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We present a numerical analysis of the cosmological evolution of scalar field dark matter (SFDM) in the Boltzmann code $\texttt{CLASS}$, based on a dynamical system analysis of previous works. We show a detailed study of the evolution of…

宇宙学与河外天体物理 · 物理学 2023-07-13 L. Arturo Ureña-López , Francisco X. Linares Cedeño

We investigate cosmological solutions of the chameleon model with a non-minimal coupling between the matter and the scalar field through a conformal factor with gravitational strength. By considering the spatially flat FLRW metric and the…

广义相对论与量子宇宙学 · 物理学 2023-11-01 Raziyeh Zaregonbadi , Nasim Saba , Mehrdad Farhoudi

In this study, we have explored a scalar field cosmological model in the axially symmetric Bianchi type-I universe. In this study, our aim is to constrain the scalar field dark energy model in an anisotropic background. For this purpose,…

广义相对论与量子宇宙学 · 物理学 2025-11-19 Vinod Kumar Bhardwaj , Anil Kumar Yadav

This article describes lcpy, an open-source python package that allows for advanced parametric Life Cycle Assessment (LCA) and Life Cycle Costing (LCC) analysis. The package is designed to allow the user to model a process with a flexible,…

新兴技术 · 计算机科学 2025-06-17 Spiros Gkousis , Evina Katsou

We investigate the late-time evolution of the Universe within a cosmological model in which dark matter and dark energy are identified with two interacting scalar fields. Using methods of qualitative analysis of dynamical systems, we…

广义相对论与量子宇宙学 · 物理学 2021-06-14 Paulo M. Sá

We introduce a Markov Chain Monte Carlo simulation and data analysis package that extends the CMBEASY software. We have taken special care in implementing an adaptive step algorithm for the Markov Chain Monte Carlo in order to improve…

天体物理学 · 物理学 2007-05-23 Michael Doran , Christian M. Mueller

Cosmological scaling solutions, which give rise to a scalar-field density proportional to a background fluid density during radiation and matter eras, are attractive to alleviate the energy scale problem of dark energy. In the presence of…

广义相对论与量子宇宙学 · 物理学 2010-03-25 Junko Ohashi , Shinji Tsujikawa

Non-minimally coupled scalar field models are well-known for providing interesting cosmological features. These include a late time dark energy behavior, a phantom dark energy evolution without singularity, an early time inflationary…

广义相对论与量子宇宙学 · 物理学 2021-09-03 Wompherdeiki Khyllep , Jibitesh Dutta

We describe scalar-bimetric theories where the dynamics of the Universe are governed by two separate metrics, each with an Einstein-Hilbert term. In this setting, the baryonic and dark matter components of the Universe couple to metrics…

广义相对论与量子宇宙学 · 物理学 2018-10-09 Philippe Brax , Patrick Valageas

We present a computational framework for "painting" galaxies on top of the Dark Matter Halo/Sub-Halo hierarchy obtained from N-body simulations. The method we use is based on the sub-halo clustering and abundance matching (SCAM) scheme…

宇宙学与河外天体物理 · 物理学 2024-02-15 Tommaso Ronconi , Andrea Lapi , Matteo Viel , Alberto Sartori

By means of the present geometrical and dynamical observational data, it is very hard to establish, from a statistical perspective, a clear preference among the vast majority of the proposed models for the dynamical dark energy and/or…

宇宙学与河外天体物理 · 物理学 2017-11-07 Tomasz Denkiewicz , Vincenzo Salzano

We look for cosmologies with a scalar field (dark energy without cosmological constant), which mimic the standard $\Lambda CDM$ cosmological model yielding exactly the same large-scale geometry described by the evolution of the Hubble…

天体物理学 · 物理学 2015-05-13 V. I. Zhdanov , G. Ivashchenko

We study the most general cosmological model with real scalar field which is minimally coupled to gravity. Our calculations are based on Friedmann-Lemaitre-Robertson-Walker (FLRW) background metric. Field equations consist of three…

广义相对论与量子宇宙学 · 物理学 2023-03-22 Medine Ildes , Metin Arik

Cosmological scaling solutions are particularly important in solving the coincidence problem of dark energy. We derive the equations of sub-Hubble linear matter perturbations for a general scalar-field Lagrangian--including quintessence,…

天体物理学 · 物理学 2009-11-11 Luca Amendola , Shinji Tsujikawa , M. Sami

The chameleon model is a modified gravity theory that introduces an additional scalar field that couples to matter through a conformal coupling. This `chameleon field' possesses a screening mechanism through a nonlinear self-interaction…

广义相对论与量子宇宙学 · 物理学 2022-01-05 Chad Briddon , Clare Burrage , Adam Moss , Andrius Tamosiunas

Markov Chain Monte Carlo (MCMC) sampler is widely used for cosmological parameter estimation from CMB and other data. However, due to the intrinsic serial nature of the MCMC sampler, convergence is often very slow. Here we present a fast…

宇宙学与河外天体物理 · 物理学 2014-08-12 Santanu Das , Tarun Souradeep

SpectraPy is an Astropy affiliated package for spectroscopic data reduction. It collects algorithms and methods for data reduction of astronomical spectra obtained by through-slits spectrographs. It has been created to fill the gap in…

天体物理仪器与方法 · 物理学 2023-02-10 Marco Fumana

The current paper provides a comprehensive examination of a dark energy cosmological model in the classical regime, in which a generic scalar field is regarded as a dark energy source. Einstein's field equations are solved in model…

广义相对论与量子宇宙学 · 物理学 2022-09-07 Ritika Nagpal , Shibesh Kumar Jas Pacif , Abhishek Parida

A simple speed-up cosmology model is proposed to account for the dark energy puzzle. We condense contributions from dark energy and curvature term into one effective parameter in order to reduce parameter degeneracies and to find any…

天体物理学 · 物理学 2007-10-10 Xin-He Meng , Meng Su , Zheng Wang