FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3104130162> ?p ?o ?g. }

• W3104130162 endingPage "016" @default.
• W3104130162 startingPage "016" @default.
• W3104130162 abstract "We investigate whether the current Hubble parameter $H(z)$ measurements could help improve the constraints on dark energy on the basis of the mainstream cosmological probes including the type Ia supernovae (SN) observation, the cosmic microwave background anisotropies (CMB) observation, and the baryon acoustic oscillations (BAO) observation. For the current $H(z)$ data, we use 30 data points measured by using a differential age method. Furthermore, we also consider the future $H(z)$ measurements based on the Sandage-Loeb (SL) test by means of the E-ELT in construction, and thus we also use 30 simulated $H(z)$ data according to a 10-year SL test observation. In this work, we choose four typical dark energy models as examples, i.e., the $Lambda$CDM model, the $w$CDM model, the $alpha$DE model, and the GCG model, to complete the analysis. We find that, when only the current $H(z)$ data are added, the constraints on these models are not improved compared to the cases using the SN+CMB+BAO data; but when further adding the 10-year SL test data, the constraint results are tremendously improved for all the four models. Therefore, we conclude that, although the current $H(z)$ measurements could not provide an evident improvement on the basis of the current mainstream cosmological probes, the future $H(z)$ measurements from the SL test would have enormous potential to change the status of the Hubble parameter measurements in constraining dark energy." @default.
• W3104130162 created "2020-11-23" @default.
• W3104130162 creator A5006651636 @default.
• W3104130162 creator A5020810072 @default.
• W3104130162 creator A5021293751 @default.
• W3104130162 creator A5042572715 @default.
• W3104130162 date "2019-05-13" @default.
• W3104130162 modified "2023-09-27" @default.
• W3104130162 title "Revisit of constraints on dark energy with Hubble parameter measurements including future redshift drift observations" @default.
• W3104130162 cites W1636808257 @default.
• W3104130162 cites W1853767801 @default.
• W3104130162 cites W1949590851 @default.
• W3104130162 cites W1970799623 @default.
• W3104130162 cites W1973047332 @default.
• W3104130162 cites W1974007811 @default.
• W3104130162 cites W1975825273 @default.
• W3104130162 cites W1998539951 @default.
• W3104130162 cites W2004975276 @default.
• W3104130162 cites W2011267614 @default.
• W3104130162 cites W2011426435 @default.
• W3104130162 cites W2014145707 @default.
• W3104130162 cites W2015155466 @default.
• W3104130162 cites W2017283350 @default.
• W3104130162 cites W2023587319 @default.
• W3104130162 cites W2030882691 @default.
• W3104130162 cites W2031579307 @default.
• W3104130162 cites W2036439761 @default.
• W3104130162 cites W2042486679 @default.
• W3104130162 cites W2045719640 @default.
• W3104130162 cites W2048178787 @default.
• W3104130162 cites W2048446165 @default.
• W3104130162 cites W2056173066 @default.
• W3104130162 cites W2056583201 @default.
• W3104130162 cites W2065743072 @default.
• W3104130162 cites W2073163146 @default.
• W3104130162 cites W2073603601 @default.
• W3104130162 cites W2073832139 @default.
• W3104130162 cites W2075884494 @default.
• W3104130162 cites W2076533122 @default.
• W3104130162 cites W2077038906 @default.
• W3104130162 cites W2088035220 @default.
• W3104130162 cites W2094133219 @default.
• W3104130162 cites W2102197207 @default.
• W3104130162 cites W2106814493 @default.
• W3104130162 cites W2110233115 @default.
• W3104130162 cites W2118265220 @default.
• W3104130162 cites W2121951791 @default.
• W3104130162 cites W2125773180 @default.
• W3104130162 cites W2130908251 @default.
• W3104130162 cites W2131279590 @default.
• W3104130162 cites W2131348239 @default.
• W3104130162 cites W2131935965 @default.
• W3104130162 cites W2135920379 @default.
• W3104130162 cites W2136725165 @default.
• W3104130162 cites W2143062629 @default.
• W3104130162 cites W2153811626 @default.
• W3104130162 cites W2156305595 @default.
• W3104130162 cites W2169866137 @default.
• W3104130162 cites W2170967203 @default.
• W3104130162 cites W2172471412 @default.
• W3104130162 cites W2199601775 @default.
• W3104130162 cites W2200531191 @default.
• W3104130162 cites W2469037972 @default.
• W3104130162 cites W2475718109 @default.
• W3104130162 cites W2479248098 @default.
• W3104130162 cites W2587754488 @default.
• W3104130162 cites W2591817099 @default.
• W3104130162 cites W2727047013 @default.
• W3104130162 cites W2751322054 @default.
• W3104130162 cites W2884850250 @default.
• W3104130162 cites W3037504478 @default.
• W3104130162 cites W3097984739 @default.
• W3104130162 cites W3098371892 @default.
• W3104130162 cites W3098728794 @default.
• W3104130162 cites W3098957675 @default.
• W3104130162 cites W3098962334 @default.
• W3104130162 cites W3099029965 @default.
• W3104130162 cites W3099263247 @default.
• W3104130162 cites W3099549144 @default.
• W3104130162 cites W3100329962 @default.
• W3104130162 cites W3100900495 @default.
• W3104130162 cites W3102228028 @default.
• W3104130162 cites W3102522994 @default.
• W3104130162 cites W3102539771 @default.
• W3104130162 cites W3103908670 @default.
• W3104130162 cites W3104123704 @default.
• W3104130162 cites W3104817562 @default.
• W3104130162 cites W3106463060 @default.
• W3104130162 cites W3122018035 @default.
• W3104130162 cites W3123803498 @default.
• W3104130162 cites W3123971863 @default.
• W3104130162 cites W4233304942 @default.
• W3104130162 cites W4292230281 @default.
• W3104130162 cites W4292875581 @default.
• W3104130162 doi "https://doi.org/10.1088/1475-7516/2019/05/016" @default.
• W3104130162 hasPublicationYear "2019" @default.
• W3104130162 type Work @default.
• W3104130162 sameAs 3104130162 @default.

• next