2011

Measuring equality horizon with the zero-crossing of the galaxy correlation function

Prada, F., Klypin, A., Yepes, G. et al.

Understand

The size of the horizon at the matter-radiation equality is a key scale of the Big Bang cosmology that is directly related to the energy-matter content of the Universe.

  • In this letter, we argue that this scale can be accurately measured from the observed clustering of galaxies in new large scale surveys.
  • We demonstrate that the zero-crossing, r_c, of the 2-point galaxy correlation function is closely related to the horizon size at matter-radiation equality for a large variety of flat LCDM models.
  • Using large-volume cosmological simulations, we also show that the pristine zero-crossing is unaltered by non-linear evolution of density fluctuations, redshift distortions and galaxy biases.

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