pith. sign in

Title resolution pending

Second Friedmann Equation The second modified Friedmann equation is obtained analogously to the first, now consideringq i =a(t) in Eq · 2023

1 Pith paper cite this work. Polarity classification is still indexing.

1 Pith paper citing it
browse 1 citing papers

Title metadata for this work has not finished resolving. The hub is built from the citation graph; the title resolver retries DOI and OpenAlex on its next pass.

fields

astro-ph.CO 1

years

2026 1

verdicts

UNVERDICTED 1

representative citing papers

Dynamical dark energy from Kretschmann scalar at low redshifts

astro-ph.CO · 2026-04-17 · unverdicted · novelty 5.0

Replacing the cosmological constant with the Kretschmann scalar yields a dynamical dark energy model that fits supernova and cosmic chronometer data and produces a phantom-crossing equation-of-state parameter w(z) similar to recent phenomenological fits.

citing papers explorer

Showing 1 of 1 citing paper.

  • Dynamical dark energy from Kretschmann scalar at low redshifts astro-ph.CO · 2026-04-17 · unverdicted · none · ref 3

    Replacing the cosmological constant with the Kretschmann scalar yields a dynamical dark energy model that fits supernova and cosmic chronometer data and produces a phantom-crossing equation-of-state parameter w(z) similar to recent phenomenological fits.