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Universe, Volume 3, Issue 2

2017 June - 24 articles

Cover Story: Does the fine structure constant depend on gravitational potential? Hot white dwarf stars are the ideal probe for a relationship between the fine-structure constant and strong gravitational fields, providing us with a direct means of testing this important question. Potential variation manifests itself as shifts in the observed wavelengths of absorption lines when compared to laboratory wavelengths. A successful detection would be the first direct measurement of a gravitational field effect on a bare constant of nature. View the paper
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Articles (24)

  • Review
  • Open Access
6 Citations
5,513 Views
52 Pages

This review discusses confinement, as well as the topological and critical phenomena, in the gauge theories which provide the condensation of magnetic monopoles. These theories include the 3D SU(N) Georgi-Glashow model, the 4D [U(1)] N - 1 -...

  • Article
  • Open Access
52 Citations
5,483 Views
24 Pages

We analyze the time evolution of a spherically-symmetric collapsing matter from the point of view that black holes evaporate by nature. We consider conformal matters and solve the semi-classical Einstein equation G μ ν = 8 π G T μ ν ...

  • Conference Report
  • Open Access
4 Citations
3,925 Views
9 Pages

The observability of the multiverse is at the very root of its physical significance as a scientific proposal. In this conference we present, within the third quantization formalism, an interacting scheme between the wave functions of different unive...

  • Review
  • Open Access
106 Citations
9,269 Views
42 Pages

In the last four decades, different programs have been carried out aiming at understanding the final fate of gravitational collapse of massive bodies once some prescriptions for the behaviour of gravity in the strong field regime are provided. The ge...

  • Article
  • Open Access
19 Citations
3,844 Views
7 Pages

We briefly review the basics of Weyl geometry and its natural extension by a general linear ”distortion” of the metric connection by a vector field. A special class of the connections has torsion but retains the Weyl’s semi-metricity condition. We pr...

  • Conference Report
  • Open Access
1 Citations
4,346 Views
8 Pages

The main task of this review is to discuss quantum cosmology minisuperspace models based on the Wheeler–DeWitt equation, which apart from the standard matter and 3-geometry configuration degrees of freedom, allow those related to the variability of p...

  • Conference Report
  • Open Access
8 Citations
3,831 Views
9 Pages

Blind Spots for Direct Detection with Simplified DM Models and the LHC

  • Arghya Choudhury,
  • Kamila Kowalska,
  • Leszek Roszkowski,
  • Enrico Maria Sessolo and
  • Andrew J. Williams

Using the existing simplified model framework, we build several dark matter models which have suppressed spin-independent scattering cross section. We show that the scattering cross section can vanish due to interference effects with models obtained...

  • Article
  • Open Access
22 Citations
4,032 Views
20 Pages

We calculate explicitly the black-hole temperature for the Schwarzschild de-Sitter solution inside massive gravity by defining the Killing-vector in the direction of the Stückelberg function. We then consider the conditions which an observer in massi...

  • Conference Report
  • Open Access
24 Citations
4,618 Views
10 Pages

Two new high-precision measurements of the deuterium abundance from absorbers along the line of sight to the quasar PKS1937–1009 were presented. The absorbers have lower neutral hydrogen column densities (N(HI) ≈ 18 cm 2 ) than for previou...

  • Article
  • Open Access
12 Citations
4,898 Views
10 Pages

Mirror QCD and Cosmological Constant

  • Roman Pasechnik,
  • George Prokhorov and
  • Oleg Teryaev

An analog of Quantum Chromo Dynamics (QCD) sector known as mirror QCD (mQCD) can affect the cosmological evolution due to a non-trivial contribution to the Cosmological Constant analogous to that induced by the ground state in non-perturbative QCD. I...

  • Article
  • Open Access
3 Citations
5,123 Views
12 Pages

In this work, we present some results relating to the issue of the Loop Quantum Black Holes (LQBH) thermodynamics by the use of the tunneling radiation formalism. The information loss paradox is also discussed in this context, and we have considered...

  • Review
  • Open Access
181 Citations
8,151 Views
25 Pages

In this contribution, we discuss the cosmological scenario where unstable domain walls are formed in the early universe and their late-time annihilation produces a significant amount of gravitational waves. After describing cosmological constraints o...

  • Article
  • Open Access
14 Citations
3,969 Views
10 Pages

Lemaître Class Dark Energy Model for Relaxing Cosmological Constant

  • Irina Dymnikova,
  • Anna Dobosz and
  • Bożena Sołtysek

Cosmological constant corresponds to the maximally symmetric cosmological term with the equation of state p = ρ . Introducing a cosmological term with the reduced symmetry, p r = ρ in the spherically symmetric case, makes cosmolo...

  • Article
  • Open Access
2 Citations
4,306 Views
21 Pages

The Cosmic Causal Mass

  • Simen Braeck,
  • Øyvind G. Grøn and
  • Ivar Farup

In order to provide a better understanding of rotating universe models, and in particular the Gödel universe, we discuss the relationship between cosmic rotation and perfect inertial dragging. In this connection, the concept of causal mass is defined...

  • Article
  • Open Access
5 Citations
4,056 Views
10 Pages

In theories where a scalar field couples nonminimally to gravity, the effective gravitational “constant” becomes dependent on the value of the scalar field. This note first gives a brief review on how the cosmological evolution provides a dynamical s...

  • Conference Report
  • Open Access
5 Citations
6,137 Views
9 Pages

Quantum Cosmology of the Big Rip: Within GR and in a Modified Theory of Gravity

  • Mariam Bouhmadi-López,
  • Imanol Albarran and
  • Che-Yu Chen

Quantum gravity is the theory that is expected to successfully describe systems that are under strong gravitational effects while at the same time being of an extreme quantum nature. When this principle is applied to the universe as a whole, we use w...

  • Conference Report
  • Open Access
6 Citations
2,983 Views
6 Pages

We describe an alternative way to use future Baryon Acoustic Oscillation observations to perform non-mainstream research. We focus on the so-called Varying Speed of Light theories, in which the speed of light is made to vary in time. Using prescripti...

  • Article
  • Open Access
18 Citations
3,641 Views
9 Pages

We recently presented a new “artificial intelligence” method for the analysis of high-resolution absorption spectra (Bainbridge and Webb, Mon. Not. R. Astron. Soc. 2017, doi:10.1093/mnras/stx179). This new method unifies three established numerical m...

  • Review
  • Open Access
7 Citations
3,436 Views
8 Pages

A Review on the Cosmology of the de Sitter Horndeski Models

  • Nelson J. Nunes,
  • Prado Martín-Moruno and
  • Francisco S. N. Lobo

We review the most general scalar-tensor cosmological models with up to second-order derivatives in the field equations that have a fixed spatially flat de Sitter critical point independent of the material content or vacuum energy. This subclass of t...

  • Conference Report
  • Open Access
33 Citations
8,168 Views
6 Pages

Probing the Gravitational Dependence of the Fine-Structure Constant from Observations of White Dwarf Stars

  • Matthew B. Bainbridge,
  • Martin A. Barstow,
  • Nicole Reindl,
  • W.-Ü Lydia Tchang-Brillet,
  • Thomas R. Ayres,
  • John K. Webb,
  • John D. Barrow,
  • Jiting Hu,
  • Jay B. Holberg and
  • Julian C. Berengut
  • + 5 authors

Hot white dwarf stars are the ideal probe for a relationship between the fine-structure constant and strong gravitational fields, providing us with an opportunity for a direct observational test. We study a sample of hot white dwarf stars, combining...

  • Article
  • Open Access
12 Citations
4,108 Views
11 Pages

From Quantum to Cosmological Regime. The Role of Forcing and Exotic 4-Smoothness

  • Jerzy Król,
  • Torsten Asselmeyer-Maluga,
  • Krzysztof Bielas and
  • Paweł Klimasara

Recently, a cosmological model based on smooth open 4-manifolds admitting non-standard smoothness structures was proposed. The manifolds are exotic versions of R 4 and S 3 × R . The model has been developed further and proven to be c...

  • Conference Report
  • Open Access
3 Citations
3,238 Views
7 Pages

Dark Energy Constraints from Espresso Tests of the Stability of Fundamental Couplings

  • Ana C. O. Leite,
  • Carlos J. A. P. Martins and
  • Paolo Molaro

ESPRESSO is a high-resolution-ultra-stable spectrograph for the Very Large Telescope (VLT), whose commissioning will start in 2017. One of its key science goals is to test the stability of nature’s fundamental couplings with unprecedented accuracy an...

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Universe - ISSN 2218-1997