Cosmic time
This article may be too technical for most readers to understand.(April 2018) |
Cosmic time, or cosmological time, is the
Cosmic time [4][5] is a measure of time by a physical clock with zero peculiar velocity in the absence of matter over-/under-densities (to prevent time dilation due to relativistic effects or confusions caused by expansion of the universe). Unlike other measures of time such as temperature, redshift, particle horizon, or Hubble horizon, the cosmic time (similar and complementary to the comoving coordinates) is blind to the expansion of the universe.
There are two main ways for establishing a reference point for the cosmic time. The most trivial way is to take the present time as the cosmic reference point (sometimes referred to as the lookback time).
Alternatively, the Big Bang may be taken as reference to define as the age of the universe, also known as time since the big bang. The current physical cosmology estimates the present age as 13.8 billion years.[6] The doesn't necessarily have to correspond to a physical event (such as the
Cosmic time is the standard time coordinate for specifying the Friedmann–Lemaître–Robertson–Walker solutions of Einstein field equations.
See also
Notes
- ^ In mathematical terms, a cosmic time on spacetime is a fibration . This fibration, having the parameter , is made of three-dimensional manifolds .
- ^ On the physical basis of cosmic time by S.E. Rugh and H. Zinkernagel
- ISBN 0-19-859686-3.
- ISBN 9780122191411.
- ISBN 9780750308106.
- ^ How Old is the Universe?
References
- Dodelson, Scott (2003). Modern Cosmology. Academic Press. ISBN 978-0-12-219141-1.
- Bonometto, Silvio (2002). Modern Cosmology. Bristol and Philadelphia: Institute of Physics Publishing. ISBN 978-0750308106.