pith. sign in

Battista, Nonsingular bouncing cosmology in general relativity: Physical analysis of the spacetime defect, Class

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it

citation-role summary

background 3

citation-polarity summary

fields

gr-qc 3

years

2026 3

verdicts

UNVERDICTED 3

roles

background 3

polarities

background 3

representative citing papers

Families of regular spacetimes and energy conditions

gr-qc · 2026-05-05 · unverdicted · novelty 7.0 · 2 refs

A classification of admissible energy density profiles with bounded Kretschmann scalar yields a unified framework for regular static spherically symmetric spacetimes satisfying the weak energy condition, recovering known models and producing new families with hypergeometric and other closed forms.

Big Bang revisited

gr-qc · 2026-03-31 · unverdicted · novelty 5.0

A degenerate spacetime metric is proposed to remove the Big Bang curvature singularity from the Friedmann solution, alongside discussion of CPT-conjugated worlds and an extended Einstein field equation.

citing papers explorer

Showing 3 of 3 citing papers.

  • Families of regular spacetimes and energy conditions gr-qc · 2026-05-05 · unverdicted · none · ref 81 · 2 links

    A classification of admissible energy density profiles with bounded Kretschmann scalar yields a unified framework for regular static spherically symmetric spacetimes satisfying the weak energy condition, recovering known models and producing new families with hypergeometric and other closed forms.

  • Energy conditions in static, spherically symmetric spacetimes and effective geometries gr-qc · 2026-04-17 · unverdicted · none · ref 67

    A logarithmic correction to Schwarzschild in static spherical symmetry obeys all classical energy conditions and serves as an effective exterior for horizon-bearing and horizonless compact objects.

  • Big Bang revisited gr-qc · 2026-03-31 · unverdicted · none · ref 14

    A degenerate spacetime metric is proposed to remove the Big Bang curvature singularity from the Friedmann solution, alongside discussion of CPT-conjugated worlds and an extended Einstein field equation.