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Oppenheimer–Phillips process

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Oppenheimer–Phillips process
NameOppenheimer–Phillips process
TypeNuclear reaction
Discovered byJ. Robert Oppenheimer and Melba Phillips
Year1935
FieldNuclear physics

Oppenheimer–Phillips process. It is a specific type of nuclear reaction involving deuterons, first described theoretically in 1935 by physicists J. Robert Oppenheimer and his graduate student Melba Phillips. The process explains the unexpectedly high reaction cross sections observed when deuterons interact with certain target nuclei at relatively low energies. This mechanism was a significant early contribution to the understanding of low-energy nuclear physics and helped refine models of the atomic nucleus.

Overview

The process is a stripping reaction where a deuteron, the nucleus of deuterium, interacts with a target nucleus. During the interaction, the loosely bound proton and neutron in the deuteron are separated by the Coulomb barrier and nuclear forces of the target. Typically, the neutron is captured by the target nucleus while the proton is repelled by the electrostatic force. This results in a transformation of the target, effectively producing an isotope one mass unit heavier, without the deuteron as a whole needing to penetrate the Coulomb barrier. This mechanism was crucial for interpreting experiments conducted at facilities like the University of California, Berkeley and the Cavendish Laboratory.

Historical background

The theoretical explanation was developed in response to experimental data from the early 1930s. Researchers such as Ernest Lawrence using his cyclotron at the University of California, Berkeley, and teams at the Cavendish Laboratory in Cambridge, including work by John Cockcroft and Ernest Walton, observed that deuteron-induced reactions occurred at energies much lower than predicted by standard Gamow factor calculations for full compound nucleus formation. Oppenheimer and Phillips published their seminal paper in the journal Physical Review in 1935, providing a quantum mechanical treatment that resolved this discrepancy. Their work built upon earlier foundations in quantum mechanics established by figures like Niels Bohr and George Gamow.

Physical mechanism

The mechanism hinges on the deuteron's low binding energy of approximately 2.2 MeV. As the deuteron approaches the target nucleus, such as an isotope of beryllium or lithium, the intense electric field distorts the deuteron's structure. The proton, due to its positive charge, experiences strong Coulomb repulsion from the target's protons. This can cause the deuteron to break apart before it reaches the distance required for the full nuclear force to act. The neutron, being neutral, continues inward and is readily captured if it passes within the range of the nuclear force, a region described by models like the liquid-drop model. This process is distinct from a full fusion or a compound nucleus reaction, as it bypasses the need for the entire deuteron to overcome the Coulomb barrier.

Applications and examples

The process was historically important for early studies in nuclear transmutation and the production of radioisotopes. A classic example is the reaction of a deuteron with a nucleus of beryllium-9, producing beryllium-10 and a proton: d + 9Be → 10Be + p. Similarly, reactions with lithium-6 could yield lithium-7. These reactions were studied extensively at institutions like the Radiation Laboratory at Berkeley and contributed to the development of nuclear chemistry. The understanding of this stripping mechanism also informed later work in nuclear astrophysics, particularly in analyzing low-energy reactions that might occur in stellar environments like the Sun.

Relation to other processes

It is a specific precursor to the broader category of direct nuclear reactions, contrasting with compound nucleus formation as described by the Bohr model. It is closely related to other stripping reactions like the deuteron stripping analyzed in later frameworks such as the distorted-wave Born approximation. The process differs fundamentally from fusion power reactions like those in the ITER project or the proton–proton chain in stars, which require full penetration of the Coulomb barrier. Its theoretical treatment also shares conceptual ground with models of nuclear structure and reactions developed at major laboratories like the Los Alamos National Laboratory and the Joint Institute for Nuclear Research.

Category:Nuclear physics Category:Nuclear reactions Category:Physics experiments