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  2. Eddington number - Wikipedia

    en.wikipedia.org/wiki/Eddington_number

    He related α to the Eddington number, which was his estimate of the number of protons in the universe. [2] This led him in 1929 to conjecture that α was exactly 1/136. [ 3 ] He devised a "proof" that N Edd = 136 × 2 256 , or about 1.57 × 10 79 .

  3. Neutron - Wikipedia

    en.wikipedia.org/wiki/Neutron

    In many substances, thermal neutron reactions show a much larger effective cross-section than reactions involving faster neutrons, and thermal neutrons can therefore be absorbed more readily (i.e., with higher probability) by any atomic nuclei that they collide with, creating a heavier – and often unstable – isotope of the chemical element ...

  4. List of states of matter - Wikipedia

    en.wikipedia.org/wiki/List_of_states_of_matter

    Neutron-degenerate matter: Found in neutron stars. Vast gravitational pressure compresses atoms so strongly that the electrons are forced to combine with protons via inverse beta decay, resulting in a super dense conglomeration of neutrons.

  5. Neutrino - Wikipedia

    en.wikipedia.org/wiki/Neutrino

    The water-based detectors Kamiokande II and IMB detected 11 and 8 antineutrinos (lepton number = −1) of thermal origin, [104] respectively, while the scintillator-based Baksan detector found 5 neutrinos (lepton number = +1) of either thermal or electron-capture origin, in a burst less than 13 seconds long. The neutrino signal from the ...

  6. List of particles - Wikipedia

    en.wikipedia.org/wiki/List_of_particles

    An atom consists of a small, heavy nucleus surrounded by a relatively large, light cloud of electrons. An atomic nucleus consists of 1 or more protons and 0 or more neutrons. Protons and neutrons are, in turn, made of quarks. Each type of atom corresponds to a specific chemical element. To date, 118 elements have been discovered or created.

  7. Deuterium - Wikipedia

    en.wikipedia.org/wiki/Deuterium

    Urey and others produced samples of heavy water in which the 2 H had been highly concentrated. The discovery of deuterium won Urey a Nobel Prize in 1934. Nearly all deuterium found in nature was synthesized in the Big Bang 13.8 billion years ago, forming the primordial ratio of 2 H to 1 H (≈26 deuterium nuclei per 10 6 hydrogen nuclei).

  8. Elementary particle - Wikipedia

    en.wikipedia.org/wiki/Elementary_particle

    Therefore, one can conclude that most of the visible mass of the universe consists of protons and neutrons, which, like all baryons, in turn consist of up quarks and down quarks. Some estimates imply that there are roughly 10 80 baryons (almost entirely protons and neutrons) in the observable universe. [11]

  9. Properties of water - Wikipedia

    en.wikipedia.org/wiki/Properties_of_water

    [23] 0.23 ppm of the earth's mass is water and 97.39% of the global water volume of 1.38 × 10 9 km 3 is found in the oceans. [ 84 ] Water is far more prevalent in the outer Solar System, beyond a point called the frost line , where the Sun's radiation is too weak to vaporize solid and liquid water (as well as other elements and chemical ...