MARATTO

article · Physics of the Dark Universe

Exploring <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si177.svg" display="inline" id="d1e1493"><mml:mrow><mml:mi>B</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>CDM models beyond <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si213.svg" display="inline" id="d1e1506"><mml:mi>Λ</mml:mi></mml:math>CDM: Observational data and cosmographic analysis

20248 citationsHassan II University Casablanca

In plain language

No abstract is available for this record, so no summary has been generated.

Research topics

  • Cosmology and Gravitation Theories
  • Galaxies: Formation, Evolution, Phenomena
  • Climate variability and models

Read the original research

This page summarises published work. The authoritative version sits with the publisher.

View on publisher siteRecord on OpenAlex

DOI: 10.1016/j.dark.2024.101555

Is something wrong with this record? Report it or request removal.

Discussion

Discuss this research

Have you built on this work, tried to replicate it, or seen it applied in practice? Share what you know. Verified researchers and MARATTO™ domain experts can open a discussion, and any member can reply. Contributions are reviewed before they appear.

No discussion yet. Open the first thread.

Sign in to join the discussion

New to MARATTO™? Create a free account.