Article
Astronomy & Astrophysics
Andreu Maso-Ferrando, Nicolas Sanchis-Gual, Jose A. Font, Gonzalo J. Olmo
Summary: In the Palatini formulation of f (R) gravity, equilibrium solutions of spherically symmetric boson stars were explored. The study compared solutions of the quadratic theory f (R) = R + xi R-2 with those in general relativity, showing similar existence curves but significant differences for negative coupling parameters leading to repulsive gravitational components. Introducing self-interactions further emphasized the similarities between f (R) and general relativity, making observational discrimination between the two theories challenging.
CLASSICAL AND QUANTUM GRAVITY
(2021)
Article
Astronomy & Astrophysics
Dhruba Jyoti Gogoi, Umananda Dev Goswami
Summary: This study investigates the behavior of dark energy f(R) gravity models along with two other cosmological models under the Palatini formalism. The results show that the new model behaves similarly to the other models in the early stages of the universe but has a unique prediction for the future history of the universe. All models show good agreement with observational data within a constrained range of parameters, with the new model showing particularly satisfactory agreement throughout its allowed parameter range.
INTERNATIONAL JOURNAL OF MODERN PHYSICS D
(2022)
Article
Astronomy & Astrophysics
Adrian Casado-Turrion, Antonio Dobado, Alvaro de la Cruz-Dombriz
Summary: This study investigates gravitational collapse in the context of f(R) theories of gravity. By generalizing the Oppenheimer-Snyder model to fit within metric f(R) gravity, novel exterior solutions are found, and it is verified that certain vacuum metrics cannot represent spacetime outside a collapsing dust star in metric f(R) gravity. Additionally, it is discovered that the Oppenheimer-Snyder model is incompatible with the junction conditions of the Palatini formulation of f(R) gravity.
Article
Astronomy & Astrophysics
A. B. Lahanas
Summary: In this study, we investigate R2 inflation in Palatini gravity with scalar fields coupled to gravity. We explore the similarities between these theories, in the Einstein frame, and K-inflation models. Additionally, we examine single-field inflationary models with monomial potentials V similar to hn, where n is a positive even integer. The analysis also includes the study of the Higgs model with nonminimal coupling to gravity. Through constraints from cosmological data, we find bounds on the inflationary scale Ms similar to 1/√(alpha) and the reheating temperature of the Universe.
Article
Astronomy & Astrophysics
Joao C. Lobato, Isabela S. Matos, Mauricio O. Calvao, Ioav Waga
Summary: The study introduces an alternative choice of variables for treating f(R) models in their Palatini formulation, leading to the derivation of general results and a complete description of the phase space for exponential gravity. It is shown that Palatini exponential gravity theories have a final attractor critical point with specific effective equation of state parameters. Comparison of analytical results with numerical solutions of the field equations is also conducted.
Article
Physics, Multidisciplinary
Stefano Camera, Salvatore Capozziello, Lorenzo Fatibene, Andrea Orizzonte
Summary: We investigate how the cosmological equation of state can be used to scrutinize extended theories of gravity, specifically the Palatini f(R) gravity. The effective equation of state produced by a given model is studied, and the inverse problem of determining which models are compatible with a given effective equation of state is also considered. We find that power-law models are capable of transforming barotropic Equations of State into effective barotropic ones, and the form of equation of state is preserved only for f(R) = R. Additionally, quadratic and non-homogeneous effective Equations of State contain the Starobinsky model and other models.
EUROPEAN PHYSICAL JOURNAL PLUS
(2023)
Article
Astronomy & Astrophysics
J. S. Goncalves, A. F. Santos
Summary: The Palatini f(R,T) gravity theory allows for the replacement of the standard Einstein-Hilbert action with an arbitrary function of the Ricci scalar R and the trace T of the energy-momentum tensor, where the metric and connection are treated as independent variables, avoiding the occurrence of noncausal solutions.
INTERNATIONAL JOURNAL OF MODERN PHYSICS D
(2021)
Article
Physics, Particles & Fields
M. Z. Bhatti, Z. Yousaf, F. Hussain
Summary: This article investigates the effects of electromagnetic field on the generalization of Lemaitre-Tolman-Bondi (LTB) spacetime while considering Palatini f(R) gravity and dissipative dust fluid. By exploring modified field equations and establishing evolution equations, the study delves into the dynamics of an inhomogeneous universe, with a focus on the scalar functions associated with metric coefficients. The properties of generalized LTB spacetime under the influence of charge and Palatini f(R) curvature terms are compared and analyzed, with symmetric properties also studied using streaming out and diffusion approximations.
EUROPEAN PHYSICAL JOURNAL C
(2021)
Article
Physics, Multidisciplinary
Amir H. Rezaei, T. Azizi, N. Rashidi
Summary: In this paper, an exponential form of modified gravity is considered. The theory is consistent with local tests and various aspects of the model are investigated, including the static solution, scalar field potential, and stability of critical points. The realization of inflation and its graceful exit in this model are also studied.
Article
Astronomy & Astrophysics
Jaakko Annala, Syksy Rasanen
Summary: In this study, we investigate inflation using the most general non-degenerate gravitational action, involving the symmetric part of the Ricci tensor coupled to a scalar field in the Palatini formulation of gravity. By employing field redefinitions, we manage to shift the impact of the Ricci terms from gravity to the scalar field, specifically focusing on slow-roll inflation. As exemplified by cases of actions quadratic and cubic in the Ricci tensor, we find that in the quadratic scenario, the tensor-to-scalar ratio r can be suppressed with no effect on the scalar spectrum, while in the cubic scenario, r can be suppressed by at most 2/9, with significant changes in the scalar spectral index n(s).
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Physics, Particles & Fields
Kinsuk Giri, Prabir Rudra
Summary: In this work, we analyze the parameter space of Einsteinian cubic gravity and f (P) gravity using observational data analysis. We use cosmic chronometer data, BAO, and CMB peak parameters for the analysis. The chi(2) statistic is used for fitting analysis and the Markov chain Monte Carlo algorithm is used to obtain parameter bounds. Furthermore, machine learning models are employed to estimate the Hubble parameter H(z) and the results are compared with observations.
Article
Physics, Particles & Fields
Georg Herzog, Helios Sanchis-Alepuz
Summary: The study focuses on solutions of stellar structure equations in modified theories of gravity, particularly in the context of neutron stars. By exploring a range of viable values of alpha and beta, the potential impacts of R-2 and Q terms are illustrated. Results suggest that modifications of general relativity can have a significant effect on the properties of stars under certain combinations of parameters and equations of state, indicating that astrophysical observations may serve as discriminators of modifications of General Relativity as the accuracy of determination of neutron star equations of state increases.
EUROPEAN PHYSICAL JOURNAL C
(2021)
Article
Astronomy & Astrophysics
Tomohiro Inagaki, Masahiko Taniguchi
Summary: We study the quadrupole radiation of gravitational waves in F(R) modified gravity, which exhibits a massive scalar mode. The explicit expressions for the quadrupole radiation and energy current of the scalar mode in general F(R) gravity models are derived. Binary stars and bouncing stars are considered as astronomical sources, and the quadrupole radiation of scalar and tensor modes are calculated. Under spherically symmetric conditions, the scalar mode radiates, while the tensor modes do not. The mass of the scalar mode is estimated for typical energy scales, and the potential detection of the scalar mode in future gravitational wave observations is discussed.
Article
Physics, Particles & Fields
Pawan Joshi, Sukanta Panda
Summary: A Hamiltonian for the nonlocal F(R) theory is constructed in this work, revealing the nature of the ghost degrees of freedom. Finally, conditions that lead to ghost-free theories are found.
EUROPEAN PHYSICAL JOURNAL C
(2022)
Article
Physics, Multidisciplinary
Aisha Siddiqa, Rubab Manzoor, Arsal Kamal
Summary: This study analyzes the propagation of polar gravitational waves in the flat FRW cosmic background using the f(R, T-f) theory. The Regge-Wheeler polar perturbation scheme is used to study the perturbation of the flat geometry of the background spacetime and the corresponding scalar field source. Field equations for both the flat and perturbed geometries are constructed and used to evaluate perturbation parameters. The results show that polar fluctuations have an impact on both the geometry and scalar field, and the behavior of these fluctuations can be observed through numerical solutions and plots.