記事
Ghost-free <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"><mml:mi>F</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="script">G</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravity
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CiNii Research
Ghost-free <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg"><mml:mi>F</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="script">G</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravity
資料詳細
要約等：
- In this work we shall address the ghost issue of F(R,G) gravity, which is known to be plagued with ghost degrees of freedom. These ghosts occur due to...
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デジタル
- 資料種別
- 記事
- 著者標目
- 出版年月日等
- 2021-12
- 出版年（W3CDTF）
- 2021-12
- 寄与者
- Ministerio de Economía y Competitividad (España)Japan Society for the Promotion of ScienceRussian Foundation for Basic ResearchConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
- タイトル（掲載誌）
- Nuclear Physics B
- 巻号年月日等（掲載誌）
- 973
- 掲載巻
- 973
- 掲載ページ
- 115617-
- 掲載年月日（W3CDTF）
- 2021-12
- ISSN（掲載誌）
- 05503213
- 出版事項（掲載誌）
- Elsevier BV
- 対象利用者
- 一般
- DOI
- 10.1016/j.nuclphysb.2021.115617
- 作成日（W3CDTF）
- 2021-11-18
- オンライン閲覧公開範囲
- インターネット公開
- 著作権情報
- https://www.elsevier.com/tdm/userlicense/1.0/http://creativecommons.org/licenses/by/4.0/
- 関連情報（URI）
- 参照
- Traversable wormholes with static spherical symmetry and their stability in higher-curvature gravity
- 参照
- Ghost-free Gauss-Bonnet theories of gravityModified gravity theories on a nutshell: Inflation, bounce and late-time evolutionUnifying inflation with early and late-time dark energy in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1046" altimg="si303.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> gravityAn alternative to quintessencePhase structure of the massive chiral Gross-Neveu model from the Hartree-Fock approachTracing the cosmic history by Gauss-Bonnet gravityBouncing cosmology in modified Gauss–Bonnet gravityUnified cosmic history in modified gravity: From <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si10.gif" display="inline" overflow="scroll"><mml:mi>F</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math> theory to Lorentz non-invariant modelsCosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with ΛCDMFinite-time future singularities in modified Gauss–Bonnet and ℱ(R,G) gravity and singularity avoidanceTowards the Einstein-Hilbert action via conformal transformationCosmological inflation in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>F</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="script">G</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravityGeneralized holographic dark energy and bouncing cosmology in Gauss–Bonnet gravityGeneralized Galileon model: Cosmological reconstruction and the Vainshtein mechanism<i>Planck</i>2018 resultsGalileon as a local modification of gravityModified Gauss–Bonnet theory as gravitational alternative for dark energyThe role of Lagrange multiplier in Gauss–Bonnet dark energyHybrid inflationGauss–Bonnet modified gravity models with bouncing behaviorThe asymptotic behavior of bouncing cosmological models in F(𝒢) gravity theoryDark energy cosmology: the equivalent description via different theoretical models and cosmography testsGeneralized Galileons: All scalar models whose curved background extensions maintain second-order field equations and stress tensorsDark energy in modified Gauss-Bonnet gravity: Late-time acceleration and the hierarchy problemCURVATURE QUINTESSENCE MATCHED WITH OBSERVATIONAL DATAMassive, massless and ghost modes of gravitational waves from higher-order gravityUnifying inflation with early and late dark energy epochs in axion <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>F</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravityInflationary universe: A possible solution to the horizon and flatness problemsSingular bouncing cosmology from Gauss-Bonnet modified gravityChaotic inflationCan higher order curvature theories explain rotation curves of galaxies?PALATINI APPROACH TO MODIFIED GRAVITY: f(R) THEORIES AND BEYONDBlack Holes, Cosmological Solutions, Future Singularities, and Their Thermodynamical Properties in Modified Gravity TheoriesDark energy exponential potential models as curvature quintessenceDark energy problem: from phantom theory to modified Gauss–Bonnet gravityInflation and the conformal structure of higher-order gravity theoriesGauss-Bonnet cosmology unifying late and early-time acceleration eras with intermediate eras<i>Planck</i>2018 resultsThe cosmological constant and dark energyDark EnergyRECONSTRUCTING DARK ENERGYLISA for cosmologists: Calculating the signal-to-noise ratio for stochastic and deterministic sourcesDynamical analysis on $f(R, \mathcal{G})$ cosmologyFurther exact cosmological solutions to higher-order gravity theoriesΛCDM epoch reconstruction from <i>F</i> ( <i>R</i> , <i>G</i> ) and modified Gauss–Bonnet gravitiesModified gravity with negative and positive powers of curvature: Unification of inflation and cosmic accelerationQuintessence and the Rest of the World: Suppressing Long-Range InteractionsOn the stability of the cosmological solutions in <i>f</i> ( <i>R</i> , <i>G</i> ) gravityDark Energy and the Accelerating UniverseCURVATURE QUINTESSENCEExtended Theories of Gravity
- 連携機関・データベース
- 国立情報学研究所 : CiNii Research
- 提供元機関・データベース
- Crossref科学研究費助成事業データベース科学研究費助成事業データベースCrossref
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