ダークエネルギーの記事

第五の力現代物理学が挑む未知の基本相互作用

Lambda-CDM, accelerated expansion of the universe. The timeline in this schematic diagram extends from the Big Bang/inflation era 13.8 billion years ago to the present cosmological time.

宇宙の加速膨張ダークエネルギーが導く時空の運命

$The ultimate fate of an expanding universe depends on the matter density Ω M {\displaystyle \Omega _{M}} and the dark energy density Ω Λ {\displaystyle \Omega _{\Lambda }} .$

宇宙の終焉ビッグバンから究極の運命まで

宇宙の終焉ビッグバン理論ダークエネルギービッグフリーズ

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$Except for the few stars in the foreground (which are bright and easily recognizable because only they have diffraction spikes), every speck of light in the composite photo is an individual galaxy, some of them as old as 13.2 billion years; the observable universe is estimated to contain more than 2 trillion galaxies.[1] From the Hubble eXtreme Deep Field.$