Section 2: Pi-Shells and Their Properties

Section 2      Pi-Shells and their properties

2.1       Overview

2.2       The Emergence of Observable Pi-Shells

2.3       What is Pi-Space?

2.4       What is Space Time then?

2.5       The Square Rule

2.6       Understanding the Properties of a Pi-Shell

2.7       The Pi-Space Laws

2.8       The importance of the Observer in a relative system

2.9       Velocity and the Observerâ??s Pi-Shell

2.10     Newtonian velocity and the Pi-Shell Diameter Line

2.11     Different Observer diameters and the need for Einsteinâ??s SR work

2.12     Einsteinâ??s Addition and Subtraction of Relative Velocities

2.13     More on the Square Rule and Defining Euclidean Space

2.14     Pi-Shell addition and Geometric Relationships

2.15     The Importance of Pythagorasâ?? Theorem

2.16     Lorentzâ??s Application of Pythagorasâ?? Theorem

2.17     Solving for Pi-Shell time

2.18     Solving for Pi-Shell unit of length

2.19     Solving for Pi-Shell mass

2.20     Calculating the distance a Pi-Shell has traveled with a constant velocity

2.21     Pi-Shells and Newtonian Acceleration

2.22     Newtonian Acceleration and the Average Velocity

2.23     Understanding E=MC²

2.24     Newtonian Kinetic Energy

2.25     Einstein Relativistic Kinetic Energy

2.26     Relative Momentum and its utility

2.27     Measuring the Energy of a Photon

2.28     The Pi-Shell Unit of Velocity and the Wavelength λ

2.29     Where does Pi-Shell momentum ultimately come from in a Pi-Shell?

2.30     Minkowski and the Invariance of the Interval

2.31     Relating Space Time Diagrams to Pi-Shells

2.32     Explaining the SR Paradoxes in Pi-Space