Gravitational waves (GWs) are predicted by Einstein's theory of general relativity. They are described as ripples in spacetime that propagate at the speed of light through space. They can apparently also be described as "graviton particles" that transfer gravitational energy, similar to photons that transfer electromagnetic energy.
Gravitational waves transfer energy quite differently to the way photons do. GWs are neither absorbed, nor reflected by matter, but pass straight through them, losing only a tiny amount of their energy. Also, while photons are emitted in legions just about everywhere in space, GW-emitting bodies are scarce, at least the ones that emit strong enough GWs to give us any hope of detection. As I understand it, GWs loose amplitude directly proportional to distance traveled, just like light waves.
GW detectors are huge (and very expensive) contraptions, mostly buried below the surface of Earth, e.g., the LIGO facility. LIGO stands for Laser Interferometer Gravitational-wave Observatory. In about 2 years of working at near-full sensitivity, LIGO has registered no GWs. Plans are now to build an even larger and more expensive GW detector in space, called LISA (Laser Interferometer Space Antenna).
GW's have been detected indirectly as the 'anomalous' in-spiraling of two pulsars orbiting each other. The rate of in-spiral matches the predictions of general relativity almost precisely, which predicts that the "lost energy" is radiated away as gravitational waves. Scientist are fairly optimistic that GWs exist and that it is just a matter of having a sensitive enough detector and then wait for an event that radiates GWs and is close enough so that we can detect it.
My question: are GW detection attempts not a huge waste of resources, while there are other more pressing needs?
SL
Comments
generating a gravity wave
March 15, 2008 by Anonymous, 1 year 36 weeks ago
Comment: 28137
Generating a gravity wave. If a large mass is shaken rather violently it should generate a spatial disturbance. The sun is a rather large mass, about 1.9891*10^30 kg, and a radius of 6.955*10^8 meters. Now the gravitational conditions at the surface or 695500 km from the center may be determined.
Surface acceleration, Sa, = 274.38 meters/ss
Escape velocity, Ve, = 617.79 km/s
Time, T’, = 0.999997876656339 seconds/proper second
Note that a proper second may be read from a clock about 1 light year distant from the sun and at rest with the sun, proper length is a rule in the same location.
Now to get is shaken, not stirred, at +/- 1000 km at about 10 times per second. Woops both GR and SR says that is a no no, but both allow me to replace the sun with a neutron star of the same mass and much smaller radius and obtain the same results at the same distances from the center. And they allow that to be shaken.
At 694500 km, +1000 km.
Sa = 275.17388 meters/ss
Ve = 618.2369 km/s
T’ = 0.999997873598969
At 696500 km, -1000 km
Sa = 273.5956 meters/ss
Ve = 617.3486 km/s
T’ = 0.9999978790493
The peak to peak time variation is 5.192*10^-7 seconds which is the same variation in length as seen compared to the proper rule. These variations are propagated away from the mass at c.
Meanwhile at earth orbit, 150133300 km from the center of mass all is quiet, the ripples will take about 8 minuets to arrive so that the gravitational conditions are;
Sa = 0.588840465 cm/ss
Ve = 42.04868 km/s
T’ = 0.999999990163505
Finally the first peak arrives.
Sa = 0.588848095 cm/ss
Ve = 42.488172 km/s
T’ = 0.999999990163439
And then the next.
Sa = 0.5888326210 cm/ss
Ve = 42.0485371 km/s
T’ = 0.999999990163570
At earth orbit the peak to peak time variation is 6.5*10^-14 as is the peak to peak length variation. These are small quantities and they continue to fall off by 1/4th every time the distance is doubled so at the intergalactic distances that we are trying to measure GWs the variations are all-most impossibly small even for super massive events.
The values of Sa, Ve and T’ fairly well describe the gravity well, and Ve and T’ show a rather neat relationship. If you pick a point r at some distance from a mass the gravitational time dilation is equal to the time dilation of an object traveling at a relative velocity of Ve.
Thanks. Con Morton
Just posted a follow-up entry on Scruffy's grav. wave question
March 12, 2008 by Fred Bortz, 1 year 37 weeks ago
Comment: 28087
http://www.scienceblog.com/cms/clear-and-interesting-newpaper-summary-gr...
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
Re: elusive points, evasive points
February 26, 2008 by Fred Bortz, 1 year 39 weeks ago
Comment: 27779
Jim,
I also said in my most recent response: "Since Jim and I both agree the discussion above is sufficient, there is no reason to resume this circular dance, even though Jim has invited me to do so."
So since your latest posting is a repetition of old arguments and accusations, I will counter a couple of personal points and one scientific point and exit this thread. (I admit it. I am rehashing old stuff. If you hadn't criticized me personally, I would not have replied at all.)
(1) General relativity is not quite a century old, so what's wrong with pointing out that no observation has challenged it in that time? Theories gain credibility as they survive more and more challenges. Of course that does not mean that they will survive future challenges. You incorrectly imply that because I give GR great credence, I am rigidly assuming that it will never need to be modified.
(2) As for "famous" scientists, whenever I cite them, it is always in the context of their work, not as authority figures. Their fame rests on the success of that work, so they have earned much more credibility than you or any other challenger who has yet to achieve that level of success.
One bit of science: Repeating previous discussion, you write, "There is no unambiguous observational support for the existence of energy-bearing gravitational waves." I agree and reiterate that absence of evidence is not evidence of absence. There have been no observations to date that would be expected to produce such unambiguous evidence.
[Emphasis added in edit, because your post states, "What sort of evidence could prove something doesn’t exist if there’s already no evidence that it exists?" The following paragraph responds directly to that question.]
When we have an observation that would unambiguously be expected to produce detectable gravitational waves by present or future instruments, that will provide evidence toward settling the argument. [Detection will support the theory; lack of detection will support the challenge.] Until then, you have made your points, and I, like everyone else reading this, have not been persuaded.
Evidence, Jim, not bluster or attacking your critics, is the only way to persuade me. So please let things rest until we have evidence to discuss. We've been going in circles long enough.
[Note to other readers: If Jim decides to insult me or demean me in response to this, as he sometimes does when people give up on having a discussion with him, please recognize that my failure to respond does not mean concurrence or inability to defend myself. It's just that I've had enough.]
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
elusive points, evasive points
February 25, 2008 by jarnold, 1 year 39 weeks ago
Comment: 27777
Fred, when you say:
"My argument rests on the success of a nearly a century of physical theory and observation that supports general relativity." (emphasis added)
you neglect to emphasize “nearly a centuryâ€, or to repeat your frequent enumeration of famous scientists, which you’ve employed elsewhere to support your position. That would have been a more pertinent response to my response to you, although admittedly, it would have undermined your argument. And you might have explicitly conceded that in your more recent message you’ve acknowledged that my position is more than “only a dispute based on not believing in gravitational waves†(a paraphrase), as if I'm taking some sort of religious position. All of this is just to clear away the peripheral objections you’ve raised that might discredit my argument without addressing it. Let’s address it.
You claim that I’m “disputing arguments that have such powerful and long standing observational support.†There is observational support for the interpretations of GR that derive from its characterization as a geometric distortion or curvature of spacetime. There is no unambiguous observational support for the existence of energy-bearing gravitational waves.
You say I’m “in the position of challenger and thus needs to cite observations that demonstrate errors or at least problems with the theory if [I] expect to be taken seriously.â€
I’ve done that. I’ve pointed out the truism often lost on mathematical physicists, that mathematics can be ambiguous in its relation to the physical world; I’ve said I can see no rational explanation of a physical transition from a theory of gravitation as a geometric distortion or curvature of spacetime to force, energy, and/or the production of energy-bearing waves; and I’ve claimed that no one has offered a coherent description of such a transition except by reference to abstract and ambiguous equations. That’s the problem. You can list all the famous scientists that share your expectation, you can count all the years they’ve been confidently expecting verification, but no one has explained how curvature can produce energy, rather than merely redirect it.
“Of course that interpretation will be subject to change if the theory is overthrown by clear evidence. But at this point, no such evidence exists.†What sort of evidence could prove something doesn’t exist if there’s already no evidence that it exists?
“Why is it so disturbing to you that people demand evidence when you are challenging a theory with so much observational support?†Again, there is no unambiguous observational support for the aspects of GR that are based on the association of gravitation with force and/or energy. You’re demanding evidence that energy-bearing gravitational waves don’t exist? So far the lack of evidence for their existence has only resulted in efforts to re-calibrate expectations. How long can that continue?
Unless someone can specifically show how the field equations require that gravitation as a geometric distortion or curvature of spacetime produces energy-bearing waves – without introducing force “through the back doorâ€, there is neither evidence nor theoretical support for gravitational waves. And no amount of ridicule or invoking time-honored authority can make 0 > 0.
Jim's elusive points are not elusive at all
February 25, 2008 by Fred Bortz, 1 year 39 weeks ago
Comment: 27772
To repeat from long ago, which Jim has just echoed:
"My argument rests on the success of a nearly a century of physical theory and observation that supports general relativity." (emphasis added)
So when Jim counters with "A modern scientific argument rests on observations and interpretations," he seems to be supporting me, not disputing me.
In this case, he is disputing arguments that have such powerful and long standing observational support to have earned the designation of "theory" (rather than "hypothesis," "conjecture," or "proposal"). He is in the position of challenger and thus needs to cite observations that demonstrate errors or at least problems with the theory if he expects to be taken seriously.
He has cited no such observations, only an interpretation which no one else finds persuasive. Without evidence to support his thesis while exposing flaws in the the theory, it seems that everyone else is persuaded by existing theory and not Jim's conjectures. I agree with Jim that evidence can change that, but the absence of evidence is not evidence of absence.
Unfortunately for Jim, the absence of evidence is all he can offer in support of his challenge. He notes that gravitational waves have yet to be observed, despite strong theoretical indications that they exist.
In the one observation we were discussing so long ago in this thread, the absence of detection could be legitimately (and was) interpreted as placing the event far beyond the detectable range.
Of course that interpretation will be subject to change if the theory is overthrown by clear evidence. But at this point, no such evidence exists.
Jim, your "elusive" points are, at best, an unsupported proposal. Why is it so disturbing to you that people demand evidence when you are challenging a theory with so much observational support?
Everyone agrees that this difference of interpretation will eventually be resolved by evidence, as discussed elsewhere in this long thread and others. That is the thrust of what people will discover "by pressing and holding the up-arrow."
Since Jim and I both agree the discussion above is sufficient, there is no reason to resume this circular dance, even though Jim has invited me to do so.
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
RE2: It isn't the names or the fame, but the science
February 25, 2008 by jarnold, 1 year 39 weeks ago
Comment: 27765
Fred has written:
Jim attacks with ad hominem nonsense:
"When all else fails your arguments rest on Famous Names, not reason."
My argument rests on the success of a nearly a century of physical theory and observation that supports general relativity as described by Einstein (hence his fame) and elaborated on by Hawking (whose fame rests on his own impressive body of work and his remarkable biography).
My point has eluded you, and therefore strikes you as nonsense. In modern science, it doesn’t matter if your argument rests on a thousand years of physical theory and the opinion of every physicist who’s ever lived, famous or not. A modern scientific argument rests on observations and interpretations, not its longevity or pedigree. One person can undo the interpretations of millennia, and of countless brilliant predecessors. By your standards, as expressed in your repeated references to the time the idea of energy-bearing gravitational waves has prevailed, and the preeminence of those who’ve supported the idea, physics would still be in lock-step with Aristotle and Ptolemy.
More from Fred:
Jim's only dispute with gravitational waves is that he doesn't believe in them.
Again, my point, my dispute has eluded you. (My dispute is available for anyone to see by pressing and holding the up-arrow.) Evidently, you sometimes (at least) read challenging arguments inattentively.
LIGO is useful
February 22, 2008 by Anonymous, 1 year 40 weeks ago
Comment: 27714
I think it is useful as a super sensitive detector for the earth's seismic activities.
Nothing will be wasted. It can be used to warn an impending tsumani and earth quake. But not for the detection of the gravity waves.
Re: Monumental cosmic event
January 10, 2008 by jarnold, 1 year 46 weeks ago
Comment: 26905
A bit ironic that someone defending the paradigm would see me as unwilling to question what's correct or wrong.
When all else fails your arguments rest on Famous Names, not reason.
I've pointed out that there doesn't seem to be a continuity between the transformation of potential to kinetic energy and changes in the distribution of mass - or even (possibly) the loss of relative energy - and a non-tidal gravitational wave. Why should anyone accept a leap as an answer, or a reason for self-doubt?
I wasn't expecting to convert you or "scruffy" anyway. You'll wait for official guidance. But it's a public forum, apparently with lots of silent readers.
And I'm done here. Laugh lots. Rest easy.
It isn't the names or the fame, but the science
January 10, 2008 by Fred Bortz, 1 year 46 weeks ago
Comment: 26907
Jim attacks with ad hominem nonsense:
"When all else fails your arguments rest on Famous Names, not reason."
My argument rests on the success of a nearly a century of physical theory and observation that supports general relativity as described by Einstein (hence his fame) and elaborated on by Hawking (whose fame rests on his own impressive body of work and his remarkable biography).
The work has held up to the scrutiny of observation and analysis by many whose names we don't know nearly as well.
Jim's only dispute with gravitational waves is that he doesn't believe in them. So far, the evidence supporting general relativity also leads the physics community to conclude to the contrary--that gravitational waves ought to exist and merit additional research to test the theories even further.
For those who are interested in a generally non-mathematical history of twentieth century physics, which includes "scientist of the decade" profiles of Einstein (1901-1910) and Hawking (1981-90), please ask your library to carry my Physics: Decade by Decade.
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
Re: It isn't the names or the fame, but the science
January 10, 2008 by Scruffy, 1 year 46 weeks ago
Comment: 26909
Fred wrote: "So far, the evidence supporting general relativity also leads the physics community to conclude to the contrary--that gravitational waves ought to exist and merit additional research to test the theories even further."
I would go one step further - that gravitational waves are ready to be exploited as observational tools. If it was just to test general relativity, I would have thought it a waste of money!
SL
Re: It isn't the names or the fame, but the science
January 11, 2008 by Halliday, 1 year 46 weeks ago
Comment: 26914
SL:
While the search for gravitational waves is fully expected to bear fruit, based upon all the other successful tests of General Relativity, it can still be considered to be both a test of General Relativity and an additional astronomical tool. In fact, the fact that it can be seen as both, in my opinion, makes it even more valuable.
For instance, the Gravity Probe B satellite was created and launched with full expectation that it would not measure anything new, since the parameters (of parameterized post-Newtonian gravity*) it would be sensitive to have already been determined to at least as high precision. However, it was considered to still be well worth it, since it would be a more direct measurement of some of the more novel predictions of General Relativity (like frame dragging).
Of course, the worth of basic scientific investigations are all in the eye of the beholder. :-)
David
* Parameterized post-Newtonian gravity is a tool for clasifying nearly all contenders for General Relativity's crown, and is particularly useful in helping researchers quantitatively see how much uncertainty exists with regard to "validating" General Relativity. (After all, one can never prove a theory, or model. One can only show that it has yet to be invalidated, since it has been upheld by all tests thus far.)
Re2: the relativity of humor
January 10, 2008 by jarnold, 1 year 46 weeks ago
Comment: 26900
"Einstein, Feynman, Hawking, etc. would have been humored!"
Maybe so. Maybe they'd stop laughing long enough to explain how "orbital energy", i.e., kinetic energy, would become "gravitational energy", i.e., non-tidal re-distributions of curvature.
Meanwhile, I'll continue to be astounded (it's too wasteful and unnecessary to be funny) until thinking like the following is finally abandoned:
"... a monumental cosmic event occurring in a nearby galaxy should have generated gravitational waves that would be easily measured by the ultra-sensitive LIGO detectors. The absence of a gravitational wave signal meant GRB070201 could not have originated in this way in Andromeda. Other causes for the event, such as a soft gamma ray repeater or a binary merger from a much further distance, are now the most likely contenders."
Monumental cosmic event
January 10, 2008 by Fred Bortz, 1 year 46 weeks ago
Comment: 26901
A true monumental cosmic event would be Jim giving the slightest credence to the possibility that Einstein, Hawking, and many others may be right about the existence of gravitational waves and he may be wrong.
I'm not holding my breath.
BTW, didn't Scruffy respectfully request that Jim open a new thread rather than hijacking this one?
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
the relativity of humor
January 10, 2008 by jarnold, 1 year 46 weeks ago
Comment: 26891
“Low earth orbit (LEO) satellites experience drag from the atmosphere, slowly robbing them of orbital energy (lost as heat that is radiated away) and they spiral downwards, increasing their orbital velocities. There is never any indication of their orbital velocities decreasing and then increasing. Ask NASA. The same thing happens with the inspiraling binary stars - no orbital velocity decrease, just an increase.â€
You’re treating “orbital energy†as if it’s a unique form of energy, something other than momentum. The atmospheric drag is a drag on “orbital energyâ€, not momentum, i.e., not on the velocity component of the momentum, i.e., not the kinetic energy?
“The binary stars ripple spacetime and that robs them of orbital energy… which is radiated as gravitational waves. The ripples cause the loss, not the other way around!â€
The “ripples†in spacetime are commonly defined as changes in curvature produced by changes in the distribution of mass. Cyclic changes in mass distribution can produce tidal effects, but there’s no legitimate PRESTO beyond that to justify some exotic non-tidal “gravitational energy†being radiated outside the system.
“It is the potential energy component of the orbital energy that is decreasing (getting more negative).â€
You’ve finally identified something specific about your “orbital energy.†The problem is, potential energy is relative. It’s relative to kinetic energy. There’s nothing absolute about it, like rest-mass-energy. If there’s a net decrease of kinetic energy to the system, then the rest of the universe is merely gravitating relative to the system, i.e., ithe expansion of the universe is being slowed by an infinitesimal amount. I don’t know if that’s plausible, but in any case it’s essentially no different than a tidal effect.
Re: the relativity of humor
January 10, 2008 by Burt, 1 year 46 weeks ago
Comment: 26894
Jim wrote: "Cyclic changes in mass distribution can produce tidal effects, but there’s no legitimate PRESTO beyond that to justify some exotic non-tidal “gravitational energy†being radiated outside the system."
You're surely joking again, Mr. Arnold!
Einstein, Feynman, Hawking, etc. would have been humored!
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
History of science podcast
January 9, 2008 by greenmue, 1 year 46 weeks ago
Comment: 26867
Interested in engaging stories about the sciences' past? Come check out my monthly podcast, The Missing Link at http://missinglinkpodcast.com (or search for Missing Link on iTunes).
The Missing Link presents essays on the history of science, medicine, and technology in an engaging and accessible format. Topics have included what African cattle herders can teach us about our desire for quantitative precision, how 1950s sci-films portrayed women scientists films (and how realistic those characters were), how we came to perceive houseflies as disease-ridden pests, what an early-20th century ethnomusicological archive in Berlin can teach us about evolution, and why our common-sense understanding of time hasn't matched many of the scientific and philosophical ways of thinking about it.
For the uninitiated, podcasts can best be described as radio programs that are downloaded from the internet (for listening on your schedule) rather than aired. You don't need an mp3 player to listen. The website (http://missinglinkpodcast.com) has links that will allow you to listen to the program from your computer.
Summary: Gravitational Waves - useful or wasteful?
January 9, 2008 by Scruffy, 1 year 46 weeks ago
Comment: 26853
I think we must accept that gravitational wave astronomy is still in its infancy and it will take decades (and billions of $) to get it fully functional and useful. Like many scientific/engineering projects that push the limits (the 'bleeding edge'), it is late and more expensive and less sensitive than originally planned. That's life. I believe the sensitivity will eventually be reached (at a price) where useful and critical observations will be made through the medium of gravitational waves.
I was initially worried about the wisdom of upgrading LIGO to "Advanced LIGO" in more or less the same time frame that LISA will be put up in space. Thanks to Burt's replies on the wavelength issues, I now understand that it is more cost effective to build shorter wavelength detectors on Earth and longer wavelength detectors in space. They are complimentary, not a duplication.
The "LIGO sheds light on cosmic event", http://www.sciencecentric.com/news/08010708.htm that I reported on earlier may have been a "non-event", but it has hinted that GWs in conjunction with other observational techniques can be very powerful.
So, thumbs up for LIGO/LISA/GEO!
Barking off - Woof!
SL
Four paws up for Scruffy and Burt
January 9, 2008 by Fred Bortz, 1 year 46 weeks ago
Comment: 26866
A great thread, with opportunities to learn about gravitational waves and to discuss political considerations about what we fund and why.
Your summary puts a cherry on the sundae, SL. And Burt's contributions were on point and excellent.
I tried to be the voice of the other readers who were trying to learn along with me, but the two of you deserve the lion's share of credit.
Even Jim's remarks were not completely diversionary, so we don't need to stick him in the doghouse. However, I don't plan to get involved in his thread on the existence or nonexistence of gravitational waves, if he takes up your suggestion. Been there, done that!
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
Re2: Jarnold's Humor
January 9, 2008 by Scruffy, 1 year 46 weeks ago
Comment: 26849
Jim wrote: "There has to be a reduction in the kinetic energy between the pulsars to reduce their mutual orbit. As the distance between them decreases, potential energy converts to kinetic energy, partially stabilizing the orbit."
Low earth orbit (LEO) satellites experience drag from the atmosphere, slowly robbing them of orbital energy (lost as heat that is radiated away) and they spiral downwards, increasing their orbital velocities. There is never any indication of their orbital velocities decreasing and then increasing. Ask NASA. The same thing happens with the inspiraling binary stars - no orbital velocity decrease, just an increase.
Jim: "According to the standard interpretation, gravitational waves are radiated as a product of the degradation of the orbits."
Woof! The binary stars ripple spacetime and that robs them of orbital energy (as Burt properly defined before) which is radiated as gravitational waves. The ripples cause the loss, not the other way around!
Jim: "So what is this “orbital energy†that is “lost†as the kinetic energy decreases and (consequently) increases?"
It is the potential energy component of the orbital energy that is decreasing (getting more negative). Read Burt's calculation above.
Jim: "And what is the primary influence that is degrading the orbit, producing the decrease of “orbital energy�"
Spacetime ripples caused by massive orbiting bodies, resulting in gravitational waves. Ask Einstein. There is no other known mechanism that can do it (not even one that Jim can dream up and defend). And BTW, using a double binary pulsar, the GR prediction has now been confirmed to within 0.1% - that's the experimental error, not a theoretical error!
I think we have exhausted this line of discussion and answered Jim's problems as patiently as possible. I want to ask Jim, if he wants to continue, to kindly open another thread on it in his own Blog, so that we can discuss the science of GWs here.
SL
one person's humor is...
January 8, 2008 by jarnold, 1 year 46 weeks ago
Comment: 26847
Burt quoted me: "… the degradation of the orbits of the pulsars is a reduction in kinetic energy of the orbits, a reduction of relative energy." Then wrote: "Surely You're Joking, Mr. Arnold!.... Ironically, as the orbital energy of the neutron stars reduces, the kinetic energy increases, in complete opposition to what Jim seems to hold."
It’s not so funny if you have to actually define “orbital energy†as something other than lost kinetic energy. And the kinetic energy issue isn’t exactly black and white, is it. There has to be a reduction in the kinetic energy between the pulsars to reduce their mutual orbit. As the distance between them decreases, potential energy converts to kinetic energy, partially stabilizing the orbit. According to the standard interpretation, gravitational waves are radiated as a product of the degradation of the orbits. So what is this “orbital energy†that is “lost†as the kinetic energy decreases and (consequently) increases? And what is the primary influence that is degrading the orbit, producing the decrease of “orbital energy�
Re: Jarnold's Humor
January 8, 2008 by Scruffy, 1 year 46 weeks ago
Comment: 26839
Burt wrote: "PS: Scruffy, sorry for this diversion, but you know how it is when arguing with Jim. I'll rest my case and let you continue with the main thread..."
Yea, I was patiently waiting to summarize the thread... Then I noted an article that may blow new life into this discussion: "LIGO sheds light on cosmic event", http://www.sciencecentric.com/news/08010708.htm
Interestingly, a failure to detect a possible event is hailed as the 'first success' of LIGO! Quote: ‘This is the first time that the field of gravitational wave physics has made a significant contribution to the gamma ray astronomical community, by searching for GRBs in a way that electromagnetic observations cannot.’
The gamma ray burst (GRB) was first thought to be coming from a merger and coalescence of two massive but compact objects, such as neutron stars or black holes in the Andromeda galaxy. LIGO was operating in science mode at the time of the GRB, but detected no gravitational waves. The GRB results then had to be reinterpreted. Interesting stuff.
SL
GW non-detection
January 8, 2008 by Fred Bortz, 1 year 46 weeks ago
Comment: 26841
Anticipating Jim, one might claim that the paper Scruffy cites is further evidence that gravitational waves do not exist or do not carry energy.
Of course, that would make the person asserting such a claim a "leaper," since they would be disputing general relativity.
Following up on Burt's diversion, Jim has two tactics, one of which Burt pointed out. The other is the claim that we are a "chorus" of people so blinded by the success of general relativity that we can't see his unique wisdom.
In one thread, I recall asking Jim why no one else in the physics community seems to share his view. His answer was that he had no idea. He never considers the possibility that his theory is either not novel or not supported by the evidence.
Anyway, the circular argumentation has begun, so I'm going to stay away from this for at least a day or two.
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
RE: GW non-detection
January 9, 2008 by Burt, 1 year 46 weeks ago
Comment: 26851
Hi Fred.
I think Jim has started to ask more pertinent questions, so perhaps he is on the brink of accepting the evidence... Anyway, I see SL has asked him rather politely to start his own thread on the "non-existence of gravitational waves", or something to that effect.
Back to the 'non-event'. I think Andromeda's distance is inside the limits of the present LIGO's ability to detect two neutron stars merging, so the non-detection probably points to some other cause of the gamma ray burst (GRB), or it must be coming from much farther out. LIGO claims 15 Mpc (~50 million light-years) range for such neutron stars, but I guess they may overstate that sensitivity a bit! Nevertheless, Andromeda is only some 0.75 Mpc away. That was the crux - there is enough faith in LIGO's ability to rule out a merger inside Andromeda as a cause of the GRB.
I read in an interview with Kip Thorne (http://discovermagazine.com/2007/nov/the-man-who-imagined-wormholes-and-...)
that he reckons there may be some GW events in the 5th science run data still to be analyzed. The detection of GWs is not like an instrument that sees it and then the bells ring and the lights flash! It can take years to fully analyze one year's worth of recorded data. Since it is government funded, the data will eventually be made available for all to look at and analyze.
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
Jarnold's Humor
January 8, 2008 by Burt, 1 year 46 weeks ago
Comment: 26837
Jim, my comment corrected what was a gross "mis-definition" of orbital energy: You wrote: "...“orbital energy†is entirely kinetic, and therefore relative". Do you recall that statement?
You then wrote: "Again, the degradation of the orbits of the pulsars is a reduction in kinetic energy of the orbits, a reduction of relative energy."
Surely You're Joking, Mr. Arnold!
Ironically, as the orbital energy of the neutron stars reduces, the kinetic energy increases, in complete opposition to what Jim seems to hold.
In order to make a positive contribution, as Jim requested, consider a simple Newtonian scenario with circular orbits and where the spin remains constant. If the orbiting neutron stars lose one unit of orbital energy very gradually, they will settle into a closer, faster circular orbit where the kinetic energy is 1 unit higher and the potential energy 2 units lower, i.e., -2 + 1 = -1 units. The calculations are very simple for the Newtonian case, coming from: E = 0.5mv^2 - GmM/r and v^2 = GM/r. The same principle holds in the relativistic case, it's just a little more complex and there are gravitational waves to consider!:))
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
PS: Scruffy, sorry for this diversion, but you know how it is when arguing with Jim. I'll rest my case and let you continue with the main thread...
Re2: absolutely scruffy
January 8, 2008 by jarnold, 1 year 46 weeks ago
Comment: 26836
"Are we seeing the familiar pattern here?"
Most definitely. Given that the gravitational waves are thought to degrade the orbits, not the rotation or binding energy of the pulsars, your comment is just a distraction. If the rotation and binding energies were thought to be degrading, and contributing to the radiation of gravitational energy, you could make a positive contribution by correcting my definition of energy being "lost", leaving my essential point modified but sustained. As it is, my point remains entirely neglected, and your original argument in support of standard gravitational wave theory unsupported, though obscured.
Again, the degradation of the orbits of the pulsars is a reduction in kinetic energy of the orbits, a reduction of relative energy.
absolutely scruffy
January 7, 2008 by jarnold, 1 year 46 weeks ago
Comment: 26832
What a chorus, you three. Whatever the cause(s) of the orbital decay of the Hulse-Taylor binary system – tidal, magnetic, or some combination, and initiated or accelerated, or not, by some external collision – the orbital decay is undisputed. But what seems to be “lost†is that “orbital energy†is entirely kinetic, and therefore relative. No one is denying what GR predicts, that “changing mass distribution can create ripples in spacetime†[Daniel Sigg, in Burt’s reference to http://www.ligo.caltech.edu/docs/P/P980007-00.pdf]. But the idea of energy-bearing waves presumes a “force†of gravity, a “gravitational energy†which would be absolute, not relative.
Re: absolutely scruffy
January 8, 2008 by Burt, 1 year 46 weeks ago
Comment: 26835
Jim wrote: "But what seems to be “lost†is that “orbital energy†is entirely kinetic, and therefore relative. "
Are we seeing the familiar pattern here? (When losing an argument, change the standard definition of something...)
The orbital energy of a point mass is the total of its kinetic and potential energies. If not a point mass, rotational energy needs to be added and if it is a large, extended mass, gravitational binding energy also comes into play. Any good textbook will tell you this.
For more on binding energy, see e.g.: http://en.wikipedia.org/wiki/Gravitational_binding_energy, with it's authoritative references.
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
Negligible Tidal Effects in Binary Pulsars
January 7, 2008 by Burt, 1 year 46 weeks ago
Comment: 26824
Hi SL, you wrote: "There must be a tiny decrease in pulsar spin rate due to tidal gravity, which works against the inspiral effect, but I have no idea of its magnitude. Perhaps Burt knows."
I didn't, but I found a comment here:
http://relativity.livingreviews.org/open?pubNo=lrr-2006-3&page=articlesu..., talking about the binary pulsar B1913+16.
Quote: "Because the orbital separation is large compared to the neutron stars’ compact size, tidal effects can be ignored."
and:
"The consistency among the constraints provides a test of the assumption that the two bodies behave as “point†masses, without complicated tidal effects, obeying the general relativistic equations of motion including gravitational radiation."
Makes sense. I guess neutron stars are so compact and gravitationally "solid" that they are not easily deformed by a relatively "distant" companion.
[Edit] I checked the last paragraph numerically and got the following: For 1.35 solar mass (each) neutron stars, orbiting at about one solar radius from one another, each star's surface gravity is about 180 Mega-g. That's how hard a neutron star squeezes itself.
The tidal gravity stretch/squeeze caused by the companion (one solar radius away) over the ~20 km diameter of the neutron star is only some 2 milli-g. Negligible.
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
Re: Replying to myself, thanks to Scruffy's comment
January 7, 2008 by Scruffy, 1 year 46 weeks ago
Comment: 26823
Fred: "Perhaps Jim is considering a rare but imaginable situation where some of the translational kinetic energy gets transferred into increasing the rotational energy of each pulsar as they pass one another one at the points of closest approach of elongated ellipses. In that case, they would spin faster as they spiral inward. That would be remarkable and observable"
Rare, imaginable, but AFAIK not what is observed on the binary pulsars. The pulsar periods are remarkably stable, definitely not increasing. There must be a tiny decrease in pulsar spin rate due to tidal gravity, which works against the inspiral effect, but I have no idea of its magnitude. Perhaps Burt knows.
SL
RE7: Gravitational Waves - useful or wasteful?
January 6, 2008 by Fred Bortz, 1 year 46 weeks ago
Comment: 26810
Jim writes:
My understanding is that the waves are a consequence of general relativity, which doesn't necessarily associate gravity with a force. In any case, the potential energy that Jim speaks of is -- TA-DA -- gravitational, not "some exotic energy."
But regardless of whether I'm understanding Jim or misinterpreting his comments, the LISA detector will test the hypothesis that gravitational waves exist. So let's wait for results instead of going in circles about this.
Also, I'm not in touch with the observation of in-spiraling pulsars, but what is the likelihood that we are catching them in a suborbital dance that is the final stages of a collision? It would seem to me that such a collision event would last a very small fraction of a double-pulsar system's lifetime.
Thus on probability grounds, I find the gravitational wave hypothesis to be much more persuasive than the not-quite orbital collision hypothesis--especially since general relativity is continuing to pass all observational tests to date.
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
Replying to myself, thanks to Scruffy's comment
January 6, 2008 by Fred Bortz, 1 year 46 weeks ago
Comment: 26817
Scruffy, you're right. There is no such thing as a "suborbital dance," which Jim was envisioning (and trapped me into considering).
Once the two pulsars are close enough that the only gravitational effects they feel are from each other, their motion will follow conic sections around their common center of mass. If they get trapped into an orbit, it will be elliptical (or circular as a special case), but if they miss each other the first time and don't transfer translational energy into rotational energy, they will continue to orbit indefinitely.
Perhaps Jim is considering a rare but imaginable situation where some of the translational kinetic energy gets transferred into increasing the rotational energy of each pulsar as they pass one another one at the points of closest approach of elongated ellipses. In that case, they would spin faster as they spiral inward. That would be remarkable and observable.
But, if I've been reading this correctly, in-spiraling pulsars have been observed and their pulse rate is not increasing.
Scruffy or Burt, please clarify what has actually been observed. I'm in this discussion only as long as you are. If it's just Jim, I'm outta here, too, Scruffy.
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
RE6: Gravitational Waves - useful or wasteful?
January 6, 2008 by jarnold, 1 year 46 weeks ago
Comment: 26807
SL, you're a leaper: "Tidal gravity makes things spiral away from each other (like the moon-earth combination)."
I wrote that the inspiralling behavior of the pulsars can be explained as the conversion of potential to kinetic energy. Massive bodies approaching each other with trajectories just short of orbital will spiral toward a collision. Your "woofs" seem always to be "goofs."
Back to the question of gravitational waves:
Burt quoted Wikipedia: "...in many cases real matter and energy can be approximated as test particles, situations arise where their appreciable mass (or equivalent thereof) can affect the background gravitational field in which they reside."
This is a description of a second-order effect which, if gravitation is a geometric effect, would seemingly be geometric too.
Consider two pulsars in a stable mutual orbit. Is there energy in their geodesics, like a static charge? I can understand their fields being more intense than would be expected by the sum of each of their particulate masses, due to second-order effects. But why would the geodesics of composite particles produce a "gravitational energy" that would be radiated if, for example, a collision between one pulsar and an asteroid knocked it into an inspiral toward the other pulsar?
The positing of gravitational energy, and its radiation in gravity waves, is a residue of the association of gravitation with force. It's often described as analogous to the electromagnetic radiation produced when an electric charge oscillates along an antenna. But orbiting pulsars are not oscillating - except in the visual field of an astronomer - they are orbiting, each following its geodesic.
There is no reason to posit the existence of some exotic energy, and its radiation, when the conversion of potential to kinetic energy serves as well with the inspiralling of pulsars as it does with any other gravitational approachment.
RE9: Gravitational Waves - useful or wasteful?
January 6, 2008 by Burt, 1 year 46 weeks ago
Comment: 26821
Jim wrote: "Consider two pulsars in a stable mutual orbit. Is there energy in their geodesics, like a static charge?"
Not like in a static charge, but the orbiting pulsars sport plenty of total orbital energy (what SL called "total mechanical energy) and that total remains constant until something robs some energy from the pulsars and take that energy completely out of the system. If there is a once-of reduction in total energy, the orbit will become slightly closer and then remain so. Only if there is a continuous energy reduction will the binary stars spiral inward. The mechanism of this energy reduction is GWs.
Jim: "But why would the geodesics of composite particles produce a "gravitational energy" that would be radiated if, for example, a collision between one pulsar and an asteroid knocked it into an inspiral toward the other pulsar?"
The sort of inspiral that you talking about here is totally different from the one I described above and which is presently being observed. Orbital mechanics demand that the sort you describe completes less than one orbit, which I think disqualifies it as a proper inspiral. However, should such an event happen, both collisions (the asteroid-star and the star-star) will radiate a nice quantity of GWs!
Jim: "The positing of gravitational energy, and its radiation in gravity waves, is a residue of the association of gravitation with force. "
Actually, it's a "residue" of Einstein's GR and although difficult to see in the field equations, there are approximations that bring it out easily (see http://www.ligo.caltech.edu/docs/P/P980007-00.pdf). There were originally misgivings about GWs, but I think the binary pulsar observations silenced all but a few. The issue is, GR is a completely consistent theory: you can't trust one piece of it and ignore another piece!
Jim: "There is no reason to posit the existence of some exotic energy, and its radiation, when the conversion of potential to kinetic energy serves as well with the inspiralling of pulsars as it does with any other gravitational approachment."
I hope that after SL's 'barks' and my discussions above, you realize your mistake and refrain from making more such orbital blunders - it is costing you dearly in credibility...
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
RE8: Gravitational Waves - useful or wasteful?
January 6, 2008 by Scruffy, 1 year 46 weeks ago
Comment: 26816
Jim wrote: "SL, you're a leaper: ''Tidal gravity makes things spiral away from each other (like the moon-earth combination).''"
These words of wisdom came from a man who apparently does not understand basic orbital mechanics, because he followed with this gem of a 'goof':
"I wrote that the inspiraling behavior of the pulsars can be explained as the conversion of potential to kinetic energy. Massive bodies approaching each other with trajectories just short of orbital will spiral toward a collision. Your "woofs" seem always to be "goofs."
Woof, woof!
Massive bodies "approaching each other with trajectories just short of orbital" will go into elliptical orbits around their common center of mass (COM). They will keep these orbits indefinitely, unless they loose total mechanical energy (TME) relative to the COM (TME = kinetic (orbital velocity) + potential + rotational energies). Binary pulsars do not "stay there", because they loose TME through gravitational wave radiation and hence spiral inwards. It may take millions of years for the inspiral to result in a collision, depending on the distance they were formed from each other.
Enough said. I'll 'bark out' and leave the rest to Fred and Burt (at least for as long as Jim is around).:(
SL
Geodesics and Gravitational Waves
January 5, 2008 by Burt, 1 year 47 weeks ago
Comment: 26786
Hi SL, you wrote: "Geodesics of two massive objects are not like the simple geodesics when we have one large mass and one small mass, with only 2nd order effects significant. I think there are higher order effects that complicate these geodesics."
You're right. Wikipedia says: "True geodesic motion is an idealization where one assumes the existence of test particles. Although in many cases real matter and energy can be approximated as test particles, situations arise where their appreciable mass (or equivalent thereof) can affect the background gravitational field in which they reside. This creates problems when performing an exact theoretical description of a gravitational system (for example, in accurately describing the motion of two stars in a binary star system)."
However, good approximations exist for such conditions and the gravitational wave radiation components can be extracted very accurately from it, e.g. http://www.ligo.caltech.edu/docs/P/P980007-00.pdf, which I used as a reference in my eBook.
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
RE: Geodesics and Gravitational Waves
January 6, 2008 by Scruffy, 1 year 46 weeks ago
Comment: 26804
Burt wrote, replying to Fred:
"From Sigg's paper that I referenced before, it appears as if the "strain" will be inside the present LIGO's range, but the frequency (~0.1 Hz) will be way to low for detection by LIGO."
I can understand that 0.1Hz requires an impossibly long 'antenna', but what puzzles me is that LIGO is supposed to be working in the 10Hz to 10kHz ("audio") band. In order to be at least quarter-wave at 1 kz (mid-range), an antenna must still be about 75km long. I believe LIGO's arms are just 4km. How do they get any sensitivity around the mid-range? Or doesn't GW antennas work like EM antennas?
SL
RE2: Geodesics and Gravitational Waves [Edit]
January 6, 2008 by Burt, 1 year 46 weeks ago
Comment: 26806
Hi SL, you asked: "I believe LIGO's arms are just 4km. How do they get any sensitivity around the mid-range? Or doesn't GW antennas work like EM antennas? "
Where EM antenna lengths need to be light-speed resonant to the signal frequency for maximum reception, GW antennas use a different scheme of resonance. It has to do with the natural resonant frequency of the system, e.g. a bar of aluminum with a 1 kHz natural frequency (depending on the speed of sound in the bar). This was the idea of the first detectors (Weber bars).
LIGO uses resonant laser light inside so-called Fabry-Perot cavities, where the laser light is amplified by being reflected backwards and forwards many times. The idea is that when a GW comes by, it will upset the resonant dimensions slightly and that change can be detected.
The length of the arms needs to be maximized, because the longer, the larger the effects of the GW. So why do we need a space-based 'long-arm' system for lower frequencies? I'm not sure, because I think the amplitude of the low frequency waves (like two supermassive black holes merging) are as high or higher than the high frequency ones.
I'll try and find the rationale behind this issue and report back (unless someone knows the answer and can give us the reference). :-)
Edit The secret lies in the "laser light is amplified by being reflected backwards and forwards many times" that I mentioned above. It works like a 'folded antenna' that gives each 4 km arm an effective ~1000 km length. (http://www.ligo.caltech.edu/docs/P/P980007-00.pdf)
LISA's space antennas cannot be 'folded' like this, because the distance between the satellite cannot be kept precisely constant. NASA plans to simply use a long enough arm (~5 million km) and strong enough lasers.
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
RE5: Gravitational Waves - useful or wasteful?
January 4, 2008 by Scruffy, 1 year 47 weeks ago
Comment: 26785
Jim wrote on the in-spiraling binary quasars and agreement with gr:
"Actually it's not in "exact correspondence." Either dynamic will produce similar results."
SL: OK, it's within 1%, which was the experimental uncertainty. If the "other dynamic" that you refer to is tidal gravity, then woof! (again). Tidal gravity makes things spiral away from each other (like the moon-earth combination).
JA: "I'd be glad just to have one scientist explain how geodesic motion can radiate energy."
SL: I have sympathy with that, because the math is horrendous. The best layman description of grav. waves that I've read has to do with the fact that tidal gravity operates like the "near field" of a transmitter antenna, which actually forms the "real antenna" for the EM radiation that propagates energy away. In a way, tidal gravity, with its short range, sets up a "near field antenna" that radiates away long range gravitational waves. (I'll have to search for the source of this description).
Geodesics of two massive objects are not like the simple geodesics when we have one large mass and one small mass, with only 2nd order effects significant. I think there are higher order effects that complicate these geodesics. Maybe Burt can help us out here.
SL
RE4: Gravitational Waves - useful or wasteful?
January 4, 2008 by jarnold, 1 year 47 weeks ago
Comment: 26764
You're a little too quick with your hind leg, scruffy.
J: "The standard interpretation of the effects of the inspiralling pulsars is an excellent example of the pre-relativistic legacy still weighing on gravitation-theory."
Woof1! The in-spiraling comes out of the heart of general relativity and is totally absent in Newtonian physics!
The interpretation of the in-spiralling comes more from Mach's influence, and the quantum association of gravitation with force.
J: "... and the "lost energy" is just a conversion of their relative potential energy to kinetic energy."
Woof2! Conversion of relative potential energy to kinetic energy is not lost energy. It happens all the time in every stable orbit.
I didn't say it's "lost energy." That's your story. I'm said the "lost energy" is just the conversion between the pulsars of potential to kinetic.
J: "'Gravitational waves' are propagated due to the periodic changes in their combined gravitational field as each orbits the other, whether they are inspirally or not, ..."
Woof3! What you describe is tidal gravity, not gravitational waves. They are two totally different animals. Woof!
You're presuming what needs to be justified. Or are you content to say "there are non-tidal gravity waves because there are non-tidal gravity waves"?
J: "... and in either case there is no reason to believe the waves carry energy - any more than the orbit of the moon propagates energy-bearing waves toward earth."
(SL): The in-spiraling of the binary pulsars is due to the fact that gravitational waves carry energy away in exact correspondence with general relativity's prediction.
Actually it's not in "exact correspondence." Either dynamic will produce similar results.
(SL): "Are we seeing the same pattern here that was apparent before: Jim against the rest of the science world?"
I understand you find that meaningful. I'd be glad just to have one scientist explain how geodesic motion can radiate energy.
Re: Gravitational wave economics
January 4, 2008 by Fred Bortz, 1 year 47 weeks ago
Comment: 26762
Far be it from me to judge whether NASA or the NSF or foreign scientific research organiztions ought to be budgeting money at this level of detail. Let the researchers make their case, as they usually do, in the form of proposals to funding agencies.
The only test of his theories that Jim has proposed is his claim that, contrary to presently accepted theory, gravitational waves should carry no energy at all.
The fact that LIGO is underway indicates that the physics community deems it important to evaluate the important prediction of general relativity that gravitational waves exist and are detectable (which means they carry energy). I'm surprised that Jim doesn't agree that these measurement are worth doing.
I think we need to look into that project to decide where this discussion ought to go, but my understanding is that the observation of two collding supermassive black holes gives the best opportunity so far to study the supposed ripples in spacetime.
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
Re2: Gravitational wave economics
January 5, 2008 by Burt, 1 year 47 weeks ago
Comment: 26787
Hi Fred, you wrote:
"I think we need to look into that project to decide where this discussion ought to go, but my understanding is that the observation of two colliding supermassive black holes gives the best opportunity so far to study the supposed ripples in spacetime."
Yea, maybe it will be the best show of gravitational waves, but rather unlikely to happen! Supermassives are at the core of galaxies and although we observe galaxies colliding, the process takes millions of years to complete. The more likely are coalescing neutron stars and black holes, with neutron stars being the more abundant, I reckon.
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
Re3: Gravitational wave economics
January 5, 2008 by Fred Bortz, 1 year 47 weeks ago
Comment: 26789
Burt agrees that the collision of two supermassive black holes "will be the best show of gravitational waves," but considers that "rather unlikely to happen."
And although the full event will take millions of years to unfold, it will be producing substantial ripples in spacetime throughout the event.
It's a big universe out there, with galactic collisions happening all the time. When I googled the exact phrase "collision of two supermassive black holes", the result was several websites, including some that discuss how LISA will be looking for such events and one credible website article that discusses the possibility that one has been spotted.
The question is not when and whether it is happening but where? Is it close enough to detect?
I guess the people who are funding LISA think it is likely enough to find such a collision, though they will be looking at other GW possibilities as well.
An interesting discussion here. Thanks Scruffy for raising the question of economics in the scientific quest.
It also applies to one of my favorite speculative searches, SETI, which is discussed in my recent middle-grade book Astrobiology.
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
Re4: Gravitational wave economics
January 5, 2008 by Burt, 1 year 47 weeks ago
Comment: 26790
Fred, could you pass the link to that "specific credible website article that discusses the possibility that one [collision of two supermassive black holes] has been spotted"?
I'm skeptical about the probability of such an event happening in out very limited time frame. AFAIK, the actual black hole merger will probably be over in less that a year, with the detectable gravitational wave signature not lasting more than a few days.
But, it will be very exiting if I'm wrong!
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
It's a Discover article from 11/02
January 5, 2008 by Fred Bortz, 1 year 47 weeks ago
Comment: 26791
http://discovermagazine.com/2002/nov/breakblack
It's a brief article called "Black Holes Flip Out" by Kathy A. Svitil. I probably overstated its content. It is an exciting prospect, but it is still no more than a prospect.
Here's the closing sentence: "So far, we have only indirect evidence of such mergers, but the LIGO detectors in Louisiana and Washington State may be able to pick up their gravitational screams."
The earlier paragraphs describe the indirect evidence.
It isn't clear for how long the waves would be detectable.
But it is clear from a 1998 Phys. Rev. D abstract that the designers of LISA expect a reasonable chance of such detection.
They write
The Google search, when the phrase is in quotation marks, turns up seven articles. It seems like a reasonable way for readers to start educating themselves on this possibility.
Waving gravitationally and otherwise,
Fred
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
RE: It's a Discover article from 11/02
January 6, 2008 by Burt, 1 year 46 weeks ago
Comment: 26801
Hi Fred.
I checked on the possible signal strength (strain) and frequency for two supermassive black holes. From Sigg's paper that I referenced before, it appears as if the "strain" will be inside the present LIGO's range, but the frequency (~0.1 Hz) will be way to low for detection by LIGO. So Kathy's closing statement:
"So far, we have only indirect evidence of such mergers, but the LIGO detectors in Louisiana and Washington State may be able to pick up their gravitational screams.",
is apparently overly journalistic optimistic! LISA should fare better. :)
Regards,
Burt Jordaan (www.Relativity-4-Engineers.com)
RE3: Gravitational Waves - useful or wasteful?
January 4, 2008 by Scruffy, 1 year 47 weeks ago
Comment: 26761
While I'm not as positive as Burt seems to be on the value of gravitational wave research, I find Jarnold's response significantly off-the-mark, e.g:
J: "The standard interpretation of the effects of the inspiralling pulsars is an excellent example of the pre-relativistic legacy still weighing on gravitation-theory."
Woof1! The in-spiraling comes out of the heart of general relativity and is totally absent in Newtonian physics!
J: "... and the "lost energy" is just a conversion of their relative potential energy to kinetic energy."
Woof2! Conversion of relative potential energy to kinetic energy is not lost energy. It happens all the time in every stable orbit.
J: "'Gravitational waves' are propagated due to the periodic changes in their combined gravitational field as each orbits the other, whether they are inspirally or not, ..."
Woof3! What you describe is tidal gravity, not gravitational waves. They are two totally different animals. Woof!
J: "... and in either case there is no reason to believe the waves carry energy - any more than the orbit of the moon propagates energy-bearing waves toward earth."
The in-spiraling of the binary pulsars is due to the fact that gravitational waves carry energy away in exact correspondence with general relativity's prediction.
J: "The periodic variations in the gravitational field the pulsars exert here on earth is infinitesimal. Their gravitational field itself is infinitesimal here."
More evidence that you describe tidal gravity (periodic periodic variations in the gravitational field) and not gravitational waves. AFAIK, tidal gravity effects fall of with the cube of distance (i.e., rapidly), while gravitational wave amplitudes fall off linearly with distance, i.e. much slower.
Are we seeing the same pattern here that was apparent before: Jim against the rest of the science world?
SL
Re4: Gravitational Waves - useful or wasteful?
January 4, 2008 by Fred Bortz, 1 year 47 weeks ago
Comment: 26763
Scruffy, you're seeing exactly the trap that Jim got himself into on some long lost discussions, where he was comparing gravitational waves to the movement of tides on Earth.
That's why I didn't want to reopen this discussion.
Anyway, I predict a reprise of the old circular argument as long as you respond to Jim. It's your choice, but I advise letting him have the last word. Your "woofs" are kinder versions of the satirical Gadfly's "bites of realism," which probably explains Gad's silence here.
Fred Bortz -- Science and technology books for young readers (www.fredbortz.com) and Science book reviews (www.scienceshelf.com)
RE2: Gravitational Waves - useful or wasteful?
January 4, 2008 by jarnold, 1 year 47 weeks ago
Comment: 26758
The standard interpretation of the effects of the inspiralling pulsars is an excellent example of the pre-relativistic legacy still weighing on gravitation-theory.
If you think of the inspiralling pulsars as each moving along its geodesic in mutual orbit, there is no force involved, and the "lost energy" is just a conversion of their relative potential energy to kinetic energy. "Gravitational waves" are propagated due to the periodic changes in their combined gravitational field as each orbits the other, whether they are inspirally or not, and in either case there is no reason to believe the waves carry energy - any more than the orbit of the moon propagates energy-bearing waves toward earth.
The periodic variations in the gravitational field the pulsars exert here on earth is infinitesimal. Their gravitational field itself is infinitesimal here. So yes, the efforts to detect the waves are wasteful, and what's worse, theoretically unjustified.
RE: Gravitational Waves - useful or wasteful? [Edit]
January 5, 2008 by Burt, 1 year 47 weeks ago
Comment: 26757
I think the reason why there were no LIGO detections to date is a slight lack of sensitivity, combined with the fact that no event strong enough (or close enough) to be detected at the achieved sensitivity has taken place. LIGO's bandwidth is roughly the audio spectrum (10 Hz to 10 KHz), which is where neutron stars that spiral into each other should radiate strongly.
I'm not sure, but I think we would need such an event inside our Local Group to be able to detect it with the present LIGO. What the probability of that is, I don't know. [Edit] From the LIGO website, the present range for detection is about 15 Mpc, just short of the Virgo super-cluster's center. They are aiming to double that range during 2008, for a new "Science run" during 2009.[/edit]
If one can increase the sensitivity tenfold, the probability increases 1000-fold, because that's the volume increase. (As SL said, the magnitude of gravitational waves decreases linearly with distance). [Edit] The 10-times increase in range must wait for "advanced LIGO" and is scheduled for operation around 2015. This will include the Coma Great Wall.[/edit]
Apart from increasing the sensitivity, it will also help if the bandwidth is increased. That's where LISA comes in. LIGO has two 4km orthogonal arms, limiting the bandwidth to the Hz range. The space-based LISA can have arms a thousand times longer (or more), giving the possibility of milli-Hz detection with a thousand times the sensitivity as well. The sensitivity on Earth is limited by many noise sources, including waves hitting the shores, Earth tremors and even traffic on the roads!
Is it worth the bother? If it was just for the sake of detecting gravitational waves, then no, but if it opens up a whole new branch of astronomy, then yes. It might then be possible to observe aspects of the universe that would otherwise have remained hidden forever.
Burt Jordaan (www.Relativity-4-Engineers.com)