Pulsation periods and stellar density
Radial stellar pulsation has a characteristic gravitational/acoustic period scale proportional to √[R³/(GM)].
Key knowledge
Radial stellar pulsation has a characteristic gravitational/acoustic period scale proportional to √[R³/(GM)]. Dimensionless mode frequencies also depend on the internal density, sound-speed and adiabatic-exponent profiles. Homologous model families share these scaled frequencies; real stellar periods cannot be inferred from mean density alone.
Values and equations
σ²=ω²R³/(GM); characteristic period∼√[R³/(GM)]
- σ
- dimensionless angular mode frequency 1
- ω
- angular mode frequency rad s⁻¹
- R,M
- stellar radius and mass m, kg
- G
- gravitational constant m³ kg⁻¹ s⁻²
Conditions and scope
- Small-amplitude adiabatic oscillations about a suitable hydrostatic model for the mode-scaling interpretation; a characteristic timescale is not an exact measured period.
- The radial order, angular degree, equilibrium structure and boundary conditions determine a mode; rotation, magnetic fields and nonadiabatic excitation add further physics.
Sources · 1
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
Read the radial dynamical-period introduction and actual dimensionless mass/radius scaling in§5.1.3, including the distinction between homologous and realistic structures; no claim of reading all276 pages or of exact solar/exoplanet inference.
2026-10-10 · Independent AI editorial review: All44 exact root-authored compact records, equations/variable units/conditions and140 origin edges accepted after independently reading final6/18 with bounded primary bodies and matching prior38/122 scientific fingerprints unchanged. Exact claim/edge review is distinct from combined inventory scope and separate CLE26 approval; no entire cited books or old-corpus experimental revalidation is asserted. Receipt: cosmos-completion-independent-content-and-inventory-review.1.
Entry details
Permanent link to this entry ↗- Record identity
- uni-cosmos-stellar-pulsation-density
- Revision
- core.1
- Structured reference record
- University core expansion