VERY SLOW LOSS. “For a black hole of the mass of our Sun, the evaporation timescale is of the order of 2 × 10(66) years. As we will see, it is mostly in strong fields, such as those occurring near the horizon of black holes, that this antigravity will lead to significant effects.”
https://lnkd.in/daA2SgMy
linkedin post 2022-06-29 05:12:48
Nigel Fleming
September 21, 2022