pith. machine review for the scientific record. sign in

Title resolution pending

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

4 Pith papers citing it

citation-role summary

background 2

citation-polarity summary

fields

hep-th 4

years

2026 4

verdicts

UNVERDICTED 4

roles

background 2

polarities

background 2

representative citing papers

Inflation and topology from the no-boundary state

hep-th · 2026-05-06 · unverdicted · novelty 7.0

The no-boundary wavefunction on the 3-torus, summed over SL(3,Z) geometries using GL(3) automorphic forms, favors large inflating universes with N ≳ 250 e-folds and induces torus-moduli corrections to the CMB spectrum.

The yes boundaries wavefunctions of the universe

hep-th · 2026-04-11 · unverdicted · novelty 6.0

Using two timelike boundaries and a nearly maximally entangled thermofield double state from dressed de Sitter Hamiltonian theories, the authors construct wavefunctions for extended cosmological spacetimes that include the future wedge and resolve entanglement entropy issues via 3D constrained path

citing papers explorer

Showing 4 of 4 citing papers.

  • A Tale of Two Hartle-Hawking Wave Functions: Fully Gravitational vs Partially Frozen hep-th · 2026-05-13 · unverdicted · none · ref 55

    In AdS the fully gravitational Hartle-Hawking wave function acquires a nontrivial one-loop phase while the partially frozen version stays real and positive; a partially frozen de Sitter sphere shows phase cancellation.

  • Inflation and topology from the no-boundary state hep-th · 2026-05-06 · unverdicted · none · ref 39

    The no-boundary wavefunction on the 3-torus, summed over SL(3,Z) geometries using GL(3) automorphic forms, favors large inflating universes with N ≳ 250 e-folds and induces torus-moduli corrections to the CMB spectrum.

  • The yes boundaries wavefunctions of the universe hep-th · 2026-04-11 · unverdicted · none · ref 70

    Using two timelike boundaries and a nearly maximally entangled thermofield double state from dressed de Sitter Hamiltonian theories, the authors construct wavefunctions for extended cosmological spacetimes that include the future wedge and resolve entanglement entropy issues via 3D constrained path

  • The Fate of Nucleated Black Holes in de Sitter Quantum Gravity hep-th · 2026-05-04 · unverdicted · none · ref 104 · 2 links

    Nucleated black holes in de Sitter space evaporate via standard Hawking radiation back to the empty vacuum, rendering nucleation a temporary fluctuation.