Search results
Jump to navigation
Jump to search
Page title matches
- ...hout electrical charge and roughly the same mass as [[w:proton |proton]]s. Neutron stars are very hot and are supported against further collapse because of th ...e]] (EOS) is used. <ref> Pawel Haensel, A.Y.Potekhin, D.G.Yakovlev (2007). Neutron Stars. Springer. {{ISBN|0387335439}}. [http://books.google.com/books?id=iIr ...10 KB (1,496 words) - 17:06, 26 January 2025
- ...escribing the internal structure, origin and evolution of the [[w:neutron| neutron]] based on the theory of [[Physics/Essays/Fedosin/Infinite Hierarchical Nes ...has a magnetic moment, which reflects its complex internal structure. The neutron’s magnetic moment is directed oppositely to the spin, while the proton’s ma ...29 KB (4,560 words) - 01:59, 5 April 2023
- This unit explores how know the sizes of white dwarfs, neutron stars, and quasars. In the process of answering these questions, we shall **Neutron star internal structure 540 (38) ...12 KB (1,993 words) - 02:55, 18 June 2015
- :___ d)d) a neutron star : - d)d) a neutron star ...22 KB (3,224 words) - 19:20, 29 May 2018
Page text matches
- ...hout electrical charge and roughly the same mass as [[w:proton |proton]]s. Neutron stars are very hot and are supported against further collapse because of th ...e]] (EOS) is used. <ref> Pawel Haensel, A.Y.Potekhin, D.G.Yakovlev (2007). Neutron Stars. Springer. {{ISBN|0387335439}}. [http://books.google.com/books?id=iIr ...10 KB (1,496 words) - 17:06, 26 January 2025
- ...ed [[../Pions/|neutron]] and [[../MuonLepton/|Muon]] Source, International Neutron Experiments Facility at Harwell (near Oxford), UK ...3 KB (346 words) - 16:15, 12 September 2020
- ...f the neutron bombardment during the irradiation process; a denser flow of neutron particles will convert more atoms of <sup>39</sup>K to <sup>39</sup>Ar than ...2 KB (336 words) - 06:40, 2 April 2022
- ...he pressure of [[electron]]s, and in [[Physics/Essays/Fedosin/Neutron star|neutron star]]s – by the pressure of degenerate [[w:nucleon |nucleon]] gas. Hence i ...ħ<sub>s</sub> = 2.8∙10<sup>41</sup> J∙s. For degenerate objects, such as neutron stars, the stellar Dirac constant is greater in magnitude: ħ’<sub>s</sub> = ...9 KB (1,361 words) - 02:00, 5 April 2023
- ...es to all of the neutrons. This prohibition does not apply to a proton and neutron occupying the same quantum state. Neutron = A<sub>r</sub> = 1, ...6 KB (1,032 words) - 13:46, 15 November 2018
- ...oms and molecules. Thus the stellar matter emerges, the basis of which are neutron stars and magnetars as the stars that carry a strong magnetic field and an The stellar Stefan–Boltzmann constant for neutron stars is: ...8 KB (1,265 words) - 02:00, 5 April 2023
- ...h a resulting `white' color, or [[../Charge/|charge]] colorless proton and neutron, as well as stable `white' nuclei `consisting of' the latter two [[../Quant ...4 KB (483 words) - 02:52, 13 November 2023
- we get for the heaviest elementary particle of the normal matter [[w:neutron|neutron]] ...assume the opposite, that the cross section for the graviton capturing by neutron (or proton) is equal to its "seen" ...8 KB (1,289 words) - 18:08, 5 November 2022
- Baryons are strongly interacting Fermions, such as a Proton or a Neutron, both of which are made up 3 Quarks. Baryons have a baryon number of 1. The * Neutron ...4 KB (769 words) - 05:36, 15 April 2024
- ...charge, another force and new particles, one of which is the neutron (the neutron contributes to the strong nuclear force, but not to the electromagnetic rep ...his mechanism, called beta decay. When a nucleus has had enough of life, a neutron might decide to turn into a proton and emit an electron (which will go into ...6 KB (986 words) - 17:20, 11 January 2024
- ...he mass of a nucleus arises from mass of its constituent [[proton]]s and [[neutron]]s. Thus, the mass excess is an expression of the [[nuclear binding energy ...same manner, the mass excess for <sup>92</sup>Kr, <sup>141</sup>Ba, and a neutron are <math>-0.073843</math> u, <math>-0.085588</math> u and <math>0.0086648< ...4 KB (682 words) - 03:40, 1 May 2017
- ...consist of [[graon]]s in a similar way as nucleons consist of praons, and neutron stars consist of nucleons. Ultrarelativistic flows of praons are one of the ...from which nucleons, electrons and other particles are composed. A typical neutron star contains approximately ''Ф'' = 1.62∙10<sup>57 </sup> nucleons, and the ...17 KB (2,812 words) - 02:01, 5 April 2023
- ...ur sun is a large collection of normal Shells. It is also possible to have neutron stars and black holes. Free neutrons and subneutrons within our sun gave ri A Hydrogen atom comprises a small Shell or neutron inside a normal Shell. When the two centers are co-located, they count as o ...13 KB (2,256 words) - 04:12, 25 February 2018
- ...escribing the internal structure, origin and evolution of the [[w:neutron| neutron]] based on the theory of [[Physics/Essays/Fedosin/Infinite Hierarchical Nes ...has a magnetic moment, which reflects its complex internal structure. The neutron’s magnetic moment is directed oppositely to the spin, while the proton’s ma ...29 KB (4,560 words) - 01:59, 5 April 2023
- ...</math> nucleus as a three--body system: <math>\alpha</math>--particle and neutron momentum distributions. ''Nuclear Physics A'' , Volume 538, 2 March 1992, P ...2 KB (276 words) - 04:16, 1 July 2015
- ..., h<sub>s</sub> = 1.8∙10<sup>42</sup> J∙s. For degenerate objects, such as neutron stars, the stellar Planck constant is slightly greater in magnitude: h’<sub ...eutron stars (in particular, the data for the proton and the corresponding neutron star are used): <ref name=com> [http://sergf.ru/com.htm Comments to the boo ...15 KB (2,374 words) - 02:00, 5 April 2023
- ...logues of muons are white dwarfs, which remain after the decay of low mass neutron stars. White dwarfs arise from the [[w:main sequence |main sequence]] stars ...kinetic energy and rebound of the envelope from the formed neutron star. A neutron star can also be formed when the mass of the carbon-oxygen white dwarf exce ...17 KB (2,862 words) - 01:59, 5 April 2023
- ...s]] at ambient [[../BoltzmannConstant/|temperatures]]. Several [[../Pions/|neutron]] inelastic, as well as Cu <math>K_\alpha</math> edge resonant inelastic [[ ...2 KB (275 words) - 04:40, 1 July 2015
- ...ystems are formed by a normal star and a compact object, a black hole or a neutron star, which accretes mass from the star. Other components conform a microqu ...hat the material evaporates thus forming the corona. In systems where the neutron star is highly magnetized this component is not present. The corona is tho ...8 KB (1,145 words) - 04:13, 16 October 2020
- This unit explores how know the sizes of white dwarfs, neutron stars, and quasars. In the process of answering these questions, we shall **Neutron star internal structure 540 (38) ...12 KB (1,993 words) - 02:55, 18 June 2015