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For describing the non-negative gravitational energy-momentum in terms of a pure Bel-Robinson type energy-momentum in a quasilocal 2-surface, both the Bel-Robinson tensor $B$ and tensor $V$ are suitable. We found that this Bel-Robinson type…

广义相对论与量子宇宙学 · 物理学 2013-12-17 Lau Loi So

For describing the non-negative gravitational energy-momentum in terms of a pure Bel-Robinson `momentum' in a quasi-local small sphere limit, the Bel-Robinson tensor $B$ is desirable. However, we found this Bel-Robinson `momentum' can be…

广义相对论与量子宇宙学 · 物理学 2018-12-31 Lau Loi So

The Bel-Robinson tensor $B$ and the tensor $V$ have the same quasilocal energy-momentum in a small sphere. Using a pseudotensor approach to evaluate the energy-momentum in a half-cylinder, we find that $B$ and $V$ have different values, not…

广义相对论与量子宇宙学 · 物理学 2022-01-06 Lau Loi So

The purpose of the classical Einstein and Landau-Lifshitz pseudotensors is for determining the gravitational energy. Neither of them can guarantee a positive energy in holonomic frames. In the small sphere approximation, it has been…

广义相对论与量子宇宙学 · 物理学 2009-09-28 Lau Loi So

Describing the gravitational energy-momentum, the super-energy Bel-Robinson tensor is the best candidate. In the past, people seems only explore the lowest order: the electric part $E_{ab}$ and magnetic part $B_{ab}$ for the Riemann tensor.…

广义相对论与量子宇宙学 · 物理学 2023-12-29 Lau Loi So

The M$\o$ller tetrad gravitational energy-momentum expression was recently evaluated for a small vacuum region using orthonormal frames adapted to Riemann normal coordinates. However the result was not proportional to the Bel-Robinson…

广义相对论与量子宇宙学 · 物理学 2008-09-24 Lau Loi So

The Bel-Robinson tensor $B_{\alpha\beta\mu\nu}$ gives a positive definite gravitational energy in the quasilocal small sphere limit approximation. However, there is an alternative tensor $V_{\alpha\beta\mu\nu}$ that was proposed recently…

广义相对论与量子宇宙学 · 物理学 2010-06-29 Lau Loi So

Moller's tetrad gravitational energy-momentum "tensor" is evaluated for a small vacuum region using an orthonormal frame adapted to Riemann normal coordinates. We find that it does satisfy the highly desired property of being a positive…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Lau Loi So , James M. Nester

Deser et al. proposed a combination of the Einstein and Landau-Lifshitz pseudotensors such that the second derivatives in vacuum are proportional to the Bel-Robinson tensor. Stimulated by their work, the present paper discuss the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Lau Loi So

The gravitational energy-momentum within a small region as determined by two tetrad-teleparallel expressions is evaluated with the aid of an orthonormal frame adapted to Riemann normal coordinates. We find that the gauge current "tensor"…

广义相对论与量子宇宙学 · 物理学 2012-07-31 Lau Loi So , James M. Nester

The specification of energy for gravitating systems has been an unsettled issue since Einstein proposed his pseudotensor. It is now understood that energy-momentum is \emph{quasi-local} (associated with a closed 2-surface). Here we consider…

广义相对论与量子宇宙学 · 物理学 2018-11-15 Chiang-Mei Chen , Jian-Liang Liu , James M. Nester

We construct an infinite number of new holonomic quasi-local gravitational energy-momentum density pseudotensors with good limits asymptotically and in small regions, both materially and in vacuum. For small vacuum regions they are all a…

广义相对论与量子宇宙学 · 物理学 2010-04-14 Lau Loi So , James M. Nester

The Bel-Robinson tensor $B_{\alpha\beta\mu\nu}$ gives a positive definite gravitational energy in the small sphere limit approximation. However, there is an alternative tensor $V_{\alpha\beta\mu\nu}$ which was proposed recently that offers…

广义相对论与量子宇宙学 · 物理学 2009-02-02 Lau Loi So

In general relativity, the local gravitational energy is best characterised by the quasilocal mass. The small sphere limit of quasilocal mass provides us the most local notion of gravitational energy. In four dimensions, the limits were…

广义相对论与量子宇宙学 · 物理学 2019-09-27 Jinzhao Wang

Although the super-energy Bel-Robinson tensor gives a desirable gravitational energy-momentum in a small sphere region, the angular-momentum is vanishing. Intuitively, it should be non-zero. Our present work shows that indeed the angular…

广义相对论与量子宇宙学 · 物理学 2024-01-09 Lau Loi So

The field theoretical description of the general relativity (GR) is further developed. The action for the gravitational field and its sources is given explicitely. The equations of motion and the energy-momentum tensor for the gravitational…

广义相对论与量子宇宙学 · 物理学 2007-05-23 S. V. Babak , L. P. Grishchuk

Describing the gravitational energy and momentum, the Bel-Robinson tensor is the best tensor. However, the classical pseudotensors can also manage the the same job. As Deser mentioned in 1999, a certain linear combination between Einstein…

广义相对论与量子宇宙学 · 物理学 2022-12-29 Lau Loi So

A proposal for the gravitational energy-momentum tensor, known in the literature as the square root of Bel-Robinson tensor, is analyzed in detail. Being constructed exclusively from the Weyl part of the Riemann tensor, such tensor…

广义相对论与量子宇宙学 · 物理学 2018-03-16 Giovanni Acquaviva , David Kofroň , Martin Scholtz

We propose a gravitational energy-momentum tensor of the general relativity obtained using Noethers theorem. It transforms as a tensor under general coordinate transformations. One of the two indices of the gravitational energy-momentum…

广义相对论与量子宇宙学 · 物理学 2017-01-05 Katsutaro Shimizu

Several energy-momentum "tensors" of gravitational field are considered and compared in the lowest approximation. Each of them together with energy-momentum tensor of point-like particles satisfies the conservation laws when equations of…

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