Matches in SemOpenAlex for { <https://semopenalex.org/work/W2085263448> ?p ?o ?g. }
- W2085263448 abstract "We perform a Markov chain Monte Carlo analysis of the self-accelerating and normal branch of Dvali-Gabadadze-Porrati braneworld gravity. By adopting a parametrized post-Friedmann description of gravity, we utilize all of the cosmic microwave background data, including the largest scales, and its correlation with galaxies in addition to the geometrical constraints from supernovae distances and the Hubble constant. We find that on both branches brane tension or a cosmological constant is required at high significance with no evidence for the unique Dvali-Gabadadze-Porrati modifications. The crossover scale must therefore be substantially greater than the Hubble scale ${H}_{0}{r}_{c}>3$ and 3.5 at the 95% C.L. with and without uncertainties from spatial curvature. With spatial curvature, the limit from the normal branch is substantially assisted by the galaxy cross correlation which highlights its importance in constraining infrared modifications to gravity." @default.
- W2085263448 created "2016-06-24" @default.
- W2085263448 creator A5025963003 @default.
- W2085263448 creator A5032638535 @default.
- W2085263448 creator A5057785475 @default.
- W2085263448 creator A5087071619 @default.
- W2085263448 date "2009-09-28" @default.
- W2085263448 modified "2023-10-11" @default.
- W2085263448 title "Cosmological constraints on DGP braneworld gravity with brane tension" @default.
- W2085263448 cites W1485300610 @default.
- W2085263448 cites W1548726628 @default.
- W2085263448 cites W1908723437 @default.
- W2085263448 cites W1944901286 @default.
- W2085263448 cites W1963983981 @default.
- W2085263448 cites W1966667130 @default.
- W2085263448 cites W1967450024 @default.
- W2085263448 cites W1980647430 @default.
- W2085263448 cites W2004485587 @default.
- W2085263448 cites W2036902403 @default.
- W2085263448 cites W2040557753 @default.
- W2085263448 cites W2056648447 @default.
- W2085263448 cites W2071937107 @default.
- W2085263448 cites W2099378658 @default.
- W2085263448 cites W2103067535 @default.
- W2085263448 cites W2106766431 @default.
- W2085263448 cites W2115324751 @default.
- W2085263448 cites W2115659244 @default.
- W2085263448 cites W2119487926 @default.
- W2085263448 cites W2124028531 @default.
- W2085263448 cites W2131260550 @default.
- W2085263448 cites W2131628703 @default.
- W2085263448 cites W2133186943 @default.
- W2085263448 cites W2135630023 @default.
- W2085263448 cites W2136696603 @default.
- W2085263448 cites W2139470207 @default.
- W2085263448 cites W2142220522 @default.
- W2085263448 cites W2143513913 @default.
- W2085263448 cites W2148386612 @default.
- W2085263448 cites W2151768910 @default.
- W2085263448 cites W2153208487 @default.
- W2085263448 cites W2169351004 @default.
- W2085263448 cites W2594609997 @default.
- W2085263448 cites W3037468666 @default.
- W2085263448 cites W3097984739 @default.
- W2085263448 cites W3099676335 @default.
- W2085263448 cites W3100776897 @default.
- W2085263448 cites W3101639755 @default.
- W2085263448 cites W3126091320 @default.
- W2085263448 doi "https://doi.org/10.1103/physrevd.80.063536" @default.
- W2085263448 hasPublicationYear "2009" @default.
- W2085263448 type Work @default.
- W2085263448 sameAs 2085263448 @default.
- W2085263448 citedByCount "79" @default.
- W2085263448 countsByYear W20852634482012 @default.
- W2085263448 countsByYear W20852634482013 @default.
- W2085263448 countsByYear W20852634482014 @default.
- W2085263448 countsByYear W20852634482015 @default.
- W2085263448 countsByYear W20852634482016 @default.
- W2085263448 countsByYear W20852634482017 @default.
- W2085263448 countsByYear W20852634482018 @default.
- W2085263448 countsByYear W20852634482019 @default.
- W2085263448 countsByYear W20852634482020 @default.
- W2085263448 countsByYear W20852634482021 @default.
- W2085263448 countsByYear W20852634482022 @default.
- W2085263448 countsByYear W20852634482023 @default.
- W2085263448 crossrefType "journal-article" @default.
- W2085263448 hasAuthorship W2085263448A5025963003 @default.
- W2085263448 hasAuthorship W2085263448A5032638535 @default.
- W2085263448 hasAuthorship W2085263448A5057785475 @default.
- W2085263448 hasAuthorship W2085263448A5087071619 @default.
- W2085263448 hasBestOaLocation W20852634482 @default.
- W2085263448 hasConcept C103874350 @default.
- W2085263448 hasConcept C108568745 @default.
- W2085263448 hasConcept C121332964 @default.
- W2085263448 hasConcept C124017977 @default.
- W2085263448 hasConcept C130044071 @default.
- W2085263448 hasConcept C166861157 @default.
- W2085263448 hasConcept C171969306 @default.
- W2085263448 hasConcept C172790937 @default.
- W2085263448 hasConcept C195065555 @default.
- W2085263448 hasConcept C207297109 @default.
- W2085263448 hasConcept C2524010 @default.
- W2085263448 hasConcept C26405456 @default.
- W2085263448 hasConcept C2776605907 @default.
- W2085263448 hasConcept C2779625871 @default.
- W2085263448 hasConcept C33332235 @default.
- W2085263448 hasConcept C33923547 @default.
- W2085263448 hasConcept C37914503 @default.
- W2085263448 hasConcept C44870925 @default.
- W2085263448 hasConcept C62520636 @default.
- W2085263448 hasConcept C68249636 @default.
- W2085263448 hasConcept C74650414 @default.
- W2085263448 hasConcept C84114770 @default.
- W2085263448 hasConcept C85725439 @default.
- W2085263448 hasConceptScore W2085263448C103874350 @default.
- W2085263448 hasConceptScore W2085263448C108568745 @default.
- W2085263448 hasConceptScore W2085263448C121332964 @default.
- W2085263448 hasConceptScore W2085263448C124017977 @default.
- W2085263448 hasConceptScore W2085263448C130044071 @default.
- W2085263448 hasConceptScore W2085263448C166861157 @default.