B Gravitational potential energy, a thought experiment

  • #101
Lok said:
I used the Sun and Sag A* as the initial bodies to underline the massive amount of energy that such a system holds as potential energy.
Again you are missing the key point: in the starting configuration of the system, it holds zero gravitational potential energy. The total mass is just ##m + M##; there is no extra "potential energy" term in there.

It is true that as the Sun falls, it gains kinetic energy, and to compensate it loses gravitational potential energy, i.e., as I have said, its gravitational potential energy becomes negative, and gets more negative as it falls. But viewing this as somehow using gravitational potential energy that was "stored" in the initial configuration is not helpful, because it makes you think there is some kind of issue involved with the total mass just being ##m + M##. There isn't. Once you properly understand this, the question you think you are asking simply evaporates.

Lok said:
In the OP I used the as in Wiki weirdly formulate value for Gravitational potential energy.
U=-GMm/R, where R is the smallest distance that can be attained by the masses
That's wrong. The formula does not depend on the "smallest distance", it depends on the actual distance. At the start it is zero because the actual distance is effectively infinity. At the end it is a negative value that exactly cancels the Sun's kinetic energy.

Lok said:
I would not state that KE cancels out GPE, but rather one transforms into another.
And your insistence on looking at it this way is why this thread keeps going on--the correct answer is staring you in the face and you are refusing to accept it.

Lok said:
either the extra 24% mass is a real thing, and this leaves me wondering where it is distributed in the initial state.
Which, again, is because you are refusing to accept the correct answer that is staring you in the face: the total mass is just ##m + M##, always, and what happens internally can't change it because the system is isolated. There is no "extra mass" anywhere.

Lok said:
Or it is a figment of equations and there should be no difference in outcome whether there is or there isn't KE in the final state.
It is impossible for the Sun to not have KE in the final state. As I have already said, there is only one valid solution to this scenario. Talking as though there were other possibilities is simply wrong. And this error appears to be part of what is confusing you and keeping you from accepting the obvious correct answer.

Lok said:
would those ##m+M+E_K+E_P## energy terms add to the mass of the box?
Yes, because ##E_P = - E_K## so ##m + M + E_K + E_P = m + M##. This is the obvious correct answer that you are refusing to accept.

Lok said:
If yes, how is that mass distributed in the initial state as the final state is less of an issue.
In the initial state, ##E_K = E_P = 0##. Which is just a special case of ##E_P = - E_K##; the latter is always true in this scenario.

Lok said:
KE does have a measurable mass via e.g. heat
Sure, but in this scenario that is irrelevant, because PE exactly cancels out KE and there is no net contribution to the total mass. For KE to appear as "extra mass" in the total mass of the system you have to look at a different scenario in which PE and KE do not exactly cancel. And for such a scenario the total mass would not be ##m + M##, even at the start (although even here calling the KE "extra mass" can be misleading, since the total mass will be less than ##m + M##). If you want to discuss such scenarios, you can start a new thread to ask about one (for example, you could consider having the Sun in a circular orbit around Sag A at some finite radius).

Lok said:
I am going for dark matter of course
That is because you keep talking as if there were some "extra mass" in this scenario, when there is none.
 
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  • #102
Lok said:
Not the gravitationally lensed mass, as my assumption is that includes the 24% extra mass somewhere somehow.
It doesn't. There is no "24% extra mass" anywhere in the system as measured from outside.

Lok said:
if the Sun can attain a higher mass by transforming GPE into KE which can be transformed into rest mass
If you want to consider the Sun's extra KE as contributing to the total mass of the system, you also must consider the Sun's negative GPE as contributing to the total mass of the system--and the two contributions exactly cancel in this scenario. So there is no "extra mass".

Basically, you are trying to consider the KE as "extra mass" but ignore the negative GPE as a negative contribution to the mass. That's wrong. You have to consider both.

Lok said:
where was that mass in the initial state?
Nowhere; it doesn't exist in this scenario. See above.

Lok said:
IMO this problem is a contradiction already.
It's not. You are just refusing to analyze it correctly. See above.

Lok said:
I strongly encourage anybody to do the most basic calculation
No such calculation is needed to give the obvious correct answer I gave above, and have given already multiple times in this thread.
 
  • #103
PeroK said:
How can the initial geometry be described by a single mass parameter?
Please, please, let's not derail the thread any further with irrelevant confusions about the Oppenheimer-Snyder model. The fact is that that scenario can be described with a constant external mass parameter: this follows from the fact that the scenario is spherically symmetric and asymptotically flat and an obvious application of Birkhoff's theorem. But discussion of that is off topic here; we're having enough trouble with the even simpler scenario the OP has posed.
 
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  • #104
Lok said:
I strongly encourage anybody to do the most basic calculation and see how much GPE is in a as OP system or galactic if one has available data and modeling software. It is above my current setup.
Are you saying that you cannot do this calculation yourself? Yet you are sure we're wrong? That's a tough, tough position to hold.

Further, the actual numbers are unnecessary. You did disregard ny suggestion to eschew the cute stories, but had you followed it, we could discuss this all symbolically.
Nugatory said:
I have no idea what you’re trying to ask here, but I do know from the timestamps that you spent no more than fifteen minutes thinking before posting, and that’s not enough.
If you're not thinking about what we are writing, why are we writing it? Skimming and reacting will not teach you anything. You have to spend the time thinking.

I suggest you stop posting for some period of time - a few hours, a day, whatever it takes - and reread the entire thread, thinking about every response carefully. If after the endn of this period, there is something you still do not understand, post as short and concise a question as you can about it, with minimal filler.
 
  • #105
PeterDonis said:
we're having enough trouble with the even simpler scenario the OP has posed.
I'm not sure I agree that the OP's scenario is simpler, but will leave it for now. Happy to discuss in another thread.
 
  • #106
Ibix said:
I'm not sure I agree that the OP's scenario is simpler
It's simpler in that no computation whatever is required to get the correct answer; at most (if you want more than just applying the obvious fact of conservation of energy for an isolated system) you just need to read it off a simple one line formula that has already been posted.
 
  • #107
PeterDonis said:
It's simpler.
Negative energy. I cannot unsee that one.
Enough! A nice day to you all.
 
  • #108
Lok said:
Negative energy. I cannot unsee that one.
Negative gravitational potential energy. That has been a useful concept in physics for several centuries now.
 
  • #109
PeterDonis said:
Negative gravitational potential energy. That has been a useful concept in physics for several centuries now.

PeterDonis said:
Negative gravitational potential energy. That has been a useful concept in physics for several centuries now.
The thing you create negative mass with.
I now understand.
Thank you!
 
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  • #110
Lok said:
Negative energy. I cannot unsee that one.
Enough! A nice day to you all.
Negative potential energy is one of the great simplifying concepts in classical physics - for example, you’ll find it very helpful when deriving Kepler’s Laws and solving orbital motion, which physics students will be doing no later than their first year of college. If you are not completely comfortable with the concept you really need to back up and review elementary classical mechanics before you try to take on relativity.
 
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  • #111
Lok said:
Negative energy. I cannot unsee that one.
Enough! A nice day to you all.
See https://en.wikipedia.org/wiki/Gravitational_energy
$$U=-\frac{GMm}{r}$$ Since ##G##, ##M##, ##m##, and ##r## are all positive, ##U## is negative. This is ordinary Newtonian physics.
 
  • #112
Lok said:
The thing you create negative mass with.
I now understand.
Thank you!

I'm not so sure you do understand - I rather suspect you do not, from your comments. I haven't read the entire thread in detail, as it is quite long, I've only skimmed it.

In Newtonian theory, if you have a planet, and you "dissassemble" it (my own term for lack of anything better) by cutting it into pieces and moving them all very far away from each other, this process requires energy.

This implies that the total energy of an assembled planet is lower than the energy of the disassembled one. This is called the "binding energy".

The total energy of a bound system is lower than the total energy of its parts.

Note that a planet orbiting a sun (or the sun orbiting Sag A) can also be considered a bound system in the same manner.

wiki said:
The gravitational binding energy of a system is the minimum energy which must be added to it in order for the system to cease being in a gravitationally bound state. A gravitationally bound system has a lower (i.e., more negative) gravitational potential energy than the sum of the energies of its parts when these are completely separated—this is what keeps the system aggregated in accordance with the minimum total potential energy principle.

Note particularly the remarks in wiki that the binding energy is negative.

This is standard usage - the potential energy of a bound system is negative because the energy of the bound system is lower than the energy of the unbound system.

As for how things actually work in GR (or even SR), I'd say it's too advanced for this thread.

I will say that SR has a concept of something called the "stress energy tensor", which GR borrows, and uses instead of "mass".

GR does also have several concepts of the mass of a system (which are derived from the stress-energy tensor) such as the "big three", Komar mass, ADM mass, and Bondi mass. The fact that it has three of them rather than one is a foreboding that things here are not simple.

However, other than dropping these names, I fear that a detailed discussion of these issues is beyond the scope of the thread.
 
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  • #113
Dale said:
See https://en.wikipedia.org/wiki/Gravitational_energy
$$U=-\frac{GMm}{r}$$ Since ##G##, ##M##, ##m##, and ##r## are all positive, ##U## is negative. This is ordinary Newtonian physics.
I said that now I understand that negative mass cancels the positive one from KE. Problem solved.
In all honesty, how old is this mess?
 
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  • #114
Lok said:
In all honesty, how old is this mess?
About 300 years.
 
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  • #115
Nugatory said:
Negative potential energy is one of the great simplifying concepts in classical physics - for example, you’ll find it very helpful when deriving Kepler’s Laws and solving orbital motion, which physics students will be doing no later than their first year of college. If you are not completely comfortable with the concept you really need to back up and review elementary classical mechanics before you try to take on relativity.

Dale said:
About 300 years.
I appreciate the honesty. Best of luck as this will crash eventually.
 
  • #116
Lok said:
The thing you create negative mass with.
No. The total mass of any system is still positive.

Lok said:
Best of luck as this will crash eventually.
What do you mean by this? If you think the concept of negative gravitational potential energy is somehow going to "crash", I strongly suggest that you think again.
 
  • #117
Lok said:
In all honesty, how old is this mess?
1666 was a turning point for England. The outbreak of the Great Plague, the eruption of the Second Dutch War and the devastating Great Fire of London all hit the country in quick succession and with devastating consequences.

Isaac Newton took refuge in the countryside.
It is not known exactly what he was doing under that tree, but they say that an apple fell on his head.
In the following year and a half, the foundations of Newton's theory of gravitation were created.

I like another consequence of the same year 1666 > Iron Maiden - The Number Of The Beast
 
  • #118
Lok said:
I said that now I understand that negative mass cancels the positive one from KE.
I recommend that you start the calculations first using Newtonian mechanics.
You calculate the speed of the Sun after some time, the kinetic energy, how long it takes to travel a certain distance...
Interesting questions are:
How long will it take the Sun to reach Sag A?
What will be its speed at that moment?
...
When you clear everything up, you move on to the special theory of relativity and compare the results.

Then you do the same using the general theory of relativity.
 
  • #119
Lok said:
I appreciate the honesty. Best of luck as this will crash eventually.
If you use Newtonian mechanics, the potential and the kinetic energy will have the same value and the opposite sign.
You can start from
$$-E_P=\frac{GMm}{r}=\frac{mv^2}{2}=E_K$$
and calculate speed for various distances (r).

Then you can fix this formula a bit because at the beginning ##E_P## is small but not quite zero and the speed ( ##v## ) is zero so ##E_P## is also zero. ( The above formula is valid for falling from infinity )
 
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  • #120
Bosko said:
If you use Newtonian mechanics, the potential and the kinetic energy will have the same value and the opposite sign.
This is also true in GR for this scenario.
 
  • #121
Bosko said:
If you use Newtonian mechanics, the potential and the kinetic energy will have the same value and the opposite sign.
We do want to be a bit careful not to overstate our case here. We can always add or subtract an arbitrary value from the potential energy, so we can always make the potential energy at any point come out positive, negative, or zero as we please. It just so happens that often (central force problems, two otherwise isolated interacting bodies as in this thread, …) it is very convenient to take the potential energy at infinity to be zero; that is the maximum of potential energy so potential energy at any finite distance will then be negative.

But in other problems we may choose different conventions. If I am standing in my front yard it may be most convenient to take the zero of gravitational potential energy to be ground level, increasing upwards. Now the mass I am holding above my head will have positive potential energy ##mgh## (reflecting the work needed to lift it to height ##h## off the ground) while the mass I dropped into the well will have negative kinetic energy (also ##mgh##, but ##h## is negative, the depth of the well below ground level).

Kinetic energy on the other hand will always be non-negative. We can choose a frame in which the kinetic energy of a given object is zero, but we can’t make it come out negative.
 
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  • #122
Lok said:
Best of luck as this will crash eventually.
There is nothing wrong with the science here, no imminent danger of a "crash". It is your expectation that energy is always positive which needs to be adjusted. The ideas of binding energy and mass deficit (or mass defect) are well known, theoretically sound, and experimentally validated.

You asked a question and you received the correct answer from multiple experts. Now it is up to you to learn. Sometimes the result of asking a question is the opportunity to learn something surprising. That is the opportunity you have now.
 
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  • #123
Nugatory said:
We can always add or subtract an arbitrary value from the potential energy
But we can't change direct observables, and as I have already pointed out, the externally measured mass of the system is a direct observable. So any convention for gravitational potential energy that does not have it go to zero at infinity means, as I pointed out, that there is now an arbitrary constant in the math that ends up dropping out of the analysis as soon as you try to evaluate any direct observable. So the only convention that actually makes physical sense for this scenario is that GPE goes to zero at infinity.

Nugatory said:
in other problems we may choose different conventions
Agreed, that's why I qualified my response to @Bosko with "in this scenario".
 
  • #124
Lok said:
In all honesty, how old is this mess?
It's over 120 posts now.
 
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  • #125
So to get on track…

Initial system: Total E: (rest)Mass + Ekin + Ep
Final system: Total E: (rest)Mass + Ekin + Ep has not changed (as long as no Energy left the system).
Ep converted to Ekin

But I stil have a question,
When we talk about the Mass of a galaxy like the Milky way, I get the impression only the (rest)Mass is meant, not the Ekin + Ep part.

But when we talk about the gravitational effects of galaxies we have to consider the Total E. Can someone please explain to me why the Ekin+ Ep part is different from dark Mass/Energy.
 
  • #126
bigbear73 said:
So to get on track…

Initial system: Total E: (rest)Mass + Ekin + Ep
Final system: Total E: (rest)Mass + Ekin + Ep has not changed (as long as no Energy left the system).
Ep converted to Ekin

But I stil have a question,
When we talk about the Mass of a galaxy like the Milky way, I get the impression only the (rest)Mass is meant, not the Ekin + Ep part.

But when we talk about the gravitational effects of galaxies we have to consider the Total E. Can someone please explain to me why the Ekin+ Ep part is different from dark Mass/Energy.
:welcome:

It might be better to start a new thread and reference this one if you need to. The mass of the Milky Way is almost entirely the rest mass of the stars and dark matter. The internal KE and GPE are negligible. The stars are generally too far apart and moving too slowly relative to each other for these other quantities to be significant.
 
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