Mohamad Shalaby

Plasma Astrophysicist | HAPI Research Associate

No cosmological constraints on dark photon dark matter from resonant conversion:
Impact of nonlinear plasma dynamics

Anson Hook, Junwu Huang, and Mohamad Shalaby arXiv:2510.13956; submitted as PRL


This work overturns all previous constraints on dark photon dark matter by showing that its resonant conversion into ordinary plasma is highly inefficient, saturating at a very low level. As a result, the limits on dark photon dark matter are weakened by a factor of 3,000 to 10 million, rendering it effectively undetectable by current and near-future cosmological observations.


In the animations below: wavemode \(k = 2\pi/\lambda\), with marked scales \(k_D = 1/\lambda_D\) and \(\omega_p = 1/\lambda_e\) where \(\lambda\) is the wavelength, \(\lambda_D\) is the Debye length, and \(\lambda_e\) is electron skin depth.



DPDM resonant driving simulations

Resonant simulation \( A_0 = 10^{-3} \)  →  \( v_q^D / v_\mathrm{th}^e \approx 0.03 \)
Resonant simulation \( A_0 = 3\times 10^{-5} \)  →  \( v_q^D / v_\mathrm{th}^e \approx 10^{-3} \)



Landau Zener (LZ) simulations

LZ simulation \( A_0 = 3\times 10^{-2} \)  →  \( v_q^D / v_\mathrm{th}^e \approx 1 \)
LZ simulation \( A_0 = 3\times 10^{-3} \)  →  \( v_q^D / v_\mathrm{th}^e \approx 0.1 \)