\begin{table}
\centering
\caption{Physicists with the lowest change scores $c_a$. $D(\bm{I_a})$ and $D(\bm{S_a})$ measure the diversity of intellectual and social capital. Numbers in parentheses indicate the share of attention dedicated to each research area. Asterisks ($\ast$) indicate physicists with a permanent position.}
\label{table:low_exitted}
\begin{tabular}{p{0.15\textwidth}|c|c|c|b{0.25\textwidth}|b{0.25\textwidth}}
\toprule
            Physicist & $c_a$ & $D(\bm{I_a})$ & $D(\bm{S_a})$ &                            Previous main area &                      Current main area \\
\midrule
        K.Gallmeister &     0 &          2.15 &          7.13 &                       Collider physics (0.81) &             Collider physics (0.47)\\ \hline
          P.D.Serpico &     0 &          4.58 &          7.66 &                            Dark matter (0.40) &                  Dark matter (0.46)\\ \hline
           C.E.Thomas &     0 &          2.70 &          4.59 &                                Hadrons (0.66) &                      Hadrons (0.38)\\ \hline
            L.Lavoura &     0 &          4.29 &          6.79 &           Neutrinos \& flavour physics (0.57) & Neutrinos \& flavour physics (0.38)\\ \hline
         R.Williams 3 &     0 &          5.07 &          7.57 &                   Perturbative methods (0.38) &         Perturbative methods (0.32)\\ \hline
             Wei Wang &     0 &          3.45 &          4.98 &                                Hadrons (0.67) &                      Hadrons (0.56)\\ \hline
    W.Grimus ($\ast$) &     0 &          4.54 &          7.24 &           Neutrinos \& flavour physics (0.56) & Neutrinos \& flavour physics (0.38)\\ \hline
           T.M.P.Tait &     0 &          5.17 &          8.35 &            Electroweak sector (0.59$\to$0.24) &         Dark matter (0.07$\to$0.43)\\ \hline
Angels Ramos ($\ast$) &     0 &          5.32 &          6.91 &                                Hadrons (0.44) &                      Hadrons (0.76)\\ \hline
           K.Ishiwata &     0 &          2.84 &          7.16 &                            Dark matter (0.70) &                  Dark matter (0.41)\\ \hline
C.E.M.Wagner ($\ast$) &     0 &          4.81 &          8.84 &                     Electroweak sector (0.63) &           Electroweak sector (0.58)\\ \hline
    C.N.Pope ($\ast$) &     0 &          5.98 &          9.31 & String theory \& supergravity (0.38$\to$0.16) &         Black holes (0.27$\to$0.39)\\ \hline
             K.C.Zapp &     0 &          1.75 &          5.33 &                       Collider physics (0.86) &             Collider physics (0.82)\\ \hline
        J.L.Diaz Cruz &     0 &          5.04 &          7.51 &                     Electroweak sector (0.56) &           Electroweak sector (0.43)\\ \hline
           A.A.Petrov &     0 &          5.86 &          8.78 &                                Hadrons (0.35) &                      Hadrons (0.42)\\ \hline
             H.A.Baer &     0 &          4.90 &          7.73 &                     Electroweak sector (0.43) &           Electroweak sector (0.54)\\ \hline
C.T.H.Davies ($\ast$) &     0 &          4.01 &          6.87 &                                    QCD (0.55) &                          QCD (0.55)\\ \hline
             Xian Gao &     0 &          4.14 &         11.20 &                     Cosmology (0.53$\to$0.18) &    Classical fields (0.09$\to$0.33)\\ \hline
             U.Sarkar &     0 &          5.98 &          8.55 &           Neutrinos \& flavour physics (0.46) & Neutrinos \& flavour physics (0.34)\\ \hline
         D.Berenstein &     0 &          4.76 &          9.89 & String theory \& supergravity (0.60$\to$0.09) &         Black holes (0.03$\to$0.23)\\ \hline
\bottomrule
\end{tabular}
\end{table}
