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arXiv · 1810.11915

The large scale structure in the 3D luminosity-distance space and its cosmological applications

Pengjie Zhang
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Abstract

Future gravitational wave (GW) observations are capable of detecting millions of compact star binary mergers in extragalactic galaxies, with $1\%$ luminosity-distance ($D_L$) measurement accuracy and better than arcminute positioning accuracy. This will open a new window of the large scale structure (LSS) of the universe, in the 3D {\bf luminosity-distance space (LDS)}, instead of the 3D redshift space of galaxy spectroscopic surveys. The baryon acoustic oscillation and the AP test encoded in the LDS LSS constrain the $D_L$-$D^{\rm co}_A$ (comoving angular diameter distance) relation and therefore the expansion history of the universe. Peculiar velocity induces the LDS distortion, analogous to the redshift space distortion, and allows for a new structure growth measure $f_L\sigma_8$. When the distance duality is enforced ($1+z=D_L/D^{\rm co}_A$), the LDS LSS by itself determines the redshift to $\sim 1\%$ level accuracy, and alleviates the need of spectroscopic follow-up of GW events.But a more valuable application is to test the distance duality to $1\%$ level accuracy, in combination with conventional BAO and supernovae measurements. This will put stringent constraints on modified gravity models in which the gravitational wave $D^{\rm GW}_L$ deviates from the electromagnetic wave $D^{EM}_L$. All these applications require no spectroscopic follow-ups.

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Pengjie Zhang. 2018-10-29. The large scale structure in the 3D luminosity-distance space and its cosmological applications. https://arxiv.org/abs/1810.11915

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