top_disruption.tex 3.9 KB

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  1. \begin{table}[H]
  2. \centering
  3. \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.}
  4. \label{table:top_disruption}
  5. \begin{tabular}{p{0.15\textwidth}|c|c|c|b{0.25\textwidth}|b{0.25\textwidth}}
  6. \toprule
  7. Physicist & $c_a$ & $D(\bm{I_a})$ & $D(\bm{S_a})$ & Previous main area & Current main area \\
  8. \midrule
  9. T.~Fuchs & 0.76 & 4.38 & 6.50 & QCD (0.53$\to$0.00) & Neutrinos \& flavour physics (0.00$\to$0.64)\\ \hline
  10. N.~G.~Sanchez ($\ast$) & 0.73 & 7.52 & 13.08 & Black holes (0.37$\to$0.03) & Dark matter (0.00$\to$0.57)\\ \hline
  11. Kwei Chou Yang ($\ast$) & 0.71 & 3.58 & 7.80 & Hadrons (0.63$\to$0.03) & Dark matter (0.00$\to$0.78)\\ \hline
  12. G.~Ferretti ($\ast$) & 0.66 & 5.22 & 6.18 & String theory \& supergravity (0.52$\to$0.00) & Electroweak sector (0.01$\to$0.58)\\ \hline
  13. A.~Mariotti & 0.63 & 3.81 & 4.91 & String theory \& supergravity (0.63$\to$0.01) & Electroweak sector (0.01$\to$0.38)\\ \hline
  14. D.~Shih & 0.62 & 5.74 & 10.21 & String theory \& supergravity (0.52$\to$0.01) & Electroweak sector (0.06$\to$0.45)\\ \hline
  15. S.~D.~Katz ($\ast$) & 0.61 & 6.50 & 10.85 & Dark matter (0.42$\to$0.03) & QCD (0.06$\to$0.47)\\ \hline
  16. K.~Bhattacharya & 0.60 & 10.79 & 10.59 & Neutrinos \& flavour physics (0.20$\to$0.00) & Cosmology (0.09$\to$0.37)\\ \hline
  17. J.~Evslin & 0.60 & 3.32 & 6.81 & String theory \& supergravity (0.71$\to$0.08) & Neutrinos \& flavour physics (0.00$\to$0.43)\\ \hline
  18. G.~B.~Cleaver ($\ast$) & 0.57 & 6.34 & 12.22 & String theory \& supergravity (0.40$\to$0.00) & Cosmology (0.03$\to$0.62)\\ \hline
  19. J.~Martin Camalich & 0.57 & 2.34 & 4.57 & QCD (0.78$\to$0.03) & Hadrons (0.06$\to$0.38)\\ \hline
  20. A.~T.~Suzuki ($\ast$) & 0.57 & 4.36 & 6.43 & Perturbative methods (0.61$\to$0.04) & Neutrinos \& flavour physics (0.01$\to$0.39)\\ \hline
  21. Qing Wang ($\ast$) & 0.55 & 7.86 & 9.76 & QCD (0.26$\to$0.05) & Dark matter (0.02$\to$0.66)\\ \hline
  22. Eiji Nakano ($\ast$) & 0.55 & 6.90 & 10.13 & QCD (0.39$\to$0.06) & Hadrons (0.04$\to$0.78)\\ \hline
  23. D.~Blas & 0.55 & 5.89 & 12.61 & Classical fields (0.33$\to$0.03) & Dark matter (0.00$\to$0.51)\\ \hline
  24. G.~Beuf & 0.54 & 8.57 & 9.07 & Collider physics (0.26) & Collider physics (0.82)\\ \hline
  25. M.~Olechowski ($\ast$) & 0.54 & 8.19 & 11.17 & Cosmology (0.28$\to$0.00) & Dark matter (0.04$\to$0.47)\\ \hline
  26. M.~Redi ($\ast$) & 0.53 & 9.81 & 12.76 & String theory \& supergravity (0.21$\to$0.01) & Dark matter (0.02$\to$0.42)\\ \hline
  27. V.~V.~Braguta ($\ast$) & 0.53 & 5.03 & 8.04 & Hadrons (0.45$\to$0.00) & QCD (0.05$\to$0.60)\\ \hline
  28. J.~Sola Peracaula & 0.52 & 6.28 & 10.50 & Electroweak sector (0.52$\to$0.03) & Cosmology (0.14$\to$0.64)\\ \hline
  29. \bottomrule
  30. \end{tabular}
  31. \end{table}