Extra Polarization Amplitudes for Gravitational Waves in Einstein-Cartan Gravity: A Computed Upper Pattern

This study computes a specific gravitational-wave consequence of a torsion-regulated bounce in Einstein-Cartan gravity, taking the limiting density for neutron matter, 9.72e+54 grams per cubic centimetre under the stated prescription, as its single input scale. Detector networks now test the polarization content of gravitational waves directly, which raises a precise question for any torsion theory: does it predict additional radiative modes, and if so, at what amplitude? The headline results of the computation are: vacuum_extra_modes = 0, NS_breathing_ratio_bound = 1.01e-20, NS_density_g_cm3 = 1.00e+15. Each quantity is evaluated by the deposited script from the assumptions stated in the Methods, and the agreement or disagreement of each quantity with published observational bounds is reported at face value, including where the conclusion is that the channel examined is closed. The study is simulated and computed from stated assumptions; it is not a measurement, and no observational data were taken for it.