pith. sign in

Kibble, Topology of Cosmic Domains and Strings , J

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

3 Pith papers citing it

citation-role summary

background 1

citation-polarity summary

years

2026 1 2025 2

roles

background 1

polarities

background 1

representative citing papers

Type II Seesaw Leptogenesis in a Majoron background

hep-ph · 2025-06-29 · unverdicted · novelty 5.0

Spontaneous wash-in leptogenesis in Type II Seesaw with Majoron pNGB background enables baryon asymmetry generation alongside dark matter cogenesis for specific v_T, v_sigma and m_j ranges.

Cosmic Strings as Dynamical Dark Energy: Novel Constraints

astro-ph.CO · 2025-05-28 · conditional · novelty 4.0

Cosmic string networks are constrained to less than ~1% of the energy density using CMB+BAO+SN data, with some models preferring mildly negative densities but no Bayesian evidence favoring them over LambdaCDM.

citing papers explorer

Showing 3 of 3 citing papers.

  • Bubble dynamics and vortex formation in holographic first-order superfluid phase transitions hep-th · 2026-04-19 · unverdicted · none · ref 30

    Holographic simulations of first-order superfluid transitions reveal that three-bubble collisions produce annihilating vortex-antivortex pairs whose lifetime scales logarithmically near critical radii, deviating from the geodesic rule.

  • Type II Seesaw Leptogenesis in a Majoron background hep-ph · 2025-06-29 · unverdicted · none · ref 162

    Spontaneous wash-in leptogenesis in Type II Seesaw with Majoron pNGB background enables baryon asymmetry generation alongside dark matter cogenesis for specific v_T, v_sigma and m_j ranges.

  • Cosmic Strings as Dynamical Dark Energy: Novel Constraints astro-ph.CO · 2025-05-28 · conditional · none · ref 1

    Cosmic string networks are constrained to less than ~1% of the energy density using CMB+BAO+SN data, with some models preferring mildly negative densities but no Bayesian evidence favoring them over LambdaCDM.