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相关论文: Building non commutative spacetimes at the Planck …

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We derive new space-time uncertainty relations (STUR) at the fundamental Planck length $L_P$ from quantum mechanics and general relativity (GR), both in flat and curved backgrounds. Contrary to claims present in the literature, our approach…

广义相对论与量子宇宙学 · 物理学 2011-03-02 Luca Tomassini , Stefano Viaggiu

We present Friedmann flat spacetime uncertainty relations (STUR) together with some cosmological implications. An interesting link between the Principle of "gravitational stability against localization of events" (PGSL) and the holographic…

广义相对论与量子宇宙学 · 物理学 2019-02-27 Stefano Viaggiu

We study the implications of the stringy space-time uncertainty relation (STUR) for inflationary cosmology. By demanding that no fluctuation modes that exit the Hubble radius are affected by the nonlocality resulting from the STUR, we find…

高能物理 - 理论 · 物理学 2024-01-09 Robert Brandenberger , Pei-Ming Ho , Hikaru Kawai , Wei-Hsiang Shao

We propose uncertainty relations for the different coordinates of spacetime events, motivated by Heisenberg's principle and by Einstein's theory of classical gravity. A model of Quantum Spacetime is then discussed where the commutation…

高能物理 - 理论 · 物理学 2015-06-26 Sergio Doplicher , Klaus Fredenhagen , John E. Roberts

Solutions of the Friedmann-Lemaitre cosmological equations of general relativity have been found with finite-time singularities that are everywhere regular, have regular Hubble expansion rate, and obey the strong-energy conditions but…

广义相对论与量子宇宙学 · 物理学 2016-11-15 John D. Barrow , S. Cotsakis , A. Tsokaros

Quantum effects are expected to modify the cosmological dynamics of the early universe while maintaining some (potentially discrete) notion of space-time structure. In one approach, loop quantum cosmology, current models are shown here to…

广义相对论与量子宇宙学 · 物理学 2026-04-29 Martin Bojowald , Manuel Diaz , Erick I. Duque

We study the potential effects of spacetime non-metricity in cosmology. In the spirit of Einstein-Cartan gravity, but with non-metricity replacing torsion, we consider the Einstein-Hilbert action and assume zero torsion. Adopting certain…

广义相对论与量子宇宙学 · 物理学 2023-03-29 Damianos Iosifidis , Ioannis Georgios Vogiatzis , Christos G. Tsagas

We consider Hilbert's sixth problem on the axiomatization of physics starting with a higher degree Heisenberg commutation relation involving the Dirac operator and the Feynman slash of scalar fields. The two sided version of the commutation…

高能物理 - 理论 · 物理学 2018-06-13 Ali H. Chamseddine

In this work quantum physics in noncommutative spacetime is developed. It is based on the work of Doplicher et al. which allows for time-space noncommutativity. The Moyal plane is treated in detail. In the context of noncommutative quantum…

高能物理 - 理论 · 物理学 2016-09-06 A. P. Balachandran , T. R. Govindarajan , C. Molina , P. Teotonio-Sobrinho

We locally classify all possible cosmological homogeneous and isotropic Landsberg-type Finsler structures, in 4-dimensions. Among them, we identify viable non-stationary Finsler spacetimes, i.e. those geometries leading to a physical causal…

We consider spatially homogeneous and isotropic cosmologies with non-zero torsion. Given the high symmetry of these universes, we adopt a specific form for the torsion tensor that preserves the homogeneity and isotropy of the spatial…

广义相对论与量子宇宙学 · 物理学 2019-05-01 D. Kranas , C. G. Tsagas , J. D. Barrow , D. Iosifidis

The phenomenologically observed flatness - or near flatness - of spacetime cannot be understood as emerging from continuum Planck (or sub-Planck) scales using known physics. Using dimensional arguments it is demonstrated that any…

广义相对论与量子宇宙学 · 物理学 2013-06-14 D. Bennett , H. B. Nielsen

It is well known that nonrelativistic quantum mechanics presents a clear asymmetry between space and time. Much of this asymmetry is attributed to the lack of Lorentz invariance of the theory. Nonetheless, a recent work [Phys. Rev. A…

量子物理 · 物理学 2017-12-12 Ricardo Ximenes , Eduardo O. Dias

We investigate the dynamics of the spatially flat universes submitted to isotropic tidal forces and adiabatic expansion under Einstein's equations. Surprisingly, the tendency to a high Hubble anisotropy at late times starts to appear as far…

广义相对论与量子宇宙学 · 物理学 2022-07-20 Fabio Scalco Dias , Leandro Gustavo Gomes , Luis Fernando Mello

We explore the possibilities of constructing bulk spacetimes in five dimensions for warped braneworld models with a spatially flat Friedmann-Robertson-Walker (FRW) line element on the 3-brane and with a time-dependent extra dimension. Our…

广义相对论与量子宇宙学 · 物理学 2009-11-06 Suman Ghosh , Sayan Kar

We consider flat Friedmann-Lema\^{\i}tre-Robertson-Walker cosmological models in the framework of general scalar-tensor theories of gravity with arbitrary coupling functions, set in the Jordan frame, in the cosmological epoch when the…

广义相对论与量子宇宙学 · 物理学 2015-06-03 Laur Järv , Piret Kuusk , Margus Saal

I give a summary review of the research program using noncommutative geometry as a framework to determine the structure of space-time. Classification of finite noncommutative spaces under few assumptions reveals why nature chose the…

高能物理 - 理论 · 物理学 2019-02-25 Ali H. Chamseddine

Together with collaborators, we introduced a noncommutative Riemannian geometry over Moyal algebras and systematically developed it for noncommutative spaces embedded in higher dimensions in the last few years. The theory was applied to…

高能物理 - 理论 · 物理学 2012-04-01 R. B. Zhang , Xiao Zhang

We study the quantum cosmology of a flat Friedmann-Lema\^{i}tre-Robertson-Walker universe filled with a (free) massless scalar field and a perfect fluid that represents radiation or a cosmological constant whose value is not fixed by the…

广义相对论与量子宇宙学 · 物理学 2020-10-01 Steffen Gielen , Lucía Menéndez-Pidal

We characterize the local instability of pressureless Friedmann spacetimes to radial perturbation at the Big Bang. The analysis is based on a formulation of the Einstein-Euler equations in self-similar variables $(t,\xi)$, with $\xi=r/t$,…

广义相对论与量子宇宙学 · 物理学 2025-10-17 Christopher Alexander , Blake Temple , Zeke Vogler
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