Sachs-Wolfe effect in a Dark Energy universe?

In summary, the integrated Sachs-Wolfe effect is a phenomenon that occurs when a photon travels through a changing gravitational potential due to spacetime expansion. This can result in a blueshift when the photon enters a gravitational well and a redshift when it exits. While dark energy is not the cause of expansion, it can contribute to accelerated expansion. However, the integrated Sachs-Wolfe effect can still occur even in a universe with only one galaxy, as long as there is some spatial variation in density. If there are no other gravity wells besides our own, then the effect would not be observed.
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Suekdccia
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TL;DR Summary
Sachs-Wolfe effect in Dark Energy universe?
The integrated Sachs-Wolfe effect occurs when a photon goes through a gravitational potential that changes due to spacetime expansion (presumably caused by dark energy). For that reason, a photon going through a gravitational well would gain energy (blueshift) when entering and it would lose energy (redshift) when exiting it. If the universe expands, the well becomes "less deep" and therefore, the photon gets more energy and becomes blueshifted.

However, would this effect still occur if we had a photon traveling in a universe with only one galaxy (the Milky Way) and the rest of it dominated by Dark Energy (that is, the Universe once the expansion separates all non-gravitationally bounded structures to us)?
 
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Suekdccia said:
The integrated Sachs-Wolfe effect occurs when a photon goes through a gravitational potential that changes due to spacetime expansion
Yes.

Suekdccia said:
(presumably caused by dark energy)
No. Dark energy is not the cause of expansion. It's only the cause of accelerated expansion. But you don't need accelerated expansion to have a nonzero integrated Sachs-Wolfe effect. All you need is some spatial variation in density.

Suekdccia said:
would this effect still occur if we had a photon traveling in a universe with only one galaxy (the Milky Way) and the rest of it dominated by Dark Energy (that is, the Universe once the expansion separates all non-gravitationally bounded structures to us)?
If you postulate that there are no other gravity wells except the one we are in, then no, we would no longer observe any Sachs-Wolfe effect, just a (small) blueshift from photons falling into our gravity well.
 
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FAQ: Sachs-Wolfe effect in a Dark Energy universe?

What is the Sachs-Wolfe effect?

The Sachs-Wolfe effect refers to the phenomenon observed in the cosmic microwave background radiation (CMB) where photons are redshifted or blueshifted as they travel through gravitational potential wells. This effect is caused by the changing gravitational fields of large-scale structures in the universe.

How does the Sachs-Wolfe effect relate to Dark Energy?

In a Dark Energy universe, the expansion of the universe is accelerating, causing the gravitational potential wells to change over time. This results in a larger Sachs-Wolfe effect on the CMB, as the photons have more time to interact with the changing gravitational fields.

What evidence supports the Sachs-Wolfe effect in a Dark Energy universe?

Observations of the CMB, such as the Planck satellite data, have shown that the CMB is affected by the Sachs-Wolfe effect. The observed patterns and fluctuations in the CMB are consistent with the predictions of the Sachs-Wolfe effect in a Dark Energy universe.

Can the Sachs-Wolfe effect be used to study Dark Energy?

Yes, the Sachs-Wolfe effect can provide valuable information about the properties of Dark Energy. By studying the patterns and fluctuations in the CMB, scientists can gain insights into the expansion rate and density of Dark Energy in the universe.

Are there any other effects that can be observed in a Dark Energy universe?

Yes, in addition to the Sachs-Wolfe effect, there are other effects that can be observed in a Dark Energy universe, such as the Integrated Sachs-Wolfe effect and the Rees-Sciama effect. These effects also involve the interaction between CMB photons and changing gravitational fields in the universe.

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