Matches in SemOpenAlex for { <https://semopenalex.org/work/W4385298910> ?p ?o ?g. }
- W4385298910 endingPage "101297" @default.
- W4385298910 startingPage "101297" @default.
- W4385298910 abstract "We study cosmological perturbations in a universe with only one matter component described by a triplet of fields. Configuration of these fields is the same as for body coordinates of a solid, and they enter the matter Lagrangian only through the kinetic term. We restrict ourselves only to cases with constant pressure to energy density ratio w. Superhorizon perturbations have no constant modes with scalar vector and tensor perturbations decaying or growing at different rates, and in cases with pressure to energy density ratio w>(19−87)/3=̇−0.722 perturbations propagate with superluminal sound speed. Regarding our universe, these results illustrate possible challenges with comparing the observational data to models similar to solid inflation, if the inflation is followed by a period during which the studied model is a sufficiently good approximation." @default.
- W4385298910 created "2023-07-28" @default.
- W4385298910 creator A5031654024 @default.
- W4385298910 date "2023-12-01" @default.
- W4385298910 modified "2023-10-15" @default.
- W4385298910 title "Evolution of perturbations in a universe with exotic solid-like matter" @default.
- W4385298910 cites W1863133017 @default.
- W4385298910 cites W1973861971 @default.
- W4385298910 cites W1978108060 @default.
- W4385298910 cites W1996501054 @default.
- W4385298910 cites W2027311184 @default.
- W4385298910 cites W2027907977 @default.
- W4385298910 cites W2032901690 @default.
- W4385298910 cites W2035433892 @default.
- W4385298910 cites W2036482104 @default.
- W4385298910 cites W2037539358 @default.
- W4385298910 cites W2039108312 @default.
- W4385298910 cites W2041876997 @default.
- W4385298910 cites W2050573442 @default.
- W4385298910 cites W2056173066 @default.
- W4385298910 cites W2067579792 @default.
- W4385298910 cites W2086249589 @default.
- W4385298910 cites W2090982346 @default.
- W4385298910 cites W2096255088 @default.
- W4385298910 cites W2108313227 @default.
- W4385298910 cites W2124601931 @default.
- W4385298910 cites W2137919480 @default.
- W4385298910 cites W2147453274 @default.
- W4385298910 cites W2149441316 @default.
- W4385298910 cites W2169912865 @default.
- W4385298910 cites W2173390048 @default.
- W4385298910 cites W2512171569 @default.
- W4385298910 cites W2773086791 @default.
- W4385298910 cites W2922355218 @default.
- W4385298910 cites W2936936436 @default.
- W4385298910 cites W2944651831 @default.
- W4385298910 cites W2964283458 @default.
- W4385298910 cites W2994984874 @default.
- W4385298910 cites W3037205021 @default.
- W4385298910 cites W3037311074 @default.
- W4385298910 cites W3037396947 @default.
- W4385298910 cites W3090120384 @default.
- W4385298910 cites W3098714636 @default.
- W4385298910 cites W3099347536 @default.
- W4385298910 cites W3099499560 @default.
- W4385298910 cites W3100587783 @default.
- W4385298910 cites W3102124281 @default.
- W4385298910 cites W3103018286 @default.
- W4385298910 cites W3103494697 @default.
- W4385298910 cites W3104378108 @default.
- W4385298910 cites W3127197122 @default.
- W4385298910 cites W3169092501 @default.
- W4385298910 cites W3174624691 @default.
- W4385298910 cites W3201365274 @default.
- W4385298910 cites W3217610788 @default.
- W4385298910 cites W4224039080 @default.
- W4385298910 cites W4225895875 @default.
- W4385298910 cites W4226242991 @default.
- W4385298910 cites W4308887399 @default.
- W4385298910 doi "https://doi.org/10.1016/j.dark.2023.101297" @default.
- W4385298910 hasPublicationYear "2023" @default.
- W4385298910 type Work @default.
- W4385298910 citedByCount "0" @default.
- W4385298910 crossrefType "journal-article" @default.
- W4385298910 hasAuthorship W4385298910A5031654024 @default.
- W4385298910 hasBestOaLocation W43852989102 @default.
- W4385298910 hasConcept C110521144 @default.
- W4385298910 hasConcept C121332964 @default.
- W4385298910 hasConcept C135889238 @default.
- W4385298910 hasConcept C166861157 @default.
- W4385298910 hasConcept C172790937 @default.
- W4385298910 hasConcept C177918212 @default.
- W4385298910 hasConcept C200941418 @default.
- W4385298910 hasConcept C20154449 @default.
- W4385298910 hasConcept C2524010 @default.
- W4385298910 hasConcept C26405456 @default.
- W4385298910 hasConcept C2779228454 @default.
- W4385298910 hasConcept C2780100471 @default.
- W4385298910 hasConcept C33332235 @default.
- W4385298910 hasConcept C33923547 @default.
- W4385298910 hasConcept C44870925 @default.
- W4385298910 hasConcept C57691317 @default.
- W4385298910 hasConcept C62520636 @default.
- W4385298910 hasConcept C74650414 @default.
- W4385298910 hasConcept C84999194 @default.
- W4385298910 hasConceptScore W4385298910C110521144 @default.
- W4385298910 hasConceptScore W4385298910C121332964 @default.
- W4385298910 hasConceptScore W4385298910C135889238 @default.
- W4385298910 hasConceptScore W4385298910C166861157 @default.
- W4385298910 hasConceptScore W4385298910C172790937 @default.
- W4385298910 hasConceptScore W4385298910C177918212 @default.
- W4385298910 hasConceptScore W4385298910C200941418 @default.
- W4385298910 hasConceptScore W4385298910C20154449 @default.
- W4385298910 hasConceptScore W4385298910C2524010 @default.
- W4385298910 hasConceptScore W4385298910C26405456 @default.
- W4385298910 hasConceptScore W4385298910C2779228454 @default.
- W4385298910 hasConceptScore W4385298910C2780100471 @default.
- W4385298910 hasConceptScore W4385298910C33332235 @default.