Exotic Scenarios for Compact Astrophysical Objects

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

Deadline for manuscript submissions: 31 December 2024 | Viewed by 1389

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Guest Editor
Institute of Experimental and Applied Physics, Czech Technical University, 11000 Prague, Czechia
Interests: the nature of dark matter; physics of neutron stars
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Guest Editor
Department of Nuclear and Elementaty Particle Physics, School of Physics, Faculty of Sciences, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
Interests: theoretical nuclear physics; nuclear astrophysics
Special Issues, Collections and Topics in MDPI journals

E-Mail Website
Guest Editor
Institute of Experimental and Applied Physics, Czech Technical University, 11000 Prague, Czechia
Interests: theoretical and experimental nuclear physics
Special Issues, Collections and Topics in MDPI journals

Special Issue Information

Dear Colleagues,

One of the most important problems of physics and astrophysics is the internal structure of compact objects, including neutron stars, boson stars, white dwarfs and compact dark objects as well. In particular, the internal structure of all the above became subject of a thorough study by researchers from different branches of physics including nuclear physics, astrophysics, particle physics, general relativity and thermodynamics. Problems such as a) the composition and properties of dense nuclear matter; b) the existence of exotic phases involving strangeness, such as hyperons, kaon or pion condensates, and deconfined quark matter; c) the possibility of dark matter being absorbed inside them; or even d) the existence of compact dark objects, all of them today are included in the researcher’s agenda. On the other hand, the accelerated improvement of the research, concerning the study of gravitational waves, has opened important perspectives to study the above theoretical predictions. We expect that in the near future, with the help of the detection of gravitational waves from events associated with compact objects (binary neutron star merger, various instability modes, etc.) and other observations including mainly the X-ray radiation and gamma-rays burst, the theoretical predictions and speculations will be able to be tested, providing us answers to some of the most fundamental problems of physics. The scope of the present Special Issue is to expose the above important problems and to highlight how they can be addressed both from the theoretical and observational point of view.

Dr. Vlasios Petousis
Dr. Charalampos Moustakidis
Dr. Martin Veselsky
Guest Editors

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Keywords

  • compacts objects
  • neutron stars
  • hybrid stars
  • strange quark stars
  • boson stars
  • white dwarfs
  • dark objects

Published Papers (1 paper)

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Research

12 pages, 563 KiB  
Article
Role of Quark Matter and Color Superconductivity in the Structure and Tidal Deformability of Strange Dwarfs
by Loïc Perot and Nicolas Chamel
Universe 2023, 9(9), 382; https://doi.org/10.3390/universe9090382 - 25 Aug 2023
Viewed by 878
Abstract
In 1995, Glendenning, Kettner and Weber postulated the existence of a new class of compact stars resembling white dwarfs but containing a small strange quark-matter core surrounded by hadronic layers attaining much higher densities than those found in white dwarfs. In our previous [...] Read more.
In 1995, Glendenning, Kettner and Weber postulated the existence of a new class of compact stars resembling white dwarfs but containing a small strange quark-matter core surrounded by hadronic layers attaining much higher densities than those found in white dwarfs. In our previous study, we have shown that it could be possible to unmask these so-called strange dwarfs through gravitational-wave observations with future space-based detectors such as the Laser Interferometer Space Antenna. We calculated more realistic equations of state for the hadronic envelope, but the quark core was treated using the simplest MIT bag model. In this paper, we investigate more closely the role of the possibly solid core in the structure and the tidal deformability of strange dwarfs in the full general relativistic framework by considering different models of strange quark matter in the crystalline color -superconducting phase. We find that the effect of the extreme rigidity of the elastic core on the tidal deformability is almost completely canceled by the surrounding hadronic layers. However, in all cases, the tidal deformability of strange dwarfs remains sufficiently lower than that of white dwarfs, to be potentially observable with gravitational waves despite the uncertainties in the strange quark-matter equation of state. Full article
(This article belongs to the Special Issue Exotic Scenarios for Compact Astrophysical Objects)
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