Pith. sign in

(4) To achieve this goal, we multiply (

in r [8]), is to multiply ( 3) by functions f (B(r, t ), r ), then rearrange the result to regain a conservation law of kind ∂tv(r, t ) + ∂rf (v(r, t ), r ) = 0

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Non-uniqueness of the shockwave dynamics in effective loop quantum gravity

gr-qc · 2025-02-05 · conditional · novelty 6.0

In effective loop quantum gravity, an infinite family of mathematically equivalent collapse equations produce different weak solutions after shell crossing, so the predicted black hole lifetime (e.g., M^2, M^3, M^4) is not uniquely determined.

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  • Non-uniqueness of the shockwave dynamics in effective loop quantum gravity gr-qc · 2025-02-05 · conditional · none · ref 3

    In effective loop quantum gravity, an infinite family of mathematically equivalent collapse equations produce different weak solutions after shell crossing, so the predicted black hole lifetime (e.g., M^2, M^3, M^4) is not uniquely determined.