gregtomko
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OK! That puts it to rest... for now... Thanks again!
phinds said:Guess I asked that one badly. What I mean is, why is that not a good explanation? What is incorrect about it?
phinds said:where did I go wrong with the "same pressure from all directions ==> no movement" explanation?
gregtomko said:If the mass of the universe is constantly being converted to energy through nuclear fusion, and nothing can travel outside of space-time, then isn't the ratio of energy to mass increasing? If so, then wouldn't the only possible option be for an acceleration of the universe's expansion?
gregtomko said:oh, OK, they don't have "rest" mass, but they aren't at rest. I wasn't aware they had mass when traveling.
gregtomko said:oh, OK, they don't have "rest" mass, but they aren't at rest. I wasn't aware they had mass when traveling.
Drakkith said:They do not have mass, ever. They have momentum and energy. Both mass and energy contribute to gravity. There is a confusing thing called "relativistic mass" that shouldn't have ever been called mass to begin with. When you think of mass only think of "rest mass" or "invariant mass". Both are the same thing. When a star emits light it does lose a small amount of mass thanks to the missing energy that the photon took. While in transit that photon is affecting the space around it through gravity. Once the photon is absorbed the energy it carried is turned back into mass, making whatever absorbed it slightly more massive.
If the mass is no longer in the star while the photons are in transit, how can the mass of the universe stay constant? Or maybe that was referring to the relativistic mass of the universe?juanrga said:No. In fact the mass M of the Universe is constant.
gregtomko said:That is exactly the way I thought it worked. How does that relate to the earlier post
If the mass is no longer in the star while the photons are in transit, how can the mass of the universe stay constant? Or maybe that was referring to the relativistic mass of the universe?
gregtomko said:What I am questioning is if the total quantity of energy released through nuclear fusion throughout the history of the universe is enough to equal the acceleration we observe. Not if we see certain effects on certain systems. As a whole, the proportion between how much energy is necessary to accelerate the universe as we see, and the amount of energy released in stars throughout time, is that a known ratio?
phinds said:you have to have a plausible mechanism for transferring the energy released in the middle of stars to points MANY light years away, and there isn't any.
gregtomko said:I only ask the question because I am not an astrophysicist. I am not asking about the mechanism, just about the relationship in energy.
What I am questioning is if the total quantity of energy released through nuclear fusion throughout the history of the universe is enough to equal the acceleration we observe
gregtomko said:It seems to me that the question of meaningless or meaningful, rests on the relationship of the quantities of energy involved.
gregtomko said:I am just curious if this is an understood proportion?
gregtomko said:I am not sure where I am going with it either, it just seems like there might be some significance if there was a similarity. It would at least be a way to disprove an intuitive, yet overly simplistic connection.
gregtomko said:What I am questioning is if the total quantity of energy released through nuclear fusion throughout the history of the universe is enough to equal the acceleration we observe. Not if we see certain effects on certain systems. As a whole, the proportion between how much energy is necessary to accelerate the universe as we see, and the amount of energy released in stars throughout time... is that a known ratio?
Drakkith said:It is not. It isn't even close.
gregtomko said:phinds, I don't want to sound sarcastic, but if the two quantities just happened to be the same, you don't think there would be some significance?
gregtomko said:Which way is it not close, and where can I find information on that?
gregtomko said:If the whole business of dark energy is so unknown, how can you be sure of that? I would think that conservation of energy in the universe, is far more unified than the international market price for fuel.
Drakkith said:It's not nearly enough. The Earth experiences around 5.823 x 10^8 Newtons of radiation pressure. The force of gravity from the Sun is about 3.5222 x 10^22 Newtons. That means that the radiation pressure reduces the net force on Earth to 35,221,999,999,999,417,700,000 Newtons. (Round it off and its 3.5222x10^22)
phinds said:you have to imagine a mechanism whereby the use of energy in stars has an effect that is STRONGER the farther away you are from the star
gregtomko said:I am not talking about the instantaneous acceleration on our solar system. The question is about the total energy released throughout time by starts in the universe, related to the total acceleration we see in the universe as a whole.
gregtomko said:That seems to be the similarity between dark energy and dark matter, they are stronger than they should be, the farther away you get. That was the inspiration for the question.
Drakkith said:Extrapolating that out, since radiation pressure is mainly produced by stars, and stars only make up about 1.5% of all matter and dark matter (the stuff that generates gravity), then we can see that the contribution of radiation pressure is absolutely miniscule compared with the combined gravity of the universe.
Drakkith said:We have no idea what to expect from either dark matter or dark energy.
Also, what about them is stronger?
gregtomko said:That seems to be the similarity between dark energy and dark matter, they are stronger than they should be, the farther away you get. That was the inspiration for the question.
gregtomko said:That would be quite informative if the whole concept of dark matter was at all understood.
I thought that's what I was saying. That dark energy is needed to explain the extra acceleration of the universe the farther away we look. That dark matter is needed to explain the gravitational pull to hold stars farther away from the center of galaxies. The farther away, the stronger the "dark" forces appear to be.
I specifically said I didn't know if radiation pressure is the mechanism. In reference to dark matter, I was saying that it appears to be more influential the farther from the centers of galaxies. Isn't that the whole concept, that galaxies rotations look odd because the outer stars rotate faster than they should? This is true or they wouldn't need to call it "dark matter" right? Just as "dark energy" is more influential on objects farther away from us. If it was a simple relationship there would be no question. Earlier in this line of posts it was stated that the reason the energy of fusion couldn't explain the acceleration of the universe, was somehow it did not fit the characteristics of the observed expansion. I am asking what is the observed relationship. I don't Know what the connection is, that's why I am asking.Drakkith said:OR you could admit that radiation pressure is not a likely possibility to explain universal expansion. That seems much more reasonable than one liners aimed at someone's post you simply don't like. In the future try to understand the subject more before shooting down someone who has actually done the math.Dark matter is spread throughout the galaxy, not concentrated in the center. It's effects don't get stronger with increasing distance. Dark energy does not either. The acceleration increases with distance because the space in between galaxies is expanding all at the same rate. IE if you break space down into chunks you will find that each piece is expanding at the same rate. Hence the reason the expansion is faster at increasing distances is because you have more pieces of space expanding between us.
gregtomko said:I specifically said I didn't know if radiation pressure is the mechanism. In reference to dark matter, I was saying that it appears to be more influential the farther from the centers of galaxies. Isn't that the whole concept, that galaxies rotations look odd because the outer stars rotate faster than they should?
This is true or they wouldn't need to call it "dark matter" right? Just as "dark energy" is more influential on objects farther away from us. If it was a simple relationship there would be no question. Earlier in this line of posts it was stated that the reason the energy of fusion couldn't explain the acceleration of the universe, was somehow it did not fit the characteristics of the observed expansion. I am asking what is the observed relationship. I don't Know what the connection is, that's why I am asking.
Drakkith said:Saying the "dark forces" appear stronger further out implies that the actual force of gravity or expansion increases as distance increases.
Drakkith said:For every million parsecs of distance from the observer, the rate of expansion increases by about 74 kilometers per second. One parsec = 3.26 light years. Is that what you wanted?
gregtomko said:That is your own conclusion, I am not sure that is the relationship.
I am looking more specifically for the ratio of the amount of energy needed to accelerate the mass of the universe as we see it, compared to the amount of energy released through nuclear fusion in the stars of the universe throughout its expansion.
Drakkith said:What? What relationship?
Drakkith said:In the future try to understand the subject more before shooting down someone who has actually done the math.
gregtomko said:"Saying the "dark forces" appear stronger further out implies that the actual force of gravity or expansion increases as distance increases."
That relationship. That is an odd conclusion.
gregtomko said:So you have done the math? I thought that nobody has ever done the math to explain dark matter, isn't that the whole point?
I am not trying to draw a conclusion, just ask a simple question.Drakkith said:That is exactly the conclusion your statement brings me to.
Drakkith said:I don't even know what you want to know about dark matter and energy that hasn't already be said.
gregtomko said:All I would like to know is the ratio of energy released from stars through fusion, to that needed for the acceleration of the expansion of the universe. If you could point me to that particular wikipedia page I would appreciate it.
Drakkith said:There isn't one because it isn't possible for radiation pressure to cause the expansion of the universe. You can't even calculate the "needed energy" because the two effects aren't even related. Radiation pressure would never result in galaxies receding from us greater than the speed of light, only expansion of space will do that.
gregtomko said:Not the radiation pressure, just the straight a = F/m
gregtomko said:Or is that what I am missing? Is the radiation pressure equal to the total energy released from stars?