Black Holes, Cosmology and Space-Time Singularities
Nobel Lecture, December 8, 2020 by
Roger Penrose, University of Oxford, Oxford, United Kingdom.

(pp.63-64)
The area that I thought might be helpful was the theory of 2-component
spinors. I should explain that I finally understood properly about
2-spinors from lectures by the great quantum physicist Paul Dirac, earlier
in the spring of 1958, in the academic year before Finkelstein’s lecture.
Dirac’s course was basically on quantum field theory, but he appeared to
have deviated from his normal course when he talked about 2-spinors. He
was famous for discovering the dynamical equation for the electron, but
this originally involved the introduction of 4-spinors. However, you can
break each of them down into a pair of 2-spinors and Dirac had become
well acquainted with this fact, having written an important paper [6]
describing higher-spin fields in these terms. Yet, these techniques were
not very familiar to most physicists at that time. I had myself heard of
2-spinors and had been intrigued by them, but I did not really understand
them until Dirac’s lectures had made them abundantly clear to me!
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(p.94)
[6] Dirac, P.A.M. (1936) Relativistic wave equations. Proc. Roy. Soc. (Lond.) A155, 447–59.