Using Derivatives of Time's Flux with Respect to Space-time in Generalized Planck-Einstein Equation and de Broglie Wavelength Relations
POSTER
Abstract
In our vision, the nature of time is wavy-like motion of the matter and nature of space is jerky-like motion of the matter. These two natures can be matched on wave-particle duality of elementary particles [Gholibeigian, et.al. APS April Meeting 2016, abstract {\#}1.032]. On the other hand, it seems that the variation of time's flux (time's dimensions) arises from different geometries of extra dimensions of string which are in face-front of the string's motion. So, we propose to use derivatives of time's flux, $R=f(mv,\sigma ,\tau )$, with respect to the space-time for modification of the Generalized Planck-Einstein equation and de Broglie wavelength relations as follows: n.t_{p} \frac{\partial R}{\partial \tau }+P^{\mu }=n.t_{p} \frac{\partial R}{\partial \sigma }+\frac{h}{2\pi }K^{\mu } In which $\sigma \& \tau $ are coordinates on the string world sheet, respectively space and time along the string, $m$ is string's mass$, \quad v$ is velocity of string's motion$, \quad n$ factor \quad depends on geometry of each extra dimension \quad which is in face-front of the motion, and $t_{p} $ is Planck's time.
Authors
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Hassan Gholibeigian
No Company Provided
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Abdolazim Amirshahkarami
Retired
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Kazem Gholibeigian
Student