Noncommutativity, Gravity and Cosmology

A special issue of Mathematics (ISSN 2227-7390). This special issue belongs to the section "Mathematical Physics".

Deadline for manuscript submissions: closed (30 April 2024) | Viewed by 1191

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Departamento de Física, Centro de Matemática e Aplicações (CMA-UBI), Universidade da Beira Interior, Rua Marquês d’Avila e Bolama, 6200-001 Covilhã, Portugal
Interests: general relativity; quantum field theory; gravitational physics; quantum mechanics; theoretical particle; physics; high energy physics
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Guest Editor
Departamento de Física, Centro de Matemática e Aplicações (CMA-UBI), Universidade da Beira Interior, Rua Marquês d’Avila e Bolama, 6200-001 Covilhã, Portugal
Interests: quantum cosmology; general relativity; mathematical physics; foundations of quantum mechanics
Special Issues, Collections and Topics in MDPI journals

Special Issue Information

Dear Colleagues,

Noncommutativity is a long-standing subject in mathematics and physics. The proposal of noncommutativity in spacetime was first put forward by Snyder. 

In addition, noncommutative field theory has also been established. Substantially further motivations for investigating the noncommutative proposals have arisen due to the advances in string and M-theory and interesting predictions made in particle physics such as predictions about the IR/UV mixing, non-locality, Lorentz violation and new physics at very short distance scales. 

Several noncommutative gravitational scenarios have been inspired by noncommutative field theory. Noncommutative cosmology is also an application of noncommutativity between fields. More specifically, noncommutative deformations modify the noncommutative fields, and the effects of non-commutative gravity could be determined by applying mini-superspace variables. 

Such procedures have been constructed by employing the Moyal product of functions in the Wheeler–DeWitt equation as well as the semiclassical approximation of quantum gravity. In addition, classical noncommutative models have been studied by modifying the Poisson brackets.

Noncommutative cosmological models have been employed to describe various aspects of the universe, such as inflation, dark energy and dark matter. As already mentioned, UV/IR mixing is one of the features of noncommutative field theories, by which short scales are effectively mixed with long scales. Therefore, the noncommutative effects could be seen in the current time of the Universe due to the presence of noncommutativity effects at small scale. In analogy to the usual quantum mechanics, the noncommutativity effects are usually related to a minimal size by a generalized uncertainty principle.

Any review and further developments of the noncommutative proposals mentioned above that are relevant to gravity and cosmology are the focus of this special issue and are welcome.

Dr. Seyed Meraj Mousavi Rasouli
Prof. Dr. Paulo Vargas Moniz
Guest Editors

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Keywords

  • noncommutative gravity/cosmology
  • noncommutative geometry
  • noncommutative quantum mechanics
  • Wheeler-DeWitt equation
  • Moyal product
  • semiclassical approximation of quantum gravity
  • noncommutative classical Poisson algebra
  • noncommutative minisuperspaces
  • minimal length

Published Papers (1 paper)

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Research

19 pages, 2044 KiB  
Article
Scalar Field Cosmology from a Modified Poisson Algebra
by Genly Leon, Alfredo D. Millano and Andronikos Paliathanasis
Mathematics 2023, 11(1), 120; https://doi.org/10.3390/math11010120 - 27 Dec 2022
Cited by 1 | Viewed by 818
Abstract
We investigate the phase space of a scalar field theory obtained by minisuperspace deformation. We consider quintessence or phantom scalar fields in the action that arises from minisuperspace deformation on the Einstein–Hilbert action. We use a modified Poisson algebra where Poisson brackets are [...] Read more.
We investigate the phase space of a scalar field theory obtained by minisuperspace deformation. We consider quintessence or phantom scalar fields in the action that arises from minisuperspace deformation on the Einstein–Hilbert action. We use a modified Poisson algebra where Poisson brackets are the α-deformed ones and are related to the Moyal–Weyl star product. We discuss early- and late-time attractors and reconstruct the cosmological evolution. We show that the model can have the ΛCDM model as a future attractor if we initially consider a massless scalar field without a cosmological constant term. Full article
(This article belongs to the Special Issue Noncommutativity, Gravity and Cosmology)
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