Matches in SemOpenAlex for { <https://semopenalex.org/work/W2962998226> ?p ?o ?g. }
- W2962998226 endingPage "1950031" @default.
- W2962998226 startingPage "1950031" @default.
- W2962998226 abstract "The currently accelerated expansion of our universe is unarguably one of the most intriguing problems in today’s physics research. Two realistic nonminimal torsion–matter coupling [Formula: see text] models have been established and studied in our previous papers [C. J. Feng, F. F. Ge, X. Z. Li, R. H. Lin and X. H. Zhai, Phys. Rev. D 92 (2015) 104038; R. H. Lin, X. H. Zhai and X. Z. Li, Eur. Phys. J. C 77 (2017) 504] aiming to explain this “dark energy” problem. In this paper, we study the generalized power-law torsion–matter coupling [Formula: see text] model. Dynamical system analysis shows that the three expansion phases of the universe, i.e. the radiation-dominated era, the matter-dominated era and the dark energy-dominated era, can all be reproduced in this generalized model. By using the statefinder and [Formula: see text] diagnostics, we find that the different cases of the model can be distinguished from each other and from other dark energy models such as the two models in our previous papers, [Formula: see text]CDM, quintessence and Chaplygin gas. Furthermore, the analyses also show that all kinds of generalized power-law torsion–matter coupling model are able to cross the [Formula: see text] divide from below to above, which is a realization of quintom scenario. The decrease of the energy density resulting from the crossing of [Formula: see text] will make the catastrophic fate of the universe avoided and a de Sitter expansion fate in the future will be approached." @default.
- W2962998226 created "2019-07-30" @default.
- W2962998226 creator A5051597478 @default.
- W2962998226 creator A5072729690 @default.
- W2962998226 creator A5080538851 @default.
- W2962998226 creator A5091383480 @default.
- W2962998226 date "2019-01-01" @default.
- W2962998226 modified "2023-10-08" @default.
- W2962998226 title "Diagnostics for generalized power-law torsion–matter coupling f(T) model" @default.
- W2962998226 cites W1541738557 @default.
- W2962998226 cites W1653780923 @default.
- W2962998226 cites W1763442943 @default.
- W2962998226 cites W1963581370 @default.
- W2962998226 cites W1968040444 @default.
- W2962998226 cites W1970210438 @default.
- W2962998226 cites W1988458471 @default.
- W2962998226 cites W1989589910 @default.
- W2962998226 cites W1992674769 @default.
- W2962998226 cites W1992720874 @default.
- W2962998226 cites W1998534512 @default.
- W2962998226 cites W1999101610 @default.
- W2962998226 cites W2003300092 @default.
- W2962998226 cites W2012122246 @default.
- W2962998226 cites W2021574561 @default.
- W2962998226 cites W2039425854 @default.
- W2962998226 cites W2046641074 @default.
- W2962998226 cites W2046681237 @default.
- W2962998226 cites W2049393017 @default.
- W2962998226 cites W2057547451 @default.
- W2962998226 cites W2073163146 @default.
- W2962998226 cites W2078466115 @default.
- W2962998226 cites W2078896402 @default.
- W2962998226 cites W2102595495 @default.
- W2962998226 cites W2118470197 @default.
- W2962998226 cites W2121951791 @default.
- W2962998226 cites W2122927372 @default.
- W2962998226 cites W2124601931 @default.
- W2962998226 cites W2131935965 @default.
- W2962998226 cites W2139937287 @default.
- W2962998226 cites W2145708901 @default.
- W2962998226 cites W2151185137 @default.
- W2962998226 cites W2156305595 @default.
- W2962998226 cites W2159874741 @default.
- W2962998226 cites W2165724764 @default.
- W2962998226 cites W2169866137 @default.
- W2962998226 cites W2177433753 @default.
- W2962998226 cites W2211043289 @default.
- W2962998226 cites W2281443567 @default.
- W2962998226 cites W2408023993 @default.
- W2962998226 cites W2478077360 @default.
- W2962998226 cites W2592749701 @default.
- W2962998226 cites W2604798180 @default.
- W2962998226 cites W2619086538 @default.
- W2962998226 cites W2622603792 @default.
- W2962998226 cites W2783381413 @default.
- W2962998226 cites W2798974155 @default.
- W2962998226 cites W3099082873 @default.
- W2962998226 cites W3099305190 @default.
- W2962998226 cites W3099718233 @default.
- W2962998226 cites W3100339959 @default.
- W2962998226 cites W3100415766 @default.
- W2962998226 cites W3103671208 @default.
- W2962998226 cites W3105647117 @default.
- W2962998226 cites W3105790464 @default.
- W2962998226 doi "https://doi.org/10.1142/s0218271819500317" @default.
- W2962998226 hasPublicationYear "2019" @default.
- W2962998226 type Work @default.
- W2962998226 sameAs 2962998226 @default.
- W2962998226 citedByCount "1" @default.
- W2962998226 countsByYear W29629982262022 @default.
- W2962998226 crossrefType "journal-article" @default.
- W2962998226 hasAuthorship W2962998226A5051597478 @default.
- W2962998226 hasAuthorship W2962998226A5072729690 @default.
- W2962998226 hasAuthorship W2962998226A5080538851 @default.
- W2962998226 hasAuthorship W2962998226A5091383480 @default.
- W2962998226 hasBestOaLocation W29629982262 @default.
- W2962998226 hasConcept C121332964 @default.
- W2962998226 hasConcept C127413603 @default.
- W2962998226 hasConcept C131584629 @default.
- W2962998226 hasConcept C141071460 @default.
- W2962998226 hasConcept C159249277 @default.
- W2962998226 hasConcept C172790937 @default.
- W2962998226 hasConcept C19262093 @default.
- W2962998226 hasConcept C20154449 @default.
- W2962998226 hasConcept C26405456 @default.
- W2962998226 hasConcept C2777515927 @default.
- W2962998226 hasConcept C2778632639 @default.
- W2962998226 hasConcept C33332235 @default.
- W2962998226 hasConcept C36429004 @default.
- W2962998226 hasConcept C37914503 @default.
- W2962998226 hasConcept C44870925 @default.
- W2962998226 hasConcept C62520636 @default.
- W2962998226 hasConcept C71924100 @default.
- W2962998226 hasConcept C74650414 @default.
- W2962998226 hasConcept C77461463 @default.
- W2962998226 hasConcept C78519656 @default.
- W2962998226 hasConcept C84999194 @default.
- W2962998226 hasConceptScore W2962998226C121332964 @default.