Detecting a Gravity Wave: What Kind of Event Could Produce It?

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Discussion Overview

The discussion revolves around the detection of gravitational waves and the types of astronomical events that could produce them. Participants explore theoretical and practical aspects of gravitational wave detection, including potential sources and the technology involved.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants propose that significant changes in mass, such as the collapse of stars into black holes or binary systems of dense objects, could generate detectable gravitational waves.
  • Others mention that gravitational wave bursts may arise from events like supernova explosions or the collision of neutron stars and black holes.
  • A participant suggests that gravitational waves could be detected from supermassive black hole collisions, although the expected occurrence rate is low.
  • There is a discussion about the limitations of current technology, with references to detectors like LISA and LIGO, and the challenges they face in detecting gravitational waves.
  • Some participants express skepticism about the ability to detect gravitational waves from certain events, arguing that they may appear symmetric and thus not produce detectable waves.
  • Technical aspects of detector design are mentioned, highlighting the complexity and challenges faced by researchers in this field.

Areas of Agreement / Disagreement

Participants express a range of views on the types of events that could produce gravitational waves, with no clear consensus on the most promising sources or the effectiveness of current detection methods. Some agree on the potential of certain events, while others remain skeptical about detection capabilities.

Contextual Notes

Participants note that gravitational waves are expected to be generated by asymmetric events, and the discussion includes various assumptions about the nature of mass and energy changes in astrophysical contexts.

Who May Find This Useful

This discussion may be of interest to those studying astrophysics, gravitational wave research, or the technological challenges associated with detecting gravitational waves.

RandallB
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I understanding there is some effort to detect a “Gravity Wave”
What kind of event are looking for that could produce one?

Assuming we are starting from a base of gravitation “tension” being exerted on us like rubber bands from all directions. I assume the wave to be detected would be in line – like someone pulling back and forth on the rubber band.
And if detected it would likely be a highly damped single Square Wave. A sudden change in the number of gravitons coming our way up or down.

So this wouldn’t be just be something moving around out in the Cosmos.
We must be looking for some significant change is Mass to generate such a wave.

The question is – What is it that we expect to be happening out there that should have such a dramatic affect. A massive release energy though the sudden elimination of mass on a scale large enough that we hope detect a G wave?

Do we have an idea of what this predicted event should “Look” like?
Should be disappointed if such an event is seen but G wave is not detected?

Randall B
 
Astronomy news on Phys.org
What kind of event are looking for that could produce one?
There is expectation to detect two classes of events, continuous sources and gravitational waves bursts. Continuous sources are for example binary pulsars, in fact the indirect detection of gravitational waves in a binary pulsar granted a Nobel prize to Taylor. GW bursts are produced for example, in the explosion of a supernova
Should be disappointed if such an event is seen but G wave is not detected?
The search for gravitational waves is not new, there is an effort of years to detect them, but our current technology has proven primitive to detect them.
There's a laser interferometer called LISA that will be launched in 2012 that possibly will detect such events
Another possible device to detect gravitational waves is a matter wave interferometer, as proposed here
http://arxiv.org/abs/gr-qc/0407039
 
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Thanks for the link, meteor. Hadn't seen that one. In addition to LISA, the Square Kilometer Array is promising and may provide some results useful for the LISA project:
Science with the Square Kilometer Array: Motivation, Key Science Projects, Standards and Assumptions
http://arxiv.org/abs/astro-ph/0409274
 
Just about any astrophysical event will generate gravity waves, however a well-known theorum on gravitational radiation is that spherically symmetric systems do not generate graviational waves, so for example (I guess) when a star collapses into a black hole (which is often cited as one of the best possible sources of g. waves), the amount of graviational wvaes will strongly depend on the degree of spherical asymmetry of the star/black hole. Binary systems of dense objects such as neutron stars orbiting each other closely should also be a copius form of graviational waves.

We are never going to see strong graviational waves from the Earth, as the waves will be string only tclose to the source, an object 'hit by a gravitational wave will appear to move to some remote observer, but from the object's point of view it stays still!
 
RandallB said:
I understanding there is some effort to detect a “Gravity Wave”
What kind of event are looking for that could produce one?

Assuming we are starting from a base of gravitation “tension” being exerted on us like rubber bands from all directions. I assume the wave to be detected would be in line – like someone pulling back and forth on the rubber band.
And if detected it would likely be a highly damped single Square Wave. A sudden change in the number of gravitons coming our way up or down.

So this wouldn’t be just be something moving around out in the Cosmos.
We must be looking for some significant change is Mass to generate such a wave.

The question is – What is it that we expect to be happening out there that should have such a dramatic affect. A massive release energy though the sudden elimination of mass on a scale large enough that we hope detect a G wave?

Do we have an idea of what this predicted event should “Look” like?
Should be disappointed if such an event is seen but G wave is not detected?

Randall B

I remember from the Elegant Universe DVD that gravity waves could be used to communitcate with intellgient life in other universe that were // with our own. Let me see if I can find the clip about it from the streaming video
 
The LIGO website has lots of good resources and links to answer all your questions RandallB.

The two key expected soures (for LIGO detection) are colliding neutron stars (or black holes) and asymmetric supernovae. Some feel that colliding SMBH (galaxy or quasar nuclei) might also be detected, even to the edge of the universe, but the expected rate of occurrence is very low.

If you're into this kind of thing, click on the Einstein@Home link on the LIGO page ... your own PC can take part in data reduction, perhaps leading to the discovery of the first gravitational wave detection!
 
What might be the relationship, coincidence or symmetry, of the fact that light and gravity travel at the same speed?
 
Rader said:
What might be the relationship, coincidence or symmetry, of the fact that light and gravity travel at the same speed?

That's as fast as anything can go. And if gravity turns out to be carried by gravitons, they are massless, which means they travel at c.
 
  • #10
Nereid said:
Some feel that colliding SMBH (galaxy or quasar nuclei) might also be detected, even to the edge of the universe, but the expected rate of occurrence is very low.
Thanks Nererd and others, LIGO has a lot of great material on how they are hopefully of see something. I’ll keep looking it over.
I just have a lot of doubt about detecting anything from orbital or explosive events even if they appear “asymmetric” when you look at it. Seems to me when you get down to it gravitationally they will likely present “symmetric”. Doesn’t seem to me that a “wave” should be expected from mass just moving about.

However the idea that the center of a couple of galaxies could collide Super Massive Black Holes scoring direct hits on each other, that might have the potential for releasing/creating a massive amount of energy converted from disappearing mass.
If enough mass disappeared that I can understand could create a true liner G wave.

Got to be impressed with the effort to even look, two SMBH’s finding each other – that would be rare.

Randall B
 
  • #11
The (experimental) detector design aspects of Gravity Wave detectors is quite an interesting area too. The Q-factors on some of the low-frequency vibration isolation systems built by these people are nothing short of mind-blowing. I remember being particularly impressed by some of the isolators built by a group in Australia (either U of New South Wales or U of S. Australia) - don't recall which one, but I have the paper saved somewhere.

I brought this up because detector design is often the make or break issue in gravity wave measurements and the people that do this incredibly (and I cannot sufficiently describe how technically challenging this job is) difficult work seldom receive recognition.

<just sticking up for my fellow experimenters :biggrin:>
 
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  • #12
RandallB said:
However the idea that the center of a couple of galaxies could collide Super Massive Black Holes scoring direct hits on each other, that might have the potential for releasing/creating a massive amount of energy converted from disappearing mass.
If enough mass disappeared that I can understand could create a true liner G wave.

Got to be impressed with the effort to even look, two SMBH’s finding each other – that would be rare.

Randall B
Rare, but nonetheless sure to happen. The best example I've seen is 3C75, two radio galaxies (they have their own pairs of jets and bright nuclei) on death spiral, at the heart of Abell 400.
 
  • #13
RandallB said:
Thanks Nererd and others, LIGO has a lot of great material on how they are hopefully of see something. I’ll keep looking it over.
I just have a lot of doubt about detecting anything from orbital or explosive events even if they appear “asymmetric” when you look at it. Seems to me when you get down to it gravitationally they will likely present “symmetric”. Doesn’t seem to me that a “wave” should be expected from mass just moving about.

All a gravitational wave is doing is telling an objects gravitational field taht the stae of an object has changed and to change itself to reflect this (infact in some sense all it is is the changes in the field). It's specifically spherically symmetric objects that do not produce graviational waves as long as spherical symmetry is maintained. To get somne clue as to why this might be you might remember the well known theorum that a spherically symmetric object behaves like a point mass, therefore under any changes that do not alter the fact that it's spherical symmetry it will go on behaving like a point mass and there will be no changes to it's gravitatioanl field (actually to be clear we're strictly talking about the field outside of the object).
 
  • #14
RandallB said:
However the idea that the center of a couple of galaxies could collide Super Massive Black Holes scoring direct hits on each other, that might have the potential for releasing/creating a massive amount of energy converted from disappearing mass.
If enough mass disappeared that I can understand could create a true liner G wave.

http://www.batse.com/index.html

What about gamma ray bursts emitting possibly detectable gravity waves? Nothing as yet has been found to emit more energy in a short period of time as they do. They are thought to be on the edge of the universe and it is unlikely that black holes would collide there, as they would have had no time to form.
 

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