Another gravity wave question

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    Gravity Wave
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Discussion Overview

The discussion centers around gravitational waves (GWs), their detectability, and the implications of their properties in various astrophysical events. Participants explore theoretical aspects, experimental challenges, and the potential for future detection methods.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant expresses skepticism about the detectability of GWs, arguing that the center of gravity remains unchanged in events like exploding stars or binary neutron stars, which may render GWs undetectable at astronomical distances.
  • Another participant agrees that the center of gravity does not change, noting that gravitational waves are quadrupole radiation and discussing the conservation of energy in relation to the intensity of GWs.
  • A different participant hopes for the success of a satellite system designed to detect differences in GWs from the Big Bang versus those from brane collisions, referencing a source that discusses the polarization of such waves.
  • Concerns are raised about the sensitivity of existing detectors like LIGO and LISA in detecting GWs from the Big Bang, with references to the WMAP findings and their implications for detecting major collisions.

Areas of Agreement / Disagreement

Participants express differing views on the detectability of gravitational waves, with some expressing skepticism and others highlighting potential future detection methods. The discussion remains unresolved regarding the implications of these viewpoints.

Contextual Notes

Participants reference various theoretical frameworks and experimental limitations, including the sensitivity of current detection methods and the nature of gravitational radiation. There is an acknowledgment of the assumptions underlying the discussions, particularly regarding general relativity and the characteristics of gravitational waves.

jnorman
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i have read quite a bit about gravity waves, and even worked (as a lab tech) on an early GW experiment at LSU back in the 70s. i have become ever more convinced that the search for GWs is relatively fruitless.

the reason i feel that way is that, given any particular example of an event which would cause GWs, such as exploding star or orbiting binary neutron stars, the center of gravity will not be changed, and local GWs will be smoothed out in very short distance (astronomically speaking).

for any GW to be actually noticeable or measureable at any astronomical distance, the center of gravity of some very massive system would need to be altered significantly, and frankly i can't even think of a single example of how that might occur.

perhaps one of you could please enlighten me on the error of my thinking on this. thanks.
 
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jnorman said:
the reason i feel that way is that, given any particular example of an event which would cause GWs, such as exploding star or orbiting binary neutron stars, the center of gravity will not be changed, and local GWs will be smoothed out in very short distance (astronomically speaking).

It's true that the center of gravity can't change. That's why gravitational waves are quadrupole radiation, not dipole radiation.

The intensity (watts/m2) falls off as 1/r^2. It can't fall off faster than that because of conservation of energy.

This is all assuming that GR's description of gravitational waves is right. However, the extremely good agreement of the Hulse-Taylor pulsar's behavior with GR suggests that GR's description is right.
 
jnorman: I hope you are wrong. here is why: There is a satellite ystem that is supposed to be able to detect subtle differences between gravitational waves emanting from a big bang that will be slightly different than those emanting from a brane collision in a cyclic universe. That would be fun if it works!

I posted details in another thread based on information from THE ENDLESS UNIVERSE by Steinhardt and Turok and all I remember is that it had to do with the polarization of such waves. Ok it's dubbed the BBO or Big Bang Observatory...and is described in the book around page 218...

I'll see if I can find the prior thread...
 
Could not find it...anyway LIGO and LISA according to the above authors are not sensitive enough for the big bang, and... WMAP came up with nothing so far...but should be able to detect major collisions, like black holes, etc...
 

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