Geodesics using 2 Variables: Time & Radius from Mass

In summary, according to this video, an object will move along a geodesic on a curved surface if it is in a free fall. The geodesic always deviates towards the "more stretched" proper time, or towards greater gravitational time dilation.
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kairama15
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TL;DR Summary
Any object will move through spacetime along its geodesic. Since mass bends spacetime, an object initially at rest near the mass will move towards the mass along a geodesic. It would be useful to simplify the multidimensional nature of general relativity to help visualize how mass bends spacetime. We could use just 3 dimensions rather than all dimensions involved to help visualize how an object would move towards another heavy mass.
*Moving this thread from 'General Math Forum' to 'General Relativity Forum' in order to generate more discussion.*

Any object will move through spacetime along its geodesic. Since mass bends spacetime, an object initially at rest near the mass will move towards the mass along a geodesic. It would be useful to simplify the multidimensional nature of general relativity to help visualize how mass bends spacetime. We could use just 3 dimensions rather than all dimensions involved to help visualize how an object would move towards another heavy mass (as long as we only care about time, the distance from the heavy mass, and ignore the other angular components that aren't needed in a simple model).

There is a video on Youtube called Beauty of Geodesics

that visualizes how objects move along geodesics on a curved 3 dimensional surface. It may be very useful to visualize the 3 dimensional surface of the Schwarzschild metric like this to "see" how an object moves through curved spacetime generated by a mass.

A strategy would be to turn the line element of spacetime into a 3d graph. There are line elements of 3 dimensional surfaces like:

For the graph of a sphere: z=sqrt(r^2-x^2-y^2), there is a line element: ds^2=dr^2+r^2*dΘ+r^2*sinΘ*dΦ.

For the graph z=x+y, there is a line element: ds^2=dx^2+dy^2+dz^2. It's just the line element for a plane.

Is there a similar 3d graph that is associated with the Schwartzchild metric? The Schwartzchild metric is dτ^2= (1-2*G*M/(c^2*r))*dt^2 - (1-2*G*M/(c^2*r))*dr^2/c^2 (assuming dΘ and dΦ are not changing and are equal to 0). The 3d graph would be a function of r and t and its third coordinate would be τ.

...So instead of some 3d graph like z=x+y, we would get some 3d graph τ as a function of r and t. As long as we keep dΘ and dΦ equal to 0, the graph would be 3 dimensional.

So if there are 3d graphs associated with line elements for planes and spheres, is there a 3d graph associated with the Schwartzchild line element for space time τ? It would be quite beautiful to try to program a geodesic video of how a mass moves along a 3d surface of curved spacetime. I envision a stationary object next to the mass moving initially only along the t dimension, then slowly curving towards the mass as its geodesic along t and r changes.

We can't easily visualize how something moves through spacetime in 5 dimensions (spacetime,r,t,theta,phi), but we can visualize how something moves through spacetime in 3 dimensions (spacetime,r,t). Like an object initially at rest (r=ro) and only traveling along the time coordinate; and allowing the spacetime to curve it towards r=0 as r and t change on a 3 dimensional graph's geodesic.
 
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kairama15 said:
So if there are 3d graphs associated with line elements for planes and spheres, is there a 3d graph associated with the Schwartzchild line element for space time τ? It would be quite beautiful to try to program a geodesic video of how a mass moves along a 3d surface of curved spacetime. I envision a stationary object next to the mass moving initially only along the t dimension, then slowly curving towards the mass as its geodesic along t and r changes.
Here is a video for the local approximation (radial)space + time:

On the global scale spacetime is intrinsically curved (as shown below). It cannot be rolled out like the cone in the video above, which approximates just a small radial range:

gravity_global_small-png.png


The red path is the geodesic world-line of a free falling object, that oscillates through a tunnel through a spherical mass. Note that the geodesic always deviates towards the "more stretched" proper time, or towards greater gravitational time dilation. Gravitational time dilation has an extreme point at the center of the mass (gradient is zero), so there is no gravity there (but the maximal gravitational time dilation).

There is an interactive Flash version of that here (note that Flash is blocked by default by modern browsers):
http://www.adamtoons.de/physics/relativity.html

See also:
http://www.relativitet.se/Webtheses/tes.pdf
And other papers by Jonsson:
http://www.relativitet.se/articles.html
 
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FAQ: Geodesics using 2 Variables: Time & Radius from Mass

1. What is a geodesic?

A geodesic is the shortest path between two points on a curved surface, such as a planet or a black hole. It is the equivalent of a straight line on a flat surface.

2. How are geodesics calculated using 2 variables?

Geodesics are calculated using the principles of differential geometry, specifically the equations of geodesic deviation. This involves using the curvature of the surface and the acceleration of an object to determine the shortest path between two points.

3. What are the 2 variables used in geodesic calculations?

The 2 variables used in geodesic calculations are time and radius from mass. Time is used to track the movement of an object along the geodesic, while radius from mass takes into account the gravitational pull of the mass on the object.

4. How does the mass of an object affect the geodesic?

The mass of an object affects the geodesic by creating a curvature in the space-time fabric. This curvature determines the path an object will take, as objects will naturally follow the shortest path on a curved surface.

5. Why are geodesics important in physics?

Geodesics are important in physics because they help us understand the behavior of objects moving in curved space-time. They are used in theories such as general relativity to explain the effects of gravity and the motion of celestial bodies. They also have practical applications in fields such as navigation and satellite communication.

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