text: 457,58,1518761665847775233,1019760963569049601,Almog Yalinewich,"New paper on the arxiv, in which we propose a model for fast radio bursts, in which fast spinning neutron stars with low magnetic fields are the progenitors, rather than magnetars (which are the progenitors in most other models) <LINK> @di_goldene_pave oops, should be equation 19. Thanks for catching it! The emission mechanism for the counterpart is the same as for the radio emission, the only difference is that the shock radius is smaller, and the Lorentz factor is higher, so the photons get boosted to a higher energy.",https://arxiv.org/abs/2204.11663,"Recent observations of coherent radiation from the Crab pulsar (Bij et al 2021) suggest the emission is driven by an ultra - relativistic ($\gamma \sim 10^4$), cold plasma flow. A relativistically expanding plasma shell can compress the ambient magnetic field, like a moving mirror, and thus produce coherent radiation whose wavelength is shorter than that of the ambient medium by $\gamma^2$. This mechanism has been studied in the past by Colgate and Noerdelinger (1971), in the context of radio loud supernova explosions. In this work we propose that a similar mechanism drives the coherent emission in fast radio bursts. The high Lorenz factors dramatically lower the implied energy and magnetic field requirements, allowing the spin down energy of regular (or even recycled), fast spinning pulsars, rather than slow spinning magnetars, to explain FRBs. We show that this model can explain the frequency and the time evolution of observed FRBs, as well as their duration, energetics and absence of panchromatic counterparts. We also predict that the peak frequency of sub pulses decline with observation time as $\omega_{\rm obs} \propto t_{\rm obs}^{-1/2}$. Unfortunately, with current capabilities it is not possible to constrain the shape of the curve $\omega_{\rm obs} \left(t_{\rm obs} \right)$. Finally, we find that a variation of this model can explain weaker radio transients, such as the one observed from a galactic magnetar. In this variant, the shock wave produces low frequency photons which are then Compton scattered to the GHz range. ",The Moving Mirror model for Fast Radio Bursts,2,"['New paper on the arxiv, in which we propose a model for fast radio bursts, in which fast spinning neutron stars with low magnetic fields are the progenitors, rather than magnetars (which are the progenitors in most other models)\n<LINK>', '@di_goldene_pave oops, should be equation 19. Thanks for catching it!\nThe emission mechanism for the counterpart is the same as for the radio emission, the only difference is that the shock radius is smaller, and the Lorentz factor is higher, so the photons get boosted to a higher energy.']",22,04,525