Gravitational and Electromagnetic Force Unification, Using a Statistical Analysis from a Signature of Supernova Explosions
Joseph Ngene Aniezi,
Gabriel Anene
Issue:
Volume 7, Issue 3, June 2019
Pages:
24-29
Received:
17 July 2019
Accepted:
23 August 2019
Published:
6 September 2019
Abstract: Unification of gravitational and electromagnetic interactions was done using statistical method. Cosmic ray intensity as a signature from supernova explosions was used to carry out some estimation. These primary cosmic rays are charged particles with an accelerating mechanism, probably electromagnetic; and because their charge is what interacts with matter and produces the effects that we can easily see here on earth. We estimated the values of the electromagnetic interaction and gravitational force of interaction of the source using previous known relations. We were able to obtain a regression equation; with a positive and strong correlation coefficient. Fa depicts the gravitational interaction and Umaa is the electromagnetic interaction. The results suggestively indicate that gravitational and electromagnetic interactions are related. The result indicates that moving charges and moving masses provide an analogy of gravitational and electromagnetic fields, which support the concept of a gravito-magnetic force. It has solved to some extend the speculations about the development in an attempt to unify the interactions of particles; and even to incorporate gravity in the “theory of everything”. Thus, the unification of forces using the explosion mechanism and gravitational waves in core-collapse supernovae has become a reality.
Abstract: Unification of gravitational and electromagnetic interactions was done using statistical method. Cosmic ray intensity as a signature from supernova explosions was used to carry out some estimation. These primary cosmic rays are charged particles with an accelerating mechanism, probably electromagnetic; and because their charge is what interacts wit...
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The Effect of Thermal Parameters on the Flow Temperature of a Magnetized Plasma in a Sphere
Tuduo Biepremene Sebastian,
Abbey Tamunoimi Michael,
Alagoa Kingsley D.,
Onwuneme Sylvester Ebere
Issue:
Volume 7, Issue 3, June 2019
Pages:
30-35
Received:
19 July 2019
Accepted:
29 August 2019
Published:
18 September 2019
Abstract: The effect of thermal parameters on the flow temperature of a magnetized plasma in a sphere was studied. The study models astrophysical environments such as the Sun, which have spherical outline. The governing equations of the problem were obtained based on the Navier-Stokes equations under the Boussinesq’s approximation. The solutions to the resulting equations were sought by means of the general perturbation method and the results were graphically represented with radial distance, r = 1.0 on the figures corresponding to the surface of the sphere. The thermal parameters; particularly, the radiation parameter, N2 and free convection parameter, Gr. were investigated in this study with a view to determine the effect of varying these parameters on the plasma flow temperature. Increasing both N2 and Gr. led to a decrease in the plasma flow temperature in the sphere. However, above the sphere (i.e. at radial distances, r >1.0) where the plasma density is sparse, increasing N2 and Gr. produced a corresponding increase in the plasma flow temperature. The decrease in the plasma flow temperature within the sphere with increase in the thermal parameters was observed to be more significant between radial distances, r = 0.25 and r = 0.7 (i.e., 0.25 ≤ r ≤ 0.7) than between r = 0.7 and r = 1.0 (i.e., 0.7 ≤ r ≤ 1.0). This is attributable to the prevalence of partially ionized heavy elements within 0.7 ≤ r ≤ 1.0 (corresponding to the convection zone of the solar interior) which trap the high energy photons thereby reducing the rate of radiative heat loss.
Abstract: The effect of thermal parameters on the flow temperature of a magnetized plasma in a sphere was studied. The study models astrophysical environments such as the Sun, which have spherical outline. The governing equations of the problem were obtained based on the Navier-Stokes equations under the Boussinesq’s approximation. The solutions to the resul...
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