期刊
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
卷 -, 期 10, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2019/10/023
关键词
cosmic web; modified gravity; dark energy theory
资金
- Leverhulme Trust
- Royal Society University Research fellowship
- STFC [ST/P000703/1] Funding Source: UKRI
One of the most pressing questions in modified gravity is how deviations from general relativity can manifest in upcoming galaxy surveys. This is especially relevant for theories exhibiting Vainshtein screening, where such deviations are efficiently suppressed within a (typically large) Vainshtein radius. However, Vainshtein screening is known to be shape dependent: it is most effective around spherical sources, weaker around cylindrical objects and completely absent for planar sources. The Cosmic Web therefore offers a testing ground, as it displays many shapes in the form of clusters, filaments and walls. In this work, we explicitly derive the signature of the shape dependence of Vainshtein screening on the matter bispectrum, by considering a cubic Galileon model with a conformal coupling to matter and a cosmological constant. We perform a second order perturbative analysis, deriving analytic, integral expressions for the bispectrum, which we integrate using hi class. We find that the shape dependence of Vainshtein screening enters the bispectrum with a unique scale-factor dependence of proportional to a(3/2). The magnitude of the effect today is up to 2% for a model whose linear growth rate deviates up to 5% from Lambda CDM.
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