Cosmic String Theory and Observations

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

Deadline for manuscript submissions: closed (15 October 2021) | Viewed by 3698

Special Issue Editors


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Guest Editor
Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky pr., 13, Moscow 119234, Russia
Interests: general relativity; cosmology; mathematical data processing; cosmic strings

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Guest Editor
Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetsky pr., 13, Moscow 119234, Russia
Interests: astrophysics; cosmology; gravitation; cosmic strings; pulsar timing; gravitational waves; CMB anisotropy and polarization; astrometry

Special Issue Information

Dear Colleagues,

This Special Issue is dedicated to the latest research on cosmic strings, both theory and observations based on modern radio and optical instruments, as well as cosmic string simulations for future experiments.

The search for cosmic strings is one of the intriguing problems of modern astronomy, cosmology, and particle physics. The complexity of the cosmological scenario regarding cosmic strings remains an obstacle to our complete understanding. Cosmic strings are hypothetical one-dimensional objects at cosmological scales that, while predicted by the theory, have not yet been detected. Their “zoo” is quite rich. They can be purely topological entities (endless or infinite and closed loops), formed as a result of phase transitions in the vacuum stages of the expansion and cooling of the early Universe, or hybrid topological and field configurations (e.g., the “necklace”: a string with monopoles at its ends and collections of such elements). There is also the possibility of fundamental F- and D-strings of cosmological sizes, which could be generated during high-energy interactions of the extra dimensions in the early Universe.

The phenomenon of cosmic strings should be conducted simultaneously in theory and in observations. This Special Issue will present scientific results of cosmic string observational strategy with a comprehensive approach. For instance, one of the most promising approaches is simultaneous string search using both gravitational lensing methods (special chains of pairs of galaxies) and analysis of the CMB anisotropy (step-like structures). In order to process SDSS datasets, as well as WMAP and “Planck” radio maps, extremely innovative suggestions and research on effective mathematical methods for data filtering (using big data analysis and artificial intelligence based on neural networks) are required.

Prof. Dr. Olga S. Sazhina
Prof. Dr. Mikhail V. Sazhin
Guest Editors

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Keywords

  • cosmic string
  • gravitational lensing
  • CMB data
  • CMB anisotropy
  • data processing
  • big data analysis
  • SDSS datasets
  • string gravitational waves
  • superstring theory

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Published Papers (1 paper)

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Research

70 pages, 5422 KiB  
Article
Cosmological Spectrum of Two-Point Correlation Function from Vacuum Fluctuation of Stringy Axion Field in De Sitter Space: A Study of the Role of Quantum Entanglement
by Sayantan Choudhury and Sudhakar Panda
Universe 2020, 6(6), 79; https://doi.org/10.3390/universe6060079 - 5 Jun 2020
Cited by 14 | Viewed by 2960
Abstract
In this work, we study the impact of quantum entanglement on the two-point correlation function and the associated primordial power spectrum of mean square vacuum fluctuation in a bipartite quantum field theoretic system. The field theory that we consider is the effective theory [...] Read more.
In this work, we study the impact of quantum entanglement on the two-point correlation function and the associated primordial power spectrum of mean square vacuum fluctuation in a bipartite quantum field theoretic system. The field theory that we consider is the effective theory of axion field arising from Type IIB string theory compacted to four dimensions. We compute the expression for the power spectrum of vacuum fluctuation in three different approaches, namely (1) field operator expansion (FOE) technique with the quantum entangled state, (2) reduced density matrix (RDM) formalism with mixed quantum state and (3) the method of non-entangled state (NES). For a massless axion field, in all three formalisms, we reproduce, at the leading order, the exact scale invariant power spectrum which is well known in the literature. We observe that due to quantum entanglement, the sub-leading terms for these thee formalisms are different. Thus, such correction terms break the degeneracy among the analysis of the FOE, RDM and NES formalisms in the super-horizon limit. On the other hand, for massive axion field we get a slight deviation from scale invariance and exactly quantify the spectral tilt of the power spectrum in small scales. Apart from that, for massless and massive axion field, we find distinguishable features of the power spectrum for the FOE, RDM, and NES on the large scales, which is the result of quantum entanglement. We also find that such large-scale effects are comparable to or greater than the curvature radius of the de Sitter space. Most importantly, in near future if experiments probe for early universe phenomena, one can detect such small quantum effects. In such a scenario, it is possible to test the implications of quantum entanglement in primordial cosmology. Full article
(This article belongs to the Special Issue Cosmic String Theory and Observations)
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