Frontiers in Numerical Precision: From Astrophysics to Cosmology

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Gravitation".

Deadline for manuscript submissions: closed (28 February 2023) | Viewed by 3167

Special Issue Editor


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Guest Editor
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Circuito Exterior C.U., A.P. 70-543, México D.F. 04510, Mexico
Interests: dark energy; modified and extended theories of gravity; cosmostatistics

Special Issue Information

Dear Colleagues,

Studies of gravity theories lie at the interface of astrophysics, cosmology, nuclear physics, and collider physics. Constraining such theories entails the capability to compare predictions to a wide range of observations. In this line of thought, over the last 30 years, growing research areas, such as precision cosmology and astrophysics, have developed, where complex numerical methods and simulations to deal with Big Data observations are employed to construct viable solutions to the current issues at hand, evoking the consideration of new theories of gravity or exotic components at cosmic and local scales. Although much has been learned through these approaches, progress has guided us to a degeneracy of proposals. We invite our colleagues to contribute their papers to inform the scientific community of the advances made on these topics.

Prof. Dr. Celia Escamilla-Rivera
Guest Editor

Manuscript Submission Information

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Keywords

  • dark energy
  • dark matter
  • structure formation
  • modified gravity
  • observational cosmology
  • observations
  • future surveys
  • neutron stars
  • gravitational waves

Published Papers (2 papers)

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Research

12 pages, 422 KiB  
Article
Construction and Evolution of Equilibrium Configurations of the Schrödinger–Poisson System in the Madelung Frame
by Iván Alvarez-Ríos and Francisco S. Guzmán
Universe 2022, 8(8), 432; https://0-doi-org.brum.beds.ac.uk/10.3390/universe8080432 - 21 Aug 2022
Cited by 3 | Viewed by 976
Abstract
We present the construction of ground state equilibrium configurations of the Schrödinger–Poisson (SP) system in the Madelung frame and evolve such configuration using finite volume methods. We compare the behavior of these configurations when evolved within the SP and Madelung frames, in terms [...] Read more.
We present the construction of ground state equilibrium configurations of the Schrödinger–Poisson (SP) system in the Madelung frame and evolve such configuration using finite volume methods. We compare the behavior of these configurations when evolved within the SP and Madelung frames, in terms of conservation of mass and energy. We also discuss the issues of the equations in the Madelung frame and others inherent to the numerical methods used to solve them. Full article
(This article belongs to the Special Issue Frontiers in Numerical Precision: From Astrophysics to Cosmology)
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10 pages, 3409 KiB  
Article
On the Degeneracy between 8 Tension and Its Gaussian Process Forecasting
by Mauricio Reyes and Celia Escamilla-Rivera
Universe 2022, 8(8), 394; https://0-doi-org.brum.beds.ac.uk/10.3390/universe8080394 - 27 Jul 2022
Cited by 3 | Viewed by 977
Abstract
In this Article, we reconstruct the growth and evolution of the cosmic structure of the Universe using Markov chain Monte Carlo algorithms for Gaussian processes. We estimate the difference between the reconstructions that are calculated through a maximization of the kernel hyperparameters and [...] Read more.
In this Article, we reconstruct the growth and evolution of the cosmic structure of the Universe using Markov chain Monte Carlo algorithms for Gaussian processes. We estimate the difference between the reconstructions that are calculated through a maximization of the kernel hyperparameters and those that are obtained with a complete exploration of the parameter space. We find that the difference between these two approaches is of the order of 1%. Furthermore, we compare our results with those obtained by Planck Collaboration 2018 assuming a ΛCDM model and we do not find a statistically significant difference in the redshift range where the reconstructions of fσ8 have been made. Full article
(This article belongs to the Special Issue Frontiers in Numerical Precision: From Astrophysics to Cosmology)
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