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2014

Distinguishing f(R) gravity with cosmic voids

Zivick, Paul, Sutter, P. M.

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We use properties of void populations identified in N-body simulations to forecast the ability of upcoming galaxy surveys to differentiate models of f(R) gravity from \Lambda CDM cosmology.

We analyze simulations designed to mimic the densities, volumes, and clustering statistics of upcoming surveys, using the public VIDE toolkit.
We examine void abundances as a basic probe at redshifts 1.0 and 0.4.
We find that stronger f(R) coupling strengths produce voids up to ~20% larger in radius, leading to a significant shift in the void number function.

Distinguishing f(R) gravity with cosmic voids · Around

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Khoury J., Weltman A., 2004, Phys. Rev. D, 69
2004
Earlier work this paper cites.
Neyrinck M. C., 2008, Mon. Not. R. Astron. Soc., 386, 2101
2008
Earlier work this paper cites.
Laureijs R., Amiaux J., Arduini S., Auguères J. ., Brinchmann J., Cole R., Cropper M., Dabin C., Duvet L., Ealet A., et al., 2011, ArXiv:1110.3193
Original
2011
Earlier work this paper cites.

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2013
Cited alongside, same era.

Then

Sutter P. M., Carlesi E., Wandelt B. D., Knebe A., 2014, ArXiv e-prints
2014
Closest in time.
Sutter P. M., et al., 2014, ArXiv e-prints: 1406.1191
2014
Closest in time.

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