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The matter creation cosmology is revisited, including the evolution of baryons and dark matter particles. The creation process affects only dark matter and not baryons. The dynamics of the $\Lambda$CDM model can be reproduced only if two…

宇宙学与河外天体物理 · 物理学 2014-07-08 J. C. Fabris , J. A. de Freitas Pacheco , O. F. Piattella

We propose an alternative, nonsingular, cosmic scenario based on gravitationally induced particle production. The model is an attempt to evade the coincidence and cosmological constant problems of the standard model ($\Lambda$CDM) and also…

宇宙学与河外天体物理 · 物理学 2015-06-05 J. A. S. Lima , S. Basilakos , F. E. M. Costa

Cosmic acceleration is widely believed to require either a source of negative pressure (i.e., dark energy), or a modification of gravity, which necessarily implies new degrees of freedom beyond those of Einstein gravity. In this paper we…

高能物理 - 理论 · 物理学 2017-06-28 Lasha Berezhiani , Justin Khoury , Junpu Wang

Non-conservation of dark matter can lead to late-time cosmic acceleration. This mechanism is known as the matter creation theory and this replaces the need of dark energy and modified gravity theories. We consider a two-fluid system…

广义相对论与量子宇宙学 · 物理学 2025-12-02 Sudip Halder , Jaume de Haro , Supriya Pan , Tapan Saha , Subenoy Chakraborty

A new kind of accelerating flat model with no dark energy that is fully dominated by cold dark matter (CDM) is investigated. The number of CDM particles is not conserved and the present accelerating stage is a consequence of the negative…

天体物理学 · 物理学 2014-11-18 J. A. S. Lima , F. E. Silva , R. C. Santos

We investigate the creation of cold dark matter (CCDM) cosmology as an alternative to explain the cosmic acceleration. Particular attention is given to the evolution of density perturbations and constraints coming from recent observations.…

宇宙学与河外天体物理 · 物理学 2014-04-11 Rudnei O. Ramos , Marcelo Vargas dos Santos , Ioav Waga

A new cosmic scenario with gravitationally induced particle creation is proposed. In this model the Universe evolves from an early to a late time de Sitter era, with the recent accelerating phase driven only by the negative creation…

广义相对论与量子宇宙学 · 物理学 2015-06-22 J. A. S. Lima , L. L. Graef , D. Pavón , S. Basilakos

We revisit a cosmological model where dark matter (DM) and dark energy (DE) follow barotropic equations of state, allowing deviations from the standard $\Lambda$CDM framework (i.e. $w_{dm} \neq 0$, $w_{de} \neq -1$), considering both flat…

宇宙学与河外天体物理 · 物理学 2025-11-24 Dorian Araya , Cristian Castillo , Genly Leon , Juan Magaña , Angie Barr Domínguez , Miguel A. García-Aspeitia

Modified dark matter (MDM) is a phenomenological model of dark matter, inspired by gravitational thermodynamics. For an accelerating Universe with positive cosmological constant ($\Lambda$), such phenomenological considerations lead to the…

宇宙学与河外天体物理 · 物理学 2018-02-14 Douglas Edmonds , Duncan Farrah , Djordje Minic , Y. Jack Ng , Tatsu Takeuchi

We discuss an interacting dark sector model featuring decaying vacuum energy and dark matter empowered by gravitationally induced matter creation. Motivated by quantum field theoretic considerations of vacuum decay and adiabatic particle…

宇宙学与河外天体物理 · 物理学 2025-09-17 Lokesh Chander , C P Singh

The standard procedure to explain the accelerated expansion of the Universe is to assume the existence of an exotic component with negative pressure, generically called dark energy. Here, we propose a new accelerating flat cosmology without…

宇宙学与河外天体物理 · 物理学 2025-02-21 P. W. R. Lima , J. A. S. Lima , J. F. Jesus

A new accelerating cosmology driven only by baryons plus cold dark matter (CDM) is proposed in the framework of general relativity. In this model the present accelerating stage of the Universe is powered by the negative pressure describing…

宇宙学与河外天体物理 · 物理学 2010-12-06 J. A. S. Lima , J. F. Jesus , F. A. Oliveira

The nature of dark matter is one of the most fundamental questions in cosmology. Using the cosmic microwave background (CMB), type Ia supernova (SN) and DESI's new measurements of baryon acoustic oscillations (BAO), we find the robust…

宇宙学与河外天体物理 · 物理学 2025-05-13 Deng Wang

A fundamental question in cosmology is whether dark energy evolves over time, a topic that has gained prominence since the discovery of cosmic acceleration. Recently, the DESI collaboration has reported increasing evidence for evolving dark…

宇宙学与河外天体物理 · 物理学 2025-11-21 Deng Wang , David Mota

The negative pressure accompanying gravitationally-induced particle creation can lead to a cold dark matter (CDM) dominated, accelerating Universe (Lima et al. 1996) without requiring the presence of dark energy or a cosmological constant.…

天体物理学 · 物理学 2009-07-22 G. Steigman , R. C. Santos , J. A. S. Lima

The universe with adiabatic matter creation is considered. It is thought that the negative pressure caused by matter creation can play the role of a dark energy component, and drive the accelerating expansion of the universe. Using the Type…

天体物理学 · 物理学 2015-06-24 Yuan Qiang , Tong-Jie Zhang , Ze-Long Yi

This article opens new window to obtain accelerating scaling attractors without any need of dark energy. We study cosmological dynamics in a two-fluid system where pressureless dark matter (DM) undergoes adiabatic particle creation and…

广义相对论与量子宇宙学 · 物理学 2026-04-24 Sudip Halder , Jaume de Haro , Supriya Pan , Emmanuel N. Saridakis , Tapan Saha , Subenoy Chakraborty

In the present article we have investigated a very natural question regarding the dynamics of the universe, namely, the possibility of its decelerating phase immediately after the present accelerating phase. To begin with, we have focused…

广义相对论与量子宇宙学 · 物理学 2022-04-26 Yu. L. Bolotin , V. A. Cherkaskiy , M. I. Konchatnyi , Supriya Pan , Weiqiang Yang

In the present lore of cosmology, matter and space-time emerged from a singularity and evolved through four different regimes: inflation, radiation, dark matter and dark energy dominated eras. In the radiation and dark matter dominated…

宇宙学与河外天体物理 · 物理学 2011-06-13 J. A. S. Lima , S. Basilakos
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