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Model of Expansive Nondecelerative Universe (ENU) due to involving Vaidya metric makes it possible to localize the energy density of gravitational field. This its capability allows for answering several open questions and supporting (or…

综合物理 · 物理学 2007-05-23 Miroslav Sukenik , Jozef Sima

Introduction of Vaidya metrics into the Expansive Nondecelerative Universe model allows to localize the energy of gravitational field. On the assumption that there is an interaction of long-range gravitational and electromagnetic fields,…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Miroslav Sukenik , Jozef Sima , Julius Vanko

Incorporation of the Vaidya metric in the model of Expansive Nondecelerative Universe allows to precisely localize gravitational energy for weak fields and obtain the components of the Einstein energy-momentum pseudotensor for strong…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Miroslav Sukenik , Jozef Sima

Vaidya metric as an integral part of the Expansive Nondecelerative Universe (ENU) model enables to localize the energy of gravitational field and, subsequently, to find a deep interrelationship between quantum mechanics and the general…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Jozef Sima , Miroslav Sukenik

It is shown that the gravity acceleration just above a chamber filled with gas or plasma at ultra-low pressure can be strongly reduced by applying an Extra Low-Frequency (ELF) electromagnetic field across the gas or the plasma. This…

综合物理 · 物理学 2013-12-03 Fran De Aquino

The contribution provides the starting points and background of the model of Expansive Nondecelerative Universe (ENU), manifests the advantage of exploitation of Vaidya metrics for the localization and quantization of gravitational energy,…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Jozef Sima , Miroslav Sukenik , Julius Vanko

Owing to Vaidya metric including, the model of Expansive Nondecelerative Universe (ENU) is able to localize gravitational energy. Based on the quantification of gravitational field of the Earth, ENU allows to rationalize and quantify the…

综合物理 · 物理学 2007-05-23 Miroslav Sukenik , Jozef Sima

In the expansive nondecelerative universe model, creation of matter occurs due to which the Vaidya metrics is applied. This fact allows for localizing gravitational energy and calculating the energy of gravitational waves using an approach…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Miroslav Sukenik , Jozef Sima

The model of Expansive Nondecelerative Universe exploiting the Vaidya metrics is used as a tool for unification of gravitation and strong interactions. The proposed approach stems from the capability to localize the energy of gravitational…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Miroslav Sukenik , Jozef Sima

Applying the Vaidya metrics in the model of Expansive Nondecelerative Universe (ENU) leads to compatibility of the ENU model both with the classic Newton gravitational theory and the general theory of relativity in weak fields

广义相对论与量子宇宙学 · 物理学 2007-05-23 Miroslav Sukenik , Jozef Sima , Julius Vanko

In the weak field limit general relativity reduces, as is well known, to the Newtonian gravitation. Alternative theories of gravity, however, do not necessarily reduce to Newtonian gravitation; some of them, for example, reduce to…

星系天体物理 · 物理学 2014-11-20 C. S. S. Brandao , J. C. N. de Araujo

We consider quantum mechanical effects of the modified Newtonian potential in the presence of extra compactified dimensions. We develop a method to solve the resulting Schroedinger equation and determine the energy shifts caused by the…

高能物理 - 唯象学 · 物理学 2011-06-27 E. G. Floratos , G. K. Leontaris , N. D. Vlachos

In a previous paper, the authors with Ann Nelson proposed that the UV and IR applicability of effective quantum field theories should be constrained by requiring that strong gravitational effects are nowhere encountered in a theory's domain…

高能物理 - 唯象学 · 物理学 2021-03-09 Andrew G. Cohen , David B. Kaplan

Alternative theories of gravity may serve to overcame several shortcomings of the standard cosmological model but, in their weak field limit, General Relativity must be recovered so as to match the tight constraints at the Solar System…

广义相对论与量子宇宙学 · 物理学 2018-06-06 Mariafelicia De Laurentis , Ivan De Martino , Ruth Lazkoz

The paper summarizes the background of Expensive Nondecelerative Universe model and its main consequences for gravitation. Applying the Vaidya metrics, the model allows for the localization and determination of the density and quantity of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Jozef Sima , Miroslav Sukenik

Since the Newtonian gravitation is largely used to model with success the structures of the universe, such as galaxies and clusters of galaxies, for example, a way to probe and constrain alternative theories, in the weak field limit, is to…

宇宙学与河外天体物理 · 物理学 2014-11-20 C. S. S. Brandao , J. C. N. de Araujo

According to the weak form of Einstein's general relativity equivalence principle, the gravitational and inertial masses are equivalent. However recent calculations (gr-qc/9910036) have revealed that they are correlated by an adimensional…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Fran De Aquino

We propose a quantum mechanical method of constraining non-Newtonian gravity at the nanometer range. In this method, a hybrid electro-optomechanical system is employed. Applying a strong driving field, we can obtain normal mode splitting of…

量子物理 · 物理学 2021-07-27 Lei Chen , Jian Liu , Ka-di Zhu

It was demonstrated (gr-qc/9910036) that the gravitational and inertial masses are correlated by an adimensional factor, which depends on the incident (or emitted)radiation upon the particle. There is a direct correlation between the…

综合物理 · 物理学 2010-06-11 Fran De Aquino

A second gradient generalization of Newtonian gravity is presented within the framework of gradient field theory. Weak nonlocality is introduced via first and second gradients of the gravitational field strength in the Lagrangian density.…

广义相对论与量子宇宙学 · 物理学 2020-12-02 Markus Lazar
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