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We consider gravitational collapse of a spherically symmetric sphere of a fluid with spin and torsion into a black hole. We use the Tolman metric and the Einstein$-$Cartan field equations with a relativistic spin fluid as a source. We show…

广义相对论与量子宇宙学 · 物理学 2026-03-24 Nikodem Popławski

We consider gravitational collapse of a fluid sphere with torsion generated by spin, which forms a black hole. We use the Tolman metric and the Einstein$-$Cartan field equations with a relativistic spin fluid as a source. We show that…

广义相对论与量子宇宙学 · 物理学 2025-11-21 Nikodem Popławski

We consider gravitational collapse of a sphere of a fluid with torsion generated by spin, which forms a black hole. We use the Tolman metric and the Einstein$-$Cartan field equations with a relativistic spin fluid as a source. We show that…

广义相对论与量子宇宙学 · 物理学 2023-09-22 Nikodem Popławski

We propose a modified form of the spontaneous birth of the universe by quantum tunneling. It proceeds through topology change and inflation, to eventually become a universe with closed spatial sections of negative curvature and nontrivial…

广义相对论与量子宇宙学 · 物理学 2007-05-23 S. S. e Costa , H. V. Fagundes

Matter collapsing to a singularity in a gravitational field is still an intriguing question. Similar situation arises when discussing the very early universe or a universe recollapsing to a singularity. It is suggested that inclusion of…

天体物理学 · 物理学 2011-07-04 C Sivaram , Kenath Arun , Venkata Manohara Reddy A

Creation of a black hole in quantum cosmology is the third way of black hole formation. In contrast to the gravitational collapse from a massive body in astrophysics or from the quantum fluctuation of matter fields in the very early…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Wu Zhong Chao

The expansion of our universe, when followed backward in time, implies that it emerged from a phase of huge density, the big bang. These stages are so extreme that classical general relativity combined with matter theories is not able to…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Martin Bojowald

Understanding gravitational collapse requires understanding how $\sim 10^{58}$ nucleons can be destroyed in $\sim 10^{-5}$ seconds. The recent proposal that the endpoint of gravitational collapse can be a "dark energy star" implies that the…

天体物理学 · 物理学 2009-11-13 George Chapline , Pawel O. Mazur

The creation of spacetimes with horizons is discussed, focussing on baby universes and black holes as examples. There is a complex interplay of quantum theory and General Relativity in both cases, leading to consequences for the future of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Tanmay Vachaspati

Quantum gravity has matured over the last decade to a theory which can tell in a precise and explicit way how cosmological singularities of general relativity are removed. A branch of the universe "before" the classical big bang is obtained…

天体物理学 · 物理学 2007-05-23 Martin Bojowald

We discuss the evolution of the universe in the context of the second law of thermodynamics from its early stages to the far future. Cosmological observations suggest that most matter and radiation will be absorbed by the cosmological…

广义相对论与量子宇宙学 · 物理学 2013-04-03 Andrew P. Lundgren , Ruxandra Bondarescu , Mihai Bondarescu

This short review is addressed to cosmologists. General relativity predicts that space-time comes to an end and physics comes to a halt at the big-bang. Recent developments in loop quantum cosmology have shown that these predictions cannot…

广义相对论与量子宇宙学 · 物理学 2011-01-25 Abhay Ashtekar

The process of quantum creation of a qusihomogeneous inflationary universe near a cosmological singularity is considered. It is shown that during the evolution quantum fluctuations of spatial topologies increase and the universe acquires…

广义相对论与量子宇宙学 · 物理学 2007-05-23 A. A. Kirillov

A scenario for a quantum big crunch to big bang transition is proposed. We first clarify the similarities between this transition and the final stages of black hole evaporation. The black hole and the universe are thought of as quantum…

高能物理 - 理论 · 物理学 2012-09-25 Ram Brustein , Maximilian Schmidt-Sommerfeld

Everybody knows what the classical black holes are. In short, this is a spacetime region beyond the so-called event horizon. The notion of the event horizon is mathematically well defined. The situation with a definition of quantum black…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Victor Berezin

This article reviews classical and quantum aspects of critical phenomena in gravitational collapse. We pay special attention to the origin of the scaling law for black hole mass, and to phase transitions in which black hole formation turns…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Patrick R Brady , Mike J Cai

We discuss the essential features of baby-universe production, starting from a description of black holes and wormholes, in terms of the causal structure of spacetime, and following a qualitative review of the connection between vacuum…

广义相对论与量子宇宙学 · 物理学 2018-09-24 S. Ansoldi , Z. Merali , E. I. Guendelman

Assuming that Quantum Mechanics is universal and that it can be applied over all scales, then the Universe is allowed to be in a quantum superposition of states, where each of them can correspond to a different space-time geometry. How can…

广义相对论与量子宇宙学 · 物理学 2024-02-27 José Luis Gaona-Reyes , Lucía Menéndez-Pidal , Mir Faizal , Matteo Carlesso

The Universe may pass through an effectively matter-dominated epoch between inflation and Big Bang Nucleosynthesis during which gravitationally bound structures can form on subhorizon scales. In particular, the inflaton field can collapse…

宇宙学与河外天体物理 · 物理学 2022-01-14 Benedikt Eggemeier , Bodo Schwabe , Jens C. Niemeyer , Richard Easther

Quantum gravity, as a fundamental theory of space-time, is expected to reveal how the universe may have started, perhaps during or before an inflationary epoch. It may then leave a potentially observable (but probably minuscule) trace in…

广义相对论与量子宇宙学 · 物理学 2015-12-17 Martin Bojowald
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