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相关论文: The no-defect conjecture in cosmic crystallography

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Under the hypothesis that the cosmological constant vanishes in the true ground state with lowest possible energy density, we argue that the observed small but finite vacuum-like energy density can be explained if we consider a theory with…

高能物理 - 理论 · 物理学 2009-11-07 Jun'ichi Yokoyama

It is shown that topological changes in space-time are necessary to make General Relativity compatible with the Newtonian limit and to solve the hierarchy of the fundamental interactions. We detail how topology and topological changes…

广义相对论与量子宇宙学 · 物理学 2012-12-10 M. D. Maia

We investigate a counterintuitive geometric interaction between defects and curvature in thin layers of superfluids, superconductors and liquid crystals deposited on curved surfaces. Each defect feels a geometric potential whose functional…

软凝聚态物质 · 物理学 2009-11-10 Vincenzo Vitelli , Ari Turner

We study the behaviour of a nonrelativistic quantum particle interacting with different potentials in the spacetimes of topological defects. We find the energy spectra and show how they differ from their free-space values.

量子物理 · 物理学 2007-05-23 Geusa de A. Marques , Valdir B. Bezerra

To provide a phenomenological theory for the various interesting transitions in restructuring networks we employ a statistical mechanical approach with detailed balance satisfied for the transitions between topological states. This enables…

统计力学 · 物理学 2007-05-23 Imre Derenyi , Illes Farkas , Gergely Palla , Tamas Vicsek

Despite our present-day inability to predict the topology of the universe it is expected that we should be able to detect it in the near future. A nontrivial detectable topology of the space section of the universe can be probed for all…

宇宙学与河外天体物理 · 物理学 2010-05-04 M. J. Reboucas , A. F. F. Teixeira

We propose a new cosmological paradigm in which our observed expanding phase is originated from an initially large contracting Universe that subsequently experienced a bounce. This category of models, being geodesically complete, is…

广义相对论与量子宇宙学 · 物理学 2008-11-07 Patrick Peter , Nelson Pinto-Neto

The idea that the cosmological term, Lambda, should be a time dependent quantity in cosmology is a most natural one. It is difficult to conceive an expanding universe with a strictly constant vacuum energy density, namely one that has…

宇宙学与河外天体物理 · 物理学 2015-03-18 Joan Sola

In this paper I discuss the formation of topological defects in quantum field theory and the relation between fractals and coherent states. The study of defect formation is particularly useful in the understanding of the same mathematical…

高能物理 - 理论 · 物理学 2008-08-22 Giuseppe Vitiello

A non-trivial spatial topology of the Universe is a potentially observable attribute, which can be probed through the circles-in-the-sky for all locally homogeneous and isotropic universes with no assumptions on the cosmological parameters.…

宇宙学与河外天体物理 · 物理学 2009-04-21 M. J. Reboucas

The relation between thermodynamic phase transitions in classical systems and topology changes in their state space is discussed for systems in which equivalence of statistical ensembles does not hold. As an example, the spherical model…

统计力学 · 物理学 2007-05-23 Michael Kastner

We investigate experimentally and numerically the defect configurations emerging when a cholesteric liquid crystal is confined to a spherical shell. We uncover a rich scenario of defect configurations, some of them non-existent in nematic…

软凝聚态物质 · 物理学 2017-09-13 Alexandre Darmon , Michael Benzaquen , Simon Čopar , Olivier Dauchot , Teresa Lopez-Leon

Topological defects are singularities in material fields that play a vital role across a range of systems: from cosmic microwave background polarization to superconductors, and biological materials. Although topological defects and their…

软凝聚态物质 · 物理学 2017-10-06 Luca Giomi , Žiga Kos , Miha Ravnik , Anupam Sengupta

Is the Universe (a spatial section thereof) finite or infinite? Knowing the global geometry of a Friedmann-Lema\^{\i}tre (FL) universe requires knowing both its curvature and its topology. A flat or hyperbolic (``open'') FL universe is {\em…

天体物理学 · 物理学 2009-10-31 Boudewijn F. Roukema

The recognition that the cosmological constant may be non-zero forces us to re-evaluate standard notions about the connection between geometry and the fate of our Universe. An open Universe can recollapse, and a closed Universe can expand…

天体物理学 · 物理学 2014-10-13 Lawrence M. Krauss , Michael S. Turner

Topological phases of matter are defined by their nontrivial patterns of ground-state quantum entanglement, which is irremovable so long as the excitation gap and the protecting symmetries, if any, are maintained. Recent studies on…

强关联电子 · 物理学 2019-03-25 Dominic V. Else , Hoi Chun Po , Haruki Watanabe

Topological defects are an essential part of the structure and dynamics of all liquid crystals, and they are particularly important in experiments and simulations on active liquid crystals. In a recent paper, Vromans and Giomi [Soft Matter,…

软凝聚态物质 · 物理学 2017-08-23 Xingzhou Tang , Jonathan V. Selinger

An old branch of mathematics, Topology, has opened the road to the discovery of new phases of matter. A hidden topology in the energy spectrum is the key for novel conducting/insulating properties of topological matter.

介观与纳米尺度物理 · 物理学 2016-07-06 Manuel Asorey

In the last decade, the study of the overall shape of the universe, called Cosmic Topology, has become testable by astronomical observations, especially the data from the Cosmic Microwave Background (hereafter CMB) obtained by WMAP and…

宇宙学与河外天体物理 · 物理学 2025-08-19 Jean-Pierre Luminet

What is the shape of the Universe? Is it finite or infinite ? Is space multi-connected to create ghost images of faraway cosmic sources? After a "dark age" period, the field of cosmic topology has now become one of the major concerns in…

宇宙学与河外天体物理 · 物理学 2015-06-17 Jean-Pierre Luminet