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Maurice Goldhaber

 
Scientist: Maurice Goldhaber

Austrian–American physicist (1911–)

Goldhaber, who was born at Lemberg (now Lvov in Ukraine), was educated at the universities of Berlin and Cambridge, where he obtained his PhD in 1936. He emigrated to America in 1938 where he first taught at the University of Illinois, becoming professor there in 1945. He moved to the Brookhaven National Laboratory in 1950, serving as its director from 1961 until 1973.

In 1934, while at the Cavendish Laboratory of Cambridge University, Goldhaber codiscovered the nuclear photoelectric effect with James Chadwick. This is the disintegration of a nucleus by high-energy x-rays or gamma rays. From this it was later established that the neutron is slightly heavier than the proton. Following Enrico Fermi's discovery of slow neutrons, Chadwick and Goldhaber also discovered (1934–35) the neutron disintegration reactions for lithium, boron, and nitrogen. The nitrogen reaction is the major source of radioactive carbon–14 on Earth.

At the University of Illinois (1938) Goldhaber and his wife, Gertrude Scharff-Goldhaber, demonstrated that electrons and beta particles are the same. In 1940 he discovered that beryllium is a good moderator, i.e., it slows down fast neutrons so that they more readily split uranium atoms.

He has also proposed a cosmological theory in which an initial ‘universon’ broke up into a ‘cosmon’ (matter) and an ‘anticosmon’ (antimatter), with the anticosmon forming a second universe made of antimatter.

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Maurice Goldhaber

Born April 18, 1911 (1911-04-18) (age 98)
Lemburg, Austria
Residence United States
Nationality  Austria
Fields Physicist
Institutions Cavendish Laboratory
Doctoral advisor James Chadwick
Known for Neutrinos and negativehelicity
Notable awards National Medal of Science (1985)
Wolf Prize (1991)
J. Robert Oppenheimer Memorial Prize (1992)
Fermi Award (1998).

Maurice Goldhaber (born April 18, 1911) is an American physicist, who in 1957 (with Lee Grodzins and Andrew Sunyar) established that neutrinos have negative helicity.

He was born in Lemberg, Austria. In 1934, working at the Cavendish Laboratory in Cambridge, England he and James Chadwick, through what they called the nuclear photo-electric effect, established that the neutron has a great enough mass over the proton to decay. In the 1940s with his wife Gertrude Scharff-Goldhaber he established that beta particles are identical to electrons. With Edward Teller he proposed that the so-called "giant-dipole nuclear resonance" was due to the neutrons in a nucleus vibrating as a group against the protons as a group (Goldhaber-Teller model).

He made a well-known bet with Hartland Snyder in about 1955 that anti-protons could not exist; when he lost the bet, he speculated that the reason anti-matter does not appear to be abundant in the universe is that before the Big Bang, a single particle, the "universon" existed that then decayed into "cosmon" and "anti-cosmon," and that the cosmon subsequently decayed to produce the known cosmos. In the 1950s also he speculated that all fermions[1] such as electrons, protons and neutrons are "doubled," that is that each is associated with a similar heavier particle. He also speculated that in what became known as the Goldhaber-Christie model, the so-called strange particles were composites of just 3 basic particles. He was Director of Brookhaven National Laboratory from 1961 to 1973.

Among his many other awards, he won the National Medal of Science in 1985, the Wolf Prize in 1991, the J. Robert Oppenheimer Memorial Prize in 1992, and the Fermi Award in 1998.

Maurice Goldhaber's brother Gerson Goldhaber is a professor of physics at Berkeley; his son Alfred Scharff Goldhaber is a professor of physics at SUNY Stony Brook; his grandson (son of Alfred) David Goldhaber-Gordon is a professor of physics at Stanford.

References

  • G. Feinberg, A.W. Sunyar, J. Weneser, A Festschrift for Maurice Goldhaber,New York Academy of Sciences (1993), ISBN 0897660862
  1. ^ Goldhaber, Maurice (2002), "A closer look at the elementary fermions.", Proc. Natl. Acad. Sci. U.S.A. 99 (1): 33–6, 2002 Jan 8, doi:10.1073/pnas.221582298, PMID 11773637 

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