Methods of Numerical Computation
The differential equation to be solved numerically is the equation given in the previous §5.1, which is converted to the following dimensionless form EQG:
(EQG) : R* ∂R* ( R*-1 ∂R*Ψ* ) = - λ V* ∂R (V*2 + V* ∂R*Ψ* ),
where R* , V* and Ψ* are dimension-less variables defined by V* =V obs /c, R*=R/L and
Ψ* =Ψ/(cL) with L a scale parameter characterizing the galaxy under investigation. The equation (EQG) is a 2nd order ordinary differential equation with the dimension-less parameter λ.
This equation describes the mechanism of how the gauge potential Ψ* is excited by the rotation velocity V* (R*) of the galaxy. The degree of excitation is controlled by the dimension-less parameter
λ = ( μ∗/G) (4π)-1 c2 , proportional to the ratio μ∗/G, signifying relative strength of two excitation mechanisms represented by two parameters μ∗ and G. The μ∗ denotes the excitation by the current flux ρ0V (see the equation (III) of §5) and the constant G denotes the excitation by the gravity. The equation (EQG) is solved by the finite-element scheme.
Regarding the boundary conditions, firstly, the radial section of R is chosen where R ∈ [R1, R2] with
R1 < R2 . Since the present study is interested in investigating the halo, the R2-value is chosen within the halo. Then we have V2 =V obs (R2) of the observed rotation velocity, and Ac(R2) =V22 /R2 .
Given the value Ac(R2), the equation Ac= F(Ag) of the main article (2) yields Ag(R2) = F-1 [Ac(R2)]
by the inversion. Then, the first derivative of Ψ at R2 is given by (16) of the main article as follows:
dΨ/dR|R2 = (-Ac(R2) + Ag(R2) ) (R2/V2) ≡ Y2
denoted as Y2 . In the diagram of §4.2, although the point (Ag(R2), Ac(R2) ) is located on the curve given by Ac= F(Ag), the other points are not necessarily located on the same curve, because the other points are determined by solving the differential equation (EQG). At the other end R1, the condition
Ψ(R1) = 0 is imposed to fix the arbitrariness of Ψ-value.
Initially, an appropriate value λ1 is chosen for the unknown parameter λ of (EQG), and the rotation curve is given by the observed function Vobs(R). Then, the two boundary conditions on both sides of the R-section are given by
(BC): Ψ* = 0 at R*1 =R1/L ; ∂R*Ψ* = Y*2 at R*2 =R2/L
To solve the second order differential equation (EQG), the initial turn of the trial computation is carried
out by the finite-element scheme for the above conditions (BC), and one finds the first trial function
Ψ(1)(R) for R ∈ [R1, R2].
From Ψ(1)(R), the equation (18) of the main text gives a trial value A(1)DM = |VR-1 ∂RΨ(1) | at R.
Then from (17) of the main article, the variable Agrav (written in place of Ag ) is given a trial value by
A(1)grav(R) =V2obs(R)/R - A(1)DM , where A(1)grav is regarded as the first trial value of | ∂RΦg | at the position R, together with Ac(1)(R) = A(1)grav + A(1)DM . In general, the diagram of MLS-plot gives ADM once the abscissa Ag-value is given. Setting the value of Ag by the computed value A(1)grav at R , one must compare the computed trial value A(1)DM with the value ADM = F(A(1)grav) - A(1)grav . Usually, both are different. Note that F(A(1)grav) ≠ Ac(1)(R) .
If those two of A(1)DM and ADM do not match, the index-parameter λ1 must be corrected to a new better value λ2, and another try of computation must be carried out to find a better matching. Iterative computation must be repeated until satisfactory matching is obtained (which is denoted by ∞ ) between the computed curve ( A(∞)grav (R), A(∞)c(R) ) and the target curve ( Ag, F(Ag) ) with Ac = F(Ag) by (2).
Thus, the triplet [ A(∞)grav (R), A(∞)c(R), A(∞)DM(R) ], R ∈ [R1, R2 ], has been found from the computation for the three selected galaxies NGC3198, NGC6503 and NGC3741 . Those are plotted in the diagram of Fig. 4 of the main article shown by the blue sequence of dots marked with c.
Matching with the curve Ac = F(Ag) marked with a is remarkable.
The curves a and c are also given in the diagram of §4.2 given above.