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Basing on the field theory of gravity and observable parameters of the expanding Universe the upper limit of $m_g \leq 4.5 . 10^{-66} g$. on the value of possible graviton mass is derived.

High Energy Physics - Theory · Physics 2016-09-06 S. S. Gershtein , A. A. Logunov , M. A. Mestvirishvili

It is noticed that the total relative density of mass in the Universe Omega_tot should exceed 1, i.e. Omega_tot=1+f^2/6 according to the field relativistic theory of gravity (RTG), which is free of the cosmological singularity and which…

Astrophysics · Physics 2009-11-07 S. S. Gershtein , A. A. Logunov , M. A. Mestvirishvili

We report new upper limits on any possible long-term time variation of the ratio of the electron to proton masses, $(m_e/m_p)$, the fine-structure constant, ($\alpha$), and the quantity $\alpha^2 g_p(m_e/m_p)$, where $g_p$ is the proton…

Astrophysics · Physics 2011-07-18 Lennox L. Cowie , Antoinette Songaila

Improved terrestrial experiment to test the equivalence principle for rotating extended bodies is presented, and a new upper limit for the violation of the equivalence principle is obtained at the level of 1.6$% \times 10^{\text{-7}}$,…

High Energy Physics - Phenomenology · Physics 2009-11-10 Z. B. Zhou , J. Luo , Q. Yan , Z. G. Wu , Y. Z. Zhang , Y. X. Nie

It is shown that using the relativistic field theory of gravity (RTG) and measured value of $\Omega_{tot}$ one can obtain the upper limit on the graviton mass with 95%C.L.: $m\leq 1.6\cdot 10^{-66}$ [g]; within the $(1\sigma)$ range its…

Astrophysics · Physics 2009-04-28 S. S. Gershtein , A. A. Logunov , M. A. Mestvirishvili , N. P. Tkachenko

White dwarfs are one of the densest form of matter following neutron star and black holes. A typical white dwarf is as massive as our sun has radius comparable to the earth. This paper reviewed the Fermi gas model Equation of State of white…

Solar and Stellar Astrophysics · Physics 2025-01-29 Tousif Raza

The maximum size of a cosmic structure is given by the maximum turnaround radius -- the scale where the attraction due to its mass is balanced by the repulsion due to dark energy. We derive generic formulae for the estimation of the maximum…

Cosmology and Nongalactic Astrophysics · Physics 2017-07-17 Sourav Bhattacharya , Konstantinos F. Dialektopoulos , Antonio Enea Romano , Constantinos Skordis , Theodore N. Tomaras

The top quark is by far the heaviest known fermion [1]. In consequence, experiment is just beginning to explore its properties, and some of them may yet prove to be distinctly non-standard. The very size of the top quark's mass even hints…

High Energy Physics - Phenomenology · Physics 2007-05-23 Elizabeth H. Simmons

The gravitational Bohr radius (GBR) characterizes the size of a hypothetical ground state hydrogen atom wherein the binding interaction between its nucleus and its electronic structure is purely gravitational. The conventional calculation…

General Physics · Physics 2008-03-11 R. L. Oldershaw

The greater part of this paper is concerned with a historical discussion of the development of the search for the origins of the highest-energy cosmic-rays together with a few remarks about future prospects. Additionally, in section 6, the…

Instrumentation and Methods for Astrophysics · Physics 2019-06-12 A A Watson

We present gravitation as a theory in which the coordinates are distances and velocities between galaxies. We show that there are three possibilities for the Universe to expand: decelerating, constant and accelerating, and it is shown that…

Astrophysics · Physics 2007-05-23 Moshe Carmeli

The Standard Model of particle physics contains about two dozen parameters - such as particle masses - whose origins are still unknown and cannot be predicted, but whose values are constrained through their interactions. In particular, the…

High Energy Physics - Experiment · Physics 2012-08-27 D0 Collaboration

Historically cosmic rays have always been at the intersection of astrophysics with particle physics. This is still and especially true in current days where experimenters routinely observe atmospheric showers from particles whose energies…

Astrophysics · Physics 2009-11-07 Guenter Sigl

It is shown that our knowledge of the mass composition of cosmic rays is deficient at all energies above 10^17 eV. Systematic differences between different measurements are discussed and, in particular, it is argued that there is no…

Astrophysics · Physics 2007-05-23 A. A. Watson

Our knowledge of the mass composition of cosmic rays is deficient at all energies above 10^17. Here systematic differences between different measurements are discussed and, in particular, it is argued that there is no compelling evidence to…

Astrophysics · Physics 2009-11-10 A. A. Watson

Recent detections of high-redshift absorption by both atomic hydrogen and molecular gas in the radio spectra of quasars have provided a powerful tool to measure possible temporal and spatial variations of physical `constants' in the…

Astrophysics · Physics 2009-10-30 M. J. Drinkwater , J. K. Webb , J. D. Barrow , V. V. Flambaum

Interpretation of the energy spectrum and arrival distribution of cosmic rays is complicated by lack of knowledge of the nature of the primaries. We review claims for the mass composition above 1017 eV where it can be determined only…

Astrophysics · Physics 2007-05-23 M. T. Dova , A. A. Watson , A. G. Mariazzi

We call attention to a simple analogy between atomic physics and cosmology. Both have two characteristic length scales. In atomic physics the lengths are the Compton wavelength of the electron and the Bohr radius; the ratio of these two…

General Relativity and Quantum Cosmology · Physics 2011-10-18 Ronald J. Adler

The bodies of snakes, such as king cobras, are very soft so that it is nearly impossible for them to raise their heads higher than around one meter. By direct measurement, we were only possible to hold the body of a freshly killed cobra…

Although cosmic rays were discovered 90 years ago, we do not know how and where they are accelerated. There is compelling evidence that the highest energy cosmic rays are extra-galactic -- they cannot be contained by our galaxy's magnetic…

Astrophysics · Physics 2009-11-07 F. Halzen
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