The age of the Universe is a direct consequence of its expansion history. By measuring the presentβday expansion rate, the Hubble constant (H_0), and how that rate has changed over time, we can infer how long the cosmos has been stretching.
In the standard (Lambda)CDM model the expansion is governed by the matter density (Omega_{m}), the darkβenergy density (Omega_{Lambda}), and any curvature term (Omega_{k}). For a flat universe (Omega_{k}=0) and the sum (Omega_{m}+Omega_{Lambda}=1). These parameters set the shape of the Friedmann equation, which determines the cosmic time as a function of redshift.
For a flat universe the age can be written analytically as
What is the Hubble constant?
How does the ΞCDM model describe the universe's expansion?
What is the significance of Omega_m in cosmology?
How does dark energy affect the age of the universe?
What is the current best estimate for the age of the universe?
How does curvature affect the calculation of the universe's age?
Can this calculator account for changes in the Hubble constant over time?
Results are for informational purposes only and do not constitute professional advice.
