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- Helena, and Hobarton. 1854 Thomas Graham, On Osmotic Force. 1855 John Tyndall, On the Nature of the Force by which Bodies are repelled from the Poles of a…25 KB (3.337 Wörter) - 22:08, 6. Dez. 2024
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- the nuclear force becomes repulsive. This repulsion is responsible for the size of nuclei, since nucleons can come no closer than the force allows. (The…29 KB (3.510 Wörter) - 03:59, 12. Jul. 2025
- Neutron star (Weiterleitung von „Stellar spin-down“)densities reach a nuclear density of 4×1017 kg/m3, a combination of strong force repulsion and neutron degeneracy pressure halts the contraction. The contracting…117 KB (13.877 Wörter) - 02:15, 3. Aug. 2025
- Nuclear fusion (Abschnitt Stellar reaction chains)electrostatic repulsion and be brought close enough such that the attractive nuclear force is greater than the repulsive Coulomb force. The strong force grows…113 KB (12.226 Wörter) - 06:19, 17. Jul. 2025
- repulsion arises from the energy density, not the Planck length, and starts taking effect far earlier than might be expected. This repulsive "force"…5 KB (555 Wörter) - 04:59, 24. Jun. 2025
- drawback is this will cause the fuel to disperse due to electrostatic repulsion.[citation needed] Launching the fuel on a trajectory so that the fuel…18 KB (1.976 Wörter) - 05:20, 25. Mai 2025
- Electron degeneracy pressure (Kategorie Stellar evolution)than the Sun. At this density gravity exerts immense force pulling the nuclei together. This force is balanced by the electron degeneracy pressure keeping…8 KB (981 Wörter) - 12:05, 1. Jul. 2025
- Nuclear binding energy (Abschnitt The nuclear force)force does not hold nuclei together, because all protons carry a positive charge and repel each other. If two protons were touching, their repulsion force…52 KB (7.079 Wörter) - 04:14, 17. Jul. 2025
- Dark energy (Weiterleitung von „Dark repulsive force theory“)This accelerating expansion effect is sometimes labeled "gravitational repulsion". In standard cosmology, there are three components of the universe: matter…89 KB (9.948 Wörter) - 14:22, 29. Jul. 2025
- of the protons is high enough to overcome their mutual electrostatic repulsion. In the Sun, deuteron-producing events are rare. Diprotons are the much…22 KB (2.250 Wörter) - 16:07, 18. Jul. 2025
- at low temperature. The term is used in astrophysics to refer to dense stellar objects such as white dwarfs and neutron stars, where thermal pressure…23 KB (3.074 Wörter) - 22:08, 24. Jun. 2025
- Nuclear physics (Abschnitt Eddington and stellar nuclear fusion)including protons and neutrons. This force explained why nuclei did not disintegrate under the influence of proton repulsion, and it also gave an explanation…43 KB (5.094 Wörter) - 22:33, 24. Mai 2025
- P-process (Kategorie Concepts in stellar astronomy)electric charge increases with each added proton, leading to an increased repulsion of the next proton to be added, according to Coulomb's law. In the context…7 KB (803 Wörter) - 12:38, 3. Feb. 2025
- the discovery will help understand the strong nuclear force and provide fresh insights into stellar nucleosynthesis. Galindo-Uribarri and co-workers chose…24 KB (2.660 Wörter) - 07:46, 23. Jul. 2025
- as 0.7 M☉. Subsequent consideration of neutron-neutron repulsion mediated by the strong force raised the estimate to approximately 1.5 M☉ to 3.0 M☉. Observations…168 KB (18.965 Wörter) - 14:04, 30. Jul. 2025
- more stable against decay, but with increasing atomic number, the mutual repulsion of the protons requires an increasing proportion of neutrons to maintain…126 KB (12.982 Wörter) - 02:39, 17. Jul. 2025
- More realistic models of neutron stars that include baryon strong force repulsion predict a neutron star mass limit of 2.2 to 2.9 M☉. The uncertainty…24 KB (3.246 Wörter) - 01:47, 26. Mai 2025
- strong nuclear force attractions. In particular, most pairs of protons in large nuclei are not far enough apart, such that electrical repulsion dominates over…4 KB (523 Wörter) - 14:51, 29. Jan. 2024
- nucleus). The nuclear force is highly attractive at the distance of typical nucleon separation, and this overwhelms the repulsion between protons due to…33 KB (3.945 Wörter) - 05:11, 28. Jun. 2025
- between the attractive properties of the strong nuclear force and the mutual coulombic repulsion of the constituent protons. Nuclear binding energy increases…19 KB (2.008 Wörter) - 20:38, 17. Jun. 2025
- particles requires that they pass through each other; for infinitely strong repulsion this cannot happen. This model is described by a quantum nonlinear Schrödinger…26 KB (3.470 Wörter) - 03:14, 27. Jul. 2025
- so large that the strong nuclear force holding it together can just barely counterbalance the electromagnetic repulsion between the protons it contains…19 KB (2.546 Wörter) - 20:43, 26. Jul. 2025