scholarly journals Constraints on the growth of structure around cosmic voids in eBOSS DR14

2020 ◽  
Vol 2020 (06) ◽  
pp. 012-012 ◽  
Author(s):  
Adam J. Hawken ◽  
Marie Aubert ◽  
Alice Pisani ◽  
Marie-Claude Cousinou ◽  
Stephanie Escoffier ◽  
...  
Keyword(s):  
2020 ◽  
Author(s):  
Laird A. Thompson
Keyword(s):  

2015 ◽  
Vol 448 (1) ◽  
pp. 642-653 ◽  
Author(s):  
Andrii Elyiv ◽  
Federico Marulli ◽  
Giorgia Pollina ◽  
Marco Baldi ◽  
Enzo Branchini ◽  
...  

2015 ◽  
Vol 455 (3) ◽  
pp. 3075-3085 ◽  
Author(s):  
Giorgia Pollina ◽  
Marco Baldi ◽  
Federico Marulli ◽  
Lauro Moscardini
Keyword(s):  

2021 ◽  
Author(s):  
Danny C. Pan
Keyword(s):  

Quasars ◽  
1986 ◽  
pp. 575-576
Author(s):  
P. M. Gondhalekar ◽  
N. Brosch
Keyword(s):  

1996 ◽  
pp. 461-461
Author(s):  
J. Vennik ◽  
B. Kovachev ◽  
U. Hopp ◽  
B. Kuhn

2019 ◽  
Vol 27 ◽  
pp. 34-52 ◽  
Author(s):  
X. Xu ◽  
J. Cisewski-Kehe ◽  
S.B. Green ◽  
D. Nagai

2014 ◽  
Vol 11 (S308) ◽  
pp. 571-574
Author(s):  
A. J. Hawken ◽  
D. Michelett ◽  
B. Granett ◽  
A. Iovino ◽  
L. Guzzo

AbstractUsing an algorithm based on searching for empty spheres we identified 245 voids in the VIMOS Public Extragalactic Redshift Survey (VIPERS). We show how by modelling the anisotropic void-galaxy cross correlation function we can probe the growth rate of structure.


2019 ◽  
Vol 1221 ◽  
pp. 012031
Author(s):  
Isidro Gómez-Vargas ◽  
Ricardo Medel-Esquivel ◽  
Ricardo García-Salcedo

2014 ◽  
Vol 11 (S308) ◽  
pp. 589-590 ◽  
Author(s):  
P. Zivick ◽  
P. M. Sutter

AbstractWe 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 \lcdm cosmology. We analyze simulations designed to mimic the densities, volumes, and clustering statistics of upcoming surveys, using the public {\tt 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. As an initial estimate of the constraining power of voids, we use this change in the number function to forecast a constraint on the coupling strength of Δ fR0 = 10-5.


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