Article
Astronomy & Astrophysics
Wenyu Wang, Wu-Long Xu, Bin Zhu
Summary: This study investigates the influence of the intrinsic interaction of dark matter self-scattering on structure formation. By introducing a simplified model and a new definition of velocity dependence, the impact of dark protons on cosmological structures is revealed.
Article
Astronomy & Astrophysics
Enis Belgacem, Tomislav Prokopec
Summary: This paper presents a detailed study of a simple model aiming to explain dark energy as quantum fluctuations in a scalar field during inflation. The study explores the spatial correlations imprinted on dark energy by its quantum origin and their possible role in alleviating the Hubble tension. The results show discrepancies between the predictions of the stochastic formalism and field theoretical treatment, but introducing a reduced speed of sound for the scalar field restores agreement. The paper also discusses an alternative approach based on the evolution of probability distributions for studying correlators within the stochastic formalism.
Article
Astronomy & Astrophysics
Miguel Correa, Mayukh R. Gangopadhyay, Nur Jaman, Grant J. Mathews
Summary: This study investigates the natural warm inflationary paradigm and reveals two significant new findings. Firstly, the observational constraints on the primordial power spectrum from the cosmic microwave background (CMB) can be met within the Planck scale of the effective field theory. Secondly, the natural warm inflationary paradigm can inevitably generate primordial black holes (PBHs) in a specific mass range, which can account for the entirety of the universe's dark matter while satisfying observational constraints.
Article
Astronomy & Astrophysics
Hao Wang, Yun-Song Piao
Summary: In studies on pre-recombination early dark energy (EDE), the post-recombination evolution of the universe is often assumed to be Lambda CDM-like, with a dark energy equation of state w = -1. However, in realistic models, w may be evolving. This research explores different models for the evolution of w with respect to redshift z in Axion-like EDE and AdSEDE models. By performing a Monte Carlo Markov chain analysis with recent cosmological data, it is found that the bestfit w(z) is compatible with a constant w(0) = -1, wa = 0 (corresponding to a cosmological constant), and the evolution of w is only marginally favored, having little effect on the bestfit value of H-0.
Article
Astronomy & Astrophysics
Rodrigo von Marttens, Javier E. Gonzalez, Jailson Alcaniz, Valerio Marra, Luciano Casarini
Summary: The study relaxes the minimum coupling assumption between dark matter and dark energy fields, reconstructs the interaction in the dark sector independent of the ACDM model, and finds consistency with the ACDM model at 3 sigma CL. However, the current background data do not rule out the possibility of interaction in the dark sector. Euclid and SKA are forecasted to distinguish interacting models with about 4% precision at z approximately 1.
Article
Astronomy & Astrophysics
Hao Wang, Yun-Song Piao
Summary: This study finds that considering the coupling between a fraction of dark matter and EDE can help alleviate the cosmic expansion tension.
Article
Astronomy & Astrophysics
Ahmad Mehrabi, Maryam Vazirnia
Summary: In this study, the DE density is reconstructed from observational data, and its evolution over time is investigated. The results show good agreement with the ΛCDM model at lower redshifts, but a weak sign of negative DE density is observed at higher redshifts.
ASTROPHYSICAL JOURNAL
(2022)
Article
Physics, Particles & Fields
Luis A. Escamilla, J. Alberto Vazquez
Summary: The main aim of this paper is to compare reconstructions of dark energy properties using different models and methods. The reconstructions were made using data from the Hubble parameter, Supernovae Type Ia, and Baryon Acoustic Oscillations. The models were compared through parameter estimation and Bayesian Evidence, revealing better fit to the data compared to ACDM and interesting features such as oscillatory behavior and transition to the phantom divide-line in the equation of state. Principal component analysis was also used to distinguish these features from noise contributions.
EUROPEAN PHYSICAL JOURNAL C
(2023)
Article
Physics, Particles & Fields
W. J. C. da Silva, R. Silva
Summary: The study examines the impact of extended viscous dark energy models on matter perturbations, showing similarities to the ΛCDM model at high redshift but slight differences at late times. Bayesian analysis using observational data indicates compatibility with cosmological probes and recovery of the ΛCDM model. The viscous models alleviate the H-0 tension by about 2 to 3 sigma and some can alleviate the sigma(8) tension. However, in the model selection framework, the extended viscous dark energy models are discarded based on the data.
EUROPEAN PHYSICAL JOURNAL C
(2021)
Article
Physics, Multidisciplinary
Muhamad Zahid Mughal, Iftikhar Ahmad
Summary: This paper investigates a multi-field model of dark energy, analyzing the system using multi-field tachyon and phantom tachyon scalars, predicting the fate of the universe, and noting that stable critical points satisfy power-law solutions. The model affects the equation of state parameter w, transitioning from greater than -1 to less than -1 during the evolutionary phase, with the phantom divide playing a decisive role in the cosmos' evolution.
EUROPEAN PHYSICAL JOURNAL PLUS
(2021)
Article
Astronomy & Astrophysics
Gabriel Gomez
Summary: Scalar fields coupled to dark matter by conformal or disformal transformations give rise to a general class of scalar-tensor theories with rich phenomenology in cosmology. However, the vector case has been barely studied. In this study, we build models based on vector fields coupled to dark matter and derive the interaction term in a covariant form independent of gravity theory, providing insights into general vector-tensor theories. Numerical calculations show that the coupling of vector fields to dark matter significantly affects the cosmological dynamics during different stages of the Universe's evolution.
Article
Astronomy & Astrophysics
Yue Nan, Kazuhiro Yamamoto
Summary: In this study, a dynamical model for dark energy based on an ultralight mass scalar field with large-scale inhomogeneities is considered. The model is found to have observable impacts on the anisotropic properties of the cosmic microwave background (CMB) intensity and luminosity distance. Numerical solutions show that the model can mimic the standard ΛCDM cosmology, including spatially dependent dark energy with flexible ranges of model parameters. Constraints on the amplitude of these inhomogeneities are also put forward through observations of the CMB anisotropies, along with discussions on their influence on the estimation of the luminosity distance.
Article
Astronomy & Astrophysics
Earl Lester, Krzysztof Bolejko
Summary: The study investigates the effects of decaying dark matter on cosmic voids, highlighting these voids as valuable locations for studying dark matter physics with less baryonic contamination. Future cosmological observations should focus on identifying signs of decaying dark matter to confirm or rule out this scenario. Lack of reported features could impose constraints on the decay rate of dark matter.
Article
Astronomy & Astrophysics
Abraham Loeb
Summary: I demonstrate that gravitational scattering of dark matter objects can provide the required cross section per unit mass for self-interacting dark matter models that address the challenges of small-scale structures in the collisionless cold dark matter model. The interaction decreases steeply with increasing velocity, which explains the lack of evidence for self-interaction in data on massive galaxies and clusters of galaxies.
ASTROPHYSICAL JOURNAL LETTERS
(2022)
Article
Astronomy & Astrophysics
Giovanni Acquaviva, Ozgur Akarsu, Nihan Katirci, J. Alberto Vazquez
Summary: This work discusses the potential of dark energy models with negative energy density values in the past to alleviate the H-0 tension and the discrepancy with the baryon acoustic oscillation (BAO) Lyman-alpha data within the Lambda CDM model. It also investigates whether two minimal extensions of the Lambda CDM model can successfully achieve such scenarios.