532 |
|
dc.subject |
FRW universe, Hubble horizon, Holographic Dark Energy, Dimensional Modified Gravity |
en_US |
dc.title |
Analysis of Barrow Holographic Dark Energy in Five- Dimensional Modified Gravity |
en_US |
dc.type |
Thesis |
en_US |