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Dynamical topological transitions in the massive Schwinger model with a {\theta}-term

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

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abstract

Aiming at a better understanding of anomalous and topological effects in gauge theories out-of-equilibrium, we study the real-time dynamics of a prototype model for CP-violation, the massive Schwinger model with a $\theta$-term. We identify dynamical quantum phase transitions between different topological sectors that appear after sufficiently strong quenches of the $\theta$-parameter. Moreover, we establish a general dynamical topological order parameter, which can be accessed through fermion two-point correlators and, importantly, which can be applied for interacting theories. Enabled by this result, we show that the topological transitions persist beyond the weak-coupling regime. Finally, these effects can be observed with table-top experiments based on existing cold-atom, superconducting-qubit, and trapped-ion technology. Our work, thus, presents a significant step towards quantum simulating topological and anomalous real-time phenomena relevant to nuclear and high-energy physics.

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2026 3

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Provable Quantum Advantage for Dynamical Phase Transition

quant-ph · 2026-06-29 · unverdicted · novelty 5.0

Proves intractability of DQPT estimation on quantum computers but equivalence of subsystem DQPT decision to quantum circuit simulation, with quadratic speedup for critical time search.

The Saddle Point of Everything

physics.gen-ph · 2026-05-28 · unverdicted · novelty 3.0

The inverted harmonic oscillator and its dual are argued to underpin a unique unitary renormalizable quantum gravity in four dimensions, yielding a non-singular universe and Starobinsky inflation.

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  • The Saddle Point of Everything physics.gen-ph · 2026-05-28 · unverdicted · none · ref 17 · internal anchor

    The inverted harmonic oscillator and its dual are argued to underpin a unique unitary renormalizable quantum gravity in four dimensions, yielding a non-singular universe and Starobinsky inflation.