pith. sign in

Substitute it into Eq

Solution IV In this solution, denote Rs = 2M, we have G = H = f = 1 − 2M r , δG = δH = δf = −2δM r , bt = b, b r = b f p 1 − f , δb t = 0, δb r = b(f − 2) 2f2√1 − f δf

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New Exact Vacuum Solutions in Extended Bumblebee Gravity

gr-qc · 2026-04-10 · unverdicted · novelty 6.0

Ten new exact vacuum solutions, including black holes with zero entropy, arise in extended bumblebee gravity because varying the action and imposing the vector VEV constraint do not commute.

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  • New Exact Vacuum Solutions in Extended Bumblebee Gravity gr-qc · 2026-04-10 · unverdicted · none · ref 11

    Ten new exact vacuum solutions, including black holes with zero entropy, arise in extended bumblebee gravity because varying the action and imposing the vector VEV constraint do not commute.