Friedmann model
(Friedmann universe, Friedmann-Lemaitre universe)
(type of model of universe incorporating general relativity)
A Friedmann model (Friedmann universe or Friedmann-Lemaitre universe)
is a type of mathematical model of the universe incorporating general relativity (GR).
Specific instances vary regarding the amount of mass, and whether
the amount is sufficient to reach or exceed the critical density.
An instance exactly at the critical density is termed an
Einstein-de Sitter model. Friedmann models are based the
Friedmann equations, a set of equations compatible with GR worked
out by Alexander Friedmann. Georges Lemaitre subsequently independently
worked out the same model.
(physics,model,cosmology)
Further reading:
https://en.wikipedia.org/wiki/Friedmann_equations
https://astronomy.swin.edu.au/cosmos/F/Friedmann-Lemaitre+Universe
http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/fried.html
http://astronomy.nmsu.edu/tharriso/ast110/class27.html
https://sites.astro.caltech.edu/~george/ay21/Ay21_Lec03.pdf
http://ned.ipac.caltech.edu/level5/Peacock/Peacock3_2.html
https://jila.colorado.edu/~pja/astr3830/lecture33.pdf
https://www.astro.umd.edu/~richard/ASTRO340/class16_RM_2014.pdf
Referenced by pages:
critical density (ρc)
Einstein-de Sitter model
redshift-angular size relation
scale factor (a)
Index