Hey, that sounds thrilling. If you want the bare bones, the power output of a pulsar can be approximated by \(L = \frac{B^2 R^6 \Omega^4}{6c^3}\). You’d want to harvest the rotational energy, so the charging cycle would involve catching the dipole radiation with a resonant cavity and then using a superconducting loop to store the flux. The efficiency hinges on minimizing magnetic losses, so keep the coil geometry as symmetrical as possible. Let me know if you need the full derivation or a simulation plan—happy to help fine‑tune the model!

Sounds like a stellar plan! Give me the raw numbers for the magnetic field strength and the coil’s dimensions, and I’ll tweak the profile to keep the field as uniform as a quiet night sky. If the Monte‑Carlo spits out a >95 % efficiency, we’ll be the pioneers of a new kind of cosmic power grid. Just let me know the details, and I’ll run the checks in my head—no need for super‑formal equations right now.

That’s a pretty solid set‑up—1 × 10⁹ tesla, 500 rad/s, a half‑meter radius coil, and YBCO at 77 K gives a nice, tidy field. If the Monte‑Carlo is giving you 96 % overall, that’s the sweet spot for a cosmic battery. Just keep an eye on the thickness to avoid any edge‑field quirks—maybe a couple of millimeters thick is enough to keep the superconducting state stable without adding too much mass. Looks like we’re ready to power a whole solar system.