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| Tags: dimensions, general, physical, relativity |
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#1
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OK we hit a temporary snag solved below. In elementary physics first
rule is to check your units and physical dimensions. Don't mix apples with oranges etc. Yet GR theorists do that nonchalantly and sloppily even in text books. For example, the SSS metric is typically written as gtt = -(1 - 2GM/c^2r) [dimensionless] grr = (1 - 2GM/c^2r)^-1 [dimensionless] But hold on gthetatheta = r^2 [area] gphiphi = r^2sin^2theta [area] Where we have the incommensurate basis set of Cartan 1-forms dx^0 = cdt dx^1 = dr dx^2 = dtheta dx^3 = dphi With the Grassmann basis sort of "Clifford" algebra" of 2^4 = 16 p-forms, p = 0,1,2,3,4 *p-form = (4 - p)-form, when N = 4. 1 dx^u dx^u/\dx^v dx^u/\dx^v/\dx^w dx^u/\dx^v/\dx^w/\dx^l This gives an incommensurate set of Levi-Civita connection field components in the hovering LNIFs (LC)^001 = [2(1 - 2GM/c^2r)]^-1 (1 - 2GM/c^2r),r [1/length] (LC)^122 = -r(1 - 2GM/c^2r) [length] (LC)^233 = -sinthetacostheta [dimensionless] (LC)^100 = (1/2)(1 - 2GM/c^2r),r(1 - 2GM/c^2r) [1/length] (LC)^133 = -(rsin^2theta)(1 - 2GM/c^2r) [length] (LC)^313 = (LC)^212 = 1/r [1/length] (LC)^111 = (1/2)(1 - 2GM/c^2r)(1 - 2GM/c^2r)^-1,r [1/length] (LC)^323 = cottheta [dimensionless] all other (LC) identically & globally zero in this FRAME BUNDLE of hovering LNIFs all over this toy model 4D space-time My original suggestion gthetatheta = gphiphi = 1 will not work here because physically we have a stretch-squeeze tidal curvature that requires the theta dependence in addition to the radial dependence. Nevertheless we MUST use commensurate infinitesimal basis sets for our local frames and the (LC) components MUST all be of the same physical dimension in order to define consistent Diff(4) covariant derivatives. For example Au;v = Au,v - (LC)uv^wAw The GRAVITY-MATTER MINIMAL COUPLING SUM (LC)uv^wAw must have physically commensurate (LC) components because Au is arbitrary! For example, Au can be the Maxwell EM vector potential, and all the components of Au have same physical dimensions. Therefore ALL the (LC) MUST obey [LC] = 1/length So, how to we accomplish this? Simple, use engineering dimensional analysis and introduce a scale L. What is L? Is L = Lp = (hG/c^3)^1/2 or is L = GM/c^2 or? For now let's call it "L". Therefore the SSS metric is now the physically commensurate dimensionless array gtt = -(1 - 2GM/c^2r) grr = (1 - 2GM/c^2r)^-1 gthetatheta = (r/L)^2 gphiphi = (r/L)^2sin^2theta Where we NOW have the commensurate set of basic 1-forms dx^0 = cdt dx^1 = dr dx^2 = Ldtheta dx^3 = Ldphi Note that ,0 = (1/c),t ,1 = ,r ,2 = (1/L),theta ,3 = (l/L),phi Therefore, all the (LC) are now [1/length] LC)^001 = [2(1 - 2GM/c^2r)]^-1 (1 - 2GM/c^2r),r (LC)^122 = -(r/L^2)(1 - 2GM/c^2r) (LC)^233 = -(1/L)sinthetacostheta (LC)^100 = (1/2)(1 - 2GM/c^2r),r(1 - 2GM/c^2r) (LC)^133 = -(rsin^2theta/L^2)(1 - 2GM/c^2r) (LC)^313 = (LC)^212 = 1/r (LC)^111 = (1/2)(1 - 2GM/c^2r)(1 - 2GM/c^2r)^-1,r (LC)^323 = (1/L)cottheta [dimensionless] The Riemann-Christoffel tensor is now dimensionally self-consistent, i.e. 1/Area Note that L cancels out of the frame invariant ds^2 = guvdx^udx^v and it must cancel out of any local physical quantity. In particular it must cancel out of the geodesic equation and the tidal geodesic deviation. It's pretty obvious that L will be physically locally unobservable. It's a bit like the Weyl gauge parameter. Note that the geodesic equation for a non-spinning point test particle is D^2x^u/ds^2 = d^2x^u/ds^2 - (LC)^uvw(dx^v/ds)(dx^w/ds) = 0 So the 1/L's in the (LC)s cancel the L's in x2 & x^3 Similarly with geodesic deviation d(x^u - x'^u)/ds = R^uvwl(x^v - x'^v)(dx^w/ds)(dx^l/ds) Note that (LC)^uvw and R^uvwl are NEVER MEASURED DIRECTLY in isolation. What is measured is D^2x^u/ds^2 and d(x^u - x'^u)/ds |
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#2
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"Jack Sarfatti" wrote in message m... OK we hit a temporary snag solved below. In elementary physics first rule is to check your units and physical dimensions. Don't mix apples with oranges etc. Yet GR theorists do that nonchalantly and sloppily even in text books. For example, the SSS metric is typically written as gtt = -(1 - 2GM/c^2r) [dimensionless] grr = (1 - 2GM/c^2r)^-1 [dimensionless] But hold on gthetatheta = r^2 [area] gphiphi = r^2sin^2theta [area] So what? Do they ever add grr to gthetatheta ? They add gtt c dt c dt (area) grr dr dr (area) gthetatheta dtheta dtheta (area) gphiphi dphi dphi (area) Dirk Vdm |
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#3
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"Dirk Van de moortel" wrote in message ... "Jack Sarfatti" wrote in message m... OK we hit a temporary snag solved below. In elementary physics first rule is to check your units and physical dimensions. Don't mix apples with oranges etc. Yet GR theorists do that nonchalantly and sloppily even in text books. For example, the SSS metric is typically written as gtt = -(1 - 2GM/c^2r) [dimensionless] grr = (1 - 2GM/c^2r)^-1 [dimensionless] But hold on gthetatheta = r^2 [area] gphiphi = r^2sin^2theta [area] So what? Do they ever add grr to gthetatheta ? They add gtt c dt c dt (area) grr dr dr (area) gthetatheta dtheta dtheta (area) gphiphi dphi dphi (area) Dirk Vdm Oops... I hadn't seen I was replying to a write only troll bot Sorry, groups. Dirk Vdm |
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#4
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Dirk Van de moortel wrote:
Oops... I hadn't seen I was replying to a write only troll bot Sorry, groups. We'll accept your apology, but just try to be more careful! |
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