Recent content by James1238765

  1. James1238765

    Undergrad Geodesic path in 2 dimensions?

    1. The Riemann curvature in terms of Christoffel coefficients are: 2. The Riemann curvature in terms of ##\{a,b,c,d,e,f,g,h,i,j\}##, ##\{a',b',c',d',e',f',g',h',i',j'\}## are: 3. The Ricci curvature in terms of ##\{a,b,c,d,e,f,g,h,i,j\}##, ##\{a',b',c',d',e',f',g',h',i',j'\}##...
  2. James1238765

    Undergrad Geodesic path in 2 dimensions?

    1. For the boundary value problem in 10 variables ##\vec r = [a,b,c,d,e,f,g,h,i,j]## : $$\frac{d^2u}{da^2} + \frac{d^2u}{db^2} + \frac{d^2u}{dc^2} + \frac{d^2u}{dd^2} + \frac{d^2u}{de^2} + \frac{d^2u}{df^2} + \frac{d^2u}{dg^2} + \frac{d^2u}{dh^2} + \frac{d^2u}{di^2} + \frac{d^2u}{dj^2} = f(\vec...
  3. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    1. Random numerical ##g_{ij}## will generate valid ##T_{ij}##, with matter everywhere: Thus, the difficulty is in generating the black vacuum (zeros), instead of the (white) matter. 2. Combinatorially, we consider a 2x2x2 universe grid, with only 2 matter states (matter ON, and matter OF)...
  4. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    @romsofia thank you, the two books seem nicely computational! I have looked at a few books/articles on 3+1 method, a lot of new structures (folliation, ##\gamma##) seem needed for ADM & harmonic differential equations solving... I would like to try and exhaust simpler methods while reading up on...
  5. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    thank you. I think I roughly understand the general analytic strategy now, ie. try to guess the functional form of the independent ##g_{ij}## components and their dependencies on ##\{t, r, \theta, \phi \}##, such that as many of ##\frac{dg_{ij}}{d?}## becomes zero, which causes many ##\Gamma##...
  6. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    I think I see the differential equations now. If every step from ##g_{ij} \rightarrow R## is expanded into single equations form, we would get 16 equations with 10 variables (the ones in the original metric ##g_{ij}##), such as from [here]. So what are the standard methods to solve (in 1 go)...
  7. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    Which Einstein field equation? The geodesic ones will just calculate trajectories, don't they? What field differential equations precisely will arise from $$ R_{ij} + Rg_{ij} = T_{ij}$$ ? I would greatly appreciate it if someone could link to a straightforward worked example in numerical...
  8. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    Starting with ##T_{ij}## we have 16 numbers for each 3D gridpoint, with particular places we want to have all 0 values. The problem seems to be trying to reverse engineer what R and ##R_{ij}## will give rise to this result, then reverse engineer the ##\Gamma^i_{jk}## and all the way to...
  9. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    Ok. will try it backward from ##T_{ij}## next. Are all the reverse algorithms ##R \rightarrow R_{ij} \rightarrow R^i_{jk} \rightarrow \Gamma^i_{jk} \rightarrow g^{ij} \rightarrow g_{ij}## well defined and calculable for all the intermediate quantities?
  10. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    all that really long chain beginning with ##g_{ij} \rightarrow g^{ij} \rightarrow \Gamma^i_{jk} \rightarrow R^i_{jkl} \rightarrow R_{ij} \rightarrow R##
  11. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    The heavyweight computations used original Schwarzchild coordinates, and I was wary if changing to Cartesian suddenly might break something. Yes otffset being time dependant would mean moving bodies, though the solution as currently obtained gives nonsensical ##T_{ij}## anyways, so it's still...
  12. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    Sorry the coordinate notation was abstract. Here's a real example, the point (1, 1, 1) in spherical coordinate is first transformed into cartesian via: $$x = r \sin \theta \ cos \phi$$ $$y = r \sin \theta \ sin \phi$$ $$z = r \ cos \theta$$ we obtain the new cartesian coordinates: Next we...
  13. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    Adding 2 sources for ##g_{ij}## could be done pointwise as follows: $$ g_{total} (r, \theta, \phi) = g_{ij} (r, \theta, \phi) + $$ $$g_{ij}(Sph_r(Cart_x(r,\theta,\phi)+dist_x, Cart_y(r,\theta,\phi)+dist_y, Cart_z(r,\theta,\phi)+dist_z))$$ Single source metric is a vacuum solution: Two...
  14. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    @Ibix from differential equations perspective, could we recover completely ##g_{ij}## from the full set of descendant ##\Gamma^i_{jk}## (post 33)? As to why I insist on trying this, even if the solution is wrong, the practice is often invaluable. We can see in a single picture if the ##T_{ij}##...
  15. James1238765

    Undergrad Modeling the Earth and Sun (2 body orbits) using general relativity?

    Is it possible to recover ##g_{ij}## completely from all the descendant ##\Gamma^i_{jk}##? Adding ##\Gamma^i_{jk}## can easily be done gridpoint-wise. The main problem is the combined metric ##g^{ij}## is needed to calculate R. This combined metric is probably ugly looking, but can it be...