Force on a neutral star at 50 pc

Line-mass gravity · Lorentz force zero · coupling term absent

Date: 2026-10-08 Status: RECORD · public page /cosmology/local-stream · no ledger row · no promote Parent: measey.com documents/a_geom_ft_stellar_condensation_cascade_chunk5.md

At the named rope radius \(50\,\mathrm{pc}\), outside that rope’s volume current, the Lorentz force on a neutral star is zero. The gas line \(1.1\times 10^{3}\,M_\odot\,\mathrm{pc^{-1}}\) gives \(g=6.13\times 10^{-12}\,\mathrm{m\,s^{-2}}\) (\(1.22\times 10^{19}\,\mathrm{N}\) on one solar mass). The orbit line \(4.65\times 10^{4}\,M_\odot\,\mathrm{pc^{-1}}\) gives \(g=2.59\times 10^{-10}\,\mathrm{m\,s^{-2}}\) (\(5.16\times 10^{20}\,\mathrm{N}\) on one solar mass). No mutual inductance and no \(j(r,\theta)\) are supplied. The clocks stand in the ratio \(3.77\times 10^{6}\).

The acceleration is \(g(r)=2G\lambda/r\). The stated distance is the rope radius already used for \(I=3.86\times 10^{15}\,\mathrm{A}\) at \(5\,\mu\mathrm{G}\). A star at that radius sits where the rope’s \(j_z\) has ended, so \(\mathbf{j}\times\mathbf{B}\) on the star is zero. The same cylindrical relation supports \(3.1\,\mathrm{km\,s^{-1}}\) on the gas line, the round of \(3.076\,\mathrm{km\,s^{-1}}\), and \(20.0\,\mathrm{km\,s^{-1}}\) on the orbit line. Those speeds do not depend on radius. The accelerations do.

The circumference, the inductances, and the rope current stay as evaluated. The ratio \(41.47\,\mathrm{Myr}/11.004\,\mathrm{yr}=3.77\times 10^{6}\) is the two clocks. A coupling would be a mutual inductance or a \(j(r,\theta)\). Neither is on the page. The particle halo is retired as inventory (§0bn1190). This page's current is not that retirement. Gate 5 stays unpaid. The tachocline seat stays closed. The live line stays §0bn1188. No chip. No promote.

Figure: public/figures/local-stream/fig2_neutral_force.png.