\begin{table}[H]
\centering
\caption{Physicists with the highest 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 during each time-period. Asterisks ($\ast$) indicate physicists with a permanent position.}
\label{table:top_disruption}
\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
                J.~Evslin &  0.88 &          3.32 &          6.81 & String theory \& supergravity (0.71$\to$0.08) &  Neutrinos \& flavour physics (0.00$\to$0.43)\\ \hline
  Kwei Chou Yang ($\ast$) &  0.84 &          3.58 &          7.80 &                       Hadrons (0.63$\to$0.03) &                   Dark matter (0.00$\to$0.78)\\ \hline
   N.~G.~Sanchez ($\ast$) &  0.80 &          7.52 &         13.08 &                   Black holes (0.37$\to$0.03) &                   Dark matter (0.00$\to$0.57)\\ \hline
                  D.~Shih &  0.74 &          5.74 &         10.21 & String theory \& supergravity (0.52$\to$0.01) &            Electroweak sector (0.06$\to$0.45)\\ \hline
                  D.~Blas &  0.72 &          5.89 &         12.61 &              Classical fields (0.33$\to$0.03) &                   Dark matter (0.00$\to$0.51)\\ \hline
              A.~Mariotti &  0.71 &          3.81 &          4.91 & String theory \& supergravity (0.63$\to$0.01) &            Electroweak sector (0.01$\to$0.38)\\ \hline
     G.~Ferretti ($\ast$) &  0.71 &          5.22 &          6.18 & String theory \& supergravity (0.52$\to$0.00) &            Electroweak sector (0.01$\to$0.58)\\ \hline
     Eiji Nakano ($\ast$) &  0.71 &          6.90 &         10.13 &                           QCD (0.39$\to$0.06) &                       Hadrons (0.04$\to$0.78)\\ \hline
          K.~Bhattacharya &  0.70 &         10.79 &         10.59 &  Neutrinos \& flavour physics (0.20$\to$0.00) &                     Cosmology (0.09$\to$0.37)\\ \hline
                  G.~Beuf &  0.70 &          8.57 &          9.07 &                       Collider physics (0.26) &                       Collider physics (0.82)\\ \hline
      S.~D.~Katz ($\ast$) &  0.70 &          6.50 &         10.85 &                   Dark matter (0.42$\to$0.03) &                           QCD (0.06$\to$0.47)\\ \hline
                 T.~Fuchs &  0.69 &          4.38 &          6.50 &                           QCD (0.53$\to$0.00) &  Neutrinos \& flavour physics (0.00$\to$0.64)\\ \hline
    A.~T.~Suzuki ($\ast$) &  0.69 &          4.36 &          6.43 &          Perturbative methods (0.61$\to$0.04) &  Neutrinos \& flavour physics (0.01$\to$0.39)\\ \hline
   G.~B.~Cleaver ($\ast$) &  0.67 &          6.34 &         12.22 & String theory \& supergravity (0.40$\to$0.00) &                     Cosmology (0.03$\to$0.62)\\ \hline
       Qing Wang ($\ast$) &  0.67 &          7.86 &          9.76 &                           QCD (0.26$\to$0.05) &                   Dark matter (0.02$\to$0.66)\\ \hline
            K.~Urbanowski &  0.66 &          8.66 &          6.80 &                      Dynamics (0.23$\to$0.14) &                     Cosmology (0.03$\to$0.54)\\ \hline
A.~R.~Zhitnitsky ($\ast$) &  0.65 &          8.76 &         12.59 &                           QCD (0.33$\to$0.06) &                   Dark matter (0.10$\to$0.64)\\ \hline
        J.~Sola Peracaula &  0.65 &          6.28 &         10.50 &            Electroweak sector (0.52$\to$0.03) &                     Cosmology (0.14$\to$0.64)\\ \hline
              G.~Macorini &  0.65 &          5.64 &          8.04 &            Electroweak sector (0.46$\to$0.00) & String theory \& supergravity (0.10$\to$0.21)\\ \hline
         M.~Redi ($\ast$) &  0.64 &          9.81 &         12.76 & String theory \& supergravity (0.21$\to$0.01) &                   Dark matter (0.02$\to$0.42)\\ \hline
\bottomrule
\end{tabular}
\end{table}
