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Posted (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. 

 

 

 


 


Edited by Dubbelosix
Posted (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]
 
 
 
 

 

 

Ya, See I get what dubblesoix  is saying here, basically Probability over Space then over time as torque.

Edited by Vmedvil
Posted (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?

 

Torque_animation.gif

torque.gif

 

 

About phi in probability theory

https://en.wikipedia.org/wiki/Probability_theory

Edited by Vmedvil
Posted

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]

Posted (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 by Vmedvil
Posted (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 by Shustaire
Posted (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. 

 

220px-Moment_of_inertia_solid_sphere.svg

 

Torque_animation.gif

 

Edited by Vmedvil
Posted

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?

 

OiqkJLo.png

Posted

 

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. 
 
 
 

 

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? 

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