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相关论文: An Approach for Modelling Tachyons with Gravitatio…

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Special theory of relativity has been formulated in a vacuum momentum-energy representation which is equivalent to Einstein special relativity and predicts just the same results as it. Although in this sense such a formulation would be at…

广义相对论与量子宇宙学 · 物理学 2007-05-23 P. F. Gonzalez-Diaz

Graviton pairing and destruction of these pairs under collisions with bodies may lead to the Newtonian attraction. It opens us a new way to a very-low-energy quantum gravity model. In the model by the author, cosmological redshifts are…

高能物理 - 理论 · 物理学 2007-05-23 Michael A. Ivanov

Axions and axion-like particles are ubiquitous in extensions of the Standard Model and offer a unifying framework for addressing open problems in cosmology. Depending on their mass and interactions, axions can act as dark matter, drive…

高能物理 - 唯象学 · 物理学 2026-05-01 Luca Visinelli

The model of creation of observable particles and particles of the dark matter, considered to be superheavy particles, due to particle creation by the gravitational field of the Friedmann model of the early Universe is given. Estimates on…

高能物理 - 唯象学 · 物理学 2009-10-31 A. A. Grib , Yu. V. Pavlov

A particular class of space-time, with a tachyon field, \phi, and a barotropic fluid constituting the matter content, is considered herein as a model for gravitational collapse. For simplicity, the tachyon potential is assumed to be of…

广义相对论与量子宇宙学 · 物理学 2013-01-23 Yaser Tavakoli , João Marto , Amir Hadi Ziaie , Paulo Vargas Moniz

Graviton-photon oscillation is the conversion of gravitational waves to electromagnetic waves and vice versa in the presence of a background electromagnetic field. We investigate this phenomenon in a cosmological scenario considering a…

广义相对论与量子宇宙学 · 物理学 2023-10-10 José A. R. Cembranos , Miguel González Ortiz , Prado Martín-Moruno

Within the thermodynamic model of gravity the dark energy is identified with the energy of collective gravitational interactions of all particles in the universe, which is missing in the standard treatments. For the model-universe we…

广义相对论与量子宇宙学 · 物理学 2014-12-01 Merab Gogberashvili

Tachyons are hypothetical particles that propagate faster than light, yet they have never been observed in nature or in the laboratory. In this work, we introduce the hydrogen molecule ion as an analogue for the dynamics of a spinless test…

广义相对论与量子宇宙学 · 物理学 2025-11-17 Davi de Moura Esposti Moreira , Matheus Elias Pereira , Alexandre Grezzi de Miranda Schmidt

In this paper a hypothesis is considered, in which neutrinos and other weakly interacting particles play a fundamental role in Universe. In addition the Newton gravitational constant $G_N$ and the Hubble constant $H$ are interpreted as…

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

In this work a tachyonization of the $\Lambda$CDM model for a spatially flat Friedmann-Robertson-Walker space-time is proposed. A tachyon field and a cosmological constant are considered as the sources of the gravitational field. Starting…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Luis P. Chimento , Mónica Forte , Gilberto M. Kremer , Marlos O. Ribas

In this paper I discuss whether superluminal particles exist in the general relativistic theory of gravity. It seems that the answer to this question is negative. In truth the result may only represent a difficulty to {\bf special} but not…

广义相对论与量子宇宙学 · 物理学 2013-06-18 Asher Yahalom

The apparent Lorentz invariance of the laws of physics does not imply that space-time is indeed minkowskian. We consider a scenario where Lorentz invariance is only an approximate property of equations of matter above a certain distance…

天体物理学 · 物理学 2008-02-03 Luis Gonzalez-Mestres

We study production of light particles due to oscillation of the Hubble parameter or the scale factor. Any coherently oscillating scalar field, irrespective of its energy fraction in the universe, imprints such an oscillating feature on…

高能物理 - 唯象学 · 物理学 2016-10-05 Yohei Ema , Ryusuke Jinno , Kyohei Mukaida , Kazunori Nakayama

It is shown by the author that if gravitons are super-strong interacting particles and the low-temperature graviton background exists, the basic cosmological conjecture about the Dopplerian nature of redshifts may be false. In this case, a…

高能物理 - 理论 · 物理学 2007-05-23 Michael A. Ivanov

The effects of physical interactions are usually incorporated into the quantum theory by including the corresponding terms in the Hamiltonian. Here we consider the effects of including the gravitational potential energy of massive particles…

高能物理 - 唯象学 · 物理学 2015-06-03 J. D. Franson

An analytical approach for studying the cosmological scenario with a homogeneous tachyon field within the framework of loop quantum gravity is developed. Our study is based on the semi-classical regime where space time can be approximated…

广义相对论与量子宇宙学 · 物理学 2009-11-11 A. A. Sen

We extend the systematic calculation of an approximately relativistic Hamiltonian for centre of mass and internal dynamics of an electromagnetically bound two-particle system by Sonnleitner and Barnett [1] to the case including a weak…

量子物理 · 物理学 2019-11-27 Philip K. Schwartz , Domenico Giulini

We revive the historically first dark matter model based on neutrinos, but with an additional assumption that neutrinos might exist in tachyonic almost sterile states. To this end, we propose a group-theoretical algorithm for the…

综合物理 · 物理学 2016-04-13 Maxim A. Makukov , Eduard G. Mychelkin , Vladimir L. Saveliev

We propose a gravitational theory in which the effective Lagrangian of the gravitational field is given by an arbitrary function of the Ricci scalar, the trace of the matter energy-momentum tensor, and the contraction of the Ricci tensor…

广义相对论与量子宇宙学 · 物理学 2014-12-30 Zahra Haghani , Tiberiu Harko , Hamid Reza Sepangi , Shahab Shahidi

The Einstein equations are non-linear and the particles of which the gravitational effect is described by these equations are lastly unknown. If renormalizable fields are assumed, then results are obtained only in the case of a at space.…

综合物理 · 物理学 2016-11-25 Alfred Kording