Cosmodynamics: Energy conditions, Hubble bounds, density bounds, time and distance bounds

Understand

We refine and extend a programme initiated by one of the current authors [Science 276 (1997) 88; Phys.

• Rev.
• D56 (1997) 7578] advocating the use of the classical energy conditions of general relativity in a cosmological setting to place very general bounds on various cosmological parameters.
• We show how the energy conditions can be used to bound the Hubble parameter H(z), Omega parameter Omega(z), density rho(z), distance d(z), and lookback time T(z) as (relatively) simple functions of the redshift z, present-epoch Hubble parameter H_0, and present-epoch Omega parameter Omega_0.