Cosmic microwave background radiation

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Discussion Overview

The discussion centers around the cosmic microwave background radiation, particularly focusing on the Wilkinson Microwave Anisotropy Probe (WMAP) and its findings. Participants explore the implications of this radiation in cosmology, as well as the potential for detecting fundamental aspects of the universe beyond electromagnetic radiation.

Discussion Character

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

Main Points Raised

  • One participant summarizes an article about WMAP, highlighting its ability to measure the energy and polarization of cosmic microwave background radiation, and its advancements over previous surveys like COBE.
  • Another participant questions the detectability of fundamental constituents of the universe, such as strings in string theory, and the geometry of the universe as described by General Relativity, beyond electromagnetic observations.
  • A clarification is sought regarding the nature of the initial question about detection methods related to gravity theories and fundamental universe components.

Areas of Agreement / Disagreement

The discussion contains multiple competing views regarding the detection of fundamental aspects of the universe, and it remains unresolved whether these components can be observed outside of electromagnetic detection methods.

Contextual Notes

Participants express uncertainty about the implications of string theory and the geometry of the universe, and there are missing assumptions regarding the methods of detection discussed.

BryceG
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i read a article and i can't really understand all of it. I get some but then its beyond me.
If someone could briefly summarise it so i can understand.

Here is the link.

http://www.aip.org/enews/physnews/2003/split/624-1.html
 
Last edited by a moderator:
Astronomy news on Phys.org
This article describes a survery of the cosmic microwave background radiation made by a satellite called the Wilkinson Microwave Anisotropy Probe (WMAP). Basically, it uses two radio telescopes to measures the energy of the radiation coming from every direction in space. The energy of the radiation can be described with a "characteristic" temperature.

WMAP is not the first such survey. The last one, done by the COsmic Background Explorer (COBE) satellite, had much lower resolution -- it could not discern details as fine as WMAP did. In addition, WMAP can also measure the polarization of the radiation, which is essentially the plane of the varying electric field of the radiation photons.

The page goes on to describe some of the first numerical cosmological results from WMAP, including the age of the universe and its matter content.

Please ask me some specific questions if you have any.

- Warren
 
all our investigationtions of the universe involve EM detection in one
way or another, but in theoreis of gravity the geometry or string holds
as the basic, "thing" of the universe can these things be detected?
 
I'm not sure I understand wolfram's question ... is it "can the fundamental constituents of the universe - strings* - be detected?" Or maybe, "can the geometry** of the universe be detected, other than by observations of electro-magnetic radiation?"

*in the sense of what's in String Theory/M Theory.

**in the sense of General Relativity.
 

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