How Do EM Waves Stretch and Interact in Space?

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Discussion Overview

The discussion revolves around the behavior of electromagnetic (EM) waves as they propagate through space, particularly focusing on how they stretch, interact, and the implications of their density and interaction from various light sources such as stars. The scope includes conceptual inquiries about light propagation and potential interactions between light from different stars.

Discussion Character

  • Exploratory
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Harish questions how EM waves stretch in a vacuum and what fills the gaps as the sphere of light spreads, expressing doubt about the continuity of light emission.
  • Harish inquires whether the density of light relates to the distance from the source, suggesting a need for clarity on how light spreads without breaking up.
  • Another participant confirms that the density of light follows an inverse square relation, indicating that photon density decreases with the square of the distance from the source.
  • Harish raises concerns about the potential loss of information from distant light sources and whether overlapping light from multiple stars can be distinguished.
  • A later reply explains that light is emitted in quanta called photons, which travel in random directions, and suggests that with enough time, at least one photon from a source will reach a detector unless obstructed.

Areas of Agreement / Disagreement

Participants express varying levels of understanding and concern about the implications of light propagation and interaction, with no consensus reached on the broader implications of these phenomena.

Contextual Notes

There are unresolved questions regarding the assumptions about light density, the nature of photon interactions, and the conditions under which light from multiple sources can be distinguished.

Who May Find This Useful

This discussion may be of interest to those exploring concepts in physics related to light propagation, electromagnetic waves, and the nature of photons.

hareeshgnair
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Hi,

I am not a student of physics, asking the question as it came to mind as I read certain articles:

1. When EM Waves is emitted by a source say star it spreads in vacuum. How does the waves Stretch? What fills in the gaps as the sphere of spread grows? If light emission is continuous does the density of light in the sphere has any relation to the distance from source? Basically I doubt how can the light spread continuously without breaking up..or something like that.

2. If all the light from different stars are accounted for..do different light spheres interact and say cancel or reinforce each other?

Advance thanks for the replies,
Harish
 
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hareeshgnair said:
1. Does the density of light in the sphere has any relation to the distance from source?

2. If all the light from different stars are accounted for..do different light spheres interact and say cancel or reinforce each other?

1. Yes, for a sphere, it is an inverse square relation [photon density = constant/(distance)^2]. If sufficiently far away, a detector may see a single photon, or none, within a certain time period.

2. At a given observing point, starlight just adds up.
 
So does it imply:
1. That lot of information from around the universe is lost, as we may not receive any photons from the light sources.
2. That if two starlight adds up..I won't be able to distinguish that these are two stars?

I hope its not so simple to conclude!:)
 
Remember that light is emitted in quanta's called Photons, the particle of light. When something such as a light bulb or a star emits light, it emits each photon in a random direction. The light in your living room emits trillions upon trillions of photons, and a star has many many many more. This means that given enough time you WILL see at least one photon from a light source as long as there is nothing to interfere with it on the way to your detector.
 

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