English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We illustrate the constraints that a possible detection of a non-trivialspatial topology may place on the cosmological density parameters byconsidering the $\Lambda$CDM model Poincar\'e dodecahedal space (PDS) topologyas a circles-in-the-sky detectable topology. To this end we reanalyze the typeIa supernovae constraints on the density parameter plane$\Omega_k$--$\Omega_{\Lambda}$ and show that a circles-in-the-sky detectablePDS topology gives rise to important constraints on this parameters plane.Comment: 5 pages, 2 figs. To appear in the Proc. of 11th Marcel Grossmann  Meeting on General Relativity. Latex2e, World Scientific proc. style file

SUPERNOVAE CONSTRAINTS ON COSMOLOGICAL DENSITY PARAMETERS AND COSMIC TOPOLOGY