Could Supermassive Black Holes Be More Common Than We Thought?

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Discussion Overview

The discussion revolves around the implications of potentially more common supermassive black holes (SMBHs) for cosmological theories, particularly the Big Bang (BB) theory, gravitational wave detection by LIGO, and the relationship between SMBH formation and galaxy evolution. Participants explore various aspects of these topics, including theoretical consistency, observational challenges, and the nature of dark matter.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants assert that the existence of SMBHs is consistent with BB theory, suggesting no significant impact on the theory itself.
  • There is debate over whether LIGO should detect signals from SMBHs, with some arguing that a single black hole does not emit gravitational waves unless it is involved in a merger.
  • Concerns are raised about the need to adjust stellar evolution models in light of SMBH findings, with some suggesting it is too early to determine the implications for galaxy formation.
  • Participants discuss the nature of gravitational waves, noting that ordinary mass in motion does not necessarily produce detectable waves without specific conditions being met.
  • Some participants question the idea that SMBHs could account for dark matter, arguing that their compact nature is inconsistent with the characteristics of dark matter as it is understood.
  • There are discussions about the observational limitations of LIGO and the conditions required for detecting gravitational waves from binary systems.
  • Some participants express skepticism about the possibility of black holes being a significant component of dark matter, referencing gravitational microlensing observations that challenge this idea.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the implications of SMBHs for BB theory, the detection of gravitational waves by LIGO, or the relationship between SMBHs and dark matter. Multiple competing views and uncertainties remain throughout the discussion.

Contextual Notes

Limitations include unresolved questions about the relationship between SMBH formation and galaxy evolution, as well as the specific conditions under which gravitational waves can be detected. The discussion also highlights the complexities of dark matter characteristics and the observational constraints faced by current detection methods.

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houlahound said:
What impact if any for BB theory.

None. BB theory is perfectly consistent with the existence of supermassive black holes.

houlahound said:
Should LIGO, detect this.

No. A black hole by itself does not emit gravitational waves. What LIGO detected was a merger of two black holes.

houlahound said:
Will stellar evolution need to be tweaked in terms of galaxy formation and such.

I would say it's too early to tell. This looks more like the end state of a galaxy than an early state.
 
houlahound said:
Supermassive black hole here;http://www.npr.org/sections/thetwo-...holes-may-be-more-common-than-anyone-imagined

What impact if any for BB theory.
None, as far as I can see.

Should LIGO, detect this.
detect WHAT? It's not merging with anything so not likely giving off gravitational waves like what you get when black holes merge.

Will stellar evolution need to be tweaked in terms of galaxy formation and such.
Don't see why. It's still an open question about the relationship between SMBH formation and galaxy formation but one more big one hardly adds anything.

EDIT: I see Peter's beat me to the punch again :smile: Only time I ever beat HIM to the punch is when it has rum in it.
 
The title doesn't seem to match the news text. They discovered a new supermassive black hole. Okay, great, but on a large scale: so what? Keep looking, and you'll find more.
 
I thought ejecting the equivalent of the milky way would cause a detectable signal.
 
houlahound said:
I thought ejecting the equivalent of the milky way would cause a detectable signal.
You are not reading the article properly. It is talking about having ejected that amount of stars from its vicinity. LIGO does not detect stars, it detects gravitational waves.
 
Any mass in motion should create a gravitational wave in principle. The problem is not that gravitational waves are not created at all, but that the gravitational waves created by ordinary activity are so faint that a detector can't see it. The entire solar system creates gravitational waves with a combined power of about 100 watts. The event LIGO observed has power greater than the EM output of every star in the universe at once. The merger of two substantial sized black holes is a powerful signal. Stars can generate gravitational waves too, and in tightly bound binary systems the magnitude of the waves might even be possible to detect. Of course, not only must you have a sufficiently powerful wave to detect at a great distance from its source, you must also have a gravitational wave with a frequency that your detector is tuned to hear, and you must, of course be looking in the right place at the right time.
 
ohwilleke said:
Any mass in motion should create a gravitational wave in principle.

That simply isn't the case. (In its rest frame, how is it emitting radiation?)
 
No expert but I doubt any LIGO is built in the rest frame of merging black holes.
 
  • #10
houlahound said:
No expert but I doubt any LIGO is built in the rest frame of merging black holes.
There IS no "rest frame of merging black holes". You can have a frame in which one of them is at rest but then the other is moving relative to it, so you have relative motion which causes gravity waves. A single star is just out there on its own.
 
  • #11
ohwilleke said:
Any mass in motion should create a gravitational wave in principle.

No, this is not correct. In order to emit gravitational waves, a system must have a time-varying quadrupole moment. That's quite a bit more complicated than just "being in motion" (which, as Vanadium50 has pointed out, is frame-dependent anyway).
 
  • #12
It makes me wonder that if there more of these than previously thought, or more black holes in general then previously thought, could that be the elusive 'dark matter'?
 
  • #13
rootone said:
It makes me wonder that if there more of these than previously thought, or more black holes in general then previously thought, could that be the elusive 'dark matter'?

Supermassive black holes could not be what we see as dark matter, because they would be much too compact--too much mass in too little space. The whole point of dark matter is that it is spread out fairly evenly throughout a galaxy; a supermassive black hole would have a substantial fraction of the galaxy's mass in a very small volume, relative to the galaxy's volume.

As I understand it, the possibility that ordinary sized black holes (stellar mass or lighter) could be what we see as dark matter has been pretty well ruled out by gravitational microlensing observations--if the dark matter were black holes, it would have lensing effects on the light coming from the stars in galaxies that we do not in fact observe.
 
  • #14
ohwilleke said:
Of course, not only must you have a sufficiently powerful wave to detect at a great distance from its source, you must also have a gravitational wave with a frequency that your detector is tuned to hear, and you must, of course be looking in the right place at the right time.
Binary stars cannot radiate in the right frequency range for LIGO. Their orbits need more than 10 minutes even for contact binaries, where ground-based detectors have way too much seismic noise. eLISA with its million kilometer arm length has some chance to detect them if they are close enough.

You don't have to look at the right place, interferometric gravitational wave detectors look at nearly the whole sky at the same time. They try to look all the time, experimental constraints allow to be sensitive about half of the time.
PeterDonis said:
As I understand it, the possibility that ordinary sized black holes (stellar mass or lighter) could be what we see as dark matter has been pretty well ruled out by gravitational microlensing observations--if the dark matter were black holes, it would have lensing effects on the light coming from the stars in galaxies that we do not in fact observe.
Right. There is a small mass range for substellar black holes (which would have to come from the big bang) that could make up some relevant fraction of dark matter, but such a large amount of black holes with a narrow mass range has no good motivation, and it would still mean that most of dark matter has to be something else.
 

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