Spacetime curvature is important for cosmology constrained with supernova emissions

DOI10.1007/S10773-008-9680-7zbMath1161.83465OpenAlexW2119693381MaRDI QIDQ1008162

Michael L. Smith, Jan Paul, Ahmet Mecit Öztaş

Publication date: 24 March 2009

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-15434

zbMATH Keywords

supernovaemissionPlanck constantredshiftFRW

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Astrophysical cosmology (85A40)

Related Items (1)

The cosmological constant constrained with Union2.1 supernovae type Ia data

Cites Work

• Carmeli's cosmology fits data for an accelerating and decelerating universe without dark matter or dark energy
• Luminosity distance, angular size and surface brightness in cosmological general relativity
• Estimating the dimension of a model
• Cosmological relativity: a new theory of cosmology
• Derivation of the Tully-Fisher law: Doubts about the necessity and existence of halo dark matter
• A model of light from ancient blue emissions
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

This page was built for publication: Spacetime curvature is important for cosmology constrained with supernova emissions