Matches in SemOpenAlex for { <https://semopenalex.org/work/W3195377489> ?p ?o ?g. }
- W3195377489 endingPage "100950" @default.
- W3195377489 startingPage "100950" @default.
- W3195377489 abstract "In this work we shall develop a quantitative approach for extracting predictions on the primordial gravitational waves energy spectrum for f(R) gravity. We shall consider two distinct models which yield different phenomenology, one pure f(R) gravity model and one Chern–Simons corrected potential-less k-essence f(R) gravity model in the presence of radiation and non-relativistic perfect matter fluids. The two f(R) gravity models were carefully chosen in order for them to describe in a unified way inflation and the dark energy era, in both cases viable and compatible with the latest Planck data. Also both models mimic the Λ-Cold-Dark-Matter model and specifically the pure f(R) model only at late times, but the Chern–Simons k-essence model during the whole evolution of the model up to the radiation domination era. In addition they guarantee a smooth transition from the inflationary era to the radiation, matter domination and subsequently to the dark energy era. Using a WKB approach introduced in the relevant literature by Nishizawa, we derive formulas depending on the redshift that yield the modified gravity effect, quantified by a multiplicative factor, a “damping” in front of the General Relativistic waveform. In order to calculate the effect of the modified gravity, which is the “damping” factor, we solve numerically the Friedmann equations using appropriate initial conditions and by introducing specific statefinder quantities. As we show, the pure f(R) gravity gravitational wave energy spectrum is slightly enhanced, but it remains well below the sensitivity curves of future gravitational waves experiments. In contrast, the Chern–Simons k-essence f(R) gravity model gravitational wave energy spectrum is significantly enhanced and two signals are predicted which can be verified by future gravitational wave experiments. We discuss in detail our findings and the future perspective of modified gravity theories in view of the upcoming second and third generation experiments on primordial gravitational waves." @default.
- W3195377489 created "2021-08-30" @default.
- W3195377489 creator A5049345198 @default.
- W3195377489 creator A5053560263 @default.
- W3195377489 creator A5070134354 @default.
- W3195377489 date "2022-03-01" @default.
- W3195377489 modified "2023-09-27" @default.
- W3195377489 title "Quantitative predictions for <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline id=d1e1172 altimg=si543.svg><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity primordial gravitational waves" @default.
- W3195377489 cites W1934775445 @default.
- W3195377489 cites W1958232190 @default.
- W3195377489 cites W1985121837 @default.
- W3195377489 cites W1987300459 @default.
- W3195377489 cites W1992950749 @default.
- W3195377489 cites W1993929115 @default.
- W3195377489 cites W1997153378 @default.
- W3195377489 cites W1998067752 @default.
- W3195377489 cites W2005917645 @default.
- W3195377489 cites W2006951416 @default.
- W3195377489 cites W2014571316 @default.
- W3195377489 cites W2019326730 @default.
- W3195377489 cites W2023818049 @default.
- W3195377489 cites W2028395442 @default.
- W3195377489 cites W2038397069 @default.
- W3195377489 cites W2058307417 @default.
- W3195377489 cites W2059177657 @default.
- W3195377489 cites W2065626203 @default.
- W3195377489 cites W2077073823 @default.
- W3195377489 cites W2094471106 @default.
- W3195377489 cites W2097544083 @default.
- W3195377489 cites W2103857591 @default.
- W3195377489 cites W2125817250 @default.
- W3195377489 cites W2132911946 @default.
- W3195377489 cites W2136954147 @default.
- W3195377489 cites W2149201030 @default.
- W3195377489 cites W2150050997 @default.
- W3195377489 cites W2155095321 @default.
- W3195377489 cites W2164721450 @default.
- W3195377489 cites W2515217099 @default.
- W3195377489 cites W2522653346 @default.
- W3195377489 cites W2603530353 @default.
- W3195377489 cites W2770133691 @default.
- W3195377489 cites W2898458607 @default.
- W3195377489 cites W2902964614 @default.
- W3195377489 cites W2914179981 @default.
- W3195377489 cites W2923252909 @default.
- W3195377489 cites W2961978464 @default.
- W3195377489 cites W2965245827 @default.
- W3195377489 cites W3004014367 @default.
- W3195377489 cites W3020506053 @default.
- W3195377489 cites W3031553230 @default.
- W3195377489 cites W3038026342 @default.
- W3195377489 cites W3041404127 @default.
- W3195377489 cites W3090384628 @default.
- W3195377489 cites W3098429340 @default.
- W3195377489 cites W3098940597 @default.
- W3195377489 cites W3099492940 @default.
- W3195377489 cites W3100762001 @default.
- W3195377489 cites W3102136416 @default.
- W3195377489 cites W3102303941 @default.
- W3195377489 cites W3102687315 @default.
- W3195377489 cites W3102947544 @default.
- W3195377489 cites W3103543020 @default.
- W3195377489 cites W3103583541 @default.
- W3195377489 cites W3104434317 @default.
- W3195377489 cites W3105647117 @default.
- W3195377489 cites W3107657953 @default.
- W3195377489 cites W3116069061 @default.
- W3195377489 cites W3118596204 @default.
- W3195377489 cites W3120540649 @default.
- W3195377489 cites W3187649365 @default.
- W3195377489 cites W67474965 @default.
- W3195377489 doi "https://doi.org/10.1016/j.dark.2022.100950" @default.
- W3195377489 hasPublicationYear "2022" @default.
- W3195377489 type Work @default.
- W3195377489 sameAs 3195377489 @default.
- W3195377489 citedByCount "37" @default.
- W3195377489 countsByYear W31953774892021 @default.
- W3195377489 countsByYear W31953774892022 @default.
- W3195377489 countsByYear W31953774892023 @default.
- W3195377489 crossrefType "journal-article" @default.
- W3195377489 hasAuthorship W3195377489A5049345198 @default.
- W3195377489 hasAuthorship W3195377489A5053560263 @default.
- W3195377489 hasAuthorship W3195377489A5070134354 @default.
- W3195377489 hasBestOaLocation W31953774892 @default.
- W3195377489 hasConcept C121332964 @default.
- W3195377489 hasConcept C124017977 @default.
- W3195377489 hasConcept C166126730 @default.
- W3195377489 hasConcept C172790937 @default.
- W3195377489 hasConcept C26405456 @default.
- W3195377489 hasConcept C33332235 @default.
- W3195377489 hasConcept C37914503 @default.
- W3195377489 hasConcept C44870925 @default.
- W3195377489 hasConcept C62520636 @default.
- W3195377489 hasConceptScore W3195377489C121332964 @default.
- W3195377489 hasConceptScore W3195377489C124017977 @default.
- W3195377489 hasConceptScore W3195377489C166126730 @default.
- W3195377489 hasConceptScore W3195377489C172790937 @default.
- W3195377489 hasConceptScore W3195377489C26405456 @default.