Cosmological Principle Evidence for Isotropy

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Cosmological Principle Evidence for Isotropy

Cosmological Principle The universe is homogeneous and isotropic on large scales. Implication: No center or special point exists in the universe • In a homogeneous universe, if one place is isotropic, then all other places are isotropic. • What do we mean by “homogeneous”? • In an inhomogeneous universe, one place might be – Homogeneous !" Inhomogeneous isotropic, but other place are anisotropic. • What do we mean by “isotropic”? – Thus, one place being isotropic does not prove – Isotropic !" Anisotropic homogeneity; however, inhomogeneity requires the existenec of “special points”. • Would it be possible that the universe is… – Homogeneous but anisotropic? • Isotropy is easier to test from one place in the – Inhomogeneous but isotropic? universe -- our place. – Inhomogeneous and anisotropic? – Homogeneity is more difficult to test because we have • Principle: Something we demand and rely on, but is to travel to other places in the universe! difficult to verify. Evidence for Isotropy • Distribution of diffuse microwave light – Cosmic Microwave Background • Distribution of radio galaxies – Afterglow of Big Bang • Observed with the Very Large Array (VLA) in New Mexico Temperature • There are 40,000 bright radio = 2.73K in all directions galaxies in the upper panel – Distribution is isotropic • There are about the same Anisotropy number of fainter radio galaxies ~ 1/100,000 in the bottom panel, which is a zoom-up of the small region in the upper panel Anisotropy ~ 1/100,000 • Distribution of diffuse X-ray light Homogeneity? – Cosmic X-ray Background – Superposition of AGNs Sloan Digital Sky Survey •The bright part of the Moon reflects X-rays from the Sun. •The dark part blocks any X- rays from behind of the Moon. •Isotropic “Cosmic X-ray Background” is seen around the Moon. •This diffuse X-ray light comes from AGNs which we don’t resolve out individually. Homogeneity on large scales • To see homogeneity, one has to “smear out” the irregularities at small distances (such as galaxies and clusters of galaxies) • Inhomogeneity does decrease at large distances – Homogeneous on large scales!.

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