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#51
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On May 12, 10:55 pm, Koobee Wublee wrote:
On May 11, 11:43 pm, JanPB wrote: On May 11, 9:53 pm, Koobee Wublee wrote: ds^2 = G c^2 dt^2 / (1 + K^2 / r^2) – 4 r^2 (1 + K^2 / r^2) dr^2 / K^2 – (r^2 + K^2)^2 dO^2 / K^2 Its Ricci and Einstein tensors both vanish. In doing so, it is also sharing the same coordinate system with the Schwarzschild metric. I meant I computed only R_theta,theta and didn't bother with the rest. Remember dO^2 consists of r, theta, and phi as the Ricci and the Einstein tensors are only valid in four dimensions. Since you have not computed the Ricci tensor, you have no right to call the above solution not a null result of the Ricci and the Einstein tensors. shrug There is no point to continue. If Ricci tensor were zero, then R_theta,theta would be zero. It isn't, hence Ricci is not zero. Looking for a generic solution that is static and spherically symmetric, we employ the spherically symmetric coordinate system that describes a segment of spacetime in general of the following. ds^2 = c^2 T(r) dt^2 – P(r) dr^2 – Q(r) dO^2 Where ** T(r), P(r), Q(r) = Functions of r only ** dO^2 = cos^2(Phi) dTheta^2 + dPhi^2 Yes. But the formula you presented: ds^2 = G c^2 dt^2 / (1 + K^2 / r^2) – 4 r^2 (1 + K^2 / r^2) dr^2 / K^2 – (r^2 + K^2)^2 dO^2 / K^2 ...is not a solution if you take r to be the same as in Schwarzschild's formula. Then, the null Einstein tensor (not Ricci) tensor (in free space) is represented by the following 3 differential equations. You are supposed to get 4, but 2 of these are identical. ** 1 + dQ/dr dP/dr / (2 P^2) + (dQ/dr)^2 / (4 P Q) – d^2Q/dr^2 / P = 0 ** 1 – dQ/dr dT/dr / (1 T P) – (dQ/dr)^2 / (4 P Q) = 0 ** - d^2T/dr^2 / T + dT/dr dP/dr / (2 T P) + (dT/dr)^2 / (2 T^2) – dQ/ dr dT/dr / (2 Q T) + dP/dr dQ/dr / (2 P Q) + (dQ/dr)^2 / (2 Q^2) – d^2Q/dr^2 / Q = 0 There are an infinite number of solutions found. No. While your statement is true in the generic case, it turns out that in those coordinates these equations become ordinary diff. equations ("ordinary" is a technical term meaning "in one variable"). And it is well-known that ordinary differential equations have unique solutions - it follows, oddly enough, from a fixed point theorem. It's a classic result called Picard-Lindeloef theorem. A few examples are the following in the order of first discovered. These include the inverse cubed law one at the beginning of the post. ** Schwarzschild’s original solution ds^2 = G c^2 dt^2 (1 - K / R) – r^4 dr^2 / R^4 / (1 - K / R) – R^2 dO^2 Where ** R = (r^3 + K^3)^(1/3) ** Schwarzschild (Hilbert’s) solution ds^2 = G c^2 (1 + K / r) dt^2 – dr^2 / (1 + K / r) – r^2 dO^2 ** ?’s solution ds^2 = G c^2 dt^2 / (1 + K / r) – dr^2 (1 + K / r) – (r + K)^2 dO^2 Same thing. If "r" in these formulas are presumed the same, then the third one does not satisfy Ricci=0. OTOH if the radial coordinates in these formulas are related by substitutions, then they are the same solution, only written in different bases. Just like dx equals cos(theta)dr - r sin(theta)dtheta - just written in different bases. You need to resolve your own mathematical errors. I cannot help you on that one. shrug The bottom line is that the Newtonian solution is not unique under the Einstein field equations, and you need to get over with that. shrug It is also time to vacate from that fat castle in the air, your majesty, the queer of England. That's nice but have you noticed that your claim that the formula: ds^2 = G c^2 dt^2 / (1 + K^2 / r^2) – 4 r^2 (1 + K^2 / r^2) dr^2 / K^2 – (r^2 + K^2)^2 dO^2 / K^2 ...with Schwarzschild's "r" was a solution has just been disproved? -- Jan Bielawski |
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#52
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On May 12, 11:05 pm, Mike wrote:
On May 13, 1:55 am, Koobee Wublee wrote: [...] There are an infinite number of solutions found. A few examples are the following in the order of first discovered. These include the inverse cubed law one at the beginning of the post. Of course there are infinite solutions. But they will not accept this. What they do is select the solution they want to get as a result. Then work the math to get that solutions. Then claim they got the solution. Nice, eh? Nice but it's baloney. Good for a Hollywood movie. It's much easier to believe in silly conspiracies than to do honest work. -- Jan Bielawski |
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#53
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On May 12, 11:24 pm, Koobee Wublee wrote:
On May 12, 11:16 pm, Eric Gisse wrote: On May 12, 9:55 pm, Koobee Wublee wrote: You continue to say "infinite number" like that's supposed to have any meaning. So, you don’t understand what infinity represents. There is an infinite number of coordinate systems Yes. shrug that the Schwarzschild solution can be projected on, The Schwarzschild metric only applies to the spherically symmetric polar coordinate system and nothing else. No, that's false. It's exactly like saying "the vector pointing to the North Star applies only to the spherically symmetric polar coordinate system and nothing else". The same North-Star-pointing vector has different component triplets in different coordinates. Do you agree? Tensors of rank higher than 1 are exactly the same way. So, you do not understand the Schwarzschild metric, either. like any other metric. Other metric as a solution to the Einstein field equations also only applies to the spherically symmetric polar coordinate system and nothing else, That's false. Would you say that a vector field (say, velocity field of a fluid) "only applies to" a particular system? -- Jan Bielawski |
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#54
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On May 12, 11:32 pm, JanPB wrote:
On May 12, 10:55 pm, Koobee Wublee wrote: ds^2 = G c^2 dt^2 / (1 + K^2 / r^2) – 4 r^2 (1 + K^2 / r^2) dr^2 / K^2 – (r^2 + K^2)^2 dO^2 / K^2 Its Ricci and Einstein tensors both vanish. In doing so, it is also sharing the same coordinate system with the Schwarzschild metric. Looking for a generic solution that is static and spherically symmetric, we employ the spherically symmetric coordinate system that describes a segment of spacetime in general of the following. ds^2 = c^2 T(r) dt^2 – P(r) dr^2 – Q(r) dO^2 Where ** T(r), P(r), Q(r) = Functions of r only ** dO^2 = cos^2(Phi) dTheta^2 + dPhi^2 Yes. But the formula you presented: ds^2 = G c^2 dt^2 / (1 + K^2 / r^2) – 4 r^2 (1 + K^2 / r^2) dr^2 / K^2 – (r^2 + K^2)^2 dO^2 / K^2 ...is not a solution if you take r to be the same as in Schwarzschild's formula. Mathematically, what you are saying is just wrong. shrug Then, the null Einstein tensor (not Ricci) tensor (in free space) is represented by the following 3 differential equations. You are supposed to get 4, but 2 of these are identical. ** 1 + dQ/dr dP/dr / (2 P^2) + (dQ/dr)^2 / (4 P Q) – d^2Q/dr^2 / P = 0 ** 1 – dQ/dr dT/dr / (1 T P) – (dQ/dr)^2 / (4 P Q) = 0 ** - d^2T/dr^2 / T + dT/dr dP/dr / (2 T P) + (dT/dr)^2 / (2 T^2) – dQ/ dr dT/dr / (2 Q T) + dP/dr dQ/dr / (2 P Q) + (dQ/dr)^2 / (2 Q^2) – d^2Q/dr^2 / Q = 0 There are an infinite number of solutions found. No. While your statement is true in the generic case, it turns out that in those coordinates these equations become ordinary diff. equations ("ordinary" is a technical term meaning "in one variable"). And it is well-known that ordinary differential equations have unique solutions - it follows, oddly enough, from a fixed point theorem. It's a classic result called Picard-Lindeloef theorem. A few examples are the following in the order of first discovered. These include the inverse cubed law one at the beginning of the post. ** Schwarzschild’s original solution ds^2 = G c^2 dt^2 (1 - K / R) – r^4 dr^2 / R^4 / (1 - K / R) – R^2 dO^2 Where ** R = (r^3 + K^3)^(1/3) ** Schwarzschild (Hilbert’s) solution ds^2 = G c^2 (1 + K / r) dt^2 – dr^2 / (1 + K / r) – r^2 dO^2 ** ?’s solution ds^2 = G c^2 dt^2 / (1 + K / r) – dr^2 (1 + K / r) – (r + K)^2 dO^2 Same thing. If "r" in these formulas are presumed the same, then the third one does not satisfy Ricci=0. Well, all these are solutions to the field equations. Closing your eyes and yelling they are not does not make them not. shrug It is all in the mathematics. shrug OTOH if the radial coordinates in these formulas are related by substitutions, then they are the same solution, only written in different bases. You are full of crap. The coordinate system is the spherically symmetric polar coordinate system and nothing else. shrug Just like dx equals cos(theta)dr - r sin(theta)dtheta - just written in different bases. Wrong analogy. As a film critic of second-rated films, you are very subjective, aren’t you? You need to resolve your own mathematical errors. I cannot help you on that one. shrug The bottom line is that the Newtonian solution is not unique under the Einstein field equations, and you need to get over with that. shrug It is also time to vacate from that fat castle in the air, your majesty, the queer of England. That's nice but have you noticed that your claim that the formula: ds^2 = G c^2 dt^2 / (1 + K^2 / r^2) – 4 r^2 (1 + K^2 / r^2) dr^2 / K^2 – (r^2 + K^2)^2 dO^2 / K^2 ...with Schwarzschild's "r" was a solution has just been disproved? I don’t know what you mean by my own claim. I have claimed that all these solutions are mathematically tested out to be the solutions to the Einstein field equations under the spherically symmetric polar coordinate system. shrug It is better for you majesty, the queer of England, to retire into that soon-to-demolished fat castle in the air, for it will not be there long. You don’t have to be such scared sh*tless. At least, you can still go back being a critic for all these second-rated films, no? |
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#55
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On May 13, 1:24*am, Koobee Wublee wrote:
On May 12, 11:16 pm, Eric Gisse wrote: On May 12, 9:55 pm, Koobee Wublee wrote: You continue to say "infinite number" like that's supposed to have any meaning. So, you don’t understand what infinity represents. There is an infinite number of coordinate systems Yes. *shrug that the Schwarzschild solution can be projected on, The Schwarzschild metric only applies to the spherically symmetric polar coordinate system and nothing else. *So, you do not understand the Schwarzschild metric, either. No, that's incorrect. The Schwarzchild metric is a *shape*. It is most conveniently described in one set of coordinates, but it can certainly be described in more than one coordinate system. Likewise, the hydrogen atom wavefunctions are most conveniently written in spherically polar coordinates, so that one can take algebraic advantage of the properties of Legendre polynomials and Bessel radial functions, and because the spherically symmetric potential allows for the quick finding of these solutions by virtue of the algebraic method called separation of variables. But if you were to say that it is simply impossible to write the hydrogen atom wavefunctions in anything other than spherically polar coordinates, you'd be daft. To take it one step further just to hammer in the point, writing the equation of a sphere of radius R is easiest in spherical polar coordinates, but it is certainly possible to write the equation for the same sphere in rectangular coordinates, or cylindrical coordinates, or any other coordinate system you choose. like any other metric. Other metric as a solution to the Einstein field equations also only applies to the spherically symmetric polar coordinate system and nothing else, and you have never understood the field equations. shrug What makes me wonder is why you think this is meaningful or even relevant to the uniqueness of the solution. You remain a multi-year super-senior. *shrug You write down multiple representations of the same thing and expect us to agree with you that they are different. It doesn't work that way. You were expecting to graduate this spring. *Did it happen? *No. shrug |
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#56
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On May 12, 10:24*pm, Koobee Wublee wrote:
On May 12, 11:16 pm, Eric Gisse wrote: On May 12, 9:55 pm, Koobee Wublee wrote: You continue to say "infinite number" like that's supposed to have any meaning. So, you don’t understand what infinity represents. I usually take it to mean "lots", or in a more general sense, "more than one". You chose the coordinate form so there is only one solution for that particular coordinate form. Ever read anything about ODE uniqueness theorems? The other solutions are clearly in different coordinate systems. There is an infinite number of coordinate systems Yes. *shrug that the Schwarzschild solution can be projected on, The Schwarzschild metric only applies to the spherically symmetric polar coordinate system and nothing else. *So, you do not understand the Schwarzschild metric, either. There are still an infinite number of spherically symmetric coordinate representations of Schwarzschild - you have shown me at least 3 of them. Who says that the metric is only true in a spherically symmetric coordinate system? I can write the line element in Cartesian, prolate spherical, or cylindrical coordinates. Or can I not do that for some reason? like any other metric. Other metric as a solution to the Einstein field equations also only applies to the spherically symmetric polar coordinate system and nothing else, and you have never understood the field equations. shrug Since when does the coordinate system determine the physics? Spherical symmetry is a property of the manifold, not the coordinate system. Writing something in spherical coordinates doesn't make it spherically symmetric - or did you not know what? Glass houses, kooby. What makes me wonder is why you think this is meaningful or even relevant to the uniqueness of the solution. You remain a multi-year super-senior. *shrug You write down multiple representations of the same thing and expect us to agree with you that they are different. It doesn't work that way. You were expecting to graduate this spring. *Did it happen? *No. shrug I was also expecting a pony. Where's my pony? I'll say this once and no mo my personal life is exactly none of your business. |
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#57
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On May 13, 12:37 am, Eric Gisse wrote:
You chose the coordinate form so there is only one solution for that particular coordinate form. [The rest of crap is mercifully snipped.] You continue to whine and distort what I have said. Go back to sit on your piles of books. |
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#58
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On May 13, 12:21 am, PD wrote:
On May 13, 1:24 am, Koobee Wublee wrote: The Schwarzschild metric only applies to the spherically symmetric polar coordinate system and nothing else. So, you do not understand the Schwarzschild metric, either. No, that's incorrect. The Schwarzchild metric is a *shape*. It is most conveniently described in one set of coordinates, but it can certainly be described in more than one coordinate system. The spacetime described by the Schwarzschild metric only applied to the spherically symmetric polar coordinate. You are welcome to transform to another coordinate system with a different metric. The segment of spacetime remains the same and thus invariant while the coordinate is your choice as well as the metric associated with this coordinate to describe the invariant segment of spacetime. This concept is so basic, but you have a lot of trouble understanding that. There is no need to go through the rest of your babbling. shrug |
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#59
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On May 12, 11:51 pm, JanPB wrote:
On May 12, 11:24 pm, Koobee Wublee wrote: The Schwarzschild metric only applies to the spherically symmetric polar coordinate system and nothing else. No, that's false. It's exactly like saying "the vector pointing to the North Star applies only to the spherically symmetric polar coordinate system and nothing else". The spacetime described by the Schwarzschild metric only applied to the spherically symmetric polar coordinate. You are welcome to transform to another coordinate system with a different metric. The segment of spacetime remains the same and thus invariant while the coordinate is your choice as well as the metric associated with this coordinate to describe the invariant segment of spacetime. shrug This concept is so basic, but you have a lot of trouble understanding that. There is no point to go through the north star nonsense. |
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#60
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On May 13, 4:46*pm, Koobee Wublee wrote:
On May 13, 12:21 am, PD wrote: On May 13, 1:24 am, Koobee Wublee wrote: The Schwarzschild metric only applies to the spherically symmetric polar coordinate system and nothing else. *So, you do not understand the Schwarzschild metric, either. No, that's incorrect. The Schwarzchild metric is a *shape*. It is most conveniently described in one set of coordinates, but it can certainly be described in more than one coordinate system. The spacetime described by the Schwarzschild metric only applied to the spherically symmetric polar coordinate. Repeating the same erroneous statement does not inch it any further toward being right. *You are welcome to transform to another coordinate system with a different metric. *The segment of spacetime remains the same and thus invariant while the coordinate is your choice as well as the metric associated with this coordinate to describe the invariant segment of spacetime. This concept is so basic, but you have a lot of trouble understanding that. *There is no need to go through the rest of your babbling. shrug |
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