Dubbelosix Posted December 31, 2017 Report Share Posted December 31, 2017 (edited) I wondered whether anyone had considered an equation of the form: [math]\frac{\partial \phi}{\partial t} = \alpha \Box^2 \phi[/math] Which is analogous to the Ricci flow but instead focuses on the potential - I soon found out it had indeed been suggested (see ref). The idea would invoke a relativistic Newton-Poisson equation of the form [math]\frac{\partial \phi}{\partial t} = \alpha \Box^2 \phi = - \alpha (\frac{\partial^2 \phi}{\partial \tau^2} - \frac{\partial^2 \phi}{\partial x^2} + \frac{\partial^2 \phi}{\partial y^2} + \frac{\partial^2 \phi}{\partial z^2}) = \alpha ( \frac{\partial^2 \phi}{\partial \tau^2} + \nabla^2\phi)[/math] We should note now, what the Newton-Poisson equation is in a standard three dimensional form [math]\nabla^2 \phi = 4 \pi G \rho[/math] It means we can write it as [math]\alpha \Box^2 \phi = \alpha (\frac{\partial^2 \phi}{\partial \tau^2} + 4\pi G \rho)[/math] This would be equivalent to a relativistic Poisson equation. You can consider a mass parameter as well and this would look like: [math]\alpha (\eta^{\mu \nu}\partial_{\mu} \partial_{\nu} \phi + |\mathbf{k}|^2 + \frac{\omega^2}{c^2}) = \alpha( \Box^2 \phi + \frac{m^2c^2}{\hbar}\phi ) = \alpha (\frac{\partial^2 \phi}{\partial \tau^2} + \nabla^2 \phi + \frac{m^2c^2}{\hbar}\phi)[/math] In which [math]- |\mathbf{k}|^2 + \frac{\omega^2}{c^2} = \frac{m^2c^2}{\hbar^2}[/math] Is the dispersion relation. In the context of curved space in general relativity, this turns into First without mass parameter. [math]\partial_t \phi \equiv \alpha g^{\mu \nu} \nabla_{\mu} \nabla_{\nu} \phi = \alpha g^{\mu \nu} \nabla_{\mu} (\partial_{\nu} \phi) = \alpha(g^{\mu \nu} \partial_{\mu}\partial_{\nu} \phi + g^{\mu \nu} \Gamma^{\sigma}_{\mu \nu}\partial_{\sigma}\phi) = \alpha(\frac{-1}{\sqrt{-g}}\partial_{\mu}(g^{\mu \nu} \sqrt{-g} \partial_{\nu} \phi)) [/math] And now with the mass parameter. [math] \alpha(g^{\mu \nu} \nabla_{\mu} \nabla_{\nu} \phi + \frac{p^{\mu}p_{\mu}}{\hbar^2}\phi) = \alpha (g^{\mu \nu} \nabla_{\mu} (\partial_{\nu} \phi) + \frac{p^{\mu}p_{\mu}}{\hbar^2}\phi) = \alpha(g^{\mu \nu} \partial_{\mu}\partial_{\nu} \phi + g^{\mu \nu} \Gamma^{\sigma}_{\mu \nu}\partial_{\sigma}\phi + \frac{p^{\mu}p_{\mu}}{\hbar^2}\phi)[/math] [math]= \alpha(g^{\mu \nu} \partial_{\mu}\partial_{\nu} \phi + g^{\mu \nu} \Gamma^{\sigma}_{\mu \nu}\partial_{\sigma}\phi + \frac{m^2}{\hbar^2} \frac{dx}{d \tau^{\mu}} \frac{d x}{d \tau^{\nu}}g^{\mu \nu}\phi)[/math] which is the curved diffusion equation with mass parameter. I have never seen the diffusion Ricci flow written like this. Ref: http://www.damtp.cam.ac.uk/user/reh10/lectures/nst-mmii-chapter2.pdf https://cmouhot.files.wordpress.com/1900/10/harmonicmaps.pdf Edited January 8, 2018 by Dubbelosix Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 (edited) I wondered whether anyone had considered an equation of the form: [math]\frac{\partial \phi}{\partial t} = \alpha \Box^2 \phi[/math] Which is analogous to the Ricci flow but instead focuses on the potential - I soon found out it had indeed been suggested (see ref). The idea would invoke a relativistic Newton-Poisson equation of the form [math]\frac{\partial \phi}{\partial t} = \alpha \Box^2 \phi = - \alpha (\frac{\partial^2 \phi}{\partial \tau^2} - \frac{\partial^2 \phi}{\partial x^2} + \frac{\partial^2 \phi}{\partial y^2} + \frac{\partial^2 \phi}{\partial z^2}) = \alpha ( \frac{\partial^2 \phi}{\partial \tau^2} + \nabla^2\phi)[/math] We should note now, what the Newton-Poisson equation is in a standard three dimensional form [math]\nabla^2 \phi = 4 \pi G \rho[/math] It means we can write it as [math]\alpha \Box^2 \phi = \alpha (\frac{\partial^2 \phi}{\partial \tau^2} + 4\pi G \rho)[/math] This would be equivalent to a relativistic Poisson equation. You can consider a mass parameter as well and this would look like: [math]\alpha \Box^2 \phi = \alpha (\frac{\partial^2 \phi}{\partial \tau^2} + \nabla^2 \phi + \frac{m^2c^2}{\hbar}\phi)[/math] In the context of curved space in general relativity, this turns into [math]\alpha \partial^{\mu}\partial_{\mu} \phi = \alpha (g^{\mu \nu} \nabla_{\mu} (\partial_{\nu} \phi) + \frac{m^2c^2}{\hbar^2}\phi) = \alpha(g^{\mu \nu} \partial_{\mu}\partial_{\nu} \phi + g^{\mu \nu} \Gamma^{\sigma}_{\mu \nu}\partial_{\sigma}\phi + \frac{m^2c^2}{\hbar^2}\phi)[/math] Ref: http://www.damtp.cam.ac.uk/user/reh10/lectures/nst-mmii-chapter2.pdf Ya, See I get what dubblesoix is saying here, basically Probability over Space then over time as torque. Edited December 31, 2017 by Vmedvil Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 (edited) [math]\phi[/math] is not a wave function, it is a gravitational potential. There is no torque in these equations either. It's a wave equation ... a four dimensional Poisson equation with diffusion coefficient. And the last equation describes it in terms of the curvature of spacetime. then why did you use the symbol phi that is probability and tau or τ which is torque? In any case, what is that like a 3rd or 4th or 5th integral? About phi in probability theoryhttps://en.wikipedia.org/wiki/Probability_theory Edited December 31, 2017 by Vmedvil Quote Link to comment Share on other sites More sharing options...
Shustaire Posted December 31, 2017 Report Share Posted December 31, 2017 Look for the 4 gradient. Anyways here is the 4d D'Alambertian operator [math]\square=\frac{1}{c^2}\frac{\partial^2}{\partial t^2}-\frac{\partial^2}{\partial x^2}-\frac{\partial^2}{\partial y^2}-\frac{\partial^2}{\partial z^2}[/math] Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 (edited) [math]\tau[/math] is spacelike time. It is composed of [math]c t[/math]. You can read about that on wiki's page on relativistic heat equation which even tells you about the difference between [math]\Box[/math] and [math]\Box^2[/math] https://en.wikipedia.org/wiki/Relativistic_heat_conduction Though their construction is using the temperature denoted as [math]\Theta[/math], in this work, in the OP, we are considered the diffusion of the potential field [math]\phi[/math]. Yes, so the time component is phi/tau = Probability per torque @ a unit of time which is the grad part. Edited December 31, 2017 by Vmedvil Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 (edited) Read the link I provided. It has it all there. No, that is torque it is a function of theta. Edited December 31, 2017 by Vmedvil Quote Link to comment Share on other sites More sharing options...
Shustaire Posted December 31, 2017 Report Share Posted December 31, 2017 (edited) Yes you can rewrite this as [math]\square = \frac{\partial^2}{\partial \tau^2}-\frac{\partial^2}{\partial x^2}-\frac{\partial^2}{\partial y^2}-\frac{\partial^2}{\partial z^2}[/math] As you can see the time derivative has absorbed the inverse speed of light squared and is the definition of the spacelike time variable. yes that's correct https://arxiv.org/pdf/1509.01543.pdf Edited December 31, 2017 by Shustaire Quote Link to comment Share on other sites More sharing options...
Shustaire Posted December 31, 2017 Report Share Posted December 31, 2017 proper time Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 (edited) Not in this work, in this work [math]\phi[/math] is the gravitational potential. And [math]\tau[/math] is a space derivative, it not a torque. The obviously you don't know what that was derived from. Edited December 31, 2017 by Vmedvil Quote Link to comment Share on other sites More sharing options...
Shustaire Posted December 31, 2017 Report Share Posted December 31, 2017 (edited) Not in this case Vmedvil https://en.wikipedia.org/wiki/Proper_time https://en.wikipedia.org/wiki/Coordinate_time anyways probably last you all will see of me have fun Edited December 31, 2017 by Shustaire Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 (edited) Not in this case VmedvilDid you even read the paper you sent me, either of you? Edited December 31, 2017 by Vmedvil Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 Those equations are not related Vmedvil with my work. The gravitational potential has dimensions of [math]-\frac{Gm}{R}[/math]. They come from Newtons laws. Has nothing to do with Torque are you so sure? Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 I constructed the equations, I should know what they are made of Vmedvil. It is missing a mass, or it would be torque. Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 And when I say dimensions, I don't mean the three space dimensions, I mean dimensional analysis. That is false, F = M a , Torque = F R C2 = V2 , a R = V2 Quote Link to comment Share on other sites More sharing options...
Vmedvil Posted December 31, 2017 Report Share Posted December 31, 2017 Oh, Dimensional analysis is important but it can if you convert the units. Quote Link to comment Share on other sites More sharing options...
Super Polymath Posted December 31, 2017 Report Share Posted December 31, 2017 I wondered whether anyone had considered an equation of the form: [math]\frac{\partial \phi}{\partial t} = \alpha \Box^2 \phi[/math] Which is analogous to the Ricci flow but instead focuses on the potential - I soon found out it had indeed been suggested (see ref). The idea would invoke a relativistic Newton-Poisson equation of the form [math]\frac{\partial \phi}{\partial t} = \alpha \Box^2 \phi = - \alpha (\frac{\partial^2 \phi}{\partial \tau^2} - \frac{\partial^2 \phi}{\partial x^2} + \frac{\partial^2 \phi}{\partial y^2} + \frac{\partial^2 \phi}{\partial z^2}) = \alpha ( \frac{\partial^2 \phi}{\partial \tau^2} + \nabla^2\phi)[/math] We should note now, what the Newton-Poisson equation is in a standard three dimensional form [math]\nabla^2 \phi = 4 \pi G \rho[/math] It means we can write it as [math]\alpha \Box^2 \phi = \alpha (\frac{\partial^2 \phi}{\partial \tau^2} + 4\pi G \rho)[/math] This would be equivalent to a relativistic Poisson equation. You can consider a mass parameter as well and this would look like: [math]\alpha \Box^2 \phi = \alpha (\frac{\partial^2 \phi}{\partial \tau^2} + \nabla^2 \phi + \frac{m^2c^2}{\hbar}\phi)[/math] In the context of curved space in general relativity, this turns into [math]\partial_t \phi \equiv \alpha \partial^{\mu}\partial_{\mu} \phi = \alpha (g^{\mu \nu} \nabla_{\mu} (\partial_{\nu} \phi) + \frac{m^2c^2}{\hbar^2}\phi) = \alpha(g^{\mu \nu} \partial_{\mu}\partial_{\nu} \phi + g^{\mu \nu} \Gamma^{\sigma}_{\mu \nu}\partial_{\sigma}\phi + \frac{m^2c^2}{\hbar^2}\phi)[/math] which is the curved diffusion equation with mass parameter. I have never seen the diffusion written like this. Ref: http://www.damtp.cam.ac.uk/user/reh10/lectures/nst-mmii-chapter2.pdf What about an ADS/CFT duality treatment for a 5 dimensional (one positive & one negative ~2.5 [2+/-1 as opposed to 3+1 dimensions [not dimensional analysis] to allow for causal sets, sub-planck micro causality for gw waves, for divisions of 1 planck length per 1 planck time aka C regimes for a non-discrete/lorentz invariant continuous spacetime with non-instantaneous quantum jumps albeit local realism] fractal dimension connected via wormhole metric) relativistic poisson equation? Could you build that for my theory in the event that I end up taking some calculus & can use it in the future? Quote Link to comment Share on other sites More sharing options...
Shustaire Posted December 31, 2017 Report Share Posted December 31, 2017 Ads/cft would not describe your personal hypothesis. Quote Link to comment Share on other sites More sharing options...
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