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R_{\mu\nu} - \frac{1}{2}Rg_{\mu\nu} + \Lambda g_{\mu\nu} = \frac{8\pi G}{c^4}T_{\mu\nu}

Einstein Field Equations actively rendering spacetime metric tensor fields.

4.31 x 10⁶

Solar Masses (M☉) Recorded

Synchronize global arrays. Observe the shadow.