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

In summary: 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?Yes, one would be disappointed if they did not detect a G wave.
  • #1
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
 
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  • #2
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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  • #3
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
 
  • #4
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!
 
  • #5
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
 
  • #6
  • #7
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 occurrance 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!
 
  • #8
What might be the relationship, coincidence or symmetry, of the fact that light and gravity travel at the same speed?
 
  • #9
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 occurrance 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 intersting 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.
 

1. What is a gravity wave?

A gravity wave, also known as a gravitational wave, is a ripple in the fabric of space-time caused by a violent and energetic event in the universe.

2. How can we detect a gravity wave?

Scientists use extremely sensitive instruments called interferometers to detect gravity waves. These instruments measure tiny changes in the distance between two objects caused by the passing of a gravity wave.

3. What kind of event could produce a detectable gravity wave?

Some possible events that could produce detectable gravity waves include the collision of two black holes, the explosion of a supernova, or the merging of two neutron stars.

4. How does the detection of a gravity wave contribute to our understanding of the universe?

The detection of a gravity wave provides evidence for the existence of certain events and phenomena in the universe that were previously only theorized. It also helps us better understand the behavior of gravity and the nature of space-time.

5. Are there any current ongoing efforts to detect gravity waves?

Yes, there are several ongoing efforts around the world, including the Laser Interferometer Gravitational-Wave Observatory (LIGO) in the United States and the Virgo interferometer in Italy. These instruments are constantly being upgraded and improved to better detect and study gravity waves.

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