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R. Scoccimarro, R. K. Sheth, L. Hui and B. Jain, Astrophys. J. 546
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E. Sefusatti, M. Crocce, S. Pueblas and R. Scoccimarro, Phys. Rev. D 74
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C. Conroy, R. H. Wechsler and A. V. Kravtsov, Astrophys. J. 647
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2017

Constraining modified theory of gravity with galaxy bispectrum

Yamauchi, Daisuke, Yokoyama, Shuichiro, Tashiro, Hiroyuki

Understand

We explore the use of galaxy bispectrum induced by the nonlinear gravitational evolution as a possible probe to test general scalar-tensor theories with second-order equations of motion.

We find that time dependence of the leading second-order kernel is approximately characterized by one parameter, the second-order index, which is expected to trace the higher-order growth history of the Universe.
We show that our new parameter can significantly carry new information about the non-linear growth of structure.
We forecast future constraints on the second-order index as well as the equation-of-state parameter and the growth index.

Built on

G. W. Horndeski, Int. J. Theor. Phys. 10
1974
Earlier work this paper cites.
N. Kaiser, Mon. Not. Roy. Astron. Soc. 227
1987
Earlier work this paper cites.
A. J. S. Hamilton, Astrophys. J. 385
1992
Earlier work this paper cites.
R. Scoccimarro, H. M. P. Couchman and J. A. Frieman, Astrophys. J. 517
1999
Earlier work this paper cites.
R. K. Sheth and G. Tormen, Mon. Not. Roy. Astron. Soc. 308
1999
Earlier work this paper cites.
R. Scoccimarro and H. M. P. Couchman, Mon. Not. Roy. Astron. Soc. 325
2001
Earlier work this paper cites.
R. Scoccimarro, R. K. Sheth, L. Hui and B. Jain, Astrophys. J. 546
2001
Earlier work this paper cites.
R. Scoccimarro, E. Sefusatti and M. Zaldarriaga, Phys. Rev. D 69
2004
Earlier work this paper cites.
E. V. Linder, Phys. Rev. D 72
2005
Earlier work this paper cites.
J. L. Tinker, D. H. Weinberg, Z. Zheng and I. Zehavi, Astrophys. J. 631
2005
Earlier work this paper cites.
E. Sefusatti, M. Crocce, S. Pueblas and R. Scoccimarro, Phys. Rev. D 74
2006
Earlier work this paper cites.
C. Conroy, R. H. Wechsler and A. V. Kravtsov, Astrophys. J. 647
2006
Earlier work this paper cites.