Matches in SemOpenAlex for { <https://semopenalex.org/work/W1880222605> ?p ?o ?g. }
- W1880222605 abstract "We present a new approach to build models of quintessence interacting with dark or baryonic matter. We use a variational approach for relativistic fluids to realize an effective description of matter fields at the Lagrangian level. The coupling is introduced directly in the action by considering a single function mixing the dynamical degrees of freedom of the theory. The resulting gravitational field equations are derived by variations with respect to the independent variables. New interesting phenomenology can be obtained at both small scales, where new screening mechanisms for scalar fields can be realized, and large scales, where one finds an original and rich class of interacting quintessence models. The background cosmology of two of these models is studied in detail using dynamical system techniques. We find a variety of interesting results: for instance, these models contain dark energy dominated late time attractors and scaling solutions, both with early time matter dominated epochs and a possible inflationary origin. In general this new approach provides the starting point for future in depth studies on new interacting quintessence models." @default.
- W1880222605 created "2016-06-24" @default.
- W1880222605 creator A5014447628 @default.
- W1880222605 creator A5025390764 @default.
- W1880222605 creator A5037833819 @default.
- W1880222605 date "2015-06-02" @default.
- W1880222605 modified "2023-09-25" @default.
- W1880222605 title "Interacting quintessence from a variational approach. I. Algebraic couplings" @default.
- W1880222605 cites W1565367151 @default.
- W1880222605 cites W1646336067 @default.
- W1880222605 cites W1804556316 @default.
- W1880222605 cites W1853767801 @default.
- W1880222605 cites W1964180654 @default.
- W1880222605 cites W1964261121 @default.
- W1880222605 cites W1966415406 @default.
- W1880222605 cites W1966588923 @default.
- W1880222605 cites W1970306483 @default.
- W1880222605 cites W1978273401 @default.
- W1880222605 cites W1982583605 @default.
- W1880222605 cites W1983072385 @default.
- W1880222605 cites W1983233159 @default.
- W1880222605 cites W1989161976 @default.
- W1880222605 cites W1990148897 @default.
- W1880222605 cites W1994846719 @default.
- W1880222605 cites W2000675576 @default.
- W1880222605 cites W2013736238 @default.
- W1880222605 cites W2023875957 @default.
- W1880222605 cites W2032901690 @default.
- W1880222605 cites W2042210831 @default.
- W1880222605 cites W2044228803 @default.
- W1880222605 cites W2048129536 @default.
- W1880222605 cites W2056180749 @default.
- W1880222605 cites W2057627651 @default.
- W1880222605 cites W2061478818 @default.
- W1880222605 cites W2073832139 @default.
- W1880222605 cites W2078353411 @default.
- W1880222605 cites W2082050761 @default.
- W1880222605 cites W2092080603 @default.
- W1880222605 cites W2092301086 @default.
- W1880222605 cites W2095195342 @default.
- W1880222605 cites W2106766431 @default.
- W1880222605 cites W2110583611 @default.
- W1880222605 cites W2114934226 @default.
- W1880222605 cites W2129729174 @default.
- W1880222605 cites W2131279590 @default.
- W1880222605 cites W2135497511 @default.
- W1880222605 cites W2139937287 @default.
- W1880222605 cites W2140950522 @default.
- W1880222605 cites W2141978587 @default.
- W1880222605 cites W2147875900 @default.
- W1880222605 cites W2152565162 @default.
- W1880222605 cites W2154422137 @default.
- W1880222605 cites W2157044609 @default.
- W1880222605 cites W2161288989 @default.
- W1880222605 cites W2161609168 @default.
- W1880222605 cites W2162982196 @default.
- W1880222605 cites W2166436681 @default.
- W1880222605 cites W3037060671 @default.
- W1880222605 cites W3037508136 @default.
- W1880222605 cites W3100190638 @default.
- W1880222605 cites W3102333229 @default.
- W1880222605 cites W3103278519 @default.
- W1880222605 cites W3105636867 @default.
- W1880222605 cites W4234933822 @default.
- W1880222605 doi "https://doi.org/10.1103/physrevd.91.123002" @default.
- W1880222605 hasPublicationYear "2015" @default.
- W1880222605 type Work @default.
- W1880222605 sameAs 1880222605 @default.
- W1880222605 citedByCount "54" @default.
- W1880222605 countsByYear W18802226052015 @default.
- W1880222605 countsByYear W18802226052016 @default.
- W1880222605 countsByYear W18802226052017 @default.
- W1880222605 countsByYear W18802226052018 @default.
- W1880222605 countsByYear W18802226052019 @default.
- W1880222605 countsByYear W18802226052020 @default.
- W1880222605 countsByYear W18802226052021 @default.
- W1880222605 countsByYear W18802226052022 @default.
- W1880222605 countsByYear W18802226052023 @default.
- W1880222605 crossrefType "journal-article" @default.
- W1880222605 hasAuthorship W1880222605A5014447628 @default.
- W1880222605 hasAuthorship W1880222605A5025390764 @default.
- W1880222605 hasAuthorship W1880222605A5037833819 @default.
- W1880222605 hasBestOaLocation W18802226052 @default.
- W1880222605 hasConcept C109214941 @default.
- W1880222605 hasConcept C110521144 @default.
- W1880222605 hasConcept C111472728 @default.
- W1880222605 hasConcept C121332964 @default.
- W1880222605 hasConcept C121864883 @default.
- W1880222605 hasConcept C124017977 @default.
- W1880222605 hasConcept C134306372 @default.
- W1880222605 hasConcept C138885662 @default.
- W1880222605 hasConcept C159249277 @default.
- W1880222605 hasConcept C164380108 @default.
- W1880222605 hasConcept C172790937 @default.
- W1880222605 hasConcept C2524010 @default.
- W1880222605 hasConcept C26405456 @default.
- W1880222605 hasConcept C33332235 @default.
- W1880222605 hasConcept C33923547 @default.
- W1880222605 hasConcept C36429004 @default.
- W1880222605 hasConcept C57691317 @default.