Schutz, page 226 - Black hole formation

In summary, Schutz, in his book "A First Course in GR", states that during the formation of a black hole from a supernova explosion, gravity waves with an amplitude of M/R are expected, where M is the mass and R is the distance to the explosion. For a black hole of 10 solar masses at a distance of 10^{23}m, this amplitude is approximately 10^{-17}. Since 1 solar mass is roughly 10^3m, the M/R for the black hole itself is 10^{-19}. This suggests that a supernova explosion from a star with a mass of 1000 solar masses is needed to create a black hole of 10 solar masses. It is not clear if
  • #1
Jimmy Snyder
1,127
20
This question involves the following statement in Schutz, A First Course in GR, but you don't need to have a copy to answer it.

He says that in the formation of a black hole from a supernova explosion, we should expect gravity waves of amplitude M/R, where M is the mass and R is the distance to the explosion. He goes on to say that for a black hole of 10 solar masses, whose distance is [itex]10^{23}m[/itex], this is about [itex]10^{-17}[/itex]. Since 1 solar mass is roughly [itex]10^3m[/itex], M/R for the black hole itself would be [itex]10^{-19}[/itex]. This seems to imply that it would take the supernova explosion of a star of 1000 solar masses to create a black hole of 10 solar masses. Is this correct?
 
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  • #2
jimmysnyder said:
This question involves the following statement in Schutz, A First Course in GR, but you don't need to have a copy to answer it.
He says that in the formation of a black hole from a supernova explosion, we should expect waves of amplitude M/R, where M is the mass and R is the distance to the explosion. He goes on to say that for a black hole of 10 solar masses, whose distance is [itex]10^{23}m[/itex], this is about [itex]10^{-17}[/itex]. Since 1 solar mass is roughly [itex]10^3m[/itex], M/R for the black hole itself would be [itex]10^{-19}[/itex]. This seems to imply that it would take the supernova explosion of a star of 1000 solar masses to create a black hole of 10 solar masses. Is this correct?

What's going on with latex lately? The syntax here seems perfect an it can't be.

Pete
 
  • #3
pmb_phy said:
What's going on with latex lately? The syntax here seems perfect an it can't be.
Pete
Can you be more specific. On my screen my posts appear as I intend them to appear on your screen. Also, please note that I just edited my first post to add the word gravity so we know what kind of waves Schutz is talking about.
 
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  • #4
jimmysnyder said:
This question involves the following statement in Schutz, A First Course in GR, but you don't need to have a copy to answer it.
He says that in the formation of a black hole from a supernova explosion, we should expect gravity waves of amplitude M/R, where M is the mass and R is the distance to the explosion. He goes on to say that for a black hole of 10 solar masses, whose distance is [itex]10^{23}m[/itex], this is about [itex]10^{-17}[/itex]. Since 1 solar mass is roughly [itex]10^3m[/itex], M/R for the black hole itself would be [itex]10^{-19}[/itex]. This seems to imply that it would take the supernova explosion of a star of 1000 solar masses to create a black hole of 10 solar masses. Is this correct?

I assume this is all in geometric units.

M/r is a dimensionless number (in geometric units, which I've assumed). So when Schutz is talking about the amplitude of gravity waves, I assume he is talking about the power. (Power is another dimensionless number in geometric units). Energy is not dimensionless in geometric units.

(I suppose I don't have to assume - I'll have to refresh my memory on the emission of gravitational waves from MTW before I can verify this. More later after breakfast).

I don't see how you go from a statement about the power emitted in gravity waves to a statement about the final masses.
 
  • #5
pervect said:
in geometric units, which I've assumed.
Thanks for taking a look at this pervect. Yes, mass is given in geometric units. The book gives a figure of [itex]1.477[/itex] x [itex]10^{3}m[/itex] for the mass of the sun. So the figures are rounded off severely.

As for the amplitude of the gravitational wave, you don't really need to concentrate on that to answer the question. The real question may not have been totally clear so I repeat it:

When a supernova creates a black hole, does it take a 1000 solar mass star to make a 10 solar mass black hole?

The rest of that post was simply to justify why I was asking the question. Schutz's text seems to imply that the answer is yes.

But if the answer is yes, then there are other questions that come to my mind. A star of that mass burns so quickly, can the protostellar material have had time to clear away? But if the material is still there when the supernova occurs, wouldn't it slow down the dispersion of the ejecta? If it does, might not the ejecta fail to reach escape velocity and come crashing back to the black hole? But if it does then won't it add to the 10 solar mass of the black hole?
 
  • #6
jimmysnyder said:
As for the amplitude of the gravitational wave, you don't really need to concentrate on that to answer the question. The real question may not have been totally clear so I repeat it:
When a supernova creates a black hole, does it take a 1000 solar mass star to make a 10 solar mass black hole?
The rest of that post was simply to justify why I was asking the question. Schutz's text seems to imply that the answer is yes.
But if the answer is yes, then there are other questions that come to my mind. A star of that mass burns so quickly, can the protostellar material have had time to clear away? But if the material is still there when the supernova occurs, wouldn't it slow down the dispersion of the ejecta? If it does, might not the ejecta fail to reach escape velocity and come crashing back to the black hole? But if it does then won't it add to the 10 solar mass of the black hole?
I don't know the answer to your question. MTW appears to be very dated on this point, so I won't repeat what they have to say here.
A couple of interesting links I stumbled across are:
http://www.ligo.caltech.edu/docs/G/G020075-00.pdf
http://arxiv.org/abs/astro-ph/0409035
The second mainly for the following very short quote
We do not yet have an agreed-upon explanation for the mechanism of corecollapse
supernovae, nor for the related phenomena of neutron star kicks and
blast debris morphology.
Space Tiger might know more, he usually posts in the general astronomy and cosmology forum, so I'm not sure if he's seen your question here.
I would tend to trust observational evidence more than theory - as the second paper points out, there appear to be a lot of elements that have to be modeled properly to explain supernova.
 
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  • #7
jimmysnyder said:
Can you be more specific. On my screen my posts appear as I intend them to appear on your screen. Also, please note that I just edited my first post to add the word gravity so we know what kind of waves Schutz is talking about.
I dunno. Sometimes the Latex appears all messed up and then at other times it appears perfect.

It is a puzzlement! :-p

Pete
 
  • #8
With respect to the original post, I have a hunch that Schutz used the value of the Sun's mass given inside the back cover of MTW, i.e., Schutz forgot to convert centimetres to metres. This would account for the missing factor of 100.

Regards,
George
 
  • #9
George Jones said:
Schutz forgot to convert centimetres to metres. This would account for the missing factor of 100.
Thanks George.
 

Related to Schutz, page 226 - Black hole formation

1. What is a black hole?

A black hole is a region in space where the gravitational pull is so strong that nothing, including light, can escape from it. It is formed when a massive star dies and collapses under its own gravity.

2. How are black holes formed?

Black holes are formed when a massive star dies and its core collapses under its own gravity. This can happen when the star runs out of fuel and can no longer support its own weight.

3. What is the event horizon of a black hole?

The event horizon is the boundary around a black hole where the escape velocity is greater than the speed of light. Once an object crosses the event horizon, it is trapped inside the black hole and cannot escape.

4. What is the singularity of a black hole?

The singularity is the center of a black hole where the gravitational pull is infinite and the laws of physics as we know them break down. It is a point of infinite density and zero volume.

5. Can black holes be observed?

Black holes cannot be observed directly because they do not emit any light. However, their effects on surrounding matter can be observed through the distortion of light and other forms of radiation. Scientists also use indirect methods, such as studying the movement of stars and gas around black holes, to infer their existence.

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