Difference between revisions of "Pressure Calculation of a Constant Density Star in the Dynamic Theory of Gravity"
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[[Category:Scientific Paper|pressure calculation constant density star dynamic theory gravity]] | [[Category:Scientific Paper|pressure calculation constant density star dynamic theory gravity]] | ||
− | [[Category:Gravity]] | + | [[Category:Gravity|pressure calculation constant density star dynamic theory gravity]] |
− | [[Category:Relativity]] | + | [[Category:Relativity|pressure calculation constant density star dynamic theory gravity]] |
− | [[Category:Cosmology]] | + | [[Category:Cosmology|pressure calculation constant density star dynamic theory gravity]] |
Latest revision as of 19:50, 1 January 2017
Scientific Paper | |
---|---|
Title | Pressure Calculation of a Constant Density Star in the Dynamic Theory of Gravity |
Read in full | Link to paper |
Author(s) | Ioannis Iraklis Haranas |
Keywords | Dynamic theory of gravity, gauge fields, Weyl?s quantum principle, field equtions, Christoffel symbols, energy-momentum tensor. |
Published | 2005 |
No. of pages | 10 |
Read the full paper here
Abstract
In a new theory called Dynamic Theory of Gravity, the gravitational potential is is derived from gauge relations and has a different form than the classical Newtonian potential. In the same theory an analytical expression for the pressure is derived from the equation of the hydrodynamic equilibrium which is solved for a star of constant density and the results are compared with those of Newtonian gravity. Changes then in the central pressure and radius are also calculated and finally a redshift calculation is performed so that the dynamic gravity effects if any might be shown to be of some detectable magnitude.