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相关论文: Inflation with scalar-tensor theory of gravity

200 篇论文

We study the inflationary phenomenology of a non-minimally coupled Einstein Gauss-Bonnet gravity theory, in the presence of a scalar potential, under the condition that the gravitational wave speed of the primordial gravitational waves is…

广义相对论与量子宇宙学 · 物理学 2020-08-26 S. D. Odintsov , V. K. Oikonomou , F. P. Fronimos

We consider an Einstein-Scalar-Gauss-Bonnet gravitational theory, and argue that at early times the Ricci scalar can be safely ignored. We then demonstrate that the pure scalar-Gauss-Bonnet theory, with a quadratic coupling function,…

高能物理 - 理论 · 物理学 2015-09-02 Panagiota Kanti , Radouane Gannouji , Naresh Dadhich

We systematically study the renormalizable three-term polynomial inflation in the supersymmetric and non-supersymmetric models. The supersymmetric inflaton potentials can be realized in supergravity theory, and only have two independent…

高能物理 - 唯象学 · 物理学 2015-10-26 Tianjun Li , Zheng Sun , Chi Tian , Lina Wu

We investigate the inflationary universe in a theory where two scalar fields non-minimally coupling to the scalar curvature and an extra $R^2$ term exist and the conformal invariance is broken. In particular, the slow-roll inflation is…

高能物理 - 理论 · 物理学 2016-03-01 Kazuharu Bamba

The nonminimal coupling of the kinetic term to Einstein's tensor helps the implementation of inflationary models due to the gravitationally enhanced friction. We calculate the parametrized post-Newtonian (PPN) parameters for the…

广义相对论与量子宇宙学 · 物理学 2016-07-21 Zhu Yi , Yungui Gong

The single scalar field inflationary models that lead to scalar and tensor perturbation spectra with amplitudes varying in direct proportion to one another are reconstructed by solving the Stewart-Lyth inverse problem to next-to-leading…

天体物理学 · 物理学 2009-11-07 C. A. Terrero-Escalante , James E. Lidsey , Alberto A. Garcia

We identify models of supersymmetric hybrid inflation in which the tensor-to-scalar ratio, a canonical measure of gravity waves produced during inflation, can be as large as 0.03 or so, which will be tested by the Planck satellite…

高能物理 - 唯象学 · 物理学 2011-03-07 Qaisar Shafi , Joshua R. Wickman

The union of high-energy particle theories and gravitation often gives rise to an evolving strength of gravity. The standard picture of the earliest universe would certainly deserve revision if the Planck mass, which defines the strength of…

广义相对论与量子宇宙学 · 物理学 2008-02-03 Janna J. Levin

We derive the first quantum gravitational corrections to the inflationary power spectra for a general single-field scalar-tensor theory which includes a non-minimal coupling to gravity, a non-standard scalar kinetic term and an arbitrary…

广义相对论与量子宇宙学 · 物理学 2020-01-08 Christian F. Steinwachs , Matthijs L. van der Wild

In this work, we consider inflection point inflation in the framework of running kinetic term inflation in supergravity. We study the inflationary dynamics and show that the predicted value of the scalar spectral index and tensor-to-scalar…

高能物理 - 唯象学 · 物理学 2017-04-19 Tie-Jun Gao , Wu-Tao Xu , Xiu-Yi Yang

In scalar-tensor theories the scalar fields generically couple nontrivially to gravity. We study the observable properties of inflationary models with non-minimally coupled inflaton and Dirac-Born-Infeld (DBI) kinetic term. Within the…

宇宙学与河外天体物理 · 物理学 2010-04-06 Damien A. Easson , Shinji Mukohyama , Brian A. Powell

In this study, we investigate swampland conjectures within the setup of matter and non-metricity nonminimal coupling theories of gravity. We examine how the inflationary solution produced by a single scalar field can be resolved with the…

广义相对论与量子宇宙学 · 物理学 2024-01-01 Sanjay Mandal , Kazuharu Bamba

We investigate a standard minimally-coupled scalar-field inflationary scenario, which is based on a new potential, with suitably generalized plateau features, that leads to extra small tensor-to-scalar ratios. In particular, we consider a…

宇宙学与河外天体物理 · 物理学 2025-11-13 Gerasimos Kouniatalis , Emmanuel N. Saridakis

We investigate perturbations in power-law monomial potentials within inflationary models driven by a single scalar field. By introducing a second term to the original potential, we study how this perturbation influences the slow-roll…

广义相对论与量子宇宙学 · 物理学 2026-02-25 Maria E. S. Antunes , Micol Benetti , Eduardo Bittencourt , Fernando A. Franco

We investigate a class of inflationary models in modified gravity theories which contain a non-minimal coupling between gravity and a scalar field $\phi$ (inflaton) as $f(R,T)=R \bigl(1+\alpha+ \kappa^4 \beta T \bigr)+\kappa^2\gamma T $…

广义相对论与量子宇宙学 · 物理学 2024-12-03 Payel Sarkar , Ashmita , Prasanta Kumar Das

The inflationary paradigm is an important cornerstone of the concordance cosmological model. However, standard inflation cannot fully address the transition from an early homogeneous and isotropic stage, to another one lacking such…

广义相对论与量子宇宙学 · 物理学 2015-12-08 Mauro Mariani , Gabriel R. Bengochea , Gabriel Leon

In this paper, we investigate the potential-driven inflation models with a disformal coupling to Einstein Gravity, to find out the effects of such a coupling on these models. We consider a simple coupling form which introduces only one…

高能物理 - 唯象学 · 物理学 2020-09-16 Taotao Qiu , Zehua Xiao , Jiaming Shi , Muhsin Aljaf

In the framework of gravitational models obtained from the Geometric Inflation's proposal, where an infinite tower of curvature scalars are included into the action, we compute the slow-roll parameters by the Hubble slow-roll approach. We…

广义相对论与量子宇宙学 · 物理学 2020-09-02 Gustavo Arciniega , Luisa Jaime , Gabriella Piccinelli

We examine the power-law Starobinsky model, a generalized version of the Starobinsky inflation model, characterized by a power-law correction to Einstein gravity. Employing the $f(R)$ formalism, the scalar and tensor power spectra were…

宇宙学与河外天体物理 · 物理学 2025-02-10 Saisandri Saini , Akhilesh Nautiyal

We consider the non-minimally kinetic coupled version of DGP brane model, where the kinetic term of the scalar field is coupled to the metric and Einstein tensor on the brane by a coupling constant $\zeta$. We obtain the corresponding field…

广义相对论与量子宇宙学 · 物理学 2016-04-12 F. Darabi , A. Parsiya , K. Atazadeh