Based on the work of ratio gravity developed in 2018, which postulates the deformation of the cross ratio to associate with the physical model of gravity, we develop a mechanism to generate dynamical dark energy – a quintessence field coupled with gravity. Such model causes the dark energy behaving differently in early and late time universe. In the radiation-dominated-era and matter-dominated-era, the related analytical solutions of the quintessence field have an interesting property – starting as a constant field, then oscillating as the universe expands. By Markov Chain Monte Carlo search of the parameter space with the local measurement (Type Ia supernovae) in the Bayesian framework, the probed range of $$H_0$$ (within $$1\sigma $$) ove...
Aims.Dark energy can be investigated in two complementary ways, by considering either general parame...
We investigate a cosmological model in which dark energy, represented by a quintessential scalar fie...
Aims.Dark energy can be investigated in two complementary ways, by considering either general parame...
We introduce a power-law parameterized quintessence model for the dark energy. An exponential potent...
We present an effective-field-theory-based reconstruction of quintessence models of dark energy dire...
We study the matter creation cosmology as an alternative theory to explain the dark energy phenomena...
A component of dark energy has been recently proposed to explain the current acceleration of the Uni...
The existence of dark energy in the universe is hypothesized to explain the accelerated expansion of...
A component of dark energy has been recently proposed to explain the current acceleration of the Uni...
We address the fine-tuning problem of dark energy cosmologies which arises when the dark energy dens...
We address the fine-tuning problem of dark energy cosmologies which arises when the dark energy dens...
We study the non-linear growth of cosmic structure in different dark energy models, using large volu...
We present a quintessence model for the dark energy in which the quintessence scalar field is produc...
In order to understand the nature of the accelerating expansion of the late-time universe, it is imp...
We address the fine-tuning problem of dark energy cosmologies which arises when the dark energy dens...
Aims.Dark energy can be investigated in two complementary ways, by considering either general parame...
We investigate a cosmological model in which dark energy, represented by a quintessential scalar fie...
Aims.Dark energy can be investigated in two complementary ways, by considering either general parame...
We introduce a power-law parameterized quintessence model for the dark energy. An exponential potent...
We present an effective-field-theory-based reconstruction of quintessence models of dark energy dire...
We study the matter creation cosmology as an alternative theory to explain the dark energy phenomena...
A component of dark energy has been recently proposed to explain the current acceleration of the Uni...
The existence of dark energy in the universe is hypothesized to explain the accelerated expansion of...
A component of dark energy has been recently proposed to explain the current acceleration of the Uni...
We address the fine-tuning problem of dark energy cosmologies which arises when the dark energy dens...
We address the fine-tuning problem of dark energy cosmologies which arises when the dark energy dens...
We study the non-linear growth of cosmic structure in different dark energy models, using large volu...
We present a quintessence model for the dark energy in which the quintessence scalar field is produc...
In order to understand the nature of the accelerating expansion of the late-time universe, it is imp...
We address the fine-tuning problem of dark energy cosmologies which arises when the dark energy dens...
Aims.Dark energy can be investigated in two complementary ways, by considering either general parame...
We investigate a cosmological model in which dark energy, represented by a quintessential scalar fie...
Aims.Dark energy can be investigated in two complementary ways, by considering either general parame...