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&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&lt;br /&gt;
For people, who are unfamilar with GR, i will cover&lt;br /&gt;
the overall issue with this quick tutorial&lt;br /&gt;
&lt;br /&gt;
The orgins of GR curved space&lt;br /&gt;
----------------------------&lt;br /&gt;
In special theory of relativity, space-time interval&lt;br /&gt;
&lt;br /&gt;
ds^2 = (cdt)^2 - (dx^2 + dz^2 +dy^2)&lt;br /&gt;
&lt;br /&gt;
is constant independent of any frame. In his persuits&lt;br /&gt;
of theory of gravity, Einstien realized that&lt;br /&gt;
&lt;br /&gt;
ds^2 = (cdt)^2 - (dx^2 + dz^2 +dy^2) Equ(1)&lt;br /&gt;
&lt;br /&gt;
was inadequeate to cover gravity. Instead he turned&lt;br /&gt;
the boarder generalization of this formula&lt;br /&gt;
&lt;br /&gt;
ds^2 &amp;lt;code&amp;gt; g&amp;#039;&amp;#039;ab x^a x^b &amp;lt;/code&amp;gt; sum&amp;#039;&amp;#039;i sum&amp;#039;&amp;#039;j g&amp;#039;&amp;#039;ij x&amp;#039;&amp;#039;i x&amp;#039;&amp;#039;j&lt;br /&gt;
Equ(2)&lt;br /&gt;
&lt;br /&gt;
This formula is the heart of curved space geometry.&lt;br /&gt;
Unlike Equ(1), which has only contributions only from&lt;br /&gt;
dx^2,dy^2,dz^2, Equ(2) has contribution from dx*dy,&lt;br /&gt;
dz&amp;#039;&amp;#039;&amp;#039;dy, dy&amp;#039;&amp;#039;&amp;#039;dx, etc.&lt;br /&gt;
&lt;br /&gt;
g_ab is called a metric. Roughly speaking, its&lt;br /&gt;
components are used to compute length of the curve.&lt;br /&gt;
&lt;br /&gt;
In SR, observers disagree on dt,dx,dz,dy components in&lt;br /&gt;
different frames. However, they all agree on space&lt;br /&gt;
time interval ds^2. In GR, observers disagree on any&lt;br /&gt;
of the components of g_ab. However, they all agree&lt;br /&gt;
with the value of ds^2.&lt;br /&gt;
&lt;br /&gt;
------&lt;br /&gt;
Origins of Einstien&amp;#039;s Geodesic Equation&lt;br /&gt;
------&lt;br /&gt;
The geodesic equation can be derived from the&lt;br /&gt;
principle of least action and from the euler lagrange&lt;br /&gt;
equations. Here&amp;#039;s the summary of what these things&lt;br /&gt;
are, for the curious ones.&lt;br /&gt;
&lt;br /&gt;
The Lagragrain is defined as K.E - P.E. In classical&lt;br /&gt;
mechanics,&lt;br /&gt;
&lt;br /&gt;
L = 1/2 m (dx/dt) ^2 - V(x)&lt;br /&gt;
&lt;br /&gt;
Action S is defined as&lt;br /&gt;
&lt;br /&gt;
S &amp;lt;code&amp;gt; int_[[t&amp;lt;/code&amp;gt;a, t=b]] L dt&lt;br /&gt;
&lt;br /&gt;
According to principle of least action, the particle&lt;br /&gt;
will travel a path the minimizes L. From the&lt;br /&gt;
principle, you ger euler-lagrange equations.&lt;br /&gt;
&lt;br /&gt;
@L/@q - d/dt(@L/@p) = 0&lt;br /&gt;
&lt;br /&gt;
Here q is the generalized position coordinate and p is&lt;br /&gt;
the generalized momentum coordinate&lt;br /&gt;
&lt;br /&gt;
In our classical case, q &amp;lt;code&amp;gt; x, p &amp;lt;/code&amp;gt; dx/dt&lt;br /&gt;
&lt;br /&gt;
@L/@x = -@/@x V(x)&lt;br /&gt;
From @L/@p &amp;lt;code&amp;gt; m (dx/dt), d/dt( @L/@p) &amp;lt;/code&amp;gt; m d^2 x/dt^2&lt;br /&gt;
&lt;br /&gt;
m d^2 x/dt^2 = - @/@x V(x)&lt;br /&gt;
&lt;br /&gt;
This is Netwon&amp;#039;s famous 2nd law. This is naturally&lt;br /&gt;
derived from principle of least action.&lt;br /&gt;
&lt;br /&gt;
Einstien&amp;#039;s geodesic equation can be derived by&lt;br /&gt;
assuming&lt;br /&gt;
&lt;br /&gt;
L = sqrt( g&amp;#039;&amp;#039;ab d&amp;#039;&amp;#039;x^a /dlamda d_x^b/ dlamda )&lt;br /&gt;
&lt;br /&gt;
where lamda is some form of proper time&lt;br /&gt;
&lt;br /&gt;
In a way, g_ab are actually a measure of gravitional&lt;br /&gt;
potential and a body travels along a line of least&lt;br /&gt;
resistances. Moroever, a body travels along a path&lt;br /&gt;
that minimizes the metric g_ab.&lt;br /&gt;
&lt;br /&gt;
-----&lt;br /&gt;
Origins of the Field Equation&lt;br /&gt;
-----&lt;br /&gt;
&lt;br /&gt;
Guv = Ruv - (1/2)Rguv&lt;br /&gt;
&lt;br /&gt;
where R is the ricci tensor, R is the radius of&lt;br /&gt;
curvature and guv our metric.&lt;br /&gt;
&lt;br /&gt;
Although i wouldnt say i fully understand where this&lt;br /&gt;
comes from, Hilbert derived it also from the principle&lt;br /&gt;
of least action.&lt;br /&gt;
&lt;br /&gt;
Hilbert&amp;#039;s action = sqrt(-g)R&lt;br /&gt;
&lt;br /&gt;
where g is determinant of the metric matrix g_uv. Btw,&lt;br /&gt;
compare this to volume element of the Jacobian&lt;br /&gt;
transformations&lt;br /&gt;
&lt;/div&gt;</summary>
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