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| author | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-14 13:31:50 +0200 |
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| committer | Jaron Kent-Dobias <jaron@kent-dobias.com> | 2022-07-14 13:31:50 +0200 |
| commit | 73a6f377a5956a2843cfbc3b983bfac762fd958f (patch) | |
| tree | 2cdc7f370e28fcbec04585397f146b7d9bcc880f | |
| parent | f523139a93054ca8d90a4ac82fa8533ef8f72146 (diff) | |
| download | PRE_107_064111-73a6f377a5956a2843cfbc3b983bfac762fd958f.tar.gz PRE_107_064111-73a6f377a5956a2843cfbc3b983bfac762fd958f.tar.bz2 PRE_107_064111-73a6f377a5956a2843cfbc3b983bfac762fd958f.zip | |
Wrong word fixes.
| -rw-r--r-- | frsb_kac-rice.tex | 2 |
1 files changed, 1 insertions, 1 deletions
diff --git a/frsb_kac-rice.tex b/frsb_kac-rice.tex index 545f239..6719d05 100644 --- a/frsb_kac-rice.tex +++ b/frsb_kac-rice.tex @@ -1082,7 +1082,7 @@ also studied before in equilibrium \cite{Crisanti_2004_Spherical, Crisanti_2006_ In the equilibrium solution, the transition temperature from RS to FRSB is $\beta_\infty=1$, with corresponding average energy $\langle E\rangle_\infty=-0.53125\ldots$. Along the supersymmetric line, the FRSB solution can be found in full, exact -function form. To treat the FRSB away from this line numerically, we result to +functional form. To treat the FRSB away from this line numerically, we resort to finite $k$RSB approximations. Since we are not trying to find the actual $k$RSB solution, but approximate the FRSB one, we drop the extremal condition \eqref{eq:cond.x} for $x_1,\ldots,x_k$ and instead set |