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  2. Maria Goeppert Mayer - Wikipedia

    en.wikipedia.org/wiki/Maria_Goeppert_Mayer

    Maria Goeppert Mayer. Maria Goeppert Mayer (German pronunciation: [maˈʁiːa ˈɡœpɛʁt ˈmaɪ̯ɐ] ⓘ, née Göppert; June 28, 1906 – February 20, 1972) was a German-American theoretical physicist, and Nobel laureate in Physics for proposing the nuclear shell model of the atomic nucleus. She was the second woman to win a Nobel Prize in ...

  3. Nuclear shell model - Wikipedia

    en.wikipedia.org/wiki/Nuclear_shell_model

    The model was developed in 1949 following independent work by several physicists, most notably Maria Goeppert Mayer and J. Hans D. Jensen, who received the 1963 Nobel Prize in Physics for their contributions to this model, and Eugene Wigner, who received the Nobel Prize alongside them for his earlier groundlaying work on the atomic nuclei. [2]

  4. Double beta decay - Wikipedia

    en.wikipedia.org/wiki/Double_beta_decay

    The idea of double beta decay was first proposed by Maria Goeppert Mayer in 1935. [1] [2] In 1937, Ettore Majorana demonstrated that all results of beta decay theory remain unchanged if the neutrino were its own antiparticle, now known as a Majorana particle. [3]

  5. Women in physics - Wikipedia

    en.wikipedia.org/wiki/Women_in_physics

    1963: Maria Goeppert Mayer became the first American woman to receive a Nobel Prize in Physics; she shared the prize with J. Hans D. Jensen "for their discoveries concerning nuclear shell structure” and Eugene Paul Wigner "for his contributions to the theory of the atomic nucleus and the elementary particles, particularly through the ...

  6. Magic number (physics) - Wikipedia

    en.wikipedia.org/wiki/Magic_number_(physics)

    According to Steven Moszkowski, a student of Goeppert Mayer, the term "magic number" was coined by Wigner: "Wigner too believed in the liquid drop model, but he recognized, from the work of Maria Mayer, the very strong evidence for the closed shells. It seemed a little like magic to him, and that is how the words 'Magic Numbers' were coined."

  7. Absorption cross section - Wikipedia

    en.wikipedia.org/wiki/Absorption_cross_section

    One GM is 10 −50 cm 4 ⋅s⋅photon −1. [1][2] In the context of ozone shielding of ultraviolet light, absorption cross section is the ability of a molecule to absorb a photon of a particular wavelength and polarization. Analogously, in the context of nuclear engineering it refers to the probability of a particle (usually a neutron) being ...

  8. Two-photon absorption - Wikipedia

    en.wikipedia.org/wiki/Two-photon_absorption

    Schematic of energy levels involved in two photons absorption. In atomic physics, two-photon absorption (TPA or 2PA), also called two-photon excitation or non-linear absorption, is the simultaneous absorption of two photons of identical or different frequencies in order to excite an atom or a molecule from one state (usually the ground state), via a virtual energy level, to a higher energy ...

  9. Nonlinear optics - Wikipedia

    en.wikipedia.org/wiki/Nonlinear_optics

    The first nonlinear optical effect to be predicted was two-photon absorption, by Maria Goeppert Mayer for her PhD in 1931, but it remained an unexplored theoretical curiosity until 1961 and the almost simultaneous observation of two-photon absorption at Bell Labs [4] and the discovery of second-harmonic generation by Peter Franken et al. at University of Michigan, both shortly after the ...