Effects of Tensor + Scaler gravity

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Discussion Overview

The discussion centers around the effects of scalar and tensor gravity models, particularly in relation to the precession of Mercury and the implications of scalar fields in contemporary dark energy theories. Participants explore historical models, current hypotheses, and seek analogies to clarify the differences between scalar and tensor fields.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Neil references the historical S+T gravity model developed by Bob Dicke and Carl Brans and questions the current understanding of scalar fields in relation to Mercury's precession.
  • Some participants suggest that scalar fields can induce gravity-like forces, with current models of dark energy (like Quintessence) positing that these fields may have undetectable interactions.
  • It is noted that the distinction between normal gravity and gravity induced by a scalar field can be observed through light deflection, with current measurements agreeing within experimental precision.
  • Neil requests analogies to better understand the differences between scalar and tensor fields, indicating difficulty in visualizing these concepts.
  • A participant explains that a scalar field is defined by a single number at each point in space, while a tensor field is defined by a tensor, providing examples such as energy density for scalar fields and stress tensors for tensor fields.

Areas of Agreement / Disagreement

Participants express varying levels of understanding and seek clarification on the concepts discussed, indicating that there is no consensus on the implications of scalar fields in contemporary physics or their effects on Mercury's precession.

Contextual Notes

The discussion includes references to historical models and current theories without resolving the complexities or assumptions involved in the relationships between scalar fields, tensor fields, and gravitational effects.

Who May Find This Useful

This discussion may be of interest to those studying gravitational theories, dark energy models, and the distinctions between scalar and tensor fields in physics.

captn
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Fifty years ago (m/l), Bob Dicke and Carl Brans developed a S+T gravity model.

Concurrently, Dicke had a project to look for a small solar oblateness. He wanted the precession of Mercury caused by the scaler part of gravity to be offset by the opposite precession caused by oblateness.

In the last ten years, a scaler field has been suggested to the dark (matter? or energy?), but I have seen nothing about that field causing a part of Mercury's precesion.

Is the effect of a scaler suggested today much less than the effect caused by dicke/brans' scaler? Please help me to understand the effects of today's sacler.

Thanks, Neil
 
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captn said:
Fifty years ago (m/l), Bob Dicke and Carl Brans developed a S+T gravity model.

Concurrently, Dicke had a project to look for a small solar oblateness. He wanted the precession of Mercury caused by the scaler part of gravity to be offset by the opposite precession caused by oblateness.

In the last ten years, a scaler field has been suggested to the dark (matter? or energy?), but I have seen nothing about that field causing a part of Mercury's precesion.

Is the effect of a scaler suggested today much less than the effect caused by dicke/brans' scaler? Please help me to understand the effects of today's sacler.

Thanks, Neil
Well, it is the case that any scalar field will necessarily also cause a gravity-like force. Typically the Quintessence models of dark energy that make use of such a scalar field having one whose interactions are such that they are undetectable.

And by the way, the way to distinguish between normal gravity and gravity induced by a scalar field is by looking at the deflection of light: the two deflect differently, and so a scalar field would cause the measurement of our Sun's mass by gravitational lensing to differ from its mass as measured through the orbits of the planets. So far the two agree to within experimental precision, so any scalar field that exists must necessarily have either very weak or very short-range interactions.
 
Chalnoth said:
... models of dark energy that make use of such a scalar field having one whose interactions are such that they are undetectable.

Okay---Thanks,

Neil
 
Can someone provide an analogy of scalar versus tensor (fields)? I've read through the wikipedia, but it's difficult to visualize. Some examples of each that could be used to differentiate the two would be great.

Thanks in advance.
 
JinChang said:
Can someone provide an analogy of scalar versus tensor (fields)? I've read through the wikipedia, but it's difficult to visualize. Some examples of each that could be used to differentiate the two would be great.

Thanks in advance.
Well, a scalar field is a field that is fully defined by a single number at every point in space, whereas a tensor field is one that is fully defined by a tensor at every point in space (typically a second rank tensor).

Now, an example of a scalar field would be energy density: energy density is just a single number at every point in space. Note that this isn't a quantum field in and of itself, but rather a property of other fields. A quantum scalar field would be a fundamental particle that can be identified in such a way.

An example of a tensor field would be the stress tensor. The stress tensor is composed of pressure along the diagonal components, and anisotropic shears on the off-diagonal components. This type of tensor is required to fully define the forces in an extended object. If I have a rod, for example, I can give it pressure in one direction or another by squeezing/stretching it. I can give it an anisotropic shear by twisting the rod.

Depending upon what you mean by a tensor field, you can also add in the momentum and energy density of the rod (to make a stress-energy tensor). The difference would be whether you just want the spatial components of the tensor, or also the space-time components.
 
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Thanks, Chalnoth. While I need to study upon some of your explanation, it's certainly a great place to start.
 

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