Helium-4 (4 He ) is a stable isotope of the element helium. It is by far the more abundant of the two naturally occurring isotopes of helium, making up...
12 KB (1,391 words) - 16:20, 25 March 2024
nuclear binding energy (per nucleon) of helium-4, with respect to the next three elements after helium. This helium-4 binding energy also accounts for why...
146 KB (16,095 words) - 03:31, 25 May 2024
Superfluid helium-4 (helium II or He-II) is the superfluid form of helium-4, an isotope of the element helium. A superfluid is a state of matter in which...
40 KB (4,819 words) - 18:11, 27 April 2024
Liquid helium is a physical state of helium at very low temperatures at standard atmospheric pressures. Liquid helium may show superfluidity. At standard...
12 KB (1,212 words) - 17:33, 6 June 2024
there are nine known isotopes of helium (2He) (standard atomic weight: 4.002602(2)), only helium-3 (3 He ) and helium-4 (4 He ) are stable. All radioisotopes...
24 KB (2,635 words) - 01:47, 19 May 2024
Helium-3 (3He see also helion) is a light, stable isotope of helium with two protons and one neutron (in contrast, the most common isotope, helium-4 has...
64 KB (7,228 words) - 00:48, 7 June 2024
Alpha particle (redirect from Helium-4 nucleus)
protons and two neutrons bound together into a particle identical to a helium-4 nucleus. They are generally produced in the process of alpha decay but...
31 KB (3,860 words) - 23:45, 14 May 2024
Big Bang nucleosynthesis (redirect from Primordial helium abundance)
universe's helium (as isotope helium-4 (4He)), along with small fractions of the hydrogen isotope deuterium (2H or D), the helium isotope helium-3 (3He)...
33 KB (4,406 words) - 23:03, 11 April 2024
Bose–Einstein condensate (section Superfluid helium-4)
include the photon and atoms with an even number of neutrons (such as helium-4 (4 He )), are allowed to share a quantum state. Einstein proposed that cooling...
79 KB (9,882 words) - 15:32, 9 June 2024
Triple-alpha process (redirect from Helium fusion)
nuclear fusion reactions by which three helium-4 nuclei (alpha particles) are transformed into carbon. Helium accumulates in the cores of stars as a result...
20 KB (2,594 words) - 18:22, 2 April 2024