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  2. Gamow factor - Wikipedia

    en.wikipedia.org/wiki/Gamow_factor

    Gamow [3] first solved the one-dimensional case of quantum tunneling using the WKB approximation.Considering a wave function of a particle of mass m, we take area 1 to be where a wave is emitted, area 2 the potential barrier which has height V and width l (at < <), and area 3 its other side, where the wave is arriving, partly transmitted and partly reflected.

  3. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    The reaction rate density between species A and B, ... the integral almost vanished everywhere except around the peak, called Gamow peak, [37]: 185 ...

  4. Pycnonuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Pycnonuclear_fusion

    Pycnonuclear fusion (Ancient Greek: πυκνός, romanized: pyknós, lit. 'dense, compact, thick') is a type of nuclear fusion reaction which occurs due to zero-point oscillations of nuclei around their equilibrium point bound in their crystal lattice.

  5. Timeline of nuclear fusion - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_nuclear_fusion

    George Gamow introduces the mathematical basis for quantum tunnelling. [2] 1929. Atkinson and Houtermans provide the first calculations of the rate of nuclear fusion in stars. Based on Gamow's tunnelling, they show fusion can occur at lower energies than previously believed.

  6. George Gamow - Wikipedia

    en.wikipedia.org/wiki/George_Gamow

    [16] [17] [18] This work, in turn, evolved from his fundamental discovery of quantum tunneling as the mechanism of nuclear alpha decay, and his application of this theory to the inverse process to calculate rates of thermonuclear reaction. At first, Gamow believed that all the elements might be produced in the very high temperature and density ...

  7. Coulomb barrier - Wikipedia

    en.wikipedia.org/wiki/Coulomb_barrier

    The consideration of barrier-penetration through tunnelling and the speed distribution gives rise to a limited range of conditions where fusion can take place, known as the Gamow window. The absence of the Coulomb barrier enabled the discovery of the neutron by James Chadwick in 1932. [1] [2]

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  9. Beta decay transition - Wikipedia

    en.wikipedia.org/wiki/Beta_decay_transition

    The Gamow–Teller transition is a pseudovector transition, that is, the selection rules for beta decay caused by such a transition involve no parity change of the nuclear state. [2] The spin of the parent nucleus can either remain unchanged or change by ±1.