Vmedvil Posted December 11, 2017 Author Share Posted December 11, 2017 (edited) Furthermore. Which I using that form. ks = (K(8π/C2)) , K = ((-Duv(g) -ktuv)Tuv-1) ∇'(x,y,z,t,ωs,ωp,M,I,k,φ,S,X,Z,μ,Y,q,a,β) = (((ħ2 /(2Erest/C2)) ∑3a =1 (d2/d((C2/Erest)∑Ni = 1 MiRi)2) + (1/2)∑3a,β = 1 μaβ(Pa - Πa)(Pβ - Πβ) + U - (ħ2/2)∑3N-6s=1(d2/dq2) + V)((|(Log(DgDaDψDφ-W)(((2ħGC2))Rs - (1/4)FaμvFaμv + i(ψ-bar)γμ(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)ψi +(ψ-bar)iLVijφψjr + (aji) - (μ2((φ-Dagger)φ) + λ((φ-Dagger)φ)2)/-(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)2)|)-e2S(r,t)/h)) - ((Erest/C2)ωs((((-Duv(g) -ktuv)Tuv-1)(8π/C2))2)1/2 + (S/ (((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp ))))Rs2/2))) / (ħ2/2(Erest/C2))))1/2(((1-(((2(Erest/C2)G / Rs) - (Isωs((((-Duv(g) -ktuv)Tuv-1)(8π/C2))2)1/2 + (S/(((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp )))))/2(Erest/C2))+ (((8πG/3)((g/(2π)3)∫(((Erelativistic2 - Erest2 / C2) + ((Ar(X) + (ENucleon binding SNF ε0 μ0 /mu) - Ar(XZ±)/Z) / mu)2)(1/2)(1/e((ERelativistic - μchemical)/TMatter)±1)(ħωs + ħωs) - ((ksC2)/ Rs2) + (((((-Duv(g) -ktuv)Tuv-1)(8π/C2))2)1/2(ΔKiloparsec)))2/(C2)))1/2) Edited December 11, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Mordred Posted December 12, 2017 Share Posted December 12, 2017 (edited) 7 hours ago, Vmedvil said: Okay, I don't see how that changes anything, I used Gaussian Curvature and set it equal to (1/2)R in EFE I didn't go to Tuv but I could have, stopped at Guv Oh, I see what you are whining about that is for gab, which the first time I used for this part. Mordred you caused this to be that way, I changed it because of you from the original form which was gab because I took it on oh Mordred must know what he is talking about but this version is worse. (1/2)R = ((-8πGTab' - Λgab + Rab) * -gab-1) sigh I give up, keep making mistakes. You have looked over dozens of papers that mention Covarient and contravariant terms and indices as per Einstein summation. Yet you replace this with Gaussian curve fitting. Replacing the entire metric tensor with a central potential (covariant term). Please study the ***^&UUGFTYYGHGD Eienstein summation rules. Then apply the *&^&^&%^&$ right hand rules to the covariant and contravariant indices. In that equation above. How can you be so bleeding blind (right hand rule=covariant) [math]\frac{8\pi G}{c^4}[/math] is only central potential force there is examples where this is not the case. Edited December 12, 2017 by Mordred Link to comment Share on other sites More sharing options...
Vmedvil Posted December 12, 2017 Author Share Posted December 12, 2017 13 minutes ago, Mordred said: sigh I give up, keep making mistakes. You have looked over dozens of papers that mention Covarient and contravariant terms and indices as per Einstein summation. Yet you replace this with Gaussian curve fitting. Replacing the entire metric tensor with a central potential (covariant term). Please study the ***^&UUGFTYYGHGD Eienstein summation rules. Then apply the *&^&^&%^&$ right hand rules to the covariant and contravariant indices. In that equation above. How can you be so bleeding blind (right hand rule=covariant) Well, it has to be uv and not ab has to be up to my standards of a non screwed up equation too, I won't use the ab form. Link to comment Share on other sites More sharing options...
Mordred Posted December 12, 2017 Share Posted December 12, 2017 (edited) No indices Einstein summation [math]G_{\mu\nu}, G^{\mu\nu}, G^{\mu_\nu}[/math] study what each of those means per the tensor your using. Edited December 12, 2017 by Mordred Link to comment Share on other sites More sharing options...
Vmedvil Posted December 12, 2017 Author Share Posted December 12, 2017 24 minutes ago, Mordred said: No indices Einstein summation Gμν,Gμν,Gμν study what each of those means per the tensor your using. Ya, Contravariant and covariant are no different, from everything I have looked at. Link to comment Share on other sites More sharing options...
Mordred Posted December 12, 2017 Share Posted December 12, 2017 Then identify the central potential Gaussian under Newtons laws then do this under the Newton limit under GR Link to comment Share on other sites More sharing options...
Vmedvil Posted December 12, 2017 Author Share Posted December 12, 2017 (edited) 4 minutes ago, Mordred said: Then identify the central potential Gaussian under Newtons laws then do this under the Newton limit under GR Yes, it is co-variant my curvature is co-variant why does this matter Co-variant ks2 = K = (1/2)R Co-variant Edited December 12, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Mordred Posted December 12, 2017 Share Posted December 12, 2017 (edited) So is your equation valid when [latex]g_{\mu\nu}=g_{\alpha\beta}=\frac{dx^{\alpha}}{dy^{\mu}}\frac{dx^{\beta}}{dy^{\nu}}[/latex] Metric tensor [latex]dx^2=(dx^0)^2+(dx^1)^2+(dx^3)^2[/latex] [latex]G_{\mu\nu}=\begin{pmatrix}g_{0,0}&g_{0,1}&g_{0,2}&g_{0,3}\\g_{1,0}&g_{1,1}&g_{1,2}&g_{1,3}\\g_{2,0}&g_{2,1}&g_{2,2}&g_{2,3}\\g_{3,0}&g_{3,1}&g_{3,2}&g_{3,3}\end{pmatrix}=\begin{pmatrix}-1&0&0&0\\0&1&0&0\\0&0&1&0\\0&0&0&1\end{pmatrix}[/latex] Which corresponds to [latex]\frac{dx^\alpha}{dy^{\mu}}=\frac{dx^\beta}{dy^{\nu}}=\begin{pmatrix}\frac{dx^0}{dy^0}&\frac{dx^1}{dy^0}&\frac{dx^2}{dy^0}&\frac{dx^3}{dy^0}\\\frac{dx^0}{dy^1}&\frac{dx^1}{dy^1}&\frac{dx^2}{dy^1}&\frac{dx^3}{dy^1}\\\frac{dx^0}{dy^2}&\frac{dx^1}{dy^2}&\frac{dx^2}{dy^2}&\frac{dx^3}{dy^2}\\\frac{dx^0}{dy^3}&\frac{dx^1}{dy^3}&\frac{dx^2}{dy^3}&\frac{dx^3}{dy^3}\end{pmatrix}[/latex] The simplest transform is the Minkowskii metric, Euclidean space or flat space. This is denoted by [latex]\eta[[/latex] Flat space [latex]\mathbb{R}^4 [/latex] with Coordinates (t,x,y,z) or alternatively (ct,x,y,z) flat space is done in Cartesian coordinates. In this metric space time is defined as [latex] ds^2=-c^2dt^2+dx^2+dy^2+dz^2=\eta_{\mu\nu}dx^{\mu}dx^{\nu}[/latex] [latex]\eta=\begin{pmatrix}-c^2&0&0&0\\0&1&0&0\\0&0&1&0\\0&0&0&1\end{pmatrix}[/latex] do you see where the (c^2 1 1 1) diagonal terms comes from ? in the diagonal components yet? Edited December 12, 2017 by Mordred Link to comment Share on other sites More sharing options...
Vmedvil Posted December 12, 2017 Author Share Posted December 12, 2017 (edited) 24 minutes ago, Mordred said: So is your equation valid when gμν=gαβ=dxαdyμdxβdyν Metric tensor dx2=(dx0)2+(dx1)2+(dx3)2 Gμν=⎛⎝⎜⎜⎜⎜g0,0g1,0g2,0g3,0g0,1g1,1g2,1g3,1g0,2g1,2g2,2g3,2g0,3g1,3g2,3g3,3⎞⎠⎟⎟⎟⎟=⎛⎝⎜⎜⎜−1000010000100001⎞⎠⎟⎟⎟ Which corresponds to dxαdyμ=dxβdyν=⎛⎝⎜⎜⎜⎜⎜⎜⎜⎜dx0dy0dx0dy1dx0dy2dx0dy3dx1dy0dx1dy1dx1dy2dx1dy3dx2dy0dx2dy1dx2dy2dx2dy3dx3dy0dx3dy1dx3dy2dx3dy3⎞⎠⎟⎟⎟⎟⎟⎟⎟⎟ The simplest transform is the Minkowskii metric, Euclidean space or flat space. This is denoted by η[ Flat space R4 with Coordinates (t,x,y,z) or alternatively (ct,x,y,z) flat space is done in Cartesian coordinates. In this metric space time is defined as ds2=−c2dt2+dx2+dy2+dz2=ημνdxμdxν η=⎛⎝⎜⎜⎜−c2000010000100001⎞⎠⎟⎟⎟ Yes, but it is in that ds solved form being Laplace prime, XYZ being Laplace that you see. Edited December 12, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Mordred Posted December 12, 2017 Share Posted December 12, 2017 NO you follow the chain rule at each infinitisimal when curve fitting via the tangent vector at each coordinate of particle travel through spacetime. That is the curve fitting under GR [latex]\frac{dx^\alpha}{dy^{\mu}}=\frac{dx^\beta}{dy^{\nu}}=\begin{pmatrix}\frac{dx^0}{dy^0}&\frac{dx^1}{dy^0}&\frac{dx^2}{dy^0}&\frac{dx^3}{dy^0}\\\frac{dx^0}{dy^1}&\frac{dx^1}{dy^1}&\frac{dx^2}{dy^1}&\frac{dx^3}{dy^1}\\\frac{dx^0}{dy^2}&\frac{dx^1}{dy^2}&\frac{dx^2}{dy^2}&\frac{dx^3}{dy^2}\\\frac{dx^0}{dy^3}&\frac{dx^1}{dy^3}&\frac{dx^2}{dy^3}&\frac{dx^3}{dy^3}\end{pmatrix}[/latex] Link to comment Share on other sites More sharing options...
Vmedvil Posted December 12, 2017 Author Share Posted December 12, 2017 (edited) 8 minutes ago, Mordred said: NO you follow the chain rule at each infinitisimal when curve fitting via the tangent vector at each coordinate of particle travel through spacetime. That is the curve fitting under GR dxαdyμ=dxβdyν=⎛⎝⎜⎜⎜⎜⎜⎜⎜⎜dx0dy0dx0dy1dx0dy2dx0dy3dx1dy0dx1dy1dx1dy2dx1dy3dx2dy0dx2dy1dx2dy2dx2dy3dx3dy0dx3dy1dx3dy2dx3dy3⎞⎠⎟⎟⎟⎟⎟⎟⎟⎟ See, this is probably why I don't understand this Welcome to the parts of Calculus I, that I hated. you said the magic word "Chain Rule" No I don't understand. If you follow that by product rule along with quotient rule, I will literally just leave the part for GR blank as not worth it. Edited December 12, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Mordred Posted December 12, 2017 Share Posted December 12, 2017 (edited) yeah variational Calculus can be a pain in the arse but no matter what direction your particle changes path at each infinitisimal this provides the required derivitaves. Your indice values give the entry required at each coordinate. This is where the term locality becomes important. As not the entire field affects the above at once due to speed of information exchange. Only the local portion of the field does at each coordinate. Local range defined by speed of information exchange from field to particle at each time dependent coordinate. I have really bad news for you Every Symmetry group uses the chain rule, so does every tensor. ODE and PDE is part of the chain rule under Taylor expansions. So does all Langrene's and Hamilton's once you understand them properly prime example Feyman path integrals http://wwwf.imperial.ac.uk/~jdg/AECHAIN.PDF the second link is the ODE as per QM QFT. http://www1.phys.vt.edu/~ersharpe/6455/ch1.pdf all these examples are detailed under MULTI-Variational calculus ie two or more variables at each coordinate. Edited December 12, 2017 by Mordred Link to comment Share on other sites More sharing options...
Vmedvil Posted December 12, 2017 Author Share Posted December 12, 2017 (edited) 45 minutes ago, Mordred said: yeah variational Calculus can be a pain in the arse but no matter what direction your particle changes path at each infinitisimal this provides the required derivitaves. Your indice values give the entry required at each coordinate. This is where the term locality becomes important. As not the entire field affects the above at once due to speed of information exchange. Only the local portion of the field does at each coordinate. Local range defined by speed of information exchange from field to particle at each time dependent coordinate. I have really bad news for you Every Symmetry group uses the chain rule, so does every tensor. ODE and PDE is part of the chain rule under Taylor expansions. So does all Langrene's and Hamilton's once you understand them properly prime example Feyman path integrals http://wwwf.imperial.ac.uk/~jdg/AECHAIN.PDF the second link is the ODE as per QM QFT. http://www1.phys.vt.edu/~ersharpe/6455/ch1.pdf all these examples are detailed under MULTI-Variational calculus ie two or more variables at each coordinate. See, but I get Multi-variable calculus, ya Simple chain rule makes no sense but the one of multi-variables perfect, oh wait, that wasn't the chain rule, I was thinking of there is another one. Product and Quotient rule, whatever that is caused from. Wait ya, I am pretty sure that is there as (i,j,k) I hated calculus I in general. 17 minutes ago, Vmedvil said: See, but I get Multi-variable calculus, ya Simple chain rule makes no sense but the one of multi-variables perfect, oh wait, that wasn't the chain rule, I was thinking of there is another one. Product and Quotient rule, whatever that is caused from. Wait ya, I am pretty sure that is there as (i,j,k) I hated calculus I in general. Where ∇'(x',y',z') = ∇(1-(((2MbG / Rs) - (Isωs2/2Mb))2/C2))1/2 is like saying, d/dx(1-(((2MbG / Rs) - (Isωs2/2Mb))2/C2))1/2 + d/dy(1-(((2MbG / Rs) - (Isωs2/2Mb))2/C2))1/2 + d/dz((1-(((2MbG / Rs) - (Isωs2/2Mb))2/C2))1/2) Where dx,dy,dz or whatever is that equation. Edited December 12, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Mordred Posted December 12, 2017 Share Posted December 12, 2017 (edited) Well its required to understand how tensors work. For example Kronecker Delta (parallel transport of two vectors)(equivalence Principle. Levi_Cevita loss of parallel transport of two vectors (tidal forces due to geometry curvature). Kronecker linear coordinates Calculus 1. Levi_Cevita is more applied under calculus 2. curvilinear coordinates [math]\partial_i,j[/math] Kronecker [math\partial_{i,j,k}[/latex] Levi inner product of two vectors returns a scalar cross product of two vectors a vector outer product is the product of two coordinate tensors ie kronecker and will return a tensor product as such Edited December 12, 2017 by Mordred Link to comment Share on other sites More sharing options...
Vmedvil Posted December 12, 2017 Author Share Posted December 12, 2017 (edited) 8 minutes ago, Mordred said: Well its required to understand how tensors work. For example Kronecker Delta (parallel transport of two vectors)(equivalence Principle. Levi_Cevita loss of parallel transport of two vectors (tidal forces due to geometry curvature) Oh, I realize what you did now okay got it. So, your saying I need to solve for u,v from a,b doing a reverse chain rule or just a chain rule in the opposite direction as that. Edited December 12, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Mordred Posted December 12, 2017 Share Posted December 12, 2017 (edited) should give you a new understanding of groups and tensors. As well as how to use them. Edited December 12, 2017 by Mordred Link to comment Share on other sites More sharing options...
Vmedvil Posted December 12, 2017 Author Share Posted December 12, 2017 (edited) well, I didn't know you could transfer ab to uv, So, it will stay like this until I can solve that mess to transfer between them. ∇'(x,y,z,t,ωs,ωp,M,I,k,φ,S,X,Z,μ,Y,q,a,β) = (((ħ2 /(2Erest/C2)) ∑3a =1 (d2/d((C2/Erest)∑Ni = 1 MiRi)2) + (1/2)∑3a,β = 1 μaβ(Pa - Πa)(Pβ - Πβ) + U - (ħ2/2)∑3N-6s=1(d2/dq2) + V)((|(Log(DgDaDψDφ-W)(((2ħGC2))Rs - (1/4)FaμvFaμv + i(ψ-bar)γμ(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)ψi +(ψ-bar)iLVijφψjr + (aji) - (μ2((φ-Dagger)φ) + λ((φ-Dagger)φ)2)/-(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)2)|)-e2S(r,t)/h)) - ((Erest/C2)ωs(((8πGTab' + Λgab - Rab) * gab-1))1/2 + (S/ (((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp ))))Rs2/2))) / (ħ2/2(Erest/C2))))1/2(((1-(((2(Erest/C2)G / Rs) - (Isωs(((8πGTab' + Λgab - Rab) * gab-1))1/2 + (S/(((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp )))))/2(Erest/C2))+ (((8πG/3)((g/(2π)3)∫(((Erelativistic2 - Erest2 / C2) + ((Ar(X) + (ENucleon binding SNF ε0 μ0 /mu) - Ar(XZ±)/Z) / mu)2)(1/2)(1/e((ERelativistic - μchemical)/TMatter)±1)(ħωs + ħωs) - ((ksC2)/ Rs2) + (((8πGTab' + Λgab - Rab) * gab-1))1/2(ΔKiloparsec)))2/(C2)))1/2) Ya, ab doesn't properly define it in free space is why it could not be used, This defines it all in non free space currently. Edited December 12, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Mordred Posted December 12, 2017 Share Posted December 12, 2017 (edited) Every expression you have above can be solved with Calculus of variations. How is that for a hint, Tensors allow us to organize them under group symmetries. Here Calculus of variations for shortest path. http://www-users.math.umn.edu/~olver/ln_/cv.pdf Here example article that is jumping ahead a great deal but it will prove my last statement "Lie Groups and Differential Equations" http://www.physics.drexel.edu/~bob/LieGroups/LG_16.pdf Edited December 12, 2017 by Mordred Link to comment Share on other sites More sharing options...
Vmedvil Posted December 12, 2017 Author Share Posted December 12, 2017 (edited) Let's see if this is still a polymorphic code. Polymorphic L2ghost QE = L1ghost QE All values equal 2 or 1, besides constants. ∇2'(x,y,z,t,ωs,ωp,M,I,k,φ,S,X,Z,μ,Y,q,a,β) = (((ħ2 /(2Erest/C2)) ∑3a =1 (d2/d((C2/Erest)∑Ni = 1 MiRi)2) + (1/2)∑3a,β = 1 μaβ(Pa - Πa)(Pβ - Πβ) + U - (ħ2/2)∑3N-6s=1(d2/dq2) + V)((|(Log(DgDaDψDφ-W)(((2ħGC2))Rs - (1/4)FaμvFaμv + i(ψ-bar)γμ(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)ψi +(ψ-bar)iLVijφψjr + (aji) - (μ2((φ-Dagger)φ) + λ((φ-Dagger)φ)2)/-(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)2)|)-e2S(r,t)/h)) - ((Erest/C2)ωs(((8πGTab' + Λgab - Rab) * gab-1))1/2 + (S/ (((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp ))))Rs2/2))) / (ħ2/2(Erest/C2))))1/2(((1-(((2(Erest/C2)G / Rs) - (Isωs(((8πGTab' + Λgab - Rab) * gab-1))1/2 + (S/(((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp )))))/2(Erest/C2))+ (((8πG/3)((g/(2π)3)∫(((Erelativistic2 - Erest2 / C2) + ((Ar(X) + (ENucleon binding SNF ε0 μ0 /mu) - Ar(XZ±)/Z) / mu)2)(1/2)(1/e((ERelativistic - μchemical)/TMatter)±1)(ħωs + ħωs) - ((ksC2)/ Rs2) + (((8πGTab' + Λgab - Rab) * gab-1))1/2(ΔKiloparsec)))2/(C2)))1/2) ∇1'(x,y,z,t,ωs,ωp,M,I,k,φ,S,X,Z,μ,Y,q,a,β) = (((ħ2 /(2Erest/C2)) ∑3a =1 (d2/d((C2/Erest)∑Ni = 1 MiRi)2) + (1/2)∑3a,β = 1 μaβ(Pa - Πa)(Pβ - Πβ) + U - (ħ2/2)∑3N-6s=1(d2/dq2) + V)((|(Log(DgDaDψDφ-W)(((2ħGC2))Rs - (1/4)FaμvFaμv + i(ψ-bar)γμ(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)ψi +(ψ-bar)iLVijφψjr + (aji) - (μ2((φ-Dagger)φ) + λ((φ-Dagger)φ)2)/-(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)2)|)-e2S(r,t)/h)) - ((Erest/C2)ωs(((8πGTab' + Λgab - Rab) * gab-1))1/2 + (S/ (((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp ))))Rs2/2))) / (ħ2/2(Erest/C2))))1/2(((1-(((2(Erest/C2)G / Rs) - (Isωs(((8πGTab' + Λgab - Rab) * gab-1))1/2 + (S/(((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp )))))/2(Erest/C2))+ (((8πG/3)((g/(2π)3)∫(((Erelativistic2 - Erest2 / C2) + ((Ar(X) + (ENucleon binding SNF ε0 μ0 /mu) - Ar(XZ±)/Z) / mu)2)(1/2)(1/e((ERelativistic - μchemical)/TMatter)±1)(ħωs + ħωs) - ((ksC2)/ Rs2) + (((8πGTab' + Λgab - Rab) * gab-1))1/2(ΔKiloparsec)))2/(C2)))1/2) which it is. Edited December 12, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Vmedvil Posted December 21, 2017 Author Share Posted December 21, 2017 (edited) Oh, I wanted to post this before someone reads this far into the post as my final change. ∇'(x,y,z,t,ωs,ωp,M,I,k,φ,S,X,Z,μ,Y,q,a,β) = (((ħ2 /(2Erest/C2)) ∑3a =1 (d2/d((C2/Erest)∑Ni = 1 MiRi)2) + (1/2)∑3a,β = 1 μaβ(Pa - Πa)(Pβ - Πβ) + U - (ħ2/2)∑3N-6s=1(d2/dq2) + V)((|(Log(DgDaDψDφ-W)(((2ħGC2))Rs - (1/4)FaμvFaμv + i(ψ-bar)γμ(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)ψi +(ψ-bar)iLVijφψjr + (aji) - (μ2((φ-Dagger)φ) + λ((φ-Dagger)φ)2)/-(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)2)|)-e2S(r,t)/h)) - ((Erest/C2)ωs((((8πGTab/C4) + Λgab - Rab) * gab-1))1/2 + (S/ (((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp ))))Rs2/2))) / (ħ2/2(Erest/C2))))1/2(((1-(((2(Erest/C2)G / Rs) - (Isωs((((8πGTab/C4) + Λgab - Rab) * gab-1))1/2 + (S/(((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp )))))/2(Erest/C2))+ (((8πG/3)((g/(2π)3)∫(((Erelativistic2 - Erest2 / C2) + ((Ar(X) + (ENucleon binding SNF ε0 μ0 /mu) - Ar(XZ±)/Z) / mu)2)(1/2)(1/e((ERelativistic - μchemical)/TMatter)±1)(ħωs + ħωs) - ((ksC2)/ Rs2) + (((8πGTab/C4) + Λgab - Rab) * gab-1))1/2(ΔKiloparsec)))2/(C2)))1/2) ∇' - (Cdt)2 = ds2 which dt in this case is tp Lastly, this was a typo (Universe Volumetric Planck State @ size of universe in radius) =(3/4)π ((1/(tpC2)) Luniverse RUniverse)3 It was supposed to be (Universe Volumetric Planck State @ size of universe in radius) =(3/4)π ((RUniverse/(tpC)) Luniverse )3 Luniverse = (∇Charge,∇Color,∇flavour,∇gravity - ∇Dark Energy) charge possible states per point (1,2/3, 1/3, 0,-1/3,-2/3,-1) Color Possible states per point(R,B,G,0,G,B,R) Flavour possible states per point (I,II,III,0,III,II,I) Gravity/Dark Energy possible states per point of space (Energy,Mass,Spin,0,Energy,mass,spin) as tpC = lp Every detail. Edited December 21, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Vmedvil Posted December 23, 2017 Author Share Posted December 23, 2017 (edited) So, people know what it says (==== (Nuclei Vibration and Molecular Coupling Hamiltonian Energy Stress =================================)(============= ∇'(x,y,z,t,ωs,ωp,M,I,k,φ,S,X,Z,μ,Y,q,a,β) = (((ħ2 /(2Erest/C2)) ∑3a =1 (d2/d((C2/Erest)∑Ni = 1 MiRi)2) + (1/2)∑3a,β = 1 μaβ(Pa - Πa)(Pβ - Πβ) + U - (ħ2/2)∑3N-6s=1(d2/dq2) + V)((|(Log(DgDaDψDφ-W) ====Maxwell Electromagnetism=Dirac========= QE Virtual Ghost particles======= Hypercharged Higgs===========Particle Coupling======Standard Higgs== (((2ħGC2))Rs - (1/4)FaμvFaμv + i(ψ-bar)γμ(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)ψi +(ψ-bar)iLVijφψjr + (aji) - (μ2((φ-Dagger)φ) + λ((φ- ============= Virtual Particles Gravity =================== and Hypercharged Higgs=Spin Q Number=)(== Energy Stress Tensor Rest Mass and Rest Energy Dagger)φ)2)/-(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)2)|)-e2S(r,t)/h)) - ((Erest/C2)ωs((((8πGTab/C4) + Λgab - Rab) * gab-1))1/2 + =Angular precession of moving Rest Mass and Rest Energy================Quantum Action of it)(=================Energy Stress angular momentum== (S/ (((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp ))))Rs2/2))) / (ħ2/2(Erest/C2))))1/2(((1-(((2(Erest/C2)G / Rs) - (Isωs((((8πGTab/C4) + Λgab - Rab) * gab-1))1/2 + Angular Precession of Angular momentum================================) (==========Energy Stress of Linear momentum== Energy Stress of Strong (S/(((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp )))))/2(Erest/C2))+ (((8πG/3)((g/(2π)3)∫(((Erelativistic2 - Erest2 / C2) + ((Ar(X) + (ENucleon binding SNF ε0 μ0 /mu) - Interaction and electron orbitals= Energy Stress of Temperature= Energy Stress of Particle Annihilation===Inverse Stress of Dark Energy=======) Ar(XZ±)/Z) / mu)2)(1/2)(1/e((ERelativistic - μchemical)/TMatter)±1)(ħωs + ħωs) - ((ksC2)/ Rs2) + (((8πGTab/C4) + Λgab - Rab) * gab-1))1/2(ΔKiloparsec)))2/(C2)))1/2) Edited December 23, 2017 by Vmedvil Link to comment Share on other sites More sharing options...
Strange Posted December 23, 2017 Share Posted December 23, 2017 On 21/12/2017 at 9:42 AM, Vmedvil said: Oh, I wanted to post this before someone reads this far into the post as my final change. ∇'(x,y,z,t,ωs,ωp,M,I,k,φ,S,X,Z,μ,Y,q,a,β) = (((ħ2 /(2Erest/C2)) ∑3a =1 (d2/d((C2/Erest)∑Ni = 1 MiRi)2) + (1/2)∑3a,β = 1 μaβ(Pa - Πa)(Pβ - Πβ) + U - (ħ2/2)∑3N-6s=1(d2/dq2) + V)((|(Log(DgDaDψDφ-W)(((2ħGC2))Rs - (1/4)FaμvFaμv + i(ψ-bar)γμ(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)ψi +(ψ-bar)iLVijφψjr + (aji) - (μ2((φ-Dagger)φ) + λ((φ-Dagger)φ)2)/-(((Lghost QE - gfabc(δμ (c-bar)a)Aμbcc) / (c-bar)aδμca) + ig(1/2)τWμ + ig'(1/2)YBμ)2)|)-e2S(r,t)/h)) - ((Erest/C2)ωs((((8πGTab/C4) + Λgab - Rab) * gab-1))1/2 + (S/ (((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp ))))Rs2/2))) / (ħ2/2(Erest/C2))))1/2(((1-(((2(Erest/C2)G / Rs) - (Isωs((((8πGTab/C4) + Λgab - Rab) * gab-1))1/2 + (S/(((3G(Erest/C2))/2C2Rs3)(RpVp) + (GIs/C2Rs3)((3Rp/Rs2)(ωp Rp) -ωp )))))/2(Erest/C2))+ (((8πG/3)((g/(2π)3)∫(((Erelativistic2 - Erest2 / C2) + ((Ar(X) + (ENucleon binding SNF ε0 μ0 /mu) - Ar(XZ±)/Z) / mu)2)(1/2)(1/e((ERelativistic - μchemical)/TMatter)±1)(ħωs + ħωs) - ((ksC2)/ Rs2) + (((8πGTab/C4) + Λgab - Rab) * gab-1))1/2(ΔKiloparsec)))2/(C2)))1/2) ∇' - (Cdt)2 = ds2 which dt in this case is tp Lastly, this was a typo (Universe Volumetric Planck State @ size of universe in radius) =(3/4)π ((1/(tpC2)) Luniverse RUniverse)3 It was supposed to be (Universe Volumetric Planck State @ size of universe in radius) =(3/4)π ((RUniverse/(tpC)) Luniverse )3 Luniverse = (∇Charge,∇Color,∇flavour,∇gravity - ∇Dark Energy) charge possible states per point (1,2/3, 1/3, 0,-1/3,-2/3,-1) Color Possible states per point(R,B,G,0,G,B,R) Flavour possible states per point (I,II,III,0,III,II,I) Gravity/Dark Energy possible states per point of space (Energy,Mass,Spin,0,Energy,mass,spin) as tpC = lp Every detail. Why are you posting screen shots of Wikipedia pages that no one can read, instead of just a link? What is wrong with you. Link to comment Share on other sites More sharing options...
Vmedvil Posted December 23, 2017 Author Share Posted December 23, 2017 Just now, Strange said: Why are you posting screen shots of Wikipedia pages that no one can read, instead of just a link? What is wrong with you. Click them to enlarge. Link to comment Share on other sites More sharing options...
Strange Posted December 23, 2017 Share Posted December 23, 2017 Just now, Vmedvil said: Click them to enlarge. They are still unreadable. And WHY post an image in the first place. It is an idiotic thing to do. Please stop. PROVIDE LINKS. Link to comment Share on other sites More sharing options...
Vmedvil Posted December 23, 2017 Author Share Posted December 23, 2017 1 minute ago, Strange said: They are still unreadable. And WHY post an image in the first place. It is an idiotic thing to do. Please stop. PROVIDE LINKS. Can you not read english strange, I thought the Chinese were taught English as a second language, assuming a "Coffee Shop" in china 珈琲店 Link to comment Share on other sites More sharing options...
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