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  • Polytrope (redirección desde Polytropic gas)
    of proportionality. The constant n is known as the polytropic index; note however that the polytropic index has an alternative definition as with n as the…
    7 kB (863 palabras) - 12:04 19 mar 2024
  • κ {\displaystyle \kappa } is the polytropic exponent (or polytropic index). The air mass integral for the polytropic model does not lend itself to a closed-form…
    35 kB (5388 palabras) - 00:20 20 ene 2024
  • gravitational potential of a Newtonian self-gravitating, spherically symmetric, polytropic fluid. It is named after astrophysicists Jonathan Homer Lane and Robert…
    20 kB (3440 palabras) - 22:00 14 abr 2024
  • gravitational potential of a Newtonian self-gravitating, spherically symmetric polytropic fluid Synestia Circumplanetary disk – Accumulation of matter around a…
    9 kB (1149 palabras) - 07:41 26 mar 2024
  • corresponds to the polytropic index of an isothermal gas).[citation needed] So the second case is the rule rather than an exception in stars. This is the reason…
    19 kB (2957 palabras) - 16:12 4 feb 2024
  • explanations for Cepheid variable stars. He began by extending Karl Schwarzschild's earlier work on radiation pressure in Emden polytropic models. These models treated…
    53 kB (6251 palabras) - 01:40 2 may 2024
  • Hayashi track (redirección desde Hayashi track stars)
    = K ρ 1 + 1 / n {\displaystyle P=K\rho ^{1+1/n}} , where n=1.5 is the polytropic index. Applying the equation to the center of the star gives: P c = (…
    24 kB (3733 palabras) - 22:39 23 nov 2023
  • {T^{4}}{P}}} so that T4 is proportional to P throughout the star. This gives the polytropic equation (with n=3): P = ( 3 c k B 4 4 σ B μ 4 1 − β β 4 ) 1 / 3 ρ 4 /…
    11 kB (1718 palabras) - 19:15 4 abr 2024
  • helium starts to fuse in the core. The Schoenberg-Chandrasekhar limit: A polytropic approximation, Martin Beech, Astrophysics and Space Science 147, #2 (August…
    3 kB (446 palabras) - 03:57 24 ene 2020
  • Note that although the equation reduces to the Lane–Emden equation with polytropic index 3/2{\displaystyle 3/2}, the initial condition is not that of the…
    6 kB (1204 palabras) - 16:13 8 feb 2024
  • be estimated from the star approximate polytropic index. Note that this does not hold for large enough stars, where the radiation pressure is larger…
    16 kB (2427 palabras) - 18:16 3 dic 2023
  • original on 2011-08-14. Retrieved 2016-02-08., and a concise treatise on stars by NASA is here "NASA - Star". Archived from the original on 2010-10-24…
    104 kB (12 973 palabras) - 02:31 30 abr 2024
  • gases, and solid states as well as the state of matter in the interior of stars. At present, there is no single equation of state that accurately predicts…
    38 kB (5388 palabras) - 05:55 25 abr 2024
  • effect is unnoticeable at everyday pressures but is significant in neutron stars, although it has not been experimentally tested. Fluid pressure is most…
    44 kB (5649 palabras) - 02:15 16 abr 2024
  • frequently not modeled directly but rather characterized by an effective polytropic equation of state. More recent simulations use a multimodal distribution…
    45 kB (5608 palabras) - 07:05 7 abr 2024
  • the increase because gravity causes dispersed matter to accumulate into stars, which collapse eventually into black holes. The entropy of a black hole…
    108 kB (13 924 palabras) - 10:50 6 abr 2024
  • of thermodynamic equilibrium. They include gravitating objects such as stars and galaxies, and also some nano-scale clusters of a few tens of atoms close…
    19 kB (2773 palabras) - 12:03 19 abr 2024
  • 2(9/8)^{2/3}}}\approx [{\text{ς}},\gamma \sigma ]_{\text{max}},} where the polytropic index γ{\displaystyle \gamma } is the sound speed in units of velocity…
    79 kB (15 411 palabras) - 08:26 12 ene 2024
  • retrieved 23 June 2016 Garfinkel, Boris (1967), "Astronomical Refraction in a Polytropic Atmosphere", The Astronomical Journal, 72 (2): 235–254, Bibcode:1967AJ…
    30 kB (3728 palabras) - 06:38 8 feb 2024
  • introducing polytropic solutions, modelling of a much broader range of stellar objects was possible. His theories also suggested that stars have a boundary…
    9 kB (809 palabras) - 13:14 23 abr 2024
  • collapse of long-destroyed supernova stars (which created these atoms). In cosmology and astronomy the phenomena of stars, nova, supernova, quasars and gamma-ray…
    59 kB (7454 palabras) - 18:40 6 abr 2024