Home / Math and Physics Files / Math / Curvilinear Systems / Tensor Doc and Support / tensor doc support 2_22_12 thru 3_8_12
appendix C fiddle
DOCX · 18.8 KB
Open DOCX file
Working note dated 3.26.05 in Phil's tensor-document support files, an idea he did not finish and judged not useful. It computes the angle ψ between the coordinate lines of an elliptical-type curvilinear system from the metric, checks |cosψ| ≤ 1 via det(g') > 0, and derives tanψ = [2ab/|b²-a²|] csc(2θ). It then integrates dρ/dθ = tanψ with Maple and ends with a divergence at θ=0, where he gives up.
AI-written summary; may contain errors. This description is approximate.
Extracted text (machine-read; may contain errors)
Idea PhL 3.26.05
Here I was just wondering if you could warp some or all of the grid lines in curvilinear x'-space to make all the angles be right. I did not finish it, does not seem at all useful.
Appendix C framework:
'θ 'ρ = e'θ e'ρ / (h'θh'ρ) = eθ eρ / (h'θh'ρ) = 'θρ / (h'θh'ρ)
= [b2-a2]ρ sin(θ)cos(θ)/ {ρ}
= [b2-a2] sin(θ)cos(θ)/ {}
= cosψ
ψ(θ) = cos-1[[b2-a2] sin(θ)cos(θ)/ {}]
Can I show that
|'θ 'ρ| ≤ 1?
| eθ eρ | < (h'θh'ρ) ?
'θρ < (h'θh'ρ)
('θρ)2< (h'θh'ρ)2
('θρ)2 < 'θθ'ρρ
det(g') > 0 ?
Yes, we do know this from Section 5 (d).
So this suggests a rather elaborate way to draw the θ-ρ picture. It is drawn in Cartesian space such that at every point, the angle between the two sets of lines is angle ψ(ρ,θ). The lines intersecting are lines of constant ρ and the lines of constant θ. These would be curves satisfying
dρ/dθ = tan[ψ(θ)]
Now
secψ = / {[b2-a2] sin(θ)cos(θ)}
sec2ψ = (a2sin2θ + b2cos2θ)( a2cos2θ + b2sin2θ) / {[b2-a2]2 sin2(θ)cos2(θ)}
tan2ψ = sec2ψ - 1
= (a2sin2θ + b2cos2θ)( a2cos2θ + b2sin2θ) / {[b2-a2]2 sin2(θ)cos2(θ)}
– {[b2-a2]2 sin2(θ)cos2(θ)} / {[b2-a2]2 sin2(θ)cos2(θ)}
NUM = (a2sin2θ + b2cos2θ)( a2cos2θ + b2sin2θ) - [b2-a2]2 sin2(θ)cos2(θ)
= a4s2c2+ a2b2c4 + a2b2s4 + b4s2c2 - b4s2c2 - a4s2c2 + 2a2b2s2c2
= [a4 +b4 - b4 -a4 + 2a2b2] s2c2 + a2b2c4+ a2b2s4
= 2a2b2 s2c2 + a2b2 (s4+c4)
= a2b2 [s4+c4 + 2s2c2] = a2b2(s2+c2)2 = a2b2
Thus we find that
tan2ψ = a2b2 / {[b2-a2]2 sin2(θ)cos2(θ)}
Therefore,
tanψ = ab / {|b2-a2|sin(θ)cos(θ)} = [ 2ab/|b2-a2| ] csc(2θ)
much simpler than I thought. Our curves for the wavy vertical constant θ lines are then set by
dρ/dθ = tan[ψ(θ)] = [ 2ab/|b2-a2| ] csc(2θ)
dρ = [ 2ab/|b2-a2| ] csc(2θ)dθ
ρ = [ 2ab/|b2-a2| ] { -(1/2)ln [csc(2θ) + cot(2θ)] + constant } //Maple
At θ = π/4 we find that csc(2θ) + cot(2θ) = 1 so
ρ(π/4) = [ 2ab/|b2-a2| ] { -(1/2)ln [1] + constant } = [ 2ab/|b2-a2| ] * constant
At θ = 0+ we find that csc(2θ) + cot(2θ) = +∞ so ρ = -∞ + constant.
I give up, this all makes no sense.