Bound on scalar potential slopes in asymptotic field space · revision history

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Superseded · first revision · record

Title
Bound on scalar potential slopes in asymptotic field space
Plain
A conjecture says that wherever string theory is weakly coupled, the vacuum energy must slope steeply downhill. Whether this holds, and how steep the slope must be, is unknown.
Precise
The refined de Sitter conjecture (2018) states that in asymptotic, weakly coupled regions of moduli space, $\mid \operatorname{grad} V \mid \ge c V/M_{P}$ or min eigenvalue(grad grad V) <= -c' V/M_P^2 with c, c' of order 1. Determine whether this holds in all asymptotic regions of string moduli spaces and find the optimal value of c in d dimensions.
Settled by
A proof over all asymptotic limits of string compactifications with the sharp constant, or an explicit asymptotic counterexample.
Kind
well-posed
Answer type
value
References
(empty)
Literature status
open
Status note
Candidate sharp values are $c = 2/\sqrt{(d-1)(d-2)}$ from the trans-Planckian censorship conjecture (Bedroya, Vafa 2019) and $c = 2/\sqrt{d-2}$ (Rudelius 2021), tested in many but not all asymptotic limits (2021-2025).
Posed since
2018