FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3021037190> ?p ?o ?g. }

• W3021037190 abstract "In this work, we obtain measurements of the Hubble constant in the context of modified gravity theories. We set up our theoretical framework by considering viable cosmological $f(R)$ and $f(T)$ models, and we analyzed them through the use of geometrical datasets obtained in a model-independent way, namely, gravitationally lensed quasars with measured time delays, standard clocks from cosmic chronometers, and standard candles from the Pantheon Supernovae Ia sample. We find ${H}_{0}=(72.4ifmmodepmelsetextpmfi{}1.4)text{ }text{ }mathrm{km}text{ }{mathrm{s}}^{ensuremath{-}1}text{ }{mathrm{Mpc}}^{ensuremath{-}1}$ and ${H}_{0}=(71.5ifmmodepmelsetextpmfi{}1.3)text{ }text{ }mathrm{km}text{ }{mathrm{s}}^{ensuremath{-}1}text{ }{mathrm{Mpc}}^{ensuremath{-}1}$ for the $f(R)$ and $f(T)$ models, respectively. Our results represent 1.9% and 1.8% measurements of the Hubble constant, which are fully consistent with the local estimate of ${H}_{0}$ by the Hubble Space Telescope. We do not find significant departures from general relativity, as our study shows that the characteristic parameters of the extensions of gravity beyond general relativity are compatible with the $mathrm{ensuremath{Lambda}}mathrm{CDM}$ cosmology. Moreover, within the standard cosmological framework, our full joint analysis suggests that it is possible to measure the dark energy equation of state parameter at 1.2% accuracy, although we find no statistical evidence for deviations from the cosmological constant case." @default.
• W3021037190 created "2020-05-13" @default.
• W3021037190 creator A5074224919 @default.
• W3021037190 creator A5086929880 @default.
• W3021037190 date "2020-05-06" @default.
• W3021037190 modified "2023-10-16" @default.
• W3021037190 title "Measurements of <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:msub><mml:mi>H</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math> in modified gravity theories: The role of lensed quasars in the late-time Universe" @default.
• W3021037190 cites W1507717731 @default.
• W3021037190 cites W1853767801 @default.
• W3021037190 cites W1980534545 @default.
• W3021037190 cites W1989263666 @default.
• W3021037190 cites W1996008893 @default.
• W3021037190 cites W1996098097 @default.
• W3021037190 cites W2004188331 @default.
• W3021037190 cites W2005098187 @default.
• W3021037190 cites W2056760934 @default.
• W3021037190 cites W2058734209 @default.
• W3021037190 cites W2073163146 @default.
• W3021037190 cites W2076533122 @default.
• W3021037190 cites W2096699295 @default.
• W3021037190 cites W2111044754 @default.
• W3021037190 cites W2113396177 @default.
• W3021037190 cites W2138309709 @default.
• W3021037190 cites W2141936689 @default.
• W3021037190 cites W2142635246 @default.
• W3021037190 cites W2168175751 @default.
• W3021037190 cites W2171317216 @default.
• W3021037190 cites W2177433753 @default.
• W3021037190 cites W2396756616 @default.
• W3021037190 cites W2480130372 @default.
• W3021037190 cites W2497600269 @default.
• W3021037190 cites W2498300276 @default.
• W3021037190 cites W2624157171 @default.
• W3021037190 cites W2706506745 @default.
• W3021037190 cites W2758860028 @default.
• W3021037190 cites W2763117186 @default.
• W3021037190 cites W2763732082 @default.
• W3021037190 cites W2765934061 @default.
• W3021037190 cites W2768510880 @default.
• W3021037190 cites W2772507432 @default.
• W3021037190 cites W2777913141 @default.
• W3021037190 cites W2782368737 @default.
• W3021037190 cites W2785172315 @default.
• W3021037190 cites W2790190762 @default.
• W3021037190 cites W2808677542 @default.
• W3021037190 cites W2883986208 @default.
• W3021037190 cites W2887785509 @default.
• W3021037190 cites W2897416025 @default.
• W3021037190 cites W2942115646 @default.
• W3021037190 cites W2944059344 @default.
• W3021037190 cites W2944575491 @default.
• W3021037190 cites W2947484566 @default.
• W3021037190 cites W2951575264 @default.
• W3021037190 cites W2952549172 @default.
• W3021037190 cites W2958585481 @default.
• W3021037190 cites W2961599138 @default.
• W3021037190 cites W2961978464 @default.
• W3021037190 cites W2978719535 @default.
• W3021037190 cites W2981720551 @default.
• W3021037190 cites W2990178751 @default.
• W3021037190 cites W3009418247 @default.
• W3021037190 cites W3098023360 @default.
• W3021037190 cites W3098728794 @default.
• W3021037190 cites W3099395704 @default.
• W3021037190 cites W3100221074 @default.
• W3021037190 cites W3100339959 @default.
• W3021037190 cites W3102136416 @default.
• W3021037190 cites W3102523060 @default.
• W3021037190 cites W3102609182 @default.
• W3021037190 cites W3102687315 @default.
• W3021037190 cites W3103428786 @default.
• W3021037190 cites W3103448631 @default.
• W3021037190 cites W3103476562 @default.
• W3021037190 cites W3104043306 @default.
• W3021037190 cites W3104405069 @default.
• W3021037190 cites W3104431204 @default.
• W3021037190 cites W3105931013 @default.
• W3021037190 cites W3106076604 @default.
• W3021037190 cites W3106235984 @default.
• W3021037190 cites W3107403142 @default.
• W3021037190 cites W3124234627 @default.
• W3021037190 cites W4235359194 @default.
• W3021037190 cites W4292230281 @default.
• W3021037190 cites W4292875581 @default.
• W3021037190 doi "https://doi.org/10.1103/physrevd.101.103505" @default.
• W3021037190 hasPublicationYear "2020" @default.
• W3021037190 type Work @default.
• W3021037190 sameAs 3021037190 @default.
• W3021037190 citedByCount "42" @default.
• W3021037190 countsByYear W30210371902020 @default.
• W3021037190 countsByYear W30210371902021 @default.
• W3021037190 countsByYear W30210371902022 @default.
• W3021037190 countsByYear W30210371902023 @default.
• W3021037190 crossrefType "journal-article" @default.
• W3021037190 hasAuthorship W3021037190A5074224919 @default.
• W3021037190 hasAuthorship W3021037190A5086929880 @default.
• W3021037190 hasBestOaLocation W30210371902 @default.
• W3021037190 hasConcept C103874350 @default.
• W3021037190 hasConcept C109214941 @default.
• W3021037190 hasConcept C121332964 @default.

• next