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Polytrope

Index Polytrope

In astrophysics, a polytrope refers to a solution of the Lane–Emden equation in which the pressure depends upon the density in the form where is pressure, is density and is a constant of proportionality. [1]

28 relations: Arthur Schuster, Astrophysics, Brown dwarf, Bulk modulus, Conceptual model, Constant (mathematics), Degenerate matter, Density, Equation of state, Fluid, Gas, Gas giant, Globular cluster, Jupiter, Lane–Emden equation, Main sequence, Murnaghan equation of state, Neutron star, Polytropic process, Pressure, Radius, Red giant, Star, Stellar structure, Sun, Terrestrial planet, Thermodynamics, White dwarf.

Arthur Schuster

Sir Franz Arthur Friedrich Schuster FRS FRSE (12 September 1851 – 17 October 1934) was a German-born British physicist known for his work in spectroscopy, electrochemistry, optics, X-radiography and the application of harmonic analysis to physics.

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Astrophysics

Astrophysics is the branch of astronomy that employs the principles of physics and chemistry "to ascertain the nature of the astronomical objects, rather than their positions or motions in space".

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Brown dwarf

Brown dwarfs are substellar objects that occupy the mass range between the heaviest gas giant planets and the lightest stars, having masses between approximately 13 to 75–80 times that of Jupiter, or approximately to about.

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Bulk modulus

The bulk modulus (K or B) of a substance is a measure of how resistant to compressibility that substance is.

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Conceptual model

A conceptual model is a representation of a system, made of the composition of concepts which are used to help people know, understand, or simulate a subject the model represents.

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Constant (mathematics)

In mathematics, the adjective constant means non-varying.

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Degenerate matter

Degenerate matter is a highly dense state of matter in which particles must occupy high states of kinetic energy in order to satisfy the Pauli exclusion principle.

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Density

The density, or more precisely, the volumetric mass density, of a substance is its mass per unit volume.

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Equation of state

In physics and thermodynamics, an equation of state is a thermodynamic equation relating state variables which describe the state of matter under a given set of physical conditions, such as pressure, volume, temperature (PVT), or internal energy.

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Fluid

In physics, a fluid is a substance that continually deforms (flows) under an applied shear stress.

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Gas

Gas is one of the four fundamental states of matter (the others being solid, liquid, and plasma).

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Gas giant

A gas giant is a giant planet composed mainly of hydrogen and helium.

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Globular cluster

A globular cluster is a spherical collection of stars that orbits a galactic core as a satellite.

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Jupiter

Jupiter is the fifth planet from the Sun and the largest in the Solar System.

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Lane–Emden equation

In astrophysics, the Lane–Emden equation is a dimensionless form of Poisson's equation for the gravitational potential of a Newtonian self-gravitating, spherically symmetric, polytropic fluid.

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Main sequence

In astronomy, the main sequence is a continuous and distinctive band of stars that appear on plots of stellar color versus brightness.

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Murnaghan equation of state

The Murnaghan equation of state is a relationship between the volume of a body and the pressure to which it is subjected.

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Neutron star

A neutron star is the collapsed core of a large star which before collapse had a total of between 10 and 29 solar masses.

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Polytropic process

A polytropic process is a thermodynamic process that obeys the relation: where p is the pressure, V is volume, n is the polytropic index, and C is a constant.

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Pressure

Pressure (symbol: p or P) is the force applied perpendicular to the surface of an object per unit area over which that force is distributed.

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Radius

In classical geometry, a radius of a circle or sphere is any of the line segments from its center to its perimeter, and in more modern usage, it is also their length.

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Red giant

A red giant is a luminous giant star of low or intermediate mass (roughly 0.3–8 solar masses) in a late phase of stellar evolution.

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Star

A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.

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Stellar structure

Stars of different mass and age have varying internal structures.

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Sun

The Sun is the star at the center of the Solar System.

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Terrestrial planet

A terrestrial planet, telluric planet, or rocky planet is a planet that is composed primarily of silicate rocks or metals.

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Thermodynamics

Thermodynamics is the branch of physics concerned with heat and temperature and their relation to energy and work.

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White dwarf

A white dwarf, also called a degenerate dwarf, is a stellar core remnant composed mostly of electron-degenerate matter.

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References

[1] https://en.wikipedia.org/wiki/Polytrope

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