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| Tags: tensors |
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#1
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In message http://groups.google.com/groups?dq=&...ing.google.com
I discuss the issue of tensors. In GR the Einstein Tensor and the Stress Energy Tensor are related by Guv=8piTuv. http://scienceworld.wolfram.com/phys...Equations.html But then I asked, what if these two things were the same thing? I ask you here too, because it's important. How do we really know that there are two seperate things 'floating out there' that just HAPPEN to be the same? What if they were in fact dual aspects of the same thing? Wouldn't this make unifying Loop Quantum Gravity and String Theory a lot easier if we could derive one from the other? That, and eliminating all ad-hoc assumptions, including that causality is unique in time at high energy scales, and that the macroscopic fundamental constants remain unperterbed at extremely high energy scales. There are a lot of ad hoc assumptions made by those who work on LQG and ST. And if I ever get involved with those communities, I plan to correct them. (...Starblade Riven Darksquall...) |
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#2
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In article ,
Starblade Darksquall wrote: In message http://groups.google.com/groups?dq=&...ing.google.com I discuss the issue of tensors. In GR the Einstein Tensor and the Stress Energy Tensor are related by Guv=8piTuv. http://scienceworld.wolfram.com/phys...Equations.html But then I asked, what if these two things were the same thing? I ask you here too, because it's important. How do we really know that there are two seperate things 'floating out there' that just HAPPEN to be the same? What if they were in fact dual aspects of the same thing? When written G = 8 pi T it doesn't look very illuminating. But expand it out and you get ten independent coupled equations, the left-hand side entirely in terms of the metric tensor, and the right-hand side mostly in terms of masses, pressures, and other mechanical effects. And they're infamously difficult to find solutions for. Geometric notation hides a lot of dirty laundry. The left hand side is the curvature tensor. It tells you in what way space is curved. It needs to be there if you're going to have a geometrical theory of gravity, so it's no accident that it's sitting there. No G - no curvature - no gravity. And gravity has sources, like mass, which are described by T, the stress-energy tensor. So again it's no accident that T is on the right hand side. It's the moral equivalent of a = -GM/r^2 from Newtonian gravity. Think it's just coincidence that there just HAPPENS to be something on the left that's equal to something on the right? That, and eliminating all ad-hoc assumptions, including that causality is unique in time at high energy scales, and that the macroscopic fundamental constants remain unperterbed at extremely high energy scales. There are a lot of ad hoc assumptions made by those who work on LQG and ST. And if I ever get involved with those communities, I plan to correct them. Nose to the grindstone, and all that. -- "When the fool walks through the street, in his lack of understanding he calls everything foolish." -- Ecclesiastes 10:3, New American Bible |
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#3
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Starblade Darksquall wrote:
In message http://groups.google.com/groups?dq=&...ing.google.com I discuss the issue of tensors. and we are all poorer for it. [snip] -- Uncle Al http://www.mazepath.com/uncleal/ (Toxic URL! Unsafe for children and most mammals) "Quis custodiet ipsos custodes?" The Net! |
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#4
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Gregory L. Hansen wrote in message ... In article , Starblade Darksquall wrote: In message http://groups.google.com/groups?dq=&...sci.physics.re search&selm=4aa861fb.0309052011.484ae963%40posting .google.com I discuss the issue of tensors. In GR the Einstein Tensor and the Stress Energy Tensor are related by Guv=8piTuv. http://scienceworld.wolfram.com/phys...Equations.html But then I asked, what if these two things were the same thing? I ask you here too, because it's important. How do we really know that there are two seperate things 'floating out there' that just HAPPEN to be the same? What if they were in fact dual aspects of the same thing? When written G = 8 pi T it doesn't look very illuminating. But expand it out and you get ten independent coupled equations, the left-hand side entirely in terms of the metric tensor, and the right-hand side mostly in terms of masses, pressures, and other mechanical effects. And they're infamously difficult to find solutions for. Geometric notation hides a lot of dirty laundry. One of the biggest problems with teaching relativity to students is that the compact nature of indical notation belies the fact that there's a hell of a lot of complexity just below the surface. The 'G' in the above equation is actually shorthand for the Ricci tensor minus one half the Ricci scalar. The problem with this is that it's *not* given in terms of the metric tensor, rather that it's given in terms of first and second derivatives of the metric. Recall that the curvature tensor can be defined in terms of the connection; this results in an expression which is quadratic in first derivatives of the metric and linear in second derivatives. That's where the real complexity comes from. It's really quite funny seeing peoples' faces when they move from standard theoretical general relativity into numerical simulations of relativity; the boundless complexity of the equations is brought home in a crushingly efficient manner when you begin to look at something like CactusCode thorns. The left hand side is the curvature tensor. Not really. In essence it's a contraction (or two ;-)) of the curvature tensor, although I do see your point. It tells you in what way space is curved. It needs to be there if you're going to have a geometrical theory of gravity, so it's no accident that it's sitting there. No G - no curvature - no gravity. I'd attack this from a different perspective and say that vacuum gives rise to a vanishing Ricci scalar, but that's purely pedagogical in nature. davidoff |
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#5
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"davidoff404" wrote in message ...
Gregory L. Hansen wrote in message ... In article , Starblade Darksquall wrote: In message http://groups.google.com/groups?dq=&...sci.physics.re search&selm=4aa861fb.0309052011.484ae963%40posting .google.com I discuss the issue of tensors. In GR the Einstein Tensor and the Stress Energy Tensor are related by Guv=8piTuv. http://scienceworld.wolfram.com/phys...Equations.html But then I asked, what if these two things were the same thing? I ask you here too, because it's important. How do we really know that there are two seperate things 'floating out there' that just HAPPEN to be the same? What if they were in fact dual aspects of the same thing? When written G = 8 pi T it doesn't look very illuminating. But expand it out and you get ten independent coupled equations, the left-hand side entirely in terms of the metric tensor, and the right-hand side mostly in terms of masses, pressures, and other mechanical effects. And they're infamously difficult to find solutions for. Geometric notation hides a lot of dirty laundry. One of the biggest problems with teaching relativity to students is that the compact nature of indical notation belies the fact that there's a hell of a lot of complexity just below the surface. The 'G' in the above equation is actually shorthand for the Ricci tensor minus one half the Ricci scalar. The problem with this is that it's *not* given in terms of the metric tensor, rather that it's given in terms of first and second derivatives of the metric. Recall that the curvature tensor can be defined in terms of the connection; this results in an expression which is quadratic in first derivatives of the metric and linear in second derivatives. That's where the real complexity comes from. It's really quite funny seeing peoples' faces when they move from standard theoretical general relativity into numerical simulations of relativity; the boundless complexity of the equations is brought home in a crushingly efficient manner when you begin to look at something like CactusCode thorns. The left hand side is the curvature tensor. Not really. In essence it's a contraction (or two ;-)) of the curvature tensor, although I do see your point. It tells you in what way space is curved. It needs to be there if you're going to have a geometrical theory of gravity, so it's no accident that it's sitting there. No G - no curvature - no gravity. I'd attack this from a different perspective and say that vacuum gives rise to a vanishing Ricci scalar, but that's purely pedagogical in nature. davidoff I think the reason we use the first and second derivitives is because they define the relation between two different metrics. In reality, we would not be able to tell WHICH metric we were on, but we could still distinguish between two different metrics. |
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#7
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Starblade Darksquall wrote in message om... It tells you in what way space is curved. It needs to be there if you're going to have a geometrical theory of gravity, so it's no accident that it's sitting there. No G - no curvature - no gravity. I'd attack this from a different perspective and say that vacuum gives rise to a vanishing Ricci scalar, but that's purely pedagogical in nature. davidoff I think the reason we use the first and second derivitives is because they define the relation between two different metrics. In reality, we would not be able to tell WHICH metric we were on, but we could still distinguish between two different metrics. I'm not sure quite what you mean by this. In general relativity we don't really speak of being *on* a metric. Instead one introduces the concept of a metric on a manifold as a means to get at important ideas like distance and orthogonality. Essentially, the reason one gets derivatives of the metric is because basis vectors in the manifold vary from point to point. This is unlike the case in flat space where the basis vectors remain constant throughout the space. This is a pretty subtle issue at first glance, and is something I think deserves to be illustrated with equations. As a result Usenet probably isn't the right place to get into it. If you really want, I'll throw together a ..pdf file and give you a link to it. davidoff |
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#8
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In article ,
davidoff404 wrote: Starblade Darksquall wrote in message . com... Essentially, the reason one gets derivatives of the metric is because basis vectors in the manifold vary from point to point. This is unlike the case in flat space where the basis vectors remain constant throughout the space. Flat space with Cartesian coordinates, anyway. Non-Cartesian coordinates in flat space (e.g. polar coordinates) have basis vectors that change with position. And so more work is required before you can look at a metric and decide whether it describes something flat. -- "When the fool walks through the street, in his lack of understanding he calls everything foolish." -- Ecclesiastes 10:3, New American Bible |
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#9
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Gregory L. Hansen wrote in message ... In article , davidoff404 wrote: Starblade Darksquall wrote in message . com... Essentially, the reason one gets derivatives of the metric is because basis vectors in the manifold vary from point to point. This is unlike the case in flat space where the basis vectors remain constant throughout the space. Flat space with Cartesian coordinates, anyway. Non-Cartesian coordinates in flat space (e.g. polar coordinates) have basis vectors that change with position. And so more work is required before you can look at a metric and decide whether it describes something flat. Yes, my apologies; I really have to stop being too hasty in posting replies. I'll post a better answer tomorrow morning when I'm not so tired. By the way, I've just been giving some thought to the original question about why we have both first and second derivatives of the metric in the curvature tensor and realised something interesting. I've started thinking about using connections that are metric compatible but which are not torsion-free and realised that some really cool stuff happens when you relax the torsion requirement. I wonder why I never looked at that when I first learned GR? davidoff |
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#10
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"davidoff404" wrote in message ...
Gregory L. Hansen wrote in message ... In article , davidoff404 wrote: Starblade Darksquall wrote in message . com... Essentially, the reason one gets derivatives of the metric is because basis vectors in the manifold vary from point to point. This is unlike the case in flat space where the basis vectors remain constant throughout the space. Flat space with Cartesian coordinates, anyway. Non-Cartesian coordinates in flat space (e.g. polar coordinates) have basis vectors that change with position. And so more work is required before you can look at a metric and decide whether it describes something flat. Yes, my apologies; I really have to stop being too hasty in posting replies. I'll post a better answer tomorrow morning when I'm not so tired. By the way, I've just been giving some thought to the original question about why we have both first and second derivatives of the metric in the curvature tensor and realised something interesting. I've started thinking about using connections that are metric compatible but which are not torsion-free and realised that some really cool stuff happens when you relax the torsion requirement. I wonder why I never looked at that when I first learned GR? If your experience was like my continuing experience, you were trying so desperately to follow the basic train of thought that you had little attention to spare on those sorts of excursions. I could never ask meaningful questions about that sort of thing on a first exposure. Uncle Al has been going on about non-metric gravity. I'll look into that when I get the metric stuff down. |
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