Uncovering the Truth: Examining the Existence of Gravitational Waves

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Discussion Overview

The discussion revolves around the existence of gravitational waves (GWs) and the implications of their detection or non-detection. Participants explore theoretical aspects, observational evidence, and the conceptual challenges related to measuring gravitational waves, particularly in the context of an expanding universe.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants express confidence in the existence of gravitational waves, citing indirect observational evidence from systems like PSR 1913+16.
  • Others raise questions about the detection of gravitational waves, comparing it to the question of whether rulers expand with the universe, suggesting that if everything embedded in space-time expands, it could lead to non-detection of GWs.
  • A participant proposes that if detectors expand with the universe, they would not be able to detect gravitational waves, as the waves would "wash over" the detectors without leaving a signal.
  • Some argue that the measuring apparatus does expand, but the effect is negligible, and they emphasize that the detection of gravitational waves should still be possible if they exist.
  • Concerns are raised about the implications of failing to detect gravitational waves in future experiments, with some attributing potential failures to experimental issues rather than theoretical ones.
  • Participants discuss the Pioneer Anomaly as a clue that may suggest issues with the standard model of cosmology, although they caution against oversimplifying its implications.
  • There is a reiteration that the forces between molecules in a ruler prevent it from expanding with the universe, maintaining that physical laws governing size do not change with cosmic expansion.

Areas of Agreement / Disagreement

Participants generally agree that gravitational waves are likely to exist based on current theories and indirect evidence. However, there is significant disagreement regarding the implications of the universe's expansion on the detection of gravitational waves, with multiple competing views presented without resolution.

Contextual Notes

The discussion highlights limitations in understanding the relationship between gravitational waves and the expansion of the universe, as well as the assumptions underlying the models used to explain these phenomena. There are unresolved questions about the nature of measurements and the physical laws at play.

  • #31
Spin_Network said:
It is obvious the article is Historical, the GW's predicted by Einstein in 1916?..the articles content deals with a peer review dispute.
I am not disputing the existence of GW's, but I do not think they will be detected (in forseeable future), for which reasons the Einstein-Rosen-Paradox must have a baring?
Something can exist, and still be beyond detection?

I don't understand your point. Yes, it was a peer review dispute, but Einstein later agreed (circuitously) that the referee was right.

On what basis are you claiming that gravitational waves won't be detected soon? And what is the Einstein-Rosen paradox?

Their result was only confusing before they realized that their chosen coordinate system was misleading. It's pretty easy to confuse yourself in GR with coordinate problems if you're not very careful. This was not as widely acknowledged then as it is today. People had little experience with recognizing and resolving these issues.
 
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  • #32
Stingray said:
On what basis are you claiming that gravitational waves won't be detected soon?
As well as this being a discussion about the interpretation of theory, GWs have not yet been detected and, if this non-detection continues indefinitely, then that interpretation may have to be revised.

As an example this eprint was posted today on the physics ArXiv: Joint LIGO and TAMA300 Search for Gravitational Waves from Inspiralling Neutron Star Binaries

Yet again:
We find no evidence of any gravitational wave signals

Garth
 
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  • #33
Garth, that paper puts an upper limit of ~50 neutron star mergers per year in the Milky Way galaxy. Are you saying you would have expected it to be larger than that?
 
  • #34
SpaceTiger said:
Garth, that paper puts an upper limit of ~50 neutron star mergers per year in the Milky Way galaxy. Are you saying you would have expected it to be larger than that?
I personally expect GWs to be eventually detected, however, after linking to an article describing Einstein's ambivalence over GWs, the OP question was "So do Gravitational Waves exist?" That question becomes more pertinent the longer their non-detection continues.

Now, as for that paper's expected limit for neutron star/BH mergers. If we, for the moment, accept that short GRBs are such mergers and they are detected about once a month, and they are relatively nearby, though not necessarily in the Milky Way, then we might expect ~ 10 neutron star mergers per year in the Milky Way galaxy. So I am not expecting it to be larger than ~50 , however the upper limit is now at last approaching the expected detection limit and the next few years should be interesting!

Of course, not all NS/BH mergers necessarily produce short GRBs, and there are other sources of GWs as well, so the expected GW detection rate is probably highter than this, but I have no expertise in this area.

Garth
 
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  • #35
Garth said:
I personally expect GWs to be eventually detected, however, after linking to an article describing Einstein's ambivalence over GWs, the OP question was "So do Gravitational Waves exist?" That question becomes more pertinent the longer their non-detection continues.

I think we're still in the stage where we would have been surprised if we had detected them. LIGO doesn't have the sensitivity to see most of the conventional gravitational wave sources, and those that it can see require a great deal of luck.


Now as for that paper's expected limit for neutron star/BH mergers. If we, for the moment, accept that short GRBs are such mergers and they are detected about once a month, and they are relatively nearby, though not necessarily in the Milky Way, then we might expect ~ 10 neutron star mergers per year in the Milky Way galaxy.

Our understanding of short GRBs is extremely crude and any failure to detect such a signal would almost certainly be due to a failure in those models, not in our theory of gravity. Given the high-quality data that came from PSR 1913+16, the only way you'll see astronomers/physicists seriously questioning the existence of gravitational waves is if we point our detectors at a source that we know is above our threshold of sensitivity and get no detection.

The only observations that tell us anything about gravitational waves have come out in favor of them. None of the direct detection experiments have been able to address GR, they've only been able to put limits on the frequency of certain astrophysical events.
 
  • #36
SpaceTiger said:
Our understanding of short GRBs is extremely crude and any failure to detect such a signal would almost certainly be due to a failure in those models, not in our theory of gravity. Given the high-quality data that came from PSR 1913+16, the only way you'll see astronomers/physicists seriously questioning the existence of gravitational waves is if we point our detectors at a source that we know is above our threshold of sensitivity and get no detection.
Agreed - but when (how many more years) will our theshold of detection increase in sensitivity to below the predicted signal from known sources?

Garth
 
  • #37
Garth said:
Agreed - but when (how many more years) will our theshold of detection increase in sensitivity to below the predicted signal from known sources?
Garth

As I've stated in these forums several times, most people would be quite surprised if any of the current detectors found anything in the next few years.

Upgrades to LIGO are expected to start being built in 2008, and observations should start around 2013. These will increase the sensitivity by a factor of 10, which is expected to be sufficient to make a detection within a year or two (at worst). If nothing is found by then, people will start to worry.
 
  • #38
Stingray said:
As I've stated in these forums several times, most people would be quite surprised if any of the current detectors found anything in the next few years.
Upgrades to LIGO are expected to start being built in 2008, and observations should start around 2013. These will increase the sensitivity by a factor of 10, which is expected to be sufficient to make a detection within a year or two (at worst). If nothing is found by then, people will start to worry.
Thank you, that is what I wanted to know!

Garth
 

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