FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2785116680> ?p ?o ?g. }

• W2785116680 abstract "The concordance cosmological model has been successfully tested over the last decades. Despite its successes, the fundamental nature of dark matter and dark energy is still unknown. Modifications of the gravitational action have been proposed as an alternative to these dark components. The straightforward modification of gravity is to generalize the action to a function, $f(R)$, of the scalar curvature. Thus one is able to describe the emergence and the evolution of the large scale structure without any additional (unknown) dark component. In the weak field limit of the $f(R)$-gravity, a modified Newtonian gravitational potential arises. This gravitational potential accounts for an extra force, generally called fifth force, that produces a precession of the orbital motion even in the classic mechanical approach. We have shown that the orbits in the modified potential can be written as Keplerian orbits under some conditions on the strength and scale length of this extra force. Nevertheless, we have also shown that this extra term gives rise to the precession of the orbit. Thus, comparing our prediction with the measurements of the precession of some planetary motions, we have found that the strength of the fifth force must be in the range $[2.70--6.70]ifmmodetimeselsetexttimesfi{}{10}^{ensuremath{-}9}$ with the characteristic scale length to fix to the fiducial values of $ensuremath{sim}5000text{ }text{ }mathrm{AU}$." @default.
• W2785116680 created "2018-02-02" @default.
• W2785116680 creator A5017935883 @default.
• W2785116680 creator A5053635230 @default.
• W2785116680 creator A5056627165 @default.
• W2785116680 date "2018-05-31" @default.
• W2785116680 modified "2023-10-10" @default.
• W2785116680 title "Analysis of the Yukawa gravitational potential in <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>f</mml:mi><mml:mo mathvariant=bold stretchy=false>(</mml:mo><mml:mi>R</mml:mi><mml:mo mathvariant=bold stretchy=false>)</mml:mo></mml:math> gravity. I. Semiclassical periastron advance" @default.
• W2785116680 cites W1504608720 @default.
• W2785116680 cites W1597395936 @default.
• W2785116680 cites W1601915929 @default.
• W2785116680 cites W1792453959 @default.
• W2785116680 cites W1966205159 @default.
• W2785116680 cites W1969383785 @default.
• W2785116680 cites W1991677108 @default.
• W2785116680 cites W2004422294 @default.
• W2785116680 cites W2004614917 @default.
• W2785116680 cites W2009463540 @default.
• W2785116680 cites W2024192612 @default.
• W2785116680 cites W2026482585 @default.
• W2785116680 cites W2027861687 @default.
• W2785116680 cites W2032853727 @default.
• W2785116680 cites W2037208905 @default.
• W2785116680 cites W2054949929 @default.
• W2785116680 cites W2062136406 @default.
• W2785116680 cites W2081932318 @default.
• W2785116680 cites W2086100864 @default.
• W2785116680 cites W2089607103 @default.
• W2785116680 cites W2096322135 @default.
• W2785116680 cites W2096512430 @default.
• W2785116680 cites W2097299707 @default.
• W2785116680 cites W2102639000 @default.
• W2785116680 cites W2103678464 @default.
• W2785116680 cites W2105240812 @default.
• W2785116680 cites W2110352019 @default.
• W2785116680 cites W2117451719 @default.
• W2785116680 cites W2129111107 @default.
• W2785116680 cites W2136471348 @default.
• W2785116680 cites W2151494416 @default.
• W2785116680 cites W2152565162 @default.
• W2785116680 cites W2160168896 @default.
• W2785116680 cites W2166436681 @default.
• W2785116680 cites W2177433753 @default.
• W2785116680 cites W2397630455 @default.
• W2785116680 cites W2555277908 @default.
• W2785116680 cites W2603530353 @default.
• W2785116680 cites W2612259467 @default.
• W2785116680 cites W2612757325 @default.
• W2785116680 cites W2618288299 @default.
• W2785116680 cites W2621266390 @default.
• W2785116680 cites W2768515601 @default.
• W2785116680 cites W2782581647 @default.
• W2785116680 cites W2782732083 @default.
• W2785116680 cites W2783178622 @default.
• W2785116680 cites W2785055545 @default.
• W2785116680 cites W2789042424 @default.
• W2785116680 cites W3097984739 @default.
• W2785116680 cites W3098164631 @default.
• W2785116680 cites W3100339959 @default.
• W2785116680 cites W3100342810 @default.
• W2785116680 cites W3100403067 @default.
• W2785116680 cites W3102136416 @default.
• W2785116680 cites W3103409678 @default.
• W2785116680 cites W3103675194 @default.
• W2785116680 cites W3104349364 @default.
• W2785116680 cites W3104614728 @default.
• W2785116680 cites W3104710637 @default.
• W2785116680 cites W3105647117 @default.
• W2785116680 cites W3105840626 @default.
• W2785116680 cites W3106084670 @default.
• W2785116680 cites W4250515138 @default.
• W2785116680 cites W4292875581 @default.
• W2785116680 doi "https://doi.org/10.1103/physrevd.97.104067" @default.
• W2785116680 hasPublicationYear "2018" @default.
• W2785116680 type Work @default.
• W2785116680 sameAs 2785116680 @default.
• W2785116680 citedByCount "41" @default.
• W2785116680 countsByYear W27851166802018 @default.
• W2785116680 countsByYear W27851166802019 @default.
• W2785116680 countsByYear W27851166802020 @default.
• W2785116680 countsByYear W27851166802021 @default.
• W2785116680 countsByYear W27851166802022 @default.
• W2785116680 countsByYear W27851166802023 @default.
• W2785116680 crossrefType "journal-article" @default.
• W2785116680 hasAuthorship W2785116680A5017935883 @default.
• W2785116680 hasAuthorship W2785116680A5053635230 @default.
• W2785116680 hasAuthorship W2785116680A5056627165 @default.
• W2785116680 hasBestOaLocation W27851166802 @default.
• W2785116680 hasConcept C121332964 @default.
• W2785116680 hasConcept C124017977 @default.
• W2785116680 hasConcept C127090403 @default.
• W2785116680 hasConcept C14257148 @default.
• W2785116680 hasConcept C151195881 @default.
• W2785116680 hasConcept C159249277 @default.
• W2785116680 hasConcept C172790937 @default.
• W2785116680 hasConcept C26405456 @default.
• W2785116680 hasConcept C37914503 @default.
• W2785116680 hasConcept C44870925 @default.
• W2785116680 hasConcept C62520636 @default.
• W2785116680 hasConcept C74650414 @default.

• next