\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
               T.~Fuchs &  0.76 &          4.38 &          6.50 &                           QCD (0.53$\to$0.00) & Neutrinos \& flavour physics (0.00$\to$0.64)\\ \hline
 N.~G.~Sanchez ($\ast$) &  0.73 &          7.52 &         13.08 &                   Black holes (0.37$\to$0.03) &                  Dark matter (0.00$\to$0.57)\\ \hline
Kwei Chou Yang ($\ast$) &  0.71 &          3.58 &          7.80 &                       Hadrons (0.63$\to$0.03) &                  Dark matter (0.00$\to$0.78)\\ \hline
   G.~Ferretti ($\ast$) &  0.66 &          5.22 &          6.18 & String theory \& supergravity (0.52$\to$0.00) &           Electroweak sector (0.01$\to$0.58)\\ \hline
            A.~Mariotti &  0.63 &          3.81 &          4.91 & String theory \& supergravity (0.63$\to$0.01) &           Electroweak sector (0.01$\to$0.38)\\ \hline
                D.~Shih &  0.62 &          5.74 &         10.21 & String theory \& supergravity (0.52$\to$0.01) &           Electroweak sector (0.06$\to$0.45)\\ \hline
    S.~D.~Katz ($\ast$) &  0.61 &          6.50 &         10.85 &                   Dark matter (0.42$\to$0.03) &                          QCD (0.06$\to$0.47)\\ \hline
        K.~Bhattacharya &  0.60 &         10.79 &         10.59 &  Neutrinos \& flavour physics (0.20$\to$0.00) &                    Cosmology (0.09$\to$0.37)\\ \hline
              J.~Evslin &  0.60 &          3.32 &          6.81 & String theory \& supergravity (0.71$\to$0.08) & Neutrinos \& flavour physics (0.00$\to$0.43)\\ \hline
 G.~B.~Cleaver ($\ast$) &  0.57 &          6.34 &         12.22 & String theory \& supergravity (0.40$\to$0.00) &                    Cosmology (0.03$\to$0.62)\\ \hline
     J.~Martin Camalich &  0.57 &          2.34 &          4.57 &                           QCD (0.78$\to$0.03) &                      Hadrons (0.06$\to$0.38)\\ \hline
  A.~T.~Suzuki ($\ast$) &  0.57 &          4.36 &          6.43 &          Perturbative methods (0.61$\to$0.04) & Neutrinos \& flavour physics (0.01$\to$0.39)\\ \hline
     Qing Wang ($\ast$) &  0.55 &          7.86 &          9.76 &                           QCD (0.26$\to$0.05) &                  Dark matter (0.02$\to$0.66)\\ \hline
   Eiji Nakano ($\ast$) &  0.55 &          6.90 &         10.13 &                           QCD (0.39$\to$0.06) &                      Hadrons (0.04$\to$0.78)\\ \hline
                D.~Blas &  0.55 &          5.89 &         12.61 &              Classical fields (0.33$\to$0.03) &                  Dark matter (0.00$\to$0.51)\\ \hline
                G.~Beuf &  0.54 &          8.57 &          9.07 &                       Collider physics (0.26) &                      Collider physics (0.82)\\ \hline
 M.~Olechowski ($\ast$) &  0.54 &          8.19 &         11.17 &                     Cosmology (0.28$\to$0.00) &                  Dark matter (0.04$\to$0.47)\\ \hline
       M.~Redi ($\ast$) &  0.53 &          9.81 &         12.76 & String theory \& supergravity (0.21$\to$0.01) &                  Dark matter (0.02$\to$0.42)\\ \hline
 V.~V.~Braguta ($\ast$) &  0.53 &          5.03 &          8.04 &                       Hadrons (0.45$\to$0.00) &                          QCD (0.05$\to$0.60)\\ \hline
      J.~Sola Peracaula &  0.52 &          6.28 &         10.50 &            Electroweak sector (0.52$\to$0.03) &                    Cosmology (0.14$\to$0.64)\\ \hline
\bottomrule
\end{tabular}
\end{table}
