Imwe yenzira dzakakosha dzekufungidzira kuti zvinhu zvose zvakasikwa zvinogona kushandiswa kune zvakasikwa zvose. Zvisinei, pane zviyero zvakakura, zvakasikwa zvedu zvinoratidzika kunge zvakagadzirwa pamwe chete nemitsara yakajeka: zvose zvinowanikwa zvino zvinoratidza kuti, paavhareji, chimiro chemuchadenga chinofanira kunge chakafanana, pasinei nechinzvimbo chechitaridzi kana kutungamira kwekucherechedza: zvakasikwa zvose zvinenge zvakafanana uye isotropic. Zvinhu zvose zvakasikwa zvakaenzaniswa zvinogona kurondedzerwa nemhinduro dzakareruka dzeEinstein's equations. Mazuva ano cosmological models of the universe are obtained by combining these simple solutions to general relativity with the theories describing the properties of the universe's content matter, namely dynamics, nuclear-modules and physics. Maererano nemashoko edu, zvinhu zvose zvakasikwa zvinobva kune dense-temperature dense-temperature state <unk> roughly statically expanding within the Big Bang <unk> roughly roughly roughly roughly roughly roughly roughly roughly roughly
Kuputika Kukuru