Matches in SemOpenAlex for { <https://semopenalex.org/work/W2394228596> ?p ?o ?g. }
- W2394228596 abstract "We perform a validation of estimates of the growth rate of structure, described by the parameter combination $fsigma_8$, in modified gravity cosmologies. We consider an analysis pipeline based on the redshift-space distortion modelling of the clustering wedges statistic of the galaxy correlation function and apply it to mock catalogues of $Lambda{rm CDM}$ and the normal branch of DGP cosmologies. We employ a halo occupation distribution approach to construct our mocks, which we ensure resemble the CMASS sample from BOSS in terms of the total galaxy number density and large scale amplitude of the power spectrum monopole. We show that the clustering wedges model successfully recovers the true growth rate difference between DGP and $Lambda{rm CDM}$, even for cases with over 40% enhancement in $fsigma_8$ compared to $Lambda{rm CDM}$. The unbiased performance of the clustering wedges model allows us to use the growth rate values estimated from the BOSS DR12 data to constrain the cross-over scale $r_c$ of DGP gravity to $left[r_cH_0right]^{-1} < 0.97$ ($2sigma$) or $r_c > 3090 {rm Mpc}/h$, cutting into the interesting region of parameter space with $r_c sim H_0^{-1}$ using constraints from the growth of structure alone." @default.
- W2394228596 created "2016-06-24" @default.
- W2394228596 creator A5028407226 @default.
- W2394228596 creator A5029557191 @default.
- W2394228596 creator A5063812458 @default.
- W2394228596 date "2016-10-13" @default.
- W2394228596 modified "2023-10-14" @default.
- W2394228596 title "Validating estimates of the growth rate of structure with modified gravity simulations" @default.
- W2394228596 cites W1492154955 @default.
- W2394228596 cites W1540356931 @default.
- W2394228596 cites W1693975748 @default.
- W2394228596 cites W1751039464 @default.
- W2394228596 cites W1836372023 @default.
- W2394228596 cites W1839233296 @default.
- W2394228596 cites W1898650658 @default.
- W2394228596 cites W1937900445 @default.
- W2394228596 cites W1938366638 @default.
- W2394228596 cites W1948874727 @default.
- W2394228596 cites W1965779302 @default.
- W2394228596 cites W1967450024 @default.
- W2394228596 cites W1969647470 @default.
- W2394228596 cites W1977102999 @default.
- W2394228596 cites W1979642537 @default.
- W2394228596 cites W1999437090 @default.
- W2394228596 cites W2003255074 @default.
- W2394228596 cites W2004110391 @default.
- W2394228596 cites W2004188331 @default.
- W2394228596 cites W2009368822 @default.
- W2394228596 cites W2009693236 @default.
- W2394228596 cites W2010862536 @default.
- W2394228596 cites W2016741569 @default.
- W2394228596 cites W2026937401 @default.
- W2394228596 cites W2034157449 @default.
- W2394228596 cites W2034231122 @default.
- W2394228596 cites W2039602465 @default.
- W2394228596 cites W2043420039 @default.
- W2394228596 cites W2043908961 @default.
- W2394228596 cites W2048021339 @default.
- W2394228596 cites W2052394465 @default.
- W2394228596 cites W2056648447 @default.
- W2394228596 cites W2062526473 @default.
- W2394228596 cites W2065889919 @default.
- W2394228596 cites W2071937107 @default.
- W2394228596 cites W2073569280 @default.
- W2394228596 cites W2079938054 @default.
- W2394228596 cites W2083612340 @default.
- W2394228596 cites W2085263448 @default.
- W2394228596 cites W2090874374 @default.
- W2394228596 cites W2096407827 @default.
- W2394228596 cites W2100213110 @default.
- W2394228596 cites W2106026473 @default.
- W2394228596 cites W2112786259 @default.
- W2394228596 cites W2114744410 @default.
- W2394228596 cites W2117592896 @default.
- W2394228596 cites W2119048669 @default.
- W2394228596 cites W2127258377 @default.
- W2394228596 cites W2128130302 @default.
- W2394228596 cites W2128759530 @default.
- W2394228596 cites W2133186943 @default.
- W2394228596 cites W2139470207 @default.
- W2394228596 cites W2144226330 @default.
- W2394228596 cites W2150746633 @default.
- W2394228596 cites W2156305595 @default.
- W2394228596 cites W2166436681 @default.
- W2394228596 cites W2167025224 @default.
- W2394228596 cites W2170327775 @default.
- W2394228596 cites W2171317216 @default.
- W2394228596 cites W2172373321 @default.
- W2394228596 cites W2172444365 @default.
- W2394228596 cites W2205003259 @default.
- W2394228596 cites W2210628759 @default.
- W2394228596 cites W2253235198 @default.
- W2394228596 cites W2262956132 @default.
- W2394228596 cites W2277581298 @default.
- W2394228596 cites W2335636997 @default.
- W2394228596 cites W2464001455 @default.
- W2394228596 cites W3097984739 @default.
- W2394228596 cites W3098436526 @default.
- W2394228596 cites W3098893043 @default.
- W2394228596 cites W3101317610 @default.
- W2394228596 cites W3101719567 @default.
- W2394228596 cites W3102474852 @default.
- W2394228596 cites W3103321780 @default.
- W2394228596 cites W3105465984 @default.
- W2394228596 cites W3105554724 @default.
- W2394228596 cites W3105631369 @default.
- W2394228596 cites W3123971863 @default.
- W2394228596 cites W3125508083 @default.
- W2394228596 cites W3126091320 @default.
- W2394228596 cites W4234678205 @default.
- W2394228596 cites W4292875581 @default.
- W2394228596 cites W4293241892 @default.
- W2394228596 cites W996914278 @default.
- W2394228596 doi "https://doi.org/10.1103/physrevd.94.084022" @default.
- W2394228596 hasPublicationYear "2016" @default.
- W2394228596 type Work @default.
- W2394228596 sameAs 2394228596 @default.
- W2394228596 citedByCount "49" @default.
- W2394228596 countsByYear W23942285962017 @default.
- W2394228596 countsByYear W23942285962018 @default.