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The Birth of the Universe Through a Wormhole

Original: "Before the Bang: Wormholes at the Dawn of the Universe"
arXiv:2605.13777v2 · 2026-05-13 · CC BY 4.0 · ⏱ 1 min · HEP Theory General Relativity
Wormholes—microscopic tunnels in the fabric of space—offer a new explanation for the birth of the universe.
Abstract

Instead of the traditional "no-boundary" beginning, physicists are now considering tiny space-time tunnels (wormholes) as the key to the Universe's birth. This solves old problems and broadens the set of possible inflation scenarios. It's as if nature had a whole cookbook instead of just one recipe — which one did our Universe pick?

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Like a wormhole in an apple, a wormhole—a microscopic tunnel in the curved fabric of space—could have served as a passage for a newborn universe. This transition replaces the baffling point of singularity with a smooth birth from 'nothing,' an idea developed by Stephen Hawking. In the throat of the tunnel, inflationa rapid expansion—is triggered by the field that gives mass to particles, along with axion fields. This scenario naturally explains the uniformity of the cosmos, and quantum theory and the Standard Model of particles fit into it without breaking. Traces of this process are sought in the cosmic microwave background—ancient light from the Big Bang. The most surprising conclusion: the Big Bang wasn't an explosion at all, but a quiet tunnel transition.

🎯 In imaginary time, the geometry of a wormhole resembles a wine glass: a narrow 'stem' connecting two expanding regions. When transitioning to real time, the glass's throat becomes the birth point of a hot, rapidly expanding universe.

🎬 The idea of a tunnel from 'nothing' echoes the plot of 'Interstellar,' where heroes travel through a wormhole, but here the tunnel becomes a scientific scenario for the origin of the entire cosmos.

ds_E^2 = d\tau^2 + a^2(\tau) d\Omega_3^2
Euclidean time τ and scale factor a(τ) describe the geometry of a closed Universe.
\frac{a'^2}{a^2} - \frac{1}{a^2} + \frac{1}{3M_P^2} \left(V(\phi) - \frac{\phi'^2}{2}\right) - \frac{\tilde{\rho}_i}{a^{n_i}} = 0
The sum of curvature, potential, kinetic energy, and matter density contributions determines the evolution of the scale factor.
Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
Wormhole big bang inflation Quantum Field spacetime curvature Standard Model Higgs boson expansion of the universe axion cosmic microwave background
Laws
Friedmann equationsHubble's lawNoether's theoremEinstein field equationsPlanck's lawequivalence principle
Original: arXiv:2605.13777v2 · CC BY 4.0 · bridge42worlds