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Cosmological continuity equation

Energy conservation in FLRW gives

\overset{ρ}{˙} = - 3 H (ρ + P)

when

ρ

and

P

are energy density and pressure.

Table of contents 71 4
- Equation-of-state parameter Cosmological continuity equation 56 3
  - Quintessence Equation-of-state parameter 42 2
    - Quintessence scale-factor solution Quintessence 18
    - Quintessence-dominated universe Quintessence 13

 Ancestors (4)

 Incoming links (1)

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