What happens to EM waves outside the universe?

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Discussion Overview

The discussion revolves around the nature of electromagnetic (EM) radiation in relation to the universe's expansion, particularly addressing the concept of an "edge" or "outside" of the universe. Participants explore theoretical implications of a finite versus infinite universe, the geometry of space, and the complexities of astrophysical concepts.

Discussion Character

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

Main Points Raised

  • One participant questions what happens to EM radiation emitted from stars at the edge of the universe if the universe is expanding at less than the speed of light.
  • Another participant asserts that there is no "outside" the universe and that it is not known if the universe is finite or infinite.
  • Some participants propose that if the universe were finite, it could still lack an edge, referencing the concept of closed manifolds and the geometry of a 3-sphere.
  • One participant expresses confusion and requests a simpler explanation of these concepts.
  • Several participants share resources, such as FAQs and analogies, to help clarify the shape and nature of the universe.
  • There is a discussion about the observable universe being finite and spherical, defined by the limits of measurement due to the speed of light and expansion.
  • One participant emphasizes the complexity of astrophysics and the existence of multiple theories illustrating a single concept, which complicates understanding for casual readers.
  • Another participant highlights the lack of confusion regarding the shape of the observable universe, describing it as a sphere centered on the observer.
  • One participant mentions the cosmological constant problem and its implications for quantum field theories, introducing a more technical aspect to the discussion.

Areas of Agreement / Disagreement

Participants express varying views on the existence of an edge to the universe and the implications of a finite versus infinite universe. While some agree on the complexity of astrophysical concepts, there is no consensus on the nature of the universe's boundaries or the implications for EM radiation.

Contextual Notes

Participants reference various theoretical frameworks and analogies, indicating that assumptions about the universe's shape and boundaries may depend on specific definitions and interpretations. The discussion includes unresolved mathematical and conceptual challenges related to the cosmological constant.

yoyopizza
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If the universe is expanding at less than the speed of light, what happens to EM radiation
that is emitted from stars at the edge of the universe?
 
Astronomy news on Phys.org
But if the universe were finite, wouldn't it then have an edge?
 
yoyopizza said:
But if the universe were finite, wouldn't it then have an edge?
Not necessarily. The simplest k = +1 geometry, the 3-sphere, is compact ("finite") but has empty manifold boundary ("unbounded"). Such objects are called closed manifolds lending to why you may see the term closed universe.
 
Is there a more in depth and simple explanation? I am very confused
 
several I've already posted the FAQ sub forum and Ned wrights FAQ.

here is a useful balloon analogy

http://www.phinds.com/balloonanalogy/

this site describes loosely a few finite shapes with no edge.

http://abyss.uoregon.edu/~js/cosmo/lectures/lec15.html

this on going thread also has tons of descriptions and information on edge and shape

https://www.physicsforums.com/showthread.php?t=684006

also keep in mind the shape of what is called the Observable universe is finite and spherical. The observable universe is simply defined as the furthest we can measure. Due to speed of light and expansion.

http://en.wikipedia.org/wiki/Observable_universe
 
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yoyopizza said:
But if the universe were finite, wouldn't it then have an edge?

Not it doesn't. If the Universe was finite and unbounded it just means that if you travel in one direction for long enough you will eventually end back at your starting point. In other words the Universe "loops" back on itself. Why is this so hard for people to understand?
 
Its hard to grasp at first, but I think I get it. So there is no outside the universe, it instead might be curved in on itself right? Does gravity cause this?
 
Flatland said:
In other words the Universe "loops" back on itself. Why is this so hard for people to understand?

Do you have a vested interest Flatland?
 
  • #10
astrophysics is complicated for the casual reader (like me) because there are usually several different theories illustrating a single concept, example the shape of the local universe or the shape of the entire universe. to make communication easier many of the theories are reduced to initials or a tag name. this complicates thing a lot for the casual reader.

Keep reading. It took me a week and a half to get thru this article the first time I read it. I had 40 pages of notes that I looked up to get through this one page

http://en.wikipedia.org/wiki/Shape_of_the_Universe
 
  • #11
rustytxrx said:
astrophysics is complicated for the casual reader (like me) because there are usually several different theories illustrating a single concept, example the shape of the local universe or the shape of the entire universe. to make communication easier many of the theories are reduced to initials or a tag name. this complicates thing a lot for the casual reader.

Keep reading. It took me a week and a half to get thru this article the first time I read it. I had 40 pages of notes that I looked up to get through this one page

http://en.wikipedia.org/wiki/Shape_of_the_Universe

I agree, I can normally read books in a day or so, but just getting through one book on relativity took me a month. Have you read "Relativity Demystified"? its a great book if you havn't read it or don;t know much on relativity
 
  • #12
rustytxrx said:
astrophysics is complicated for the casual reader (like me) because there are usually several different theories illustrating a single concept, example the shape of the local universe or the shape of the entire universe. [/url]

I've never seen ANY confusion about the shape of the "local" universe, assuming you mean what is more commonly called the "observable" universe. It is a sphere with a radius based on the speed of light and the age of the universe and it is centered on you. Right now it's about 47 billion light years in radius. There is no confusion or contention about that and I'm not aware of any other theories about it.
 
  • #13
yes of course. I should have given more thought in selecting my example.

Edit - maybe my point was to read astrophysics you have to have a vast underpinning of knowledge. how I got here is I was reading quantum physics. read how the quantum vacuum was related to the cosmological constant. Thus came into search around the forum. Interesting place
 
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  • #14
You are missing the point. And making a point that has no basis in fact. Show the math.
 
  • #15
A major outstanding problem is that most quantum field theories predict a huge value for the quantum vacuum. A common assumption is that the quantum vacuum is equivalent to the cosmological constant. Although no theory exists that supports this assumption, arguments can be made in its favor.

Such arguments are usually based on dimensional analysis and effective field theory. If the universe is described by an effective local quantum field theory down to the Planck scale, then we would expect a cosmological constant of the order of M_{\rm pl}^4. As noted above, the measured cosmological constant is smaller than this by a factor of 10−120. This discrepancy has been called "the worst theoretical prediction in the history of physics!".

Some supersymmetric theories require a cosmological constant that is exactly zero, which further complicates things. This is the cosmological constant problem, the worst problem of fine-tuning in physics: there is no known natural way to derive the tiny cosmological constant used in cosmology from particle physics. Structural Quantum Gravity is an approach of Quantum Gravity that predicts Einsteins field equations with cosmological constant as the classical limit of the action of Structural Quantum Gravity.



Sorry to step on your thread , yoyopizza
 

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