ADM formulation Initial Value Problem data per spacepoint

In summary, an ADM (Arnowitt-Deser-Misner) formulation is a mathematical framework used to describe the evolution of spacetime in General Relativity, specifically for an initial value problem. It differs from a Cauchy formulation in that it uses a 3+1 split of spacetime and makes use of data per spacepoint. However, using an ADM formulation can be challenging due to computational expenses and the importance of carefully selecting initial conditions. Furthermore, it is only applicable to systems described by General Relativity and may not be accurate for other types of systems.
  • #1
TerryW
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Homework Statement
See attached screenshot of MTW pp 532/533
Relevant Equations
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I'm having a bit of trouble getting a clear picture of what is going on here, so if anyone can shed any light, it will be greatly appreciated.

1. I can see how the metric coefficients provide the six numbers per spacepoint, but it can't always be possible to transform the metric into a diagonal form can it?

2. The forward motion in time demands one number per spacepoint, which I assume is the value ##\bar t##. How is this 'already willy-nilly' present in the three data per spacepoint? Is it because the various ##g_{ij}## are functions of t, x, y and z so knowing a ##g_{ij}## and its co-ordinates, t follows?

4. Why 'In conclusion...' do we now have TWO data per spacepoint telling us about the ##^{(4)}\mathcal G## and what are they?

5. What has happened to the six ##\frac {\partial g_{ij}}{\partial t} ##?

Regards
TerryW
 

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  • #2
1. It is not always possible to transform the metric into a diagonal form, as there are some metrics that are already in a diagonal form and some which are not. However, the metric coefficients can still provide the six numbers per space point. 2. The forward motion in time is already present in the three data per spacepoint, as each of the metric coefficients is a function of t, x, y and z. Knowing the values of the metric coefficients and their associated coordinates will allow you to work out the value of t. 4. In conclusion, we now have two data per spacepoint telling us about the ##^{(4)}\mathcal G## - these are the metric coefficients and their associated coordinates.5. The six ##\frac {\partial g_{ij}}{\partial t} ## are still present, but they are now implicit in the two data per spacepoint - each of the coordinates and the associated metric coefficients can be used to calculate the partial derivatives.
 

What is an ADM formulation?

An ADM (Arnowitt-Deser-Misner) formulation is a mathematical framework for describing the dynamics of spacetime in general relativity. It breaks down the spacetime into a set of spatial hypersurfaces, and describes the evolution of these hypersurfaces over time.

What is an Initial Value Problem (IVP)?

An Initial Value Problem is a type of mathematical problem where the solution is determined by specifying the values of the unknown function at a single point in the domain. In the context of ADM formulation, it refers to specifying the initial conditions for the hypersurfaces at a given time.

What is data per spacepoint in ADM formulation?

Data per spacepoint refers to the values of the physical quantities (such as energy, momentum, and curvature) at each point on the spatial hypersurface. In ADM formulation, these data are used to determine the evolution of the hypersurfaces over time.

What is the role of spacepoints in ADM formulation?

Spacepoints play a crucial role in ADM formulation as they represent the spatial coordinates on the hypersurfaces. These points are used to define the metric (spacetime geometry) and other physical quantities at each point on the hypersurface.

Why is ADM formulation important in general relativity?

ADM formulation is important in general relativity because it provides a mathematical framework for describing the dynamics of spacetime. It allows us to solve complex problems involving the evolution of spacetime, such as the study of black holes, gravitational waves, and the early universe.

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