Euclidean Relativity

July 9,2021

July 9,2021

Many texts on relativity often present it in a way that makes it seem unintuitive and difficult to visualize . However, we can easily formulate relativity in terms of ordinary Euclidean geometry.

An easy way to see this is by starting with the Minskowski approach and switching the roles of time and proper time to get \(t^2 = \tau^2 + x^2\) (using * natural units * \(c=1\)).
This means we now treat proper time as the 4th coordinate rather than common time. This approach is also sometimes referred to as * Proper Time Geometry * or * Circular Function Geometry *.
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My first article

December 14,2020

The following is an equation.

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December 14,2020

**Hello World**This is the test page for the blog.

The following is an equation.

$$R_{\mu\nu} - \frac12 g_{\mu\nu} R = \frac{8\pi G}{c^4} T_{\mu\nu}$$

The following is a TikZ picture:

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