electron-capture transition
61Cadmium — (pronEng|ˈkædmiəm) is a chemical element with the symbol Cd and atomic number 48. A relatively abundant (price 3.55 USD/lb as of 2008 02 15), soft, bluish white, transition metal, cadmium is known to cause cancer and occurs with zinc ores.… …
62Decay energy — Nuclear physics Radioactive decay Nuclear fission Nuclear fusion Classical decays …
63Emanuel Kamber — Emanuel Kamber, Ph. D. is an Assyrian Physics professor at Western Michigan University and was the Secretary General of the Assyrian Universal Alliance. He was born in the small Assyrian village of Darbandokeh in Iraq. In 1983, Emanuel Kamber… …
64White dwarf — For other uses, see White dwarf (disambiguation). Image of Sirius A and Sirius B taken by the Hubble Space Telescope. Sirius B, which is a white dwarf, can be seen as a faint pinprick of light to the lower left of the much brighter Sirius A …
65Nuclear medicine — Intervention ICD 10 PCS C ICD 9: 92 …
66Neutron emission — Neutron emitters to left of lower dashed line Z → 0 1 2 n ↓ n H He 3 4 0 1H Li Be 5 6 1 …
67Artem Alikhanian — Infobox Scientist name = Artem Alikhanian image width = 225px caption = birth date = 1908 birth place = death date = 1978 death place = Moscow residence = citizenship = nationality = Armenian ethnicity = field = work institution = Yerevan Physics …
68Neon-burning process — The neon burning process is a set of nuclear fusion reactions that take place in massive stars (at least 8 Solar masses). Neon burning requires high temperatures and densities (around 1.2×109 K or 100 KeV and 4×109 kg/m3). At such high… …
69Oxygen-burning process — The oxygen burning process is a set of nuclear fusion reactions that take place in massive stars that have used up the lighter elements in their cores. It occurs at temperatures around 1.5×109 K / 130 keV and densities of 1010 kg/m3. The… …
70Naine Blanche — Traduction terminée White dwarf → …
