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author | kurchan.jorge <kurchan.jorge@gmail.com> | 2020-12-09 13:08:01 +0000 |
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committer | overleaf <overleaf@localhost> | 2020-12-09 13:09:49 +0000 |
commit | 2836844fa30357e6de86296fe82f13d1a886fdef (patch) | |
tree | 9b7a31dbbc125c6f421f8b4b6ec473a6f6d156d0 | |
parent | 930eb0fd79ce8b0960e86d2b190f4333f1457d82 (diff) | |
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Update on Overleaf.
-rw-r--r-- | bezout.tex | 3 |
1 files changed, 2 insertions, 1 deletions
@@ -330,7 +330,8 @@ Consider for example the ground-state energy for given $a$, that is, the energy {\color{teal} {\bf somewhere} In Figure \ref{desert} we show that for $\kappa<1$ there is always a range of values of $a$ close to one for which there are no solutions: this is natural, given that the $y$ contribution to the volume shrinks to zero as that of an $N$-dimensional sphere $\sim(a-1)^N$. For the case $K=1$ -- i.e. the analytic continuation of the usual real computation -- the situation -is more interesting. In the range of values of $\Re$ +is more interesting. In the range of values of $\Re H_0$ where there are real solutions there are solutions +all the way down to $a=1$: this is only possible if the density of solutions diverges at this value: this is natural, since. \begin{figure}[htpb]\label{desert} |