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New Frontiers in Cosmology and Astrophysics

A special issue of Entropy (ISSN 1099-4300). This special issue belongs to the section "Astrophysics, Cosmology, and Black Holes".

Deadline for manuscript submissions: closed (20 May 2022) | Viewed by 1955

Special Issue Editor


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Guest Editor
National Institute for Space Research, São José dos Campos, São Paulo 12227-010, Brazil
Interests: cosmological parameters; dark matter; dark energy; gravitational waves; modified gravity; tests of general relativity

Special Issue Information

Dear Colleagues,

The accumulation of large amounts of data by the most varied observations in recent years has brought new challenges to modern cosmology. These challenges include i) the tension in the measurements of the Hubble constant (H0) and the amplitude of late-time matter fluctuations (S8); ii) challenges in cosmology with gravitational waves; iii) the best modeling of the universe at early and late times, including the nature of the dark species, that is, dark matter and dark energy; and iv) improvements and new techniques for parameter estimation. Accompanied by these advances, a plethora of new theories have been proposed in order to address unresolved issues.

This Special Issue aims to collect work with particular regard to (keywords):

-Observational cosmology.

-Proposals for a new physics or systematic effects behind the data in light of the H0 and S8 tensions.

-Dark matter, dark energy, and modified gravity models.

-Data analysis techniques and parameter estimation in cosmology and gravitational waves.

-Cosmology and fundamental physics with gravitational waves.

-Gravitational waves and the nature of compact objects (neutron stars, black holes, white dwarves, primordial black holes, and exotic compact objects).

Dr. Rafael Nunes
Guest Editor

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Entropy is an international peer-reviewed open access monthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 2600 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

Published Papers (1 paper)

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Research

11 pages, 553 KiB  
Article
Search for Sub-Solar Mass Binaries with Einstein Telescope and Cosmic Explorer
by Rafael C. Nunes
Entropy 2022, 24(2), 262; https://0-doi-org.brum.beds.ac.uk/10.3390/e24020262 - 11 Feb 2022
Cited by 3 | Viewed by 1477
Abstract
A possible detection of sub-solar mass ultra-compact objects would lead to new perspectives on the existence of black holes that are not of astrophysical origin and/or pertain to formation scenarios of exotic ultra-compact objects. Both possibilities open new perspectives for better understanding of [...] Read more.
A possible detection of sub-solar mass ultra-compact objects would lead to new perspectives on the existence of black holes that are not of astrophysical origin and/or pertain to formation scenarios of exotic ultra-compact objects. Both possibilities open new perspectives for better understanding of our universe. In this work, we investigate the significance of detection of sub-solar mass binaries with components mass in the range: 102M up to 1M, within the expected sensitivity of the ground-based gravitational waves detectors of third generation, viz., the Einstein Telescope (ET) and the Cosmic Explorer (CE). Assuming a minimum of amplitude signal-to-noise ratio for detection, viz., ρ=8, we find that the maximum horizon distances for an ultra-compact binary system with components mass 102M and 1M are 40 Mpc and 1.89 Gpc, respectively, for ET, and 125 Mpc and 5.8 Gpc, respectively, for CE. Other cases are also presented in the text. We derive the merger rate and discuss consequences on the abundances of primordial black hole (PBH), fPBH. Considering the entire mass range [102–1]M, we find fPBH<0.70 (<0.06) for ET (CE), respectively. Full article
(This article belongs to the Special Issue New Frontiers in Cosmology and Astrophysics)
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