Interacting dark energy with CPL admits exact solutions via incomplete gamma functions; Q proportional to dark energy density modestly improves AIC fit but BIC prefers LambdaCDM, showing phantom-to-quintessence transition and possible future transient acceleration.
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Neutrino and HDM wakes provide a smoking-gun signature of free-streaming effects in large-scale structure that cannot be mimicked by dynamical dark energy, detectable at high SNR in idealistic 3D HDM tracer maps for k_fs,0 ≳ 0.1 Mpc^{-1} when HDM is ~1% of total dark matter.
A Z2-symmetric SM extension with vector-like fermions and an inert scalar doublet generates neutrino masses radiatively, accounts for (g-2)e,μ anomalies, and yields the observed DM relic abundance while satisfying LFV, direct detection, BBN, and CMB bounds.
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Cosmological evolution of interacting dark energy with a CPL equation of state
Interacting dark energy with CPL admits exact solutions via incomplete gamma functions; Q proportional to dark energy density modestly improves AIC fit but BIC prefers LambdaCDM, showing phantom-to-quintessence transition and possible future transient acceleration.
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Dark winds on the horizon: Prospects for detecting neutrino and hot dark matter wakes in large-scale structure
Neutrino and HDM wakes provide a smoking-gun signature of free-streaming effects in large-scale structure that cannot be mimicked by dynamical dark energy, detectable at high SNR in idealistic 3D HDM tracer maps for k_fs,0 ≳ 0.1 Mpc^{-1} when HDM is ~1% of total dark matter.
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Neutrino masses, anomalous magnetic moments and dark matter with vector-like fermions and an inert scalar doublet
A Z2-symmetric SM extension with vector-like fermions and an inert scalar doublet generates neutrino masses radiatively, accounts for (g-2)e,μ anomalies, and yields the observed DM relic abundance while satisfying LFV, direct detection, BBN, and CMB bounds.