Einstein-scalar field action -> Einstein-scalar field equations

In summary, the conversation discusses the derivation of the Einstein-scalar field equations from the Einstein-scalar field action. This can be done by varying the action and requiring the functional to remain constant. The equations can also be derived by taking the functional with respect to the metric in [1,1] form. Familiarity with functionals is necessary for this derivation.
  • #1
bookworm_vn
9
0
Einstein-scalar field action --> Einstein-scalar field equations

Dear friends,

Just a small question I do not know how to derive.

From the Einstein-scalar field action defined by

[tex]S\left( {g,\psi } \right) = \int_{} {\left( {R(g) - \frac{1}{2}\left| {\nabla \psi } \right|_g^2 - V\left( \psi \right)} \right)d{\eta _g}}[/tex]

one gets the so-called Einstein-scalar field equations given by

[tex]{\rm Eins}_{\alpha \beta} = {\nabla _\alpha }\psi {\nabla _\beta }\psi - \frac{1}{2}{g_{\alpha \beta }}{\nabla _\mu }\psi {\nabla ^\mu }\psi - {g_{\alpha \beta }}V(\psi ).[/tex]

My question is how to derive such equations. It seems that we need to take derivative... but how? Thanks.
 
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  • #2


you will find this derivation in most test books on GR, you can derive it by varying
the action and requiring that the functional remain constant i.e that the functional is zero
are you familar with functionals? one must take the functional w.r.t the metric itself
it is actually easier to take the functional w.r.t the metric in [1,1] form, thus write the
other components in term of this
 

1. What is the Einstein-scalar field action?

The Einstein-scalar field action is a mathematical expression that describes the dynamics of a scalar field in the presence of gravity. It is a fundamental part of the Einstein-scalar field theory, which combines the principles of general relativity and quantum field theory.

2. How does the Einstein-scalar field action lead to the Einstein-scalar field equations?

The Einstein-scalar field equations are derived from the Einstein-scalar field action using the principle of least action. This principle states that the actual path that a system follows is the one that minimizes the action. By varying the action with respect to the scalar field and the metric tensor, we can obtain the equations that govern the behavior of the scalar field and the spacetime curvature.

3. What role does the scalar field play in the Einstein-scalar field equations?

The scalar field is a fundamental component of the Einstein-scalar field equations. It represents a quantum field that interacts with the gravitational field, and its energy density and pressure contribute to the overall curvature of spacetime. This allows for a more complete and unified understanding of the relationship between gravity and matter.

4. How do the Einstein-scalar field equations differ from the original Einstein field equations?

The original Einstein field equations describe the curvature of spacetime in the presence of matter and energy. The Einstein-scalar field equations, on the other hand, take into account the additional effects of a scalar field. This allows for a more comprehensive understanding of the dynamics of spacetime and the behavior of matter and energy within it.

5. What are the applications of the Einstein-scalar field equations?

The Einstein-scalar field equations have many applications in theoretical physics, particularly in the study of cosmology and the early universe. They have also been used in attempts to reconcile general relativity with quantum mechanics and to explore the behavior of black holes and other extreme astrophysical objects. Additionally, these equations have been used to make predictions about the structure and evolution of our universe.

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