adaptation_specialization_material/output/etm_20_pretrained/top_entered.tex

\begin{table}
\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_entered}
\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
 W.Buchmuller ($\ast$) &     1 &          8.09 &         10.87 &  Neutrinos \& flavour physics (0.26$\to$0.06) & String theory \& supergravity (0.12$\to$0.36)\\ \hline
   T.R.Morris ($\ast$) &     1 &          7.48 &         11.61 &          Perturbative methods (0.35$\to$0.05) &                       AdS/CFT (0.07$\to$0.27)\\ \hline
                N.Ohta &     1 &          7.00 &          9.05 &                            Black holes (0.36) &                            Black holes (0.22)\\ \hline
  E.M.C.Abreu ($\ast$) &     1 &          9.23 &         10.40 &                   Quantum Field Theory (0.19) &                   Quantum Field Theory (0.21)\\ \hline
Joaquim Gomis ($\ast$) &     1 &          7.16 &          8.94 & String theory \& supergravity (0.32$\to$0.15) &          Quantum Field Theory (0.27$\to$0.34)\\ \hline
   A.T.Suzuki ($\ast$) &     1 &          4.36 &          6.43 &          Perturbative methods (0.61$\to$0.04) &  Neutrinos \& flavour physics (0.01$\to$0.39)\\ \hline
  Y.A.Sitenko ($\ast$) &     1 &          9.56 &          5.65 &                                    QCD (0.19) &                                    QCD (0.29)\\ \hline
 H.Verschelde ($\ast$) &     1 &          7.27 &         10.70 &          Perturbative methods (0.31$\to$0.05) &                   Black holes (0.01$\to$0.33)\\ \hline
 M.Olechowski ($\ast$) &     1 &          8.19 &         11.17 &                     Cosmology (0.28$\to$0.00) &                   Dark matter (0.04$\to$0.47)\\ \hline
 K.A.Meissner ($\ast$) &     1 &         12.07 &         10.96 &                      Dynamics (0.12$\to$0.01) &                   Dark matter (0.01$\to$0.18)\\ \hline
      F.Lizzi ($\ast$) &     1 &          4.72 &          8.88 &                   Quantum Field Theory (0.65) &                   Quantum Field Theory (0.43)\\ \hline
      Y.Satoh ($\ast$) &     1 &          7.62 &          5.74 &                       AdS/CFT (0.23$\to$0.10) & String theory \& supergravity (0.20$\to$0.42)\\ \hline
             M.Zabzine &     1 &          5.11 &          7.10 &          String theory \& supergravity (0.53) &          String theory \& supergravity (0.68)\\ \hline
              M.Visser &     1 &          9.06 &          7.97 &                            Black holes (0.22) &                            Black holes (0.38)\\ \hline
  Subir Ghosh ($\ast$) &     1 &          6.88 &          8.18 &                   Quantum Field Theory (0.43) &                   Quantum Field Theory (0.21)\\ \hline
        F.D.Mazzitelli &     1 &          8.93 &         13.57 &                Thermodynamics (0.20$\to$0.15) &                       AdS/CFT (0.19$\to$0.22)\\ \hline
      Z.Lalak ($\ast$) &     1 &          7.31 &          9.95 &                              Cosmology (0.32) &                              Cosmology (0.26)\\ \hline
           A.Falkowski &     1 &          7.93 &         10.92 &                     Electroweak sector (0.37) &                     Electroweak sector (0.36)\\ \hline
         Jorge G.Russo &     1 &          9.19 &          9.20 &          String theory \& supergravity (0.38) &          String theory \& supergravity (0.30)\\ \hline
 T.A.Jacobson ($\ast$) &     1 &          9.71 &          9.97 &                            Black holes (0.34) &                            Black holes (0.49)\\ \hline
\bottomrule
\end{tabular}
\end{table}