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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

The conservation law for the angular momentum in curved spacetime, consistent with relativistic quantum mechanics, requires that the antisymmetric part of the affine connection (torsion tensor) is a variable in the principle of least…

广义相对论与量子宇宙学 · 物理学 2026-05-28 Nikodem Popławski

We show that the radial geodesic motion of a particle inside a black hole in isotropic coordinates (the Einstein-Rosen bridge) is physically different from the radial motion inside a Schwarzschild black hole. A particle enters the interior…

广义相对论与量子宇宙学 · 物理学 2009-01-21 Nikodem J. Poplawski

It is shown, using the Einstein-Cartan-Sciama-Kibble theory of gravity, that gravitational collapse of spin-fluid fermionic matter with a stiff equation of state in a black hole of mass $M$ forms a new universe of mass $\sim M_\ast=M^2…

宇宙学与河外天体物理 · 物理学 2011-03-24 Nikodem J. Poplawski

We analyze the dynamics of a homogeneous and isotropic universe in the Einstein$--$Cartan theory of gravity. The coupling between the spin and torsion prevents gravitational singularities and replaces the Big Bang with a nonsingular big…

广义相对论与量子宇宙学 · 物理学 2019-03-05 Gabriel Unger , Nikodem Popławski

A black universe is a nonsingular black hole where, beyond the horizon, there is an expanding, asymptotically isotropic universe. Such spherically symmetric configurations have been recently found as solutions to the Einstein equations with…

广义相对论与量子宇宙学 · 物理学 2010-03-19 K. A. Bronnikov , E. V. Donskoy

In a landscape of compactifications with different numbers of macroscopic dimensions, it is possible that our universe has nucleated from a vacuum where some of our four large dimensions were compact while other, now compact, directions…

高能物理 - 理论 · 物理学 2012-01-11 Julian Adamek , David Campo , Jens C. Niemeyer

We use the phenomenological approach to study properties of space-time in the vicinity of the Schwarzschild black-hole singularity. Requiring finiteness of the Schwarzschild-like metrics we come to the notion of integrable singularity that…

广义相对论与量子宇宙学 · 物理学 2013-01-24 Vladimir N. Lukash , Vladimir N. Strokov

If spacetime torsion couples to the intrinsic spin of matter according to the Einstein-Cartan-Sciama-Kibble theory of gravity, then the resulting gravitational repulsion at supranuclear densities prevents the formation of singularities in…

宇宙学与河外天体物理 · 物理学 2011-10-26 Nikodem J. Poplawski

If our universe was born as a baby universe on the other side of the event horizon of a black hole existing in a parent universe, then the corresponding white hole at rest provides the absolute frame of reference in the universe. In this…

科普物理 · 物理学 2025-06-02 Nikodem Popławski

We propose a mechanism for origin of matter in the universe in the framework of Einstein-Gauss-Bonnet gravity in higher dimensions. The recently discovered new static black hole solution by the authors \cite{md2006} with the Kaluza-Klein…

高能物理 - 理论 · 物理学 2008-11-26 Naresh Dadhich , Hideki Maeda

We address the question of universes inside a $\Lambda$ black hole which is described by a spherically symmetric globally regular solution to the Einstein equations with a variable cosmological term $\Lambda_{\mu\nu}$, asymptotically…

广义相对论与量子宇宙学 · 物理学 2009-11-07 I. G. Dymnikova , A. Dobosz , M. L. Fil'chenkov , A. Gromov

We study the `initial state' of an anisotropic universe in Eddington-inspired Born-Infeld gravity filled with a scalar field, whose potential has various forms. With this purpose, the evolution of a spatially-flat, homogeneous anisotropic…

广义相对论与量子宇宙学 · 物理学 2015-06-18 Hyeong-Chan Kim

We propose a simple scenario which explains why our Universe appears spatially flat, homogeneous and isotropic. We use the Einstein-Cartan-Kibble-Sciama (ECKS) theory of gravity which naturally extends general relativity to include the spin…

宇宙学与河外天体物理 · 物理学 2011-07-20 Nikodem J. Poplawski

We show that the Einstein-Cartan-Sciama-Kibble theory of gravity with torsion not only extends general relativity to account for the intrinsic spin of matter, but it may also eliminate major problems in gravitational physics and answer…

广义相对论与量子宇宙学 · 物理学 2016-10-25 Nikodem J. Poplawski

In the Einstein-Cartan-Sciama-Kibble theory of gravity, the intrinsic spin of fermionic matter generates spacetime torsion and induces gravitational repulsion at extremely high densities. This repulsion prevents the collapsing spin-fluid…

广义相对论与量子宇宙学 · 物理学 2011-08-09 Nikodem J. Poplawski

We give a comparative description of different types of regular static, spherically symmetric black holes (BHs) and discuss in more detail their particular type, which we suggest to call black universes. The latter have a Schwarzschild-like…

广义相对论与量子宇宙学 · 物理学 2008-11-26 K. A. Bronnikov , H. Dehnen , V. N. Melnikov

We analyze the dynamics of a homogeneous and isotropic universe in the Einstein--Cartan theory of gravity. The spin of fermions produces spacetime torsion that prevents gravitational singularities and replaces the big bang with a…

广义相对论与量子宇宙学 · 物理学 2019-12-30 Jordan L. Cubero , Nikodem J. Popławski
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