Axion-like-particle dark matter beyond the standard paradigm
Cem Er\"oncel

TL;DR
This paper explores alternative mechanisms for axion-like particle (ALP) dark matter production beyond the standard misalignment scenario, highlighting exponential growth of fluctuations and potential observational signatures in extended parameter spaces.
Contribution
It introduces and discusses non-standard ALP production models that allow for exponential fluctuation growth, expanding the viable dark matter parameter space beyond traditional assumptions.
Findings
Standard paradigm cannot explain dark matter in certain parameter regions.
Alternative mechanisms enable exponential growth of ALP fluctuations.
Some ALP models become testable through gravitational interactions.
Abstract
Axions and axion-like particles (ALPs) are among the most popular candidates that explain the origin of the mysterious dark matter. The most popular ALP production mechanism studied in the literature is the misalignment mechanism, where an ALP field with a quadratic or cosine potential has negligible kinetic energy initially, and it starts oscillating when its mass becomes comparable to the Hubble scale. Recently, there has been an interest in models that go beyond the standard assumptions. These models not only extend the ALP dark matter parameter space, but also provide a rich phenomenology which is absent in the standard scenario. In particular, the ALP fluctuations grow exponentially via parametric resonance and tachyonic instabilities. In this proceeding, we will first demonstrate why the standard paradigm cannot explain dark matter in experimentally interesting parts of the…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Particle physics theoretical and experimental studies
