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- ...ties can be measured at the level of stars. A considerable part of stellar constants was introduced by [[User:Fedosin | Sergey Fedosin]] in 1999. <ref name="Fed == Constants for systems with main-sequence stars == ...20 KB (2,999 words) - 08:57, 12 March 2025
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- ...t relates the average [[w:luminosity |luminosity]] of a sufficiently large stellar system with the area of its outer surface and the average [[temperature]] o ...tomic and stellar levels of matter. This allowed finding various [[stellar constants]] based on the dimensional equations. ...8 KB (1,265 words) - 02:00, 5 April 2023
- ...he average [[energy]] of motion in a certain set of typical objects of the stellar level of matter with the kinetic [[temperature]] characterizing this set. ...constants, inherent in the level of elementary particles, to the physical constants of other scale levels. ...8 KB (1,237 words) - 02:00, 5 April 2023
- ...angular momentum and [[w:action (physics) |action]] for the objects of the stellar level of matter. ...constant|stellar Planck constant]] h<sub>s</sub>, which was related to the stellar Dirac constant by a factor 2''π'' : h<sub>s</sub> = 2π ħ<sub>s</sub>. ...9 KB (1,361 words) - 02:00, 5 April 2023
- ...<ref> Latest (2010) values of the constants. [http://physics.nist.gov/cuu/Constants/index.html] </ref> === Coupling constants === ...10 KB (1,390 words) - 16:15, 26 January 2025
- ...ties can be measured at the level of stars. A considerable part of stellar constants was introduced by [[User:Fedosin | Sergey Fedosin]] in 1999. <ref name="Fed == Constants for systems with main-sequence stars == ...20 KB (2,999 words) - 08:57, 12 March 2025
- ...Value?alph "CODATA Value: fine-structure constant"]. The NIST Reference on Constants, Units, and Uncertainty. US National Institute of Standards and Technology. Some equivalent definitions of ''α'' in terms of other fundamental physical constants are: ...7 KB (1,028 words) - 13:52, 26 January 2025
- ...diagram |Feynman diagram]]s. Dimensionless parameters are used as coupling constants, as well as quantities associated with them that characterize interaction a ...teraction |fundamental interaction]]s, values of dimensionless interaction constants, found by general rule, show relative strength of these interactions. The [ ...15 KB (2,082 words) - 13:36, 28 February 2025
- ...mentum]] and [[w:action (physics) |action]] inherent in the objects of the stellar level of matter. ...2''π'') we can obtain the [[Physics/Essays/Fedosin/Stellar Dirac constant|stellar Dirac constant]]. ...15 KB (2,374 words) - 02:00, 5 April 2023
- ...Units |International System of Units]], the first mention of gravitational constants was possibly due to Forward (1961).<ref name = Forward1>R. L. Forward, Proc In gravitational wave representation, the set of gravitational constants depends on the speed of propagation of gravity, in contrast to electromagne ...13 KB (1,937 words) - 16:06, 29 January 2025
- ...edosin/Selfconsistent gravitational constants|selfconsistent gravitational constants]], ...ational characteristic impedance of free space may be connected with other constants: ...12 KB (1,479 words) - 13:27, 26 January 2025
- = Chapter 7: Units, Dimensions, and Fundamental Constants in Cosmic Influx Theory (CIT) = ...also explores the relationship between vacuum properties, electromagnetic constants, and gravitational interactions. These involve: ...9 KB (1,148 words) - 06:34, 20 March 2025
- ==Table of universal constants== ==Table of electromagnetic constants== ...8 KB (1,182 words) - 17:01, 4 April 2023
- ...dosin/Selfconsistent gravitational constants |selfconsistent gravitational constants]] in the field of strong gravitation, ...of Matter|Infinite Hierarchical Nesting of Matter]] where different action constants connected to different matter levels. ...20 KB (3,027 words) - 15:12, 27 January 2025
- ...in velocities is equal to <math>S_0=7.338\cdot 10^{-4}</math>, then at the stellar level we have seven characteristic speeds for different classes of objects: ...<math>C_7= 52</math> km/s, otherwise such a planet should be considered a stellar object. ...15 KB (2,432 words) - 01:58, 5 April 2023
- ...edosin/Selfconsistent gravitational constants|selfconsistent gravitational constants]], and ...the gravitomagnetic gravitational constant of selfconsistent gravitational constants, <math> \beta = \frac {1}{4\alpha} \ </math> is the gravitational torsion c ...18 KB (2,792 words) - 09:26, 27 January 2025
- Similarly, for gravitational constant at the stellar level of matter, there is a relationship between corresponding energy densi ...\cdot 10^{34}</math> J/m³ is the energy density of graviton fluxes at the stellar level for cubic distribution; <math>~ \vartheta_s = \vartheta P'^2 = 5.2 \c ...12 KB (1,804 words) - 17:57, 29 January 2025
- == Stellar and galactic hydrogen systems == ...<math>~ 0.145 M_c </math> (where <math>~ M_c </math> is Solar mass), are stellar analogue of hydrogen atom with mass <math> ~M_p </math>. <ref>Robert L. Ol ...28 KB (4,330 words) - 09:10, 5 March 2025
- ...number of nucleons, and at the level of stars we observe [[discreteness of stellar parameters]] and the similarity between atoms and stars, including correspo Since the stellar matter is held by gravitational forces, the [[characteristic speed]] of mat ...62 KB (10,046 words) - 01:58, 5 April 2023
- ...utput of unification’. The same idea can be applied to the atomic physical constants also. Sitting in a grand unified roof one cannot make an ‘absolute measure ...speed, respectively, for the degenerate quantum objects at the atomic and stellar levels of matter.<ref name="fed"/> The powers of similarity coefficients i ...34 KB (5,250 words) - 15:38, 16 December 2024
- ...31-433. DOI: 10.107/s10509-007-9557-x. </ref> Oldershaw attributes atomic, stellar and galactic levels of matter to the main levels in observable world, and i ...n matter level considered [[black hole]] can be a proton or an appropriate stellar or galactic object. ...43 KB (6,665 words) - 08:43, 19 February 2025