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<p>The axion-like particle (ALP), a pseudo Nambu-Goldstone boson that couples to two photons, has been studied extensively in recent years as a dark matter candidate. For initial field configurations in a minimal ALP model explaining the observed dark matter abundance, we need the potential height to exceed the ALP energy density at redshift <i>z</i> ≈ 5.5 × 10<sup>6</sup> leading to:<InlineEquation ID="IEq1"> <EquationSource Format="TEX">\({f}_{\phi }\gtrsim 4\times {10}^{13}{\text{GeV}}\left(\frac{{10}^{-18}{\text{eV}}}{{m}_{\phi }}\right),\)</EquationSource> </InlineEquation></p><p>where <i>m</i><sub><i>ϕ</i></sub> and <i>f</i><sub><i>ϕ</i></sub> denote the ALP mass and decay constant, respectively. This bound is known for the ALP dark matter dominated by the homogeneous zero-momentum mode, under the requirement that coherent oscillations begin early enough to satisfy the late-forming dark matter constraint. One loop hole to evade this limit may be to introduce a large amount of the non-relativistic modes of the ALP with non-vanishing momenta. Here we show that the same limit remains valid even if nonzero-momentum modes dominate. Interestingly, when <i>nonrelativistic</i> gradient and kinetic modes prevail, the ALP behaves <i>relativistic</i> radiation rather than matter, if it violates the limit. Moreover, if the typical momentum is sufficiently small, Baumkuchen-like domain walls form, which play an important role in understanding the transition.</p>

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Relativistic axion with nonrelativistic momenta: a robust bound on minimal ALP dark matter

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  • 发表日期：

    2026年1月21日

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  • Yuma Narita,
  • Wen Yin

摘要

The axion-like particle (ALP), a pseudo Nambu-Goldstone boson that couples to two photons, has been studied extensively in recent years as a dark matter candidate. For initial field configurations in a minimal ALP model explaining the observed dark matter abundance, we need the potential height to exceed the ALP energy density at redshift z ≈ 5.5 × 106 leading to: \({f}_{\phi }\gtrsim 4\times {10}^{13}{\text{GeV}}\left(\frac{{10}^{-18}{\text{eV}}}{{m}_{\phi }}\right),\)

where mϕ and fϕ denote the ALP mass and decay constant, respectively. This bound is known for the ALP dark matter dominated by the homogeneous zero-momentum mode, under the requirement that coherent oscillations begin early enough to satisfy the late-forming dark matter constraint. One loop hole to evade this limit may be to introduce a large amount of the non-relativistic modes of the ALP with non-vanishing momenta. Here we show that the same limit remains valid even if nonzero-momentum modes dominate. Interestingly, when nonrelativistic gradient and kinetic modes prevail, the ALP behaves relativistic radiation rather than matter, if it violates the limit. Moreover, if the typical momentum is sufficiently small, Baumkuchen-like domain walls form, which play an important role in understanding the transition.