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In this article we discuss the role of current and future CMB measurements in pinning down the model of inflation responsible for the generation of primordial curvature perturbations. By considering a parameterization of the effective field…

高能物理 - 理论 · 物理学 2014-10-03 Rhiannon Gwyn , Gonzalo A. Palma , Mairi Sakellariadou , Spyros Sypsas

This paper examines the late-time accelerating Universe and the formation of large-scale structures within the modified symmetric teleparallel gravity framework, specifically using the $f(Q)$-gravity model, in light of recent cosmological…

广义相对论与量子宇宙学 · 物理学 2024-12-31 Shambel Sahlu , Amare Abebe

In this work, we introduce a parametrization of early dark energy that mimics radiation at early times and governs the present acceleration of the Universe. We show that such parametrization models non-linear electrodynamics in the early…

广义相对论与量子宇宙学 · 物理学 2023-07-13 H. B. Benaoum , Luz Ángela García , Leonardo Castañeda

The occurrence of the phenomenon known as photon acceleration is a natural prediction of nonlinear electrodynamics (NLED). This would appear as an anomalous frequency shift in any modeling of the electromagnetic field that only takes into…

天体物理学 · 物理学 2008-11-26 Jean Paul Mbelek , Herman J. Mosquera Cuesta , M. Novello , Jose M. Salim

Observations of SN 1997ff at z ~ 1.7 favor the accelerating Universe interpretation of the high-redshift type Ia supernova data over simple models of intergalactic dust or SN luminosity evolution. Taken at face-value, they provide direct…

天体物理学 · 物理学 2009-12-30 Michael S. Turner , Adam Riess

Recently, few cosmological models with additional non-Riemannian volume form(s) have been proposed. In this article we use Supernovae type Ia experimental data to test one of these models which provides a unified description of both dark…

广义相对论与量子宇宙学 · 物理学 2018-10-05 Denitsa Staicova , Michail Stoilov

Starting from pure multidimensional gravity with curvature-nonlinear terms but no matter fields in the initial action, we obtain a cosmological model with two effective scalar fields related to the size of two extra factor spaces. The model…

广义相对论与量子宇宙学 · 物理学 2010-04-21 K. A. Bronnikov , S. G. Rubin , I. V. Svadkovsky

We attempt a novel mechanism to understand the underlying cause of late-time cosmic acceleration using a distinguished physical process taking place in the late Universe. The turning of massive neutrinos from relativistic to…

广义相对论与量子宇宙学 · 物理学 2020-07-07 M. Sami , Shynaray Myrzakul , Mudhahir Al Ajm

Recent astronomical observations indicate that the Universe is presently almost flat and undergoing a period of accelerated expansion. Basing on Einstein's general relativity all these observations can be explained by the hypothesis of a…

天体物理学 · 物理学 2007-06-13 Marek Szydlowski , Aleksandra Kurek , Adam Krawiec

The cosmological constant, which was introduced by Einstein a century ago to allow for a static universe, experienced a revival two decades ago under the label dark energy as a parameter to model the observed accelerated expansion of the…

综合物理 · 物理学 2019-01-08 Jan O. Stenflo

Creation of Cold Dark Matter (CCDM) can macroscopically be described by a negative pressure, and, therefore, the mechanism is capable to accelerate the Universe, without the need of an additional dark energy component. In this framework we…

宇宙学与河外天体物理 · 物理学 2015-05-28 J. F. Jesus , F. A. Oliveira , S. Basilakos , J. A. S. Lima

In order to explain the current acceleration of the Universe, the fine tuning problem of the cosmological constant $\Lambda$ and the cosmic coincidence problem, different alternative models have been proposed in the literature. We use the…

宇宙学与河外天体物理 · 物理学 2019-05-13 Alexander Bonilla Rivera , Jorge García Farieta

Inflation is a necessary cosmic mechanism to cure basic inconsistencies of the standard model of cosmology. These problems are usually `fixed' by postulating the existence of a scalar field (called the ``inflaton''). However, other less ad…

广义相对论与量子宇宙学 · 物理学 2026-01-16 Joan Solà Peracaula , Àlex González-Fuentes , Cristian Moreno-Pulido

In this work, we perform reconstruction of \( f(Q) \) gravity inspired by the New Agegraphic Dark Energy (NADE) model, aiming to account for the Universe's late time acceleration without invoking a cosmological constant. Utilizing a power…

宇宙学与河外天体物理 · 物理学 2025-07-02 Rajdeep Mazumdar , Kalyan Malakar , Mrinnoy M. Gohain , Kalyan Bhuyan

Supersymmetric hybrid inflation is an exquisite framework to connect inflationary cosmology to particle physics at the scale of grand unification. Ending in a phase transition associated with spontaneous symmetry breaking, it can naturally…

高能物理 - 唯象学 · 物理学 2014-07-31 Wilfried Buchmuller , Valerie Domcke , Kohei Kamada , Kai Schmitz

The accelerating expansion of the universe is the most surprising cosmological discovery in many decades. In this short review, we briefly summarize theories for the origin of cosmic acceleration and the observational methods being used to…

宇宙学与河外天体物理 · 物理学 2014-01-03 Michael J. Mortonson , David H. Weinberg , Martin White

Cosmology is investigated within a new, scalar theory of gravitation, which is a preferred-frame bimetric theory with flat background metric. Before coming to cosmology, the motivation for an " ether theory " is exposed at length; the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Mayeul Arminjon

I propose a unified model of particle physic and cosmology based on both a new extension of the standard particle model and the fundamental principle of the standard cosmology. Beyond the SM, I introduce several species of dark fields with…

综合物理 · 物理学 2025-05-13 Wei-Min Yang

The absence of guidance from fundamental physics about the mechanism behind cosmic acceleration has given rise to a number of alternative cosmological scenarios. These are based either on modifications of general relativistic gravitation…

宇宙学与河外天体物理 · 物理学 2015-05-20 M. A. Dantas , J. S. Alcaniz , D. Mania , Bharat Ratra

We explore the late time cosmological dynamics of the Universe within the framework of $f(Q,\mathcal{L}_{m})$ gravity by considering the specific form $f(Q, \mathcal{L}_m)=-Q+2\mathcal{L}_m+\gamma$. To describe the cosmic pressure…

广义相对论与量子宇宙学 · 物理学 2025-08-08 Amit Samaddar , S. Surendra Singh