Luminosity distance, angular size and surface brightness in cosmological general relativity
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Publication:879983
DOI10.1007/S10701-007-9108-XzbMath1117.85023OpenAlexW2044056821MaRDI QIDQ879983
Firmin J. Oliveira, John G. Hartnett
Publication date: 10 May 2007
Published in: Foundations of Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10701-007-9108-x
Related Items (3)
Extending the redshift-distance relation in cosmological general relativity to higher redshifts ⋮ Cosmological general relativity with scale factor and dark energy ⋮ Spacetime curvature is important for cosmology constrained with supernova emissions
Cites Work
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- The distance modulus determined from Carmeli's cosmology fits the accelerating universe data of the high-redshift type ia supernovae without dark matter
- Carmeli's cosmology fits data for an accelerating and decelerating universe without dark matter or dark energy
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
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