Chamberlain-Segrè antiproton identification 2026-10-18
In 1955, Owen Chamberlain, Emilio Segrè, Clyde Wiegand, and Thomas Ypsilantis used Bevatron protons on copper, selecting negative secondaries. Magnetic fields selected ; scintillation counters S1 and S2 measured time of flight over . Cherenkov detector C1 flagged ; C2 accepted after material losses. S3 checked traversal. The cuts rejected negative pions.[ref]
Chamberlain's 1959 account describes C2's quartz radiator, mirrors, and photomultiplier readout. The trigger combined delayed scintillation counter signals with C2; photographed oscilloscope traces exposed fast particles and accidental coincidences through C1 pulses or extra pulses. Reversing the magnetic fields provided a positive-proton control and revealed an alignment error. Changing selected momentum at fixed velocity acceptance tested for a proton-mass peak.[ref]
The early antiproton work by Owen Chamberlain. 1959 lecture, pp. 496–501, Figs. 7–11; Columbia scan
Terminal-event studies remained unfinished; the 1955 identification did not rely on annihilation.[ref]
https://escholarship.org/content/qt46p0z8w7/qt46p0z8w7.pdf. UCRL-3172, p. 13
The logic is useful far beyond this experiment. A magnetic field separates electric charge signs and magnetic rigidity, but particles of different rest masses can share both. A time of flight signal adds velocity, while a Cherenkov detector independently checks whether that velocity is plausible. An accidental coincidence can imitate the delay of a slow particle without being one particle traversing the apparatus. Agreement between independent measurements is therefore part of the inference, rather than a redundant decoration.
Nobel Prize in Physics in 1959 2026-10-18
Awarded jointly to Emilio Segrè and Owen Chamberlain for discovering the antiproton.[ref]
The Nobel Prize in Physics 1959 by Nobel Prize Outreach. Both laureates, equal shares and antiproton-discovery motivation
Owen Chamberlain Created 2026-10-18 Updated 2026-11-05
Owen Chamberlain helped establish the antiproton by distinguishing a rare massive negative particle from an intense background of lighter particles. Magnetic analysis fixed momentum, while time-of-flight and Cherenkov radiation measurements constrained speed. Together these quantities tested whether the inferred mass matched that of the proton. His lecture emphasizes both the apparatus and the inference drawn from the particle's existence, separating discovery from later studies of its interactions.[ref]
The early antiproton work by Owen Chamberlain. 1959 lecture, magnetic selection, velocity measurements and antiproton identification
A physicist.[ref]
https://www.nasonline.org/wp-content/uploads/2024/06/chamberlain-owen.pdf. Independent professional profile
Portrait of Owen Chamberlain
. Nobel Foundation; individual photographer unidentified. Commons PD-Sweden designation in primary File category and upload history. No independent United States or worldwide determination., via Wikimedia Commons. Source.
