mitosis
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Does anyone know, and is there an instrument that could?
The discussion centers on the capabilities of LIGO in detecting collisions of supermassive black holes (SMBHs) and explores the reasons behind its limitations. Participants consider the differences between stellar mass black holes and supermassive black holes, the frequency of gravitational waves emitted during collisions, and the potential for other instruments to detect such events.
Participants express differing views on the definitions and implications of supermassive black holes, the capabilities of LIGO, and the nature of gravitational waves emitted during collisions. There is no consensus on the reasons for LIGO's limitations in detecting SMBH collisions.
Some discussions reference specific frequency ranges and detection capabilities of LIGO, indicating limitations based on the size and mass of black holes involved. The conversation also touches on the potential for indirect detection methods, which may not align with LIGO's operational focus.
Vanadium 50 said:We are indulging in that favorite PF activity "guess what the poster meant". Maybe we should let him or her tell us what he or she means.
phyzguy said:I disagree. The phrase "super massive black hole" has a well-defined astrophysical meaning. For example, Wikipedia says:
"A supermassive black hole (SMBH or sometimes SBH) is the largest type of black hole, containing a mass of the order of hundreds of thousands, to billions times, the mass of the Sun (M☉)."
mitosis said:but I thought I heard
I guess if you had to pick one range to measure it is logical to select the one to record the much more frequently occurring events. It still blows my mind that LIGO could be made to be sensitive enough to measure such small changes.Ibix said:Figure 3 in this paper suggests that LIGO isn't sensitive to signals from the inspiral of black holes above about 1000 solar masses (the chirp mass isn't the same as individual masses, but you get the idea). I think it's simply the frequency of the waves emitted by that size of binary black hole. Like any antenna, LIGO only works well for picking up waves in a limited range of frequencies.
I think that isn't quite the same issue. That article is proposing using an indirect detection - observing the effect of gravitational waves on the detected tick rate of distant pulsars. And they are proposing looking for much much longer times before the final inspiral - millions of years, not seconds. I don't think this methodology would have the sensitivity to pick up what LIGO looks for. On the other hand, I think it can detect enormously lower frequencies. Which is why they're looking at SMBHs (huge power output) early in the inspiral (enormous wavelength).jedishrfu said:Heres an article on it
https://www.simonsfoundation.org/2017/11/13/gravitational-waves-supermassive-black-hole-merger/
They say it happens too fast relative to what is detected today.
Thanks for solving IBEX!Ibix said:Figure 3 in this paper suggests that LIGO isn't sensitive to signals from the inspiral of black holes above about 1000 solar masses (the chirp mass isn't the same as individual masses, but you get the idea). I think it's simply the frequency of the waves emitted by that size of binary black hole. Like any antenna, LIGO only works well for picking up waves in a limited range of frequencies.