Extra (boundary?) term in Brans Dicke field equations

In summary, the paper discusses the implications of an extra boundary term in the Brans-Dicke field equations, which are used in scalar-tensor theories of gravity. It analyzes how this boundary term affects the dynamics of the gravitational field and the solutions to the equations, particularly in relation to the coupling between the scalar field and the curvature of spacetime. The authors explore the physical significance of this term and its potential impact on cosmological models and the interpretation of gravitational interactions.
  • #1
ergospherical
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Here is the action:
##S = \frac{1}{16\pi} \int d^4 x \sqrt{-g} (R\phi - \frac{\omega}{\phi} g^{ab} \phi_{,a} \phi_{,b} + 16\pi L_m)##
the ordinary matter is included via ##L_m##. Zeroing the variation ##\delta/\delta g^{\mu \nu}## in the usual way gives

##\frac{\delta}{\delta g^{\mu \nu}}[R\phi - \frac{\omega}{\phi} g^{ab} \phi_{,a} \phi_{,b}] + \frac{1}{\sqrt{-g}}(R\phi - \frac{\omega}{\phi} g^{ab} \phi_{,a} \phi_{,b}) \frac{\delta(\sqrt{-g})}{\delta g^{\mu \nu}} - 8\pi T_{\mu \nu} = 0##

where ##T_{\mu \nu} = \frac{-2}{\sqrt{-g}} \frac{\delta(\sqrt{-g}L_m)}{\delta g^{\mu \nu}}## is the stress energy of the matter. Inserting the variations of ##R## and ##\sqrt{-g}## (which are ##R_{\mu \nu}## and ##-\frac{1}{2} \sqrt{-g} g_{\mu \nu}## respectively) gives

##G_{\mu \nu} + \frac{\omega}{\phi^2}(\frac{1}{2}g^{ab} \phi_{,a} \phi_{,b} g_{\mu \nu} - \phi_{,\mu} \phi_{,\nu}) = 8\pi T_{\mu \nu}/\phi##

On Wikipedia (https://en.wikipedia.org/wiki/Brans–Dicke_theory#The_field_equations) there is another term ##\frac{1}{\phi}(\nabla_a \nabla_b \phi - g_{ab} \square \phi)##. I suspect it is a boundary term? Where did it come from.
 
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  • #2
ergospherical said:
I suspect it is a boundary term? Where did it come from.
Your suspicion is correct. By the Palatini identity, the general variation of the Ricci scalar is:$$\delta R=R_{\mu\nu}\delta g^{\mu\nu}+\nabla_{\sigma}\left(g^{\mu\nu}\delta\Gamma_{\mu\nu}^{\sigma}-g^{\mu\sigma}\delta\Gamma_{\lambda\mu}^{\lambda}\right)\tag{1}$$For the Einstein-Hilbert action, the last term on the right is dropped because it's a total divergence that integrates to an ignorable boundary term. But for the Brans-Dicke action, we multiply the full variation (1) by ##\phi## to get:$$\phi\delta R=\phi R_{\mu\nu}\delta g^{\mu\nu}+\phi\nabla_{\sigma}\left(g^{\mu\nu}\delta\Gamma_{\mu\nu}^{\sigma}-g^{\mu\sigma}\delta\Gamma_{\lambda\mu}^{\lambda}\right)$$$$=\phi R_{\mu\nu}\delta g^{\mu\nu}-\left(\nabla_{\sigma}\phi\right)\left(g^{\mu\nu}\delta\Gamma_{\mu\nu}^{\sigma}-g^{\mu\sigma}\delta\Gamma_{\lambda\mu}^{\lambda}\right)+\nabla_{\sigma}\left(\phi\left(g^{\mu\nu}\delta\Gamma_{\mu\nu}^{\sigma}-g^{\mu\sigma}\delta\Gamma_{\lambda\mu}^{\lambda}\right)\right)$$Again we ignore the last term as a divergence, but the second part is non-zero whenever ##\phi \neq \text{constant}##, and is responsible for the additional terms in the Brans-Dicke field-equations that involve second-derivatives of ##\phi##.
 
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Likes ergospherical
  • #3
Interesting - thank you.
 

FAQ: Extra (boundary?) term in Brans Dicke field equations

What is the extra term in the Brans-Dicke field equations?

The extra term in the Brans-Dicke field equations arises from the scalar-tensor theory of gravitation. It is associated with the scalar field, often denoted by φ, and its derivatives. This term modifies the usual Einstein-Hilbert action by introducing a coupling between the scalar field and the Ricci scalar, which leads to an additional term in the field equations.

How does the extra term affect the solutions of the Brans-Dicke field equations?

The extra term affects the solutions by introducing additional degrees of freedom related to the scalar field. This can lead to different gravitational behavior compared to General Relativity, such as variations in the effective gravitational constant and modifications to the dynamics of cosmological and astrophysical systems.

Why is the extra term important in the context of scalar-tensor theories?

The extra term is crucial because it encapsulates the influence of the scalar field on the geometry of spacetime. In scalar-tensor theories like Brans-Dicke theory, this term allows for a varying gravitational "constant" and can provide explanations for phenomena that are not easily addressed by General Relativity alone, such as the accelerated expansion of the universe.

How is the extra term derived in the Brans-Dicke theory?

The extra term is derived from the Brans-Dicke action, which includes a non-minimal coupling between the scalar field φ and the Ricci scalar R. By varying this action with respect to the metric and the scalar field, one obtains the modified field equations, which include the extra term involving the derivatives of the scalar field.

Can the extra term be neglected in certain limits or approximations?

In certain limits, such as when the Brans-Dicke parameter ω becomes very large, the effects of the extra term can become negligible, and the theory approaches General Relativity. However, in general scenarios where ω is finite, the extra term plays a significant role and cannot be ignored if accurate predictions are to be made.

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