FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2005276626> ?p ?o ?g. }

• W2005276626 endingPage "1322" @default.
• W2005276626 startingPage "1316" @default.
• W2005276626 abstract "The outstanding cosmological problems (horizon, flatness, . . .) which may be solved by the usual inflationary models may also find a solution in the frame of a ``generalized'' inflationary cosmology which is characterized by a suitable phase of accelerated expansion. The usual exponential growth of the scale factor S is just a particular case of such a general idea. Following this line of thought, we study in some detail a simple inflationary model characterized by a scale factor which grows like Sensuremath{sim}${t}^{p}$, with p a constant greater than one, which we call power-law inflation (PLI). Some properties of PLI have been analyzed, in different contexts, also by other authors. We consider the constraints on this model coming from the requirement of solving the horizon, flatness, ``good'' reheating, and ``convenient'' perturbation-spectrum problems. In order to obtain the perturbation spectrum when re-entering the horizon during the Friedmann phase, we extend to PLI the gauge-invariant approach developed by Bardeen et al. for the usual inflationary models. We find that the above constraints can be suitably satisfied. Finally, we outline possible connections between PLI and particular inflationary models which have recently been proposed." @default.
• W2005276626 created "2016-06-24" @default.
• W2005276626 creator A5016282067 @default.
• W2005276626 creator A5087020542 @default.
• W2005276626 date "1985-09-15" @default.
• W2005276626 modified "2023-10-11" @default.
• W2005276626 title "Power-law inflation" @default.
• W2005276626 cites W1963931725 @default.
• W2005276626 cites W1973861971 @default.
• W2005276626 cites W1976030533 @default.
• W2005276626 cites W1977446312 @default.
• W2005276626 cites W1987010236 @default.
• W2005276626 cites W1987984506 @default.
• W2005276626 cites W1991824329 @default.
• W2005276626 cites W1998135368 @default.
• W2005276626 cites W2000705863 @default.
• W2005276626 cites W2001109079 @default.
• W2005276626 cites W2011458123 @default.
• W2005276626 cites W2012869970 @default.
• W2005276626 cites W2021573208 @default.
• W2005276626 cites W2022680703 @default.
• W2005276626 cites W2025849140 @default.
• W2005276626 cites W2029434458 @default.
• W2005276626 cites W2029623174 @default.
• W2005276626 cites W2029886567 @default.
• W2005276626 cites W2033101727 @default.
• W2005276626 cites W2034898285 @default.
• W2005276626 cites W2035784745 @default.
• W2005276626 cites W2036281917 @default.
• W2005276626 cites W2046034046 @default.
• W2005276626 cites W2058269106 @default.
• W2005276626 cites W2061147052 @default.
• W2005276626 cites W2064980993 @default.
• W2005276626 cites W2072646999 @default.
• W2005276626 cites W2080465298 @default.
• W2005276626 cites W2084178876 @default.
• W2005276626 cites W2086432683 @default.
• W2005276626 cites W2086984930 @default.
• W2005276626 cites W2090982372 @default.
• W2005276626 cites W2095034832 @default.
• W2005276626 cites W2122083363 @default.
• W2005276626 cites W2134251287 @default.
• W2005276626 cites W2134990923 @default.
• W2005276626 cites W2136682975 @default.
• W2005276626 cites W2164459358 @default.
• W2005276626 cites W2169912865 @default.
• W2005276626 cites W2178041771 @default.
• W2005276626 cites W2232908915 @default.
• W2005276626 cites W4233829554 @default.
• W2005276626 doi "https://doi.org/10.1103/physrevd.32.1316" @default.
• W2005276626 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/9956284" @default.
• W2005276626 hasPublicationYear "1985" @default.
• W2005276626 type Work @default.
• W2005276626 sameAs 2005276626 @default.
• W2005276626 citedByCount "750" @default.
• W2005276626 countsByYear W20052766262012 @default.
• W2005276626 countsByYear W20052766262013 @default.
• W2005276626 countsByYear W20052766262014 @default.
• W2005276626 countsByYear W20052766262015 @default.
• W2005276626 countsByYear W20052766262016 @default.
• W2005276626 countsByYear W20052766262017 @default.
• W2005276626 countsByYear W20052766262018 @default.
• W2005276626 countsByYear W20052766262019 @default.
• W2005276626 countsByYear W20052766262020 @default.
• W2005276626 countsByYear W20052766262021 @default.
• W2005276626 countsByYear W20052766262022 @default.
• W2005276626 countsByYear W20052766262023 @default.
• W2005276626 crossrefType "journal-article" @default.
• W2005276626 hasAuthorship W2005276626A5016282067 @default.
• W2005276626 hasAuthorship W2005276626A5087020542 @default.
• W2005276626 hasConcept C105795698 @default.
• W2005276626 hasConcept C121332964 @default.
• W2005276626 hasConcept C121864883 @default.
• W2005276626 hasConcept C1276947 @default.
• W2005276626 hasConcept C135593079 @default.
• W2005276626 hasConcept C159176650 @default.
• W2005276626 hasConcept C168110828 @default.
• W2005276626 hasConcept C177918212 @default.
• W2005276626 hasConcept C190470478 @default.
• W2005276626 hasConcept C200941418 @default.
• W2005276626 hasConcept C26405456 @default.
• W2005276626 hasConcept C2778530986 @default.
• W2005276626 hasConcept C33332235 @default.
• W2005276626 hasConcept C33923547 @default.
• W2005276626 hasConcept C37914503 @default.
• W2005276626 hasConcept C62520636 @default.
• W2005276626 hasConcept C87040749 @default.
• W2005276626 hasConceptScore W2005276626C105795698 @default.
• W2005276626 hasConceptScore W2005276626C121332964 @default.
• W2005276626 hasConceptScore W2005276626C121864883 @default.
• W2005276626 hasConceptScore W2005276626C1276947 @default.
• W2005276626 hasConceptScore W2005276626C135593079 @default.
• W2005276626 hasConceptScore W2005276626C159176650 @default.
• W2005276626 hasConceptScore W2005276626C168110828 @default.
• W2005276626 hasConceptScore W2005276626C177918212 @default.
• W2005276626 hasConceptScore W2005276626C190470478 @default.
• W2005276626 hasConceptScore W2005276626C200941418 @default.
• W2005276626 hasConceptScore W2005276626C26405456 @default.

• next