Matches in SemOpenAlex for { <https://semopenalex.org/work/W1996044250> ?p ?o ?g. }
- W1996044250 abstract "We study cosmological perturbations around self-accelerating solutions to two extensions of nonlinear massive gravity: the quasi-dilaton theory and the mass-varying theory. We examine stability of the cosmological solutions, and the extent to which the vanishing of the kinetic terms for scalar and vector perturbations of self-accelerating solutions in massive gravity is generic when the theory is extended. We find that these kinetic terms are in general non-vanishing in both extensions, though there are constraints on the parameters and background evolution from demanding that they have the correct sign. In particular, the self-accelerating solutions of the quasi-dilaton theory are always unstable to scalar perturbations with wavelength shorter than the Hubble length." @default.
- W1996044250 created "2016-06-24" @default.
- W1996044250 creator A5015706916 @default.
- W1996044250 creator A5016245139 @default.
- W1996044250 creator A5047518661 @default.
- W1996044250 creator A5064758601 @default.
- W1996044250 creator A5088891944 @default.
- W1996044250 date "2013-07-16" @default.
- W1996044250 modified "2023-10-05" @default.
- W1996044250 title "Cosmological perturbations in extended massive gravity" @default.
- W1996044250 cites W1639730669 @default.
- W1996044250 cites W1977415523 @default.
- W1996044250 cites W1980796615 @default.
- W1996044250 cites W1988373934 @default.
- W1996044250 cites W1993657465 @default.
- W1996044250 cites W1993856682 @default.
- W1996044250 cites W2002230242 @default.
- W1996044250 cites W2016830897 @default.
- W1996044250 cites W2019269886 @default.
- W1996044250 cites W2025576938 @default.
- W1996044250 cites W2030885218 @default.
- W1996044250 cites W2044039892 @default.
- W1996044250 cites W2050191873 @default.
- W1996044250 cites W2055257339 @default.
- W1996044250 cites W2059937895 @default.
- W1996044250 cites W2062884529 @default.
- W1996044250 cites W2069536822 @default.
- W1996044250 cites W2069671340 @default.
- W1996044250 cites W2070298862 @default.
- W1996044250 cites W2073819085 @default.
- W1996044250 cites W2078259986 @default.
- W1996044250 cites W2080992744 @default.
- W1996044250 cites W2091210293 @default.
- W1996044250 cites W2092787791 @default.
- W1996044250 cites W2095011189 @default.
- W1996044250 cites W2097968935 @default.
- W1996044250 cites W2102567952 @default.
- W1996044250 cites W2114832931 @default.
- W1996044250 cites W2134082872 @default.
- W1996044250 cites W2168780325 @default.
- W1996044250 cites W2177175366 @default.
- W1996044250 cites W2207701757 @default.
- W1996044250 cites W2299104082 @default.
- W1996044250 cites W3037181838 @default.
- W1996044250 cites W3037580761 @default.
- W1996044250 cites W3099078861 @default.
- W1996044250 cites W3101011733 @default.
- W1996044250 cites W3101328926 @default.
- W1996044250 cites W3101475444 @default.
- W1996044250 cites W3101851303 @default.
- W1996044250 cites W3102713954 @default.
- W1996044250 cites W3102938524 @default.
- W1996044250 cites W3103743842 @default.
- W1996044250 cites W3104448831 @default.
- W1996044250 doi "https://doi.org/10.1103/physrevd.88.024023" @default.
- W1996044250 hasPublicationYear "2013" @default.
- W1996044250 type Work @default.
- W1996044250 sameAs 1996044250 @default.
- W1996044250 citedByCount "63" @default.
- W1996044250 countsByYear W19960442502013 @default.
- W1996044250 countsByYear W19960442502014 @default.
- W1996044250 countsByYear W19960442502015 @default.
- W1996044250 countsByYear W19960442502016 @default.
- W1996044250 countsByYear W19960442502017 @default.
- W1996044250 countsByYear W19960442502018 @default.
- W1996044250 countsByYear W19960442502019 @default.
- W1996044250 countsByYear W19960442502020 @default.
- W1996044250 countsByYear W19960442502021 @default.
- W1996044250 countsByYear W19960442502022 @default.
- W1996044250 crossrefType "journal-article" @default.
- W1996044250 hasAuthorship W1996044250A5015706916 @default.
- W1996044250 hasAuthorship W1996044250A5016245139 @default.
- W1996044250 hasAuthorship W1996044250A5047518661 @default.
- W1996044250 hasAuthorship W1996044250A5064758601 @default.
- W1996044250 hasAuthorship W1996044250A5088891944 @default.
- W1996044250 hasBestOaLocation W19960442501 @default.
- W1996044250 hasConcept C103874350 @default.
- W1996044250 hasConcept C110521144 @default.
- W1996044250 hasConcept C121332964 @default.
- W1996044250 hasConcept C124017977 @default.
- W1996044250 hasConcept C130044071 @default.
- W1996044250 hasConcept C134306372 @default.
- W1996044250 hasConcept C135889238 @default.
- W1996044250 hasConcept C139676723 @default.
- W1996044250 hasConcept C172790937 @default.
- W1996044250 hasConcept C174256460 @default.
- W1996044250 hasConcept C2524010 @default.
- W1996044250 hasConcept C26405456 @default.
- W1996044250 hasConcept C2776605907 @default.
- W1996044250 hasConcept C2779228454 @default.
- W1996044250 hasConcept C33332235 @default.
- W1996044250 hasConcept C33923547 @default.
- W1996044250 hasConcept C44870925 @default.
- W1996044250 hasConcept C57691317 @default.
- W1996044250 hasConcept C62520636 @default.
- W1996044250 hasConcept C74650414 @default.
- W1996044250 hasConcept C8369393 @default.
- W1996044250 hasConceptScore W1996044250C103874350 @default.
- W1996044250 hasConceptScore W1996044250C110521144 @default.
- W1996044250 hasConceptScore W1996044250C121332964 @default.