Conformal symmetry of FRW spacetime

In summary, the standard spatially flat FRW metric in Cartesian co-moving co-ordinates suggests that the Universe is both spatially homogeneous and isotropic. However, by writing the metric in a different form using conformal time, it reveals a conformal symmetry that stretches equally in time and space. This implies that photons, which obey Maxwell's equations, propagate with constant energy/frequency. It is also possible that the time we measure is actually conformal time and the observed redshift is due to the increasing energy scales with the age of the Universe. Overall, using conformal time in local systems may lead to unnecessary complexities in equations due to the dependence on the scale factor, ##a(\tau)##.
  • #1
jcap
170
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The standard spatially flat FRW metric in Cartesian co-moving co-ordinates is given by:

$$ds^2=dt^2-a(t)^2(dx^2+dy^2+dz^2)$$
As far as I understand it the fact that the metric can be written in a form that is independent of ##x,y,z## implies that the Universe has the physical qualities of being spatially homogeneous and isotropic.

But by writing the FRW metric in another way one can see that the Universe has another symmetry.

$$ds^2 = a(t)^2(\frac{dt^2}{a(t)^2}-dx^2-dy^2-dz^2)$$

If we introduce conformal time ##\tau## defined by:

$$d\tau = \frac{dt}{a(t)}$$

we get:

$$ds^2 = a(\tau)^2(d\tau^2-dx^2-dy^2-dz^2)$$
This way of writing the metric displays a conformal symmetry: it stretches equally in (conformal) time and space.

What physical quality does this conformal symmetry imply for the Universe?

Here are some of my speculations:

Photons obey Maxwell's source free equations which are conformally invariant.

Does the conformal symmetry of the FRW metric imply that photons actually propagate with constant energy/frequency?

Maybe the time we actually measure is conformal time and the redshift that we see is due to our energy scales increasing with the age of the Universe. If expanding photon wavelengths have constant energy then as our atoms have a fixed size their energies will increase with the scale of the Universe.
 
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  • #2
The time we actually measure is the integral ##\int ds## of the metric over a path where ##dx = dy = dz = 0##. So in these coordinates, ##s = \int a(\tau)d\tau = \int dt##.

Essentially, if we were to use conformal time to do physics in local systems, we'd end up with a whole bunch of extraneous factors that depend upon ##a(\tau)## that unnecessarily complicate the equations.
 

FAQ: Conformal symmetry of FRW spacetime

What is conformal symmetry?

Conformal symmetry is a mathematical property of a system or space that remains unchanged under certain transformations, specifically those that preserve angles and relative distances between points. In physics, this symmetry is often associated with the conformal group, a set of transformations that preserve the shape of spacetime.

What is FRW spacetime?

FRW spacetime, also known as Friedmann-Robertson-Walker spacetime, is a mathematical model used in cosmology to describe the large-scale structure of the universe. It is a solution to Einstein's field equations of general relativity and is based on the assumptions of homogeneity and isotropy, meaning that the universe looks the same in all directions and at all locations.

How does conformal symmetry relate to FRW spacetime?

Conformal symmetry plays a crucial role in the study of FRW spacetime as it allows for the transformation of the metric, the mathematical description of spacetime, without changing the physical properties of the universe. This symmetry allows us to simplify and analyze the equations describing the evolution of the universe in a more efficient manner.

What are the applications of studying conformal symmetry of FRW spacetime?

Understanding the conformal symmetry of FRW spacetime can help us gain a deeper understanding of the fundamental laws of physics and the behavior of the universe. It can also aid in the development of new theories and models, as well as in the interpretation of observational data from cosmological observations.

Are there any limitations to the conformal symmetry of FRW spacetime?

While conformal symmetry is a powerful tool in studying FRW spacetime, it does have some limitations. It only applies to homogeneous and isotropic universes, which may not accurately describe our own universe on smaller scales. Additionally, it does not take into account the effects of matter and energy, which play a significant role in the evolution of the universe.

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