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Ultra-relativistic oscillon collisions

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arxiv 1410.1822 v2 pith:BVCKAVDQ submitted 2014-10-07 hep-th astro-ph.HEnlin.PS

classification hep-thastro-ph.HEnlin.PS
keywords collisionsamplitudeoscillonsultra-relativisticleadingorderphasetemporal
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abstract

In this short note we investigate the ultra-relativistic collisions of small amplitude oscillons in 1+1 dimensions. Using the amplitude of the oscillons and the inverse relativistic boost factor $\gamma^{-1}$ as the perturbation variables, we analytically calculate the leading order spatial and temporal phase shifts, and the change in the amplitude of the oscillons after the collisions. At leading order, we find that only the temporal phase shift receives a nonzero contribution, and that the collision is elastic. This work is also the first application of the general kinematic framework for understanding ultra-relativistic collisions (arXiv:1308.0606) to intrinsically time-dependent solitons.

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  1. Generating Moving Field Initial Conditions with Spatially Varying Boost

    physics.comp-ph 2025-06 conditional novelty 7.0 of 10

    A 'spatially varying boost' algorithm assigns arbitrary, position-dependent bulk velocities to field initial data by composing local Lorentz boosts, demonstrated on solitons, Proca fields, and spin-1 wave dark matter.

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