Table 1 The αΩ dynamo period prediction and simulation data at several radii
From: A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers
R (km) | αϕϕ (cm s−1) | Ω (rad s−1) | Shear rate | kz (cm−1) | Ptheory (s) | \({P}_{{{{\rm{sim}}}}}\) (s) |
|---|---|---|---|---|---|---|
20 | −8.1 × 106 | 4,025 | q = 1.00 | 6.3 × 10−6 | 0.020 | 0.018 |
30 | −1.0 × 107 | 2,515 | q = 1.34 | 4.2 × 10−6 | 0.021 | 0.018–0.024 |
40 | −1.0 × 107 | 1,688 | q = 1.44 | 3.3 × 10−6 | 0.037 | 0.018–0.030 |
50 | −4.4 × 106 | 1,200 | q = 1.50 | 2.6 × 10−6 | 0.062 | 0.030–0.040 |
