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The interactions between the spin of fermionic matter and torsion in the Einstein-Cartan-Sciama-Kibble (ECSK) theory of gravity provides a repulsive gravitational potential at the very dense states of fermionic matter, which prevents the…

综合物理 · 物理学 2021-10-27 Emre Dil

The Einstein-Cartan-Kibble-Sciama ({\sf ECKS}) theory of gravity naturally extends Einstein\rq{}s general relativity ({\sf GR}) to include intrinsic angular momentum (spin) of matter. The main feature of this theory consists of an algebraic…

广义相对论与量子宇宙学 · 物理学 2018-06-04 Hamid Shabani , Amir Hadi Ziaie

Compton wavelength and Schwarzschild radius are considered here as limiting cases of a unified length scale. Using this length, it is shown that the Dirac equation and the Einstein equations for a point mass are limiting cases of an…

广义相对论与量子宇宙学 · 物理学 2018-11-12 Swanand Khanapurkar , Tejinder P. Singh

We show that the electron in the Riemann-Cartan spacetime with extra dimensions has a finite size that is much larger than the experimental upper limit on its radius. Thus the Arkani-Hamed-Dimopoulos-Dvali and Randall-Sundrum models of the…

高能物理 - 理论 · 物理学 2010-01-26 Nikodem J. Poplawski

We study a complex Dirac field in the chiral representation minimally coupled to gravity in 3+1 dimensions in the context of Einstein-Cartan theory. Generically the matter content gravitates in two different ways: On the one hand, the…

广义相对论与量子宇宙学 · 物理学 2015-03-12 Adolfo Toloza

We consider the ESK theory, based on the principle for which the space is filled with matter fields in such a way that Cartan torsion is spin; in the geometry in which Cartan torsion tensor is completely antisymmetric, spin has to be…

广义相对论与量子宇宙学 · 物理学 2012-06-20 Luca Fabbri

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

Einstein-Cartan theory is an extension of the standard formulation of General Relativity where torsion (the antisymmetric part of the affine connection) is non-vanishing. Just as the space-time metric is sourced by the stress-energy tensor…

广义相对论与量子宇宙学 · 物理学 2019-12-30 Francisco Cabral , Francisco S. N. Lobo , Diego Rubiera-Garcia

There are various generalizations of Einstein's theory of gravity (GR); one of which is the Einstein-Cartan (EC) theory. It modifies the geometrical structure of manifold and relaxes the notion of affine connection being symmetric. The…

广义相对论与量子宇宙学 · 物理学 2018-04-04 Swanand Khanapurkar

We propose a simple mechanism that may explain the observed particle-antiparticle asymmetry in the Universe. In the Einstein-Cartan-Sciama-Kibble theory of gravity, the intrinsic spin of matter generates spacetime torsion. Classical Dirac…

高能物理 - 唯象学 · 物理学 2011-05-04 Nikodem J. Poplawski

We have recently proposed a new action principle for combining Einstein equations and the Dirac equation for a point mass. We used a length scale $L_{CS}$, dubbed the Compton-Schwarzschild length, to which the Compton wavelength and…

广义相对论与量子宇宙学 · 物理学 2018-03-16 Tejinder P. Singh

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

The Einstein-Cartan-Sciama-Kibble theory of gravity naturally extends general relativity to account for the intrinsic spin of matter. Spacetime torsion, generated by spin of Dirac fields, induces gravitational repulsion in fermionic matter…

宇宙学与河外天体物理 · 物理学 2012-09-03 Nikodem J. Poplawski

The conservation law for the orbital plus spin angular momentum of a free Dirac particle in curved spacetime requires that the affine connection has the antisymmetric part: the torsion tensor, which extends general relativity to the…

广义相对论与量子宇宙学 · 物理学 2026-04-28 Nikodem Popławski

The Einstein-Cartan-Sciama-Kibble theory of gravity removes the constraint of general relativity that the affine connection be symmetric by regarding its antisymmetric part, the torsion tensor, as a dynamical variable. The minimal coupling…

广义相对论与量子宇宙学 · 物理学 2012-07-06 Nikodem Poplawski

A stellar-mass compact object spiraling into a supermassive black hole, an extreme-mass-ratio inspiral (EMRI), is one of the targets of future gravitational-wave detectors and it offers a unique opportunity to test General Relativity (GR)…

广义相对论与量子宇宙学 · 物理学 2012-08-07 Nicolas Yunes , Paolo Pani , Vitor Cardoso

Einstein-Cartan theory is formulated in (1+2)-dimensions using the algebra of exterior differential forms. A Dirac spinor is coupled to gravity and the field equations are obtained by a variational principle. The space-time torsion is found…

广义相对论与量子宇宙学 · 物理学 2010-02-05 T. Dereli , N. Ozdemir , O. Sert

In this project, we try to find the correlation between the non-local pressure inside the massive neutron stars resisting the gravitational collapse of the core and ECSK dark energy led by the effect of spin-torsion coupling between quark…

综合物理 · 物理学 2020-12-03 Emre Dil

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

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
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