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Heat transfer between baryons and millicharged dark matter has been invoked as a possible explanation for the anomalous 21-cm absorption signal seen by EDGES. Prior work has shown that the solution requires that millicharged particles make up only a fraction $(m_chi/{rm MeV}) 0.0115% lesssim f lesssim 0.4%$ of the dark matter and that their mass $m_chi$ and charge $q_chi$ have values $0.1 lesssim (m_chi/{rm MeV})lesssim 10$ and $10^{-6} lesssim (q_chi/e)lesssim 10^{-4}$. Here we show that such particles come into chemical equilibrium before recombination, and so are subject to a constraint on the effective number $N_{rm eff}$ of relativistic degrees of freedom, which we update using Planck 2018 data. We moreover determine the precise relic abundance $f$ that results for a given mass $m_chi$ and charge $q_chi$ and incorporate this abundance into the constraints on the millicharged-dark-matter solution to EDGES. With these two results, the solution is ruled out if the relic abundance is set by freeze-out.
We consider the implications of an ultra-light fermionic dark matter candidate that carries baryon number. This naturally arises if dark matter has a small charge under standard model baryon number whilst having an asymmetry equal and opposite to tha
We investigate the hypothesis that Coulomb-type interactions between dark matter (DM) and baryons explain the anomalously low 21cm brightness-temperature minimum at redshift z ~ 17 that was recently measured by the EDGES experiment. In particular, we
The next generation of axion direct detection experiments may rule out or confirm axions as the dominant source of dark matter. We develop a general likelihood-based framework for studying the time-series data at such experiments, with a focus on the
We present a possible explanation of the recently observed 511 keV $gamma$-ray anomaly with a new ``millicharged fermion. The new fermion is light (${cal O}({rm MeV})$) but has never been observed by any collider experiments mainly because of its tin
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