diff options
author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2023-05-28 12:21:20 +0200 |
---|---|---|
committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2023-05-28 12:21:20 +0200 |
commit | 9e542247c14cfa5a9df6844b6c8272bfa626b9a7 (patch) | |
tree | ffa9efb2eecdeaa1091593ea24961cf3dbbb6fb3 | |
parent | f66f0b27de5f24022c72e2e07a91e136456f148b (diff) | |
download | SciPostPhys_16_001-9e542247c14cfa5a9df6844b6c8272bfa626b9a7.tar.gz SciPostPhys_16_001-9e542247c14cfa5a9df6844b6c8272bfa626b9a7.tar.bz2 SciPostPhys_16_001-9e542247c14cfa5a9df6844b6c8272bfa626b9a7.zip |
Fixed formatting of 1RSB.
-rw-r--r-- | 2-point.tex | 2 |
1 files changed, 1 insertions, 1 deletions
diff --git a/2-point.tex b/2-point.tex index 6d3c437..1cc3687 100644 --- a/2-point.tex +++ b/2-point.tex @@ -194,7 +194,7 @@ $\chi(q)=f''(q)^{-1/2}$ is convex. The complexity at the ground state must reflect the structure of equilibrium, and therefore be replica symmetric. We are not aware of any result guaranteeing this for the complexity away from the ground state, but we check that our replica-symmetric solutions satisfy the -saddle point equations at 1RSB. +saddle point equations at {\oldstylenums1}\textsc{rsb}. To enforce the spherical constraint at stationary points, we make use of a Lagrange multiplier $\omega$. This results in the extremal problem \begin{equation} |