We study the possibility of testing a dark matter (DM) scenario embedded in a global lepton number symmetry U(1)L via gravitational waves (GWs) and cosmic microwave background (CMB) observations. The spontaneous breaking of U(1)L symmetry generates the seesaw scale as well as DM mass dynamically. The (pseudo-)Nambu-Goldstone boson, known as a Majoron, acquires nonzero mass due to soft symmetry-breaking terms of quadratic type in the scalar potential, which eventually breaks U(1)L to its Z2 subgroup. The spontaneous symmetry breaking, which effectively breaks Z2, leads to the formation of domain walls (DWs), posing a threat to successful cosmology, if allowed to dominate. As gravity does not respect any global symmetries, we consider higher-dimensional operators suppressed by the scale of quantum gravity (QG), namely, ΛQG, which introduces the required bias leading to DW annihilation and emission of stochastic GWs observable at near future experiments. The same operators also lead to decay of DM bringing interesting indirect detection aspects. While DM is produced nonthermally via scalar portal interactions, light Majorons can give rise to additional ΔNeff within reach of future CMB experiments. Published by the American Physical Society 2024
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