Astronomy and astrophysics Definition
Virial mass
Builds on Friedmann equationsHubble's lawSpherical collapse modelVirial theorem
Definition
Let be the Hubble parameter at redshift , as in Hubble's law, and let be the critical density of the Friedmann equations. Fix an overdensity . Let a roughly spherical object have mass density at distance from its centre. Its virial radius is the radius at which the mean density inside equals : The virial mass is
Remarks
Common choices are , giving , and , the value the spherical collapse model predicts for a collapsed object in a universe of matter only. Some authors use the mean matter density instead of . The name comes from the virial theorem, which the matter inside approximately satisfies.
Example: a singular isothermal sphere has mean density inside . Setting this equal to gives and .
Non-example: a density that is constant out to infinity has mean density equal to that constant at every radius. If the constant is below , no radius satisfies the condition, and no virial mass is defined.
Reading path
To understand this page from the ground up, read these 91 pages in order. The foundations come first.
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- Additivity of the integral over intervals statement
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- C^k function characterised by continuous derivatives statement
- Integral equation form of an initial value problem statement
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- Classical mechanics definition
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- Virial theorem statement
- Virial mass definition
Further reading
About this page
| Tag | 8K5AM6EMWH |
|---|---|
| URI | m2://8K5AM6EMWH |
| Kind | definition |
| Writing | W0 stub |
| MSC | 85A15, 85A40 |
| Defines | Virial mass |
| Uses | Friedmann equations, Hubble's law, Spherical collapse model, Virial theorem |
| Changed | 3 November 2026 |
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