Gamma ray burst associated with LIGO GW event

In summary, a gamma ray burst was detected in conjunction with the LIGO GW event, providing strong evidence for the merger of two neutron stars. This event marked the first time that gravitational waves and electromagnetic radiation were observed simultaneously, confirming the existence of kilonovae and shedding light on the origins of heavy elements in the universe. The detection of the gamma ray burst also provided valuable information about the properties of the merging neutron stars, furthering our understanding of these mysterious objects.
  • #36
Jonathan Scott said:
The paper looks into the statistics quite thoroughly.

True. But I don't find the statistics convincing: a common flaw of a posteriori significance calculations. What does the paper say? It says there were no events passing their requirement. They they changed this, and changed that, until they got a signal compatible with LIGO (and two dozen other signals). Now I don't want to say this procedure is generating a fake signal, but I am saying that once you go down this path it becomes pretty much impossible to calculate a p-value for whatever you find.
 
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  • #37
My point is only stronger if the probability is 0.22% that the gamma-ray detection is real. The core of Bayesian thinking is the recognition that you only rule out unlikely things if likelier ones already exist. But if you already know that something unlikely has happened, then the least unlikely becomes the probable. So here, we have a 0.22% chance that noise could look like a signal, but we must compare that to the chance that a black-hole mergers have been going on all this time, and were not previously noticeable by Fermi, but suddenly we can see them if we know when to look. That is already quite unlikely, and we cannot assess the significance of a 0.22% chance of noise looking like a signal, until we can assess the relative likelihood of Fermi having all these detections just below our ability to notice.
 
  • #38
Ken G said:
My point is only stronger if the probability is 0.22% that the gamma-ray detection is real. The core of Bayesian thinking is the recognition that you only rule out unlikely things if likelier ones already exist. But if you already know that something unlikely has happened, then the least unlikely becomes the probable. So here, we have a 0.22% chance that noise could look like a signal, but we must compare that to the chance that a black-hole mergers have been going on all this time, and were not previously noticeable by Fermi, but suddenly we can see them if we know when to look. That is already quite unlikely, and we cannot assess the significance of a 0.22% chance of noise looking like a signal, until we can assess the relative likelihood of Fermi having all these detections just below our ability to notice.
Again, I'm fairly sure this is addressed in the Fermi GBM paper by V Connaughton et al. Their normal trigger for a checking for an event is an unusually high count. However, in this case the number of counts in the relevant interval was not very significantly far above average for anyone energy bin, but the fact that a whole range of energy bins all gave somewhat above-average counts at the same time, specifically for the second after the event, is very interesting. Applying similar filtering to an extended period, they got a few other occasional matches, and they used that to determine the probability of a random timing match. I don't fully understand the details, but they are explained in the paper.
 
  • #39
They do not include any Bayesian analysis that involves the prior unlikeliness that exactly the kind of signal that flies under their radar, but is accessible after the fact, is what is sent out by exactly the kind of event that is the first type detectable by LIGO.
 
  • #40
Ken G said:
They do not include any Bayesian analysis that involves the prior unlikeliness that exactly the kind of signal that flies under their radar, but is accessible after the fact, is what is sent out by exactly the kind of event that is the first type detectable by LIGO.
The "kind of signal" is merely a weak one, below their normal trigger threshold, that would normally be of no interest. It is only the timing relative to the LIGO event that is highly suggestive.

I'd be interested to know how you think the statistics should be modified. Are you saying that you'd assign some prior probability that there would be no gamma ray burst, based on some theoretical expectations about this situation which has never been experimentally observed before?
 
  • #41
Jonathan, as a layman, I wonder how is it possible to assume that the gravitational waves are coming from black holes, considering that we have zero convincing proof that black holes exist. Wouldn't make more sense to, first proove the black holes existence, and then, try to detect their gravitational waves?
 
  • #42
Jonathan Scott said:
The "kind of signal" is merely a weak one, below their normal trigger threshold, that would normally be of no interest. It is only the timing relative to the LIGO event that is highly suggestive.
Which is entirely my point. Whenever one is asking the question "how likely is this to be random chance", one always has to know what one is comparing the likelihood to. It's a complicated situation when the only reason the signal is regarded as interesting is when it happened. It means that something unexpected occurred, but it is no simple matter to decide which is the more likely unexpected result: that black hole mergers produce just enough gamma rays to make a signal that is only detectable by virtue of its timing (when it could have made no signal at all, or a signal that is easy to detect without timing), or that an unlucky noise event just happened to occur at that time. Fortunately, the issue will quickly be decided, as this merger event is not regarded as unique, and correlations between multiple observations should easily resolve the issue. I'm just saying I'm not convinced the 0.22% number means anything at all, until the careful comparison I'm talking about has been made in some more formal Bayesian sense.
I'd be interested to know how you think the statistics should be modified.
The Bayesian approach would be to assess some kind of prior expectation that a black hole merger would produce a gamma ray signal that is only detectable if you include its timing. The fact that this prior expectation is not easy to assess is merely the evidence that whether or not the result can be viewed as significant may depend on initial assumptions. It is certainly a logical fallacy to conclude that because something non-generic happened, implies that a detection has occurred, rather than simply an unlikely noise event. The issue is the difference between absolute probabilities and relative probabilities.
Are you saying that you'd assign some prior probability that there would be no gamma ray burst, based on some theoretical expectations about this situation which has never been experimentally observed before?
It is essential to include theoretical expectations of that nature. This is clear, you only have to ask yourself what if that exact same paper had appeared, except that the timing was not the black hole merger, but rather the event of the death of some famous world figure. No one would take it seriously that the death of a world figure can produce gamma rays, so the 0.22% would have no importance posed against our extreme skepticism of its plausibility. So it's all Bayesian analysis, it's merely a question of whether it is formally acknowledged, or simply implied informally. It certainly is reason to look for correlations of a similar type for all other gravitational wave events, but it will be a long time before there can be any confidence in this detection.
 
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  • #43
myuncle said:
Jonathan, as a layman, I wonder how is it possible to assume that the gravitational waves are coming from black holes, considering that we have zero convincing proof that black holes exist. Wouldn't make more sense to, first proove the black holes existence, and then, try to detect their gravitational waves?
Gravitational waves depend on the mass and motion of the bodies, and are not affected by whether they are black holes. The point at which the amplitude of the wave peaked and then tapered off is presumably the point at which the bodies merged, so it gives some clues as to their sizes, which must clearly have been extremely dense, compatible with GR predictions of black holes.
 
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  • #44
Jonathan Scott said:
Black holes are not even supposed to be able to have magnetic fields (unlike neutron stars which can have extremely strong magnetic fields)!

A *stationary* black hole can have only electric field, not magnetic, yes.

But a *moving* electric change (any change, including a charged black hole) is seen as generating magnetic field.

This is just a consequence of the fact that electromagnetic potential is a four-vector, and if it has only temporal non-zero component in one coordinate system, it will have non-zero spatial components too in other coordinate systems after Lorentz transform.
 
  • #45
nikkkom said:
A *stationary* black hole can have only electric field, not magnetic, yes.

But a *moving* electric change (any change, including a charged black hole) is seen as generating magnetic field.

True. To be more accurate I should have said that a black hole doesn't have any intrinsic magnetic field.

However, that's not really very relevant. Note that black holes are not expected to be able to pick up much electric charge anyway (since that would generally repel particles with the same charge more strongly than gravity would attract it).
 
  • #46
Do they really need to have "much" electric charge?
A "slightly" charged pair of 30 Msun objects, orbiting each other with nearly light-speed velocities, may end up having a substantial magnetic field. Whet it all decays, where all its energy goes? I say don't discount electromagnetics yet for this case.
 
  • #47
nikkkom said:
Do they really need to have "much" electric charge?
A "slightly" charged pair of 30 Msun objects, orbiting each other with nearly light-speed velocities, may end up having a substantial magnetic field. Whet it all decays, where all its energy goes? I say don't discount electromagnetics yet for this case.
You're welcome to try a calculation, but I'd guess that's many orders of magnitude too small to be relevant.
 
  • #48
Jonathan Scott said:
Gravitational waves depend on the mass and motion of the bodies, and are not affected by whether they are black holes. The point at which the amplitude of the wave peaked and then tapered off is presumably the point at which the bodies merged, so it gives some clues as to their sizes, which must clearly have been extremely dense, compatible with GR predictions of black holes.
Extremely dense, ok, but is it enought as a proof of black holes existence? Considering that something like a black hole is incredibly big to claim, don't you think that an incredibly strong proof should be need to support this claim?
 
  • #49
myuncle said:
Extremely dense, ok, but is it enought as a proof of black holes existence? Considering that something like a black hole is incredibly big to claim, don't you think that an incredibly strong proof should be need to support this claim?
No-one has said that this proves black holes exist. The gravitational wave observation gave results which indicated two massive objects spiralling together and merging, and various parameters used to fit the results show that the objects had masses sufficiently large and radii sufficiently small that GR says they have to be black holes, if it is still correct in this extreme case, which is what is generally assumed. It was a really beautiful experimental result which neatly confirmed theoretical predictions.

However, the apparent gamma ray burst raises a challenge. If it is real and really associated with the GW event, then one potential "simple" explanation would be that GR isn't quite right and what collided was actually something like a pair of neutron stars or quark stars, so the gamma ray burst was energy being given off from that collision. Given that GR is the best theory of gravity that we have, that would be a nasty surprise to have to face, so even though the evidence for an associated gamma ray event seems fairly clear at first glance, it is a case where extraordinary claims require extraordinary proof. My guess is that any explanation that appears to be consistent with current GR, however contrived, will be considered far more plausible that the idea that black holes may not exist, although I'm personally very interested in that possibility.
 
  • #50
Jonathan Scott said:
No-one has said that this proves black holes exist. The gravitational wave observation gave results which indicated two massive objects spiralling together and merging, and various parameters used to fit the results show that the objects had masses sufficiently large and radii sufficiently small that GR says they have to be black holes, if it is still correct in this extreme case, which is what is generally assumed. It was a really beautiful experimental result which neatly confirmed theoretical predictions.

However, the apparent gamma ray burst raises a challenge. If it is real and really associated with the GW event, then one potential "simple" explanation would be that GR isn't quite right and what collided was actually something like a pair of neutron stars or quark stars, so the gamma ray burst was energy being given off from that collision. Given that GR is the best theory of gravity that we have, that would be a nasty surprise to have to face, so even though the evidence for an associated gamma ray event seems fairly clear at first glance, it is a case where extraordinary claims require extraordinary proof. My guess is that any explanation that appears to be consistent with current GR, however contrived, will be considered far more plausible that the idea that black holes may not exist, although I'm personally very interested in that possibility.

Thanks Jonathan.
 
  • #51
myuncle said:
Jonathan, as a layman, I wonder how is it possible to assume that the gravitational waves are coming from black holes, considering that we have zero convincing proof that black holes exist. Wouldn't make more sense to, first proove the black holes existence, and then, try to detect their gravitational waves?

Science doesn't prove anything exists. Proofs are for mathematics. What science does is give evidence for models. There is evidence for black holes, though perhaps not conclusive evidence. (IMO, the evidence is pretty conclusive.)

The detection of these gravity waves is another solid piece of that evidence. The gamma burst both confirms the broad model (blackholes exist) and undermines the specifics (black holes "look" like what we think they look like) of that model. So the data holds exciting possibilities of a closer matching of the model with reality (whatever that is).

But we need to remember science is about the observable and the repeatable. So one data point has no meaning on its own. Ideally we will detect a lot more gravity waves with or without gamma bursts. Then we will know more.
 
  • #52
The Model I found most feasible to generate a GWave and GRBurst
was the Merger of Two Large Stars.

As Yen and Yang merged, their combined Gravitational Field caused
each to collapse into 2 counter rotating Black Holes
which then formed a rotating QuadroPole which generated the GWave
seems the infall of the 2 star's remaining fuel supply then created a GRBlast a fraction of a Second later?

A portion of this GRBurst could have occurred Inside the Event Horizon
thus weakening the strength of the signal received on Earth, imo.
 
  • #53
A number of off-topic posts have been removed. Please stick to the facts of the topic and not to personal opinions about science in general.
 
  • #54
Both of the detections were also poorly localized. I'm curious, would it be expected that IceCube would detect anything?
 
  • #55
Neutrinos are produced by nuclear fusion, so none would be expected for a black hole merger. Even for a hypothetical neutron star merger, most of the material would already be fused into neutronium, so very little neutrino emissions would be expected. Huge amounts of neutrinos are however produced by stellar collapse to a neutron star as in a supernova.

The Wikipedia article First observation of gravitational waves has brought together a lot of useful information. It mentions that Icecube only saw three neutrinos around that time, which is compatible with background levels, and that none of them was in a direction which matched the likely direction of the gravitational wave or gamma ray detection.

In John Baez's blog entry mentioned by Greg earlier in this thread, he mentions that Tony Wells pointed out to him that the lack of neutrinos is evidence against the event having taken place inside a large collapsing star, as suggested by Loeb. However, neutrinos are of course very difficult to detect, so the absence of detection only places weak constraints on possible theories.
 
  • #56
Jonathan Scott said:
Quite unexpectedly, it seems that the Fermi Gamma-ray Burst Monitor spotted what appears to be a hard gamma-ray burst about 0.4s after the LIGO GW event, lasting about 1s: http://arxiv.org/abs/1602.03920

Maybe this burst came from another astronomical event?
 
  • #57
greswd said:
Maybe this burst came from another astronomical event?
Yes, that is of course possible, but it occurred within a second of the LIGO event and probably within the same less than 1% of the sky. Based on the average rate of such weak events, the Fermi GBM team estimated what they called the "false alarm" probability as 0.0022. Read the paper for more details of what that means.
 
  • #58
Yes, the "false alarm" probability applies to ruling out other astrophysical events. My point is that it does not apply to ruling out a non-event, because that would require comparison of the small probability of a noise event to the small probability that a black hole merger makes a signal that cannot be identified as such without coincident gravitational wave detections. Both of those likelihoods are quite small, so the question that is not addressed by the false alarm probability is the question of which of those likelihoods is the smaller. That depends on assumptions about the source, as per my analogy with the death of a famous world figure.
 
  • #59
Jonathan Scott said:
. The gravitational wave observation gave results which indicated two massive objects spiralling together and merging, and various parameters used to fit the results show that the objects had masses sufficiently large and radii sufficiently small that GR says they have to be black holes, if it is still correct in this extreme case, which is what is generally assumed.
It was a really beautiful experimental result which neatly confirmed theoretical predictions..

Apparently we can expect this experimental Result to be repeated about Once every year ?

Gravitational Waves are the Result of the rapid Acceleration of Mass that is distributed unevenly, ie nonSpherical ?
apparently this Configuration of Matter is predicted by GR to be a QuadruPole

As I understand it, Two Masses in rapid orbit will Not generate a significant GW
until they rapidly Accelerate towards each other
when their Combined Gravity overcomes the Centrifugal Forces pulling them apart.

It is hard to imagine all the dynamics involved in these 2 Masses merging
given we have no exact Values of the Parameters in this Experiment nature has provided in such a timely manner.

Monte Carlo modeling of possible combinations of Mass, Density, Elements Involved, Orbit Velocities,
Rotational Directions and Velocities, Etc... can only suggest what actually happened
and many Models might explain what we can barely observe;
due to the exxxxxxxxxtremely small measurements required to detect a GWave originating thousands of LightYears away..

So, What ShapeS would the Surface of 2 Black Holes form during collapse/merger into a single Singularity ??

First theSimplest Example: With No Orbital Velocities and No Rotational Velocities .

Seems the 2 Spheres would form a Dumbell or Hour Glass Shape very briefly
if there are no Centrifugal Forces to overcome ?
Also brief because the Radius of Black Holes is relatively small considering their MASS.

Adding Orbital Velocities and Rotational Spins near Light Speed to the above
could complicate the mathematical models a bit .
 
  • #60
Two highly confident observations of an event within microseconds of each other.
Yet one of them supports what GR predicts, and the other is unexpected.
I'd say this one should run for a while.
 
  • #61
looking4sophia said:
Apparently we can expect this experimental Result to be repeated about Once every year ?

I'm curious why?

The rapidity of the first observation would indicate lots more to come, but with a sample size of one, even that's just a guess/hope.

Given how big space is, these might be going off all the time, but probably not as large/strong and perhaps most of them are undetectable with current detectors.

I'm guessing budget increases might give better equipment and more data.
 
  • #62
rootone said:
Two highly confident observations of an event within microseconds of each other.

Well, within 400,000 microseconds of each other...
 
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  • #63
Jeff Rosenbury said:
I'm curious why?

The rapidity of the first observation would indicate lots more to come, but with a sample size of one, even that's just a guess/hope.

Given how big space is, these might be going off all the time, but probably not as large/strong and perhaps most of them are undetectable with current detectors.

...

I am pretty sure I read they expect maybe 1 BH Merger event Per Year, but can not find the article.
I'll keep looking
I was wrong about it being thousands of Light Years away. It was over 1 BILLion Light Years out there.

I did find this article that says the GWave carried away 3 Solar Masses of ENergy in less than 1 Second
making it 10 times more Powerful than all the stars in the observable Universe for that brief moment.

http://www.ligo.org/science/Publication-GW150914/index.php

This Article also answered a question I had concerning the Surface of the Hour Glass Shaped merger.

They said the Surface Oscillated before settling into a Sphere.
This Oscillation may be part of the Acceleration and Deceleration that induces a GWaves and Frequencies.
 
  • #64
I did find an Estimate, that the space based eLISA proposed for launch in 2034,
could detect as many as 35 GWave events over a 3 Year period from MASSIVE Bianary Black Hole Mergers
with another 55 less Massive mergers at too high frequencies to be observe by eLISA.

This higher Estimate of ~10 to 12 Events per Year may be due to eLISA having really long arms to detect changes in Length due to GWs.

https://en.wikipedia.org/wiki/Evolved_Laser_Interferometer_Space_Antenna

" The LISA concept has a constellation of three spacecraft , arranged in an equilateral triangle with million-kilometre arms (5 million km for classic LISA, 1 million km for eLISA) ... The distance between the satellites is precisely monitored to detect a passing gravitational wave. "
 
  • #65
Interesting Simulation of 2 Neutron Stars merging into a BH

 
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  • #66
More dramatic Views of 2 Neutron Stars as they 'Ringdown' into a Singularity.

Seems some portion of the Fuel Rich remnants of these 2 stars
would reach Critical Mass conditions Inside the Event Horizon
so their released Energy in the form of Light photons etc..
would be Trapped by the BH ?

 
  • #67
looking4sophia said:
More dramatic Views of 2 Neutron Stars as they 'Ringdown' into a Singularity.

Seems some portion of the Fuel Rich remnants of these 2 stars
would reach Critical Mass conditions Inside the Event Horizon
so their released Energy in the form of Light photons etc..
would be Trapped by the BH ?
As I understand it, there is no "inside" the event horizon. However infalling stuff tends to heat up and speed up flinging some mass/energy out of orbit. (Conservation of angular momentum causes some of this.)
 
  • #68
Note that for the LIGO GW event analysis of the wave indicated that the two masses involved were well over the theoretical maximum mass for a neutron star so they are assumed to be already black holes, not neutron stars.
 
  • #69
There is an "inside" the EH, it's all the stuff that could never avoid being pulled into the singularity. Also, neutron stars would not normally be regarded as fuel rich, though once inside the EH it wouldn't matter.
 
  • #70
Ken G said:
neutron stars would not normally be regarded as fuel rich

For conditions like those on neutron stars, even thermonuclear fuels have rather modest energy densities. When they burn, 1% of their mass converted to energy? Phew, when *any matter* (even completely inert as fuel - say, iron) falls onto a neutron star, ~20% of its rest mass gets converted to energy on impact. This potential well is *that deep*. Even just rearranging matter (and/or EM field) on a neutron star surface into a "slightly" less energetic configuration unleashes a mother of all solar flares.

A neutron star being shredded by a black hole ought to emit a torrent of gamma rays.
 

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