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The view from the boundary: a new void stacking method

Cautun, M.; Cai, Y.-C.; Frenk, C.S.

The view from the boundary: a new void stacking method Thumbnail


M. Cautun

Y.-C. Cai


We introduce a new method for stacking voids and deriving their profile that greatly increases the potential of voids as a tool for precision cosmology. Given that voids are distinctly non-spherical and have most of their mass at their edge, voids are better described relative to their boundary rather than relative to their centre, as in the conventional spherical stacking approach. The boundary profile is obtained by computing the distance of each volume element from the void boundary. Voids can then be stacked and their profiles computed as a function of this boundary distance. This approach enhances the weak lensing signal of voids, both shear and convergence, by a factor of 2 when compared to the spherical stacking method. It also results in steeper void density profiles that are characterized by a very slow rise inside the void and a pronounced density ridge at the void boundary. The resulting boundary density profile is self-similar when rescaled by the thickness of the density ridge, implying that the average rescaled profile is independent of void size. The boundary velocity profile is characterized by outflows in the inner regions whose amplitude scales with void size, and by a strong inflow into the filaments and walls delimiting the void. This new picture enables a straightforward discrimination between collapsing and expanding voids both for individual objects as well as for stacked samples.


Cautun, M., Cai, Y., & Frenk, C. (2016). The view from the boundary: a new void stacking method. Monthly Notices of the Royal Astronomical Society, 457(3), 2540-2553.

Journal Article Type Article
Acceptance Date Jan 15, 2016
Online Publication Date Feb 10, 2016
Publication Date Apr 11, 2016
Deposit Date Apr 5, 2016
Publicly Available Date Apr 7, 2016
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 457
Issue 3
Pages 2540-2553


Published Journal Article (2.9 Mb)

Copyright Statement
This article has been published in Monthly Notices of the Royal Astronomical Society ©: 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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