Sommerfeld parameter

The Sommerfeld parameter η, named after Arnold Sommerfeld, is a dimensionless quantity used in nuclear astrophysics in the calculation of reaction rates between two nuclei and also appears in the definition of the astrophysical S-factor. It is defined as^[1]

[math]\displaystyle{ \eta = \frac{Z_1 Z_2 e^2}{4 \pi \epsilon_0 \hbar v} = \alpha Z_1 Z_2 \sqrt{\frac{\mu c^2}{2E}} }[/math],

where e is the elementary charge, Z₁ and Z₂ are the atomic numbers of two interacting nuclides, v is the magnitude of the relative incident velocity in the center-of-mass frame, α is the unitless fine-structure constant, c is the speed of light, and μ is the reduced mass of the two nuclides of interest.

One of its best-known applications is in the exponent of the Gamow factor P (also known as the penetrability factor),

[math]\displaystyle{ P = \exp(-2 \pi \eta) }[/math],

which is the probability of an s-wave nuclide to penetrate the Coulomb barrier, according to the WKB approximation. This factor is particularly helpful in characterizing the nuclear contribution to low-energy nucleon-scattering cross-sections - namely, through the astrophysical S-factor.

One of the first articles in which the Sommerfeld parameter appeared was published in 1967.^[2]

References

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